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709.0635
Poisson Sigma Model with branes and hyperelliptic Riemann surfaces
We derive the explicit form of the superpropagators in presence of general boundary conditions (coisotropic branes) for the Poisson Sigma Model. This generalizes the results presented in Cattaneo and Felder's previous works for the Kontsevich angle function used in the deformation quantization program of Poisson manifolds without branes or with at most two branes. The relevant superpropagators for n branes are defined as gauge fixed homotopy operators of a complex of differential forms on n sided polygons P_n with particular "alternating" boundary conditions. In presence of more than three branes we use first order Riemann theta functions with odd singular characteristics on the Jacobian variety of a hyperelliptic Riemann surface (canonical setting). In genus g the superpropagators present g zero modes contributions.
math-ph hep-th math.CV math.MP
we derive the explicit form of the superpropagators in presence of general boundary conditions coisotropic branes for the poisson sigma model this generalizes the results presented in cattaneo and felders previous works for the kontsevich angle function used in the deformation quantization program of poisson manifolds without branes or with at most two branes the relevant superpropagators for n branes are defined as gauge fixed homotopy operators of a complex of differential forms on n sided polygons p_n with particular alternating boundary conditions in presence of more than three branes we use first order riemann theta functions with odd singular characteristics on the jacobian variety of a hyperelliptic riemann surface canonical setting in genus g the superpropagators present g zero modes contributions
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709.0636
Internal chemo-dynamical Modeling of Gas Exchange within Galaxies and with their Environment
By a few but important examples as models of combined radiative and wind-driven HII regions and galactic winds we demonstrate the importance of refined small-to-medium scale studies of chemo-dynamical effects. These processes determine the internal dynamics and energetic of the ISM and affect its observational signatures, e.g. by abundance contributions, but are not yet reliably and satisfactorily explored.
astro-ph
by a few but important examples as models of combined radiative and winddriven hii regions and galactic winds we demonstrate the importance of refined smalltomedium scale studies of chemodynamical effects these processes determine the internal dynamics and energetic of the ism and affect its observational signatures eg by abundance contributions but are not yet reliably and satisfactorily explored
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709.0637
Sample path properties of the local time of multifractional Brownian motion
We establish estimates for the local and uniform moduli of continuity of the local time of multifractional Brownian motion, $B^H=(B^{H(t)}(t),t\in\mathbb{R}^+)$. An analogue of Chung's law of the iterated logarithm is studied for $B^H$ and used to obtain the pointwise H\"{o}lder exponent of the local time. A kind of local asymptotic self-similarity is proved to be satisfied by the local time of $B^H$.
math.PR
we establish estimates for the local and uniform moduli of continuity of the local time of multifractional brownian motion bhbhtttinmathbbr an analogue of chungs law of the iterated logarithm is studied for bh and used to obtain the pointwise holder exponent of the local time a kind of local asymptotic selfsimilarity is proved to be satisfied by the local time of bh
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709.0638
Asymptotic behavior of grafting rays
In this paper we study the convergence behavior of grafting rays to the Thurston boundary of Teichmuller space. When the grafting is done along a weighted system of simple closed curves or along a maximal uniquely ergodic lamination this behavior is the same as for Teichmuller geodesics and lines of minima. We also show that the ray grafted along a weighted system of simple closed curves is at bounded distance from Teichmuller geodesic.
math.GT
in this paper we study the convergence behavior of grafting rays to the thurston boundary of teichmuller space when the grafting is done along a weighted system of simple closed curves or along a maximal uniquely ergodic lamination this behavior is the same as for teichmuller geodesics and lines of minima we also show that the ray grafted along a weighted system of simple closed curves is at bounded distance from teichmuller geodesic
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709.0639
Atomic Diffusion and Mixing in Old Stars I. VLT/FLAMES-UVES Observations of Stars in NGC 6397
We present a homogeneous photometric and spectroscopic analysis of 18 stars along the evolutionary sequence of the metal-poor globular cluster NGC 6397 ([Fe/H] = -2), from the main-sequence turnoff point to red giants below the bump. The spectroscopic stellar parameters, in particular stellar-parameter differences between groups of stars, are in good agreement with broad-band and Stroemgren photometry calibrated on the infrared-flux method. The spectroscopic abundance analysis reveals, for the first time, systematic trends of iron abundance with evolutionary stage. Iron is found to be 31% less abundant in the turnoff-point stars than in the red giants. An abundance difference in lithium is seen between the turnoff-point and warm subgiant stars. The impact of potential systematic errors on these abundance trends (stellar parameters, the hydrostatic and LTE approximations) is quantitatively evaluated and found not to alter our conclusions significantly. Trends for various elements (Li, Mg, Ca, Ti and Fe) are compared with stellar-structure models including the effects of atomic diffusion and radiative acceleration. Such models are found to describe the observed element-specific trends well, if extra (turbulent) mixing just below the convection zone is introduced. It is concluded that atomic diffusion and turbulent mixing are largely responsible for the sub-primordial stellar lithium abundances of warm halo stars. Other consequences of atomic diffusion in old metal-poor stars are also discussed.
astro-ph
we present a homogeneous photometric and spectroscopic analysis of 18 stars along the evolutionary sequence of the metalpoor globular cluster ngc 6397 feh 2 from the mainsequence turnoff point to red giants below the bump the spectroscopic stellar parameters in particular stellarparameter differences between groups of stars are in good agreement with broadband and stroemgren photometry calibrated on the infraredflux method the spectroscopic abundance analysis reveals for the first time systematic trends of iron abundance with evolutionary stage iron is found to be 31 less abundant in the turnoffpoint stars than in the red giants an abundance difference in lithium is seen between the turnoffpoint and warm subgiant stars the impact of potential systematic errors on these abundance trends stellar parameters the hydrostatic and lte approximations is quantitatively evaluated and found not to alter our conclusions significantly trends for various elements li mg ca ti and fe are compared with stellarstructure models including the effects of atomic diffusion and radiative acceleration such models are found to describe the observed elementspecific trends well if extra turbulent mixing just below the convection zone is introduced it is concluded that atomic diffusion and turbulent mixing are largely responsible for the subprimordial stellar lithium abundances of warm halo stars other consequences of atomic diffusion in old metalpoor stars are also discussed
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709.064
Algebraic theta functions and Eisenstein-Kronecker numbers
In this paper, we give an overview of our previous paper concerning the investigation of the algebraic and $p$-adic properties of Eisenstein-Kronecker numbers using Mumford's theory of algebraic theta functions.
math.NT math.AG
in this paper we give an overview of our previous paper concerning the investigation of the algebraic and padic properties of eisensteinkronecker numbers using mumfords theory of algebraic theta functions
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709.0641
Coherent control for the spherical symmetric box potential in short and intensive XUV laser fields
Coherent control calculations are presented for a spherically symmetric box potential for non-resonant two photon transition probabilities. With the help of a genetic algorithm (GA) the population of the excited states are maximized and minimized. The external driving field is a superposition of three intensive extreme ultraviolet (XUV) linearly polarized laser pulses with different frequencies in the femtosecond duration range. We solved the quantum mechanical problem within the dipole approximation. Our investigation clearly shows that the dynamics of the electron current has a strong correlation with the optimized and neutralizing pulse shape.
physics.optics physics.atom-ph
coherent control calculations are presented for a spherically symmetric box potential for nonresonant two photon transition probabilities with the help of a genetic algorithm ga the population of the excited states are maximized and minimized the external driving field is a superposition of three intensive extreme ultraviolet xuv linearly polarized laser pulses with different frequencies in the femtosecond duration range we solved the quantum mechanical problem within the dipole approximation our investigation clearly shows that the dynamics of the electron current has a strong correlation with the optimized and neutralizing pulse shape
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709.0642
Geometry of Liquid Crystals and the alignment of HIV-1 virus helical filaments
Geometry of Liquid crystals as detectors of HIV twisted helical filaments is presented.
cond-mat.mtrl-sci cond-mat.soft
geometry of liquid crystals as detectors of hiv twisted helical filaments is presented
[['geometry', 'of', 'liquid', 'crystals', 'as', 'detectors', 'of', 'hiv', 'twisted', 'helical', 'filaments', 'is', 'presented']]
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709.0643
Effects of interactions in transport through Aharonov-Bohm-Casher interferometers
We study the conductance through a ring described by the Hubbard model (such as an array of quantum dots), threaded by a magnetic flux and subject to Rashba spin-orbit coupling (SOC). We develop a formalism that is able to describe the interference effects as well as the Kondo effect when the number of electrons in the ring is odd. In the Kondo regime, the SOC reduces the conductance from the unitary limit, and in combination with the magnetic flux, the device acts as a spin polarizer.
cond-mat.str-el
we study the conductance through a ring described by the hubbard model such as an array of quantum dots threaded by a magnetic flux and subject to rashba spinorbit coupling soc we develop a formalism that is able to describe the interference effects as well as the kondo effect when the number of electrons in the ring is odd in the kondo regime the soc reduces the conductance from the unitary limit and in combination with the magnetic flux the device acts as a spin polarizer
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709.0644
One-loop Self-energy and Counterterms in a Massive Yang-Mills Theory based on the Nonlinearly Realized Gauge Group
In this paper we evaluate the self-energy of the vector mesons at one loop in our recently proposed subtraction scheme for massive nonlinearly realized SU(2) Yang-Mills theory. We check the fulfillment of physical unitarity. The resulting self-mass can be compared with the value obtained in the massive Yang-Mills theory based on the Higgs mechanism, consisting in extra terms due to the presence of the Higgs boson (tadpoles included). Moreover we evaluate all the one-loop counterterms necessary for the next order calculations. By construction they satisfy all the equations of the model (Slavnov-Taylor, local functional equation and Landau gauge equation). They are sufficient to make all the one-loop amplitudes finite through the hierarchy encoded in the local functional equation.
hep-th hep-ph
in this paper we evaluate the selfenergy of the vector mesons at one loop in our recently proposed subtraction scheme for massive nonlinearly realized su2 yangmills theory we check the fulfillment of physical unitarity the resulting selfmass can be compared with the value obtained in the massive yangmills theory based on the higgs mechanism consisting in extra terms due to the presence of the higgs boson tadpoles included moreover we evaluate all the oneloop counterterms necessary for the next order calculations by construction they satisfy all the equations of the model slavnovtaylor local functional equation and landau gauge equation they are sufficient to make all the oneloop amplitudes finite through the hierarchy encoded in the local functional equation
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709.0645
A Substellar Companion to the Intermediate-Mass Giant 11 Com
We report the detection of a substellar companion orbiting the intermediate-mass giant star 11 Com (G8 III). Precise Doppler measurements of the star from Xinglong station and Okayama Astrophysical Observatory (OAO) revealed Keplerian velocity variations with an orbital period of 326.03 +/- 0.32 days, a semiamplitude of 302.8 +/- 2.6 m/s, and an eccentricity of 0.231 +/- 0.005. Adopting a stellar mass of 2.7 +/- 0.3 M_solar, the minimum mass of the companion is 19.4 +/- 1.5 M_Jup, well above the deuterium burning limit, and the semimajor axis is 1.29 +/- 0.05 AU. This is the first result from the joint planet search program between China and Japan aiming at revealing statistics of substellar companions around intermediate-mass giants. 11 Com b emerged from 300 targets of the planet search program at OAO. The current detection rate of a brown dwarf candidate seems to be comparable to that around solar-type stars within orbital separations of $\sim$3 AU.
astro-ph
we report the detection of a substellar companion orbiting the intermediatemass giant star 11 com g8 iii precise doppler measurements of the star from xinglong station and okayama astrophysical observatory oao revealed keplerian velocity variations with an orbital period of 32603 032 days a semiamplitude of 3028 26 ms and an eccentricity of 0231 0005 adopting a stellar mass of 27 03 m_solar the minimum mass of the companion is 194 15 m_jup well above the deuterium burning limit and the semimajor axis is 129 005 au this is the first result from the joint planet search program between china and japan aiming at revealing statistics of substellar companions around intermediatemass giants 11 com b emerged from 300 targets of the planet search program at oao the current detection rate of a brown dwarf candidate seems to be comparable to that around solartype stars within orbital separations of sim3 au
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709.0646
Algebraic solution of a graphene layer in a transverse electric and perpendicular magnetic fields
We present an exact algebraic solution of a single graphene plane in transverse electric and perpendicular magnetic fields. The method presented gives both the eigen-values and the eigen-functions of the graphene plane. It is shown that the eigen-states of the problem can be casted in terms of coherent states, which appears in a natural way from the formalism.
cond-mat.mes-hall
we present an exact algebraic solution of a single graphene plane in transverse electric and perpendicular magnetic fields the method presented gives both the eigenvalues and the eigenfunctions of the graphene plane it is shown that the eigenstates of the problem can be casted in terms of coherent states which appears in a natural way from the formalism
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709.0647
Sharp constants related to the triangle inequality in Lorentz spaces
We study the Lorentz spaces $L^{p,s}(R,\mu)$ in the range $1<p<s\le \infty$, for which the standard functional $$ ||f||_{p,s}=(\int_0^\infty (t^{1/p}f^*(t))^s\frac{dt}{t})^{1/s} $$ is only a quasi-norm. We find the optimal constant in the triangle inequality for this quasi-norm, which leads us to consider the following decomposition norm: $$ ||f||_{(p,s)}=\inf\bigg\{\sum_{k}||f_k||_{p,s}\bigg\}, $$ where the infimum is taken over all finite representations $f=\sum_{k}f_k. $ We also prove that the decomposition norm and the dual norm $$ ||f||_{p,s}'= \sup\left\{\int_R fg d\mu: ||g||_{p',s'}=1\right\} $$ agree for all values $p,s>1$.
math.FA math.CA
we study the lorentz spaces lpsrmu in the range 1psle infty for which the standard functional f_psint_0infty t1pftsfracdtt1s is only a quasinorm we find the optimal constant in the triangle inequality for this quasinorm which leads us to consider the following decomposition norm f_psinfbiggsum_kf_k_psbigg where the infimum is taken over all finite representations fsum_kf_k we also prove that the decomposition norm and the dual norm f_ps supleftint_r fg dmu g_ps1right agree for all values ps1
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709.0648
Rearrangement transformations on general measure spaces
For a general set transformation ${\cal R}$ between two measure spaces, we define the rearrangement of a measurable function by means of the Layer's cake formula. We study some functional properties of the Lorentz spaces defined in terms of ${\cal R}$, giving a unified approach to the classical rearrangement, Steiner's symmetrization, the multidimensional case, and the discrete setting of trees.
math.FA
for a general set transformation cal r between two measure spaces we define the rearrangement of a measurable function by means of the layers cake formula we study some functional properties of the lorentz spaces defined in terms of cal r giving a unified approach to the classical rearrangement steiners symmetrization the multidimensional case and the discrete setting of trees
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709.0649
Oscillation of Tc depending on the number of CuO2 planes in the cuprates
Using the Tc formula given by BCS, together with a shear modulus varying with the numbering of planes, we can demonstrate that Tc oscillates depending on the number of the cuprate planes. The maximum of Tc in these oscillations appears for three planes irrespective of the cuprate family. Comparison with experimental data shows good agreement and suggests that the electron-phonon coupling predominate in the superconductivity of these materials. This model predicts that such oscillations can also occur in many others physical quantities that depend on Tc. The new Tc formula shows interesting prospects towards room temperature superconductors.
cond-mat.supr-con cond-mat.mtrl-sci
using the tc formula given by bcs together with a shear modulus varying with the numbering of planes we can demonstrate that tc oscillates depending on the number of the cuprate planes the maximum of tc in these oscillations appears for three planes irrespective of the cuprate family comparison with experimental data shows good agreement and suggests that the electronphonon coupling predominate in the superconductivity of these materials this model predicts that such oscillations can also occur in many others physical quantities that depend on tc the new tc formula shows interesting prospects towards room temperature superconductors
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709.065
Limit theorems for functionals on the facets of stationary random tessellations
We observe stationary random tessellations $X=\{\Xi_n\}_{n\ge1}$ in $\mathbb{R}^d$ through a convex sampling window $W$ that expands unboundedly and we determine the total $(k-1)$-volume of those $(k-1)$-dimensional manifold processes which are induced on the $k$-facets of $X$ ($1\le k\le d-1$) by their intersections with the $(d-1)$-facets of independent and identically distributed motion-invariant tessellations $X_n$ generated within each cell $\Xi_n$ of $X$. The cases of $X$ being either a Poisson hyperplane tessellation or a random tessellation with weak dependences are treated separately. In both cases, however, we obtain that all of the total volumes measured in $W$ are approximately normally distributed when $W$ is sufficiently large. Structural formulae for mean values and asymptotic variances are derived and explicit numerical values are given for planar Poisson--Voronoi tessellations (PVTs) and Poisson line tessellations (PLTs).
math.PR
we observe stationary random tessellations xxi_n_nge1 in mathbbrd through a convex sampling window w that expands unboundedly and we determine the total k1volume of those k1dimensional manifold processes which are induced on the kfacets of x 1le kle d1 by their intersections with the d1facets of independent and identically distributed motioninvariant tessellations x_n generated within each cell xi_n of x the cases of x being either a poisson hyperplane tessellation or a random tessellation with weak dependences are treated separately in both cases however we obtain that all of the total volumes measured in w are approximately normally distributed when w is sufficiently large structural formulae for mean values and asymptotic variances are derived and explicit numerical values are given for planar poissonvoronoi tessellations pvts and poisson line tessellations plts
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709.0651
GRB970228 and a class of GRBs with an initial spikelike emission
(Shortened) The Swift and HETE-2 discovery of an afterglow associated possibly with short GRBs opened the new problematic of their nature and classification. This has been further enhanced by the GRB060614 observation and by a re-analysis of the BATSE catalog leading to the identification of a new GRB class with "an occasional softer extended emission lasting tenths of seconds after an initial spikelike emission". We plan: a) to fit this new class of "hybrid" sources within our "canonical GRB" scenario, where all GRBs are generated by a "common engine" (i.e. the gravitational collapse to a black hole); b) to propose GRB970228 as the prototype of the such a class. We analyze BeppoSAX data on GRB970228 in the 40-700 keV and 2-26 keV energy bands within the "fireshell" model. We find that GRB970228 is a "canonical GRB", like e.g. GRB050315, with the main peculiarity of a particularly low CircumBurst Medium (CBM) average density n_{cbm}~10^{-3} #/cm^3. We also simulate the light curve corresponding to a rescaled CBM density profile with n_{cbm}=1 #/cm^3. From such a comparison it follows that the total time-integrated luminosity is a faithful indicator of the GRB nature, contrary to the peak luminosity which is merely a function of the CBM density. We call attention on discriminating the short GRBs between the "genuine" and the "fake" ones. The "genuine" ones are intrinsically short, with baryon loading B \la 10^{-5}, as stated in our original classification. The "fake" ones, characterized by an initial spikelike emission followed by an extended emission lasting tenths of seconds, have a baryon loading 10^{-4} \la B \leq 10^{-2}. They are observed as such only due to an underdense CBM consistent with a galactic halo environment which deflates the afterglow intensity.
astro-ph
shortened the swift and hete2 discovery of an afterglow associated possibly with short grbs opened the new problematic of their nature and classification this has been further enhanced by the grb060614 observation and by a reanalysis of the batse catalog leading to the identification of a new grb class with an occasional softer extended emission lasting tenths of seconds after an initial spikelike emission we plan a to fit this new class of hybrid sources within our canonical grb scenario where all grbs are generated by a common engine ie the gravitational collapse to a black hole b to propose grb970228 as the prototype of the such a class we analyze bepposax data on grb970228 in the 40700 kev and 226 kev energy bands within the fireshell model we find that grb970228 is a canonical grb like eg grb050315 with the main peculiarity of a particularly low circumburst medium cbm average density n_cbm103 cm3 we also simulate the light curve corresponding to a rescaled cbm density profile with n_cbm1 cm3 from such a comparison it follows that the total timeintegrated luminosity is a faithful indicator of the grb nature contrary to the peak luminosity which is merely a function of the cbm density we call attention on discriminating the short grbs between the genuine and the fake ones the genuine ones are intrinsically short with baryon loading b la 105 as stated in our original classification the fake ones characterized by an initial spikelike emission followed by an extended emission lasting tenths of seconds have a baryon loading 104 la b leq 102 they are observed as such only due to an underdense cbm consistent with a galactic halo environment which deflates the afterglow intensity
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709.0652
Many Body Symmetrical Dynamical Systems
We investigate the stability of few body symmetrical dynamical systems which include four and five body symmetrical dynamical systems. Research presented in this thesis includes the following original investigations: determination of some analytical solutions of the four body problem; stability analysis of the near symmetric coplanar CSFBP ; derivation of the analytical stability criterion valid for all time for a special symmetric configuration of the general five-body problem, the CS5BP, which exhibits many of the salient characteristics of the general five body problem; numerical investigation of the hierarchical stability of the CS5BP and derivation of the stability criterion for the CSNBP.
math-ph math.MP
we investigate the stability of few body symmetrical dynamical systems which include four and five body symmetrical dynamical systems research presented in this thesis includes the following original investigations determination of some analytical solutions of the four body problem stability analysis of the near symmetric coplanar csfbp derivation of the analytical stability criterion valid for all time for a special symmetric configuration of the general fivebody problem the cs5bp which exhibits many of the salient characteristics of the general five body problem numerical investigation of the hierarchical stability of the cs5bp and derivation of the stability criterion for the csnbp
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709.0653
Creating and preserving multi-partite entanglement with spin chains
We show how multi-partite entanglement, such as of W-state form, can be created in branched spin chain systems. We also discuss the preservation of such entanglement, once created. The technique could be applied to actual spin chain systems, or to other physical systems such as strings of coupled quantum dots, molecules or atoms.
quant-ph
we show how multipartite entanglement such as of wstate form can be created in branched spin chain systems we also discuss the preservation of such entanglement once created the technique could be applied to actual spin chain systems or to other physical systems such as strings of coupled quantum dots molecules or atoms
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709.0654
Mapping Neutral Hydrogen During Reionization with the Ly-alpha Emission from Quasar Ionization Fronts
We present a new method to directly map the neutral-hydrogen distribution during the reionization epoch and to constrain the emission properties of the highest-redshift quasars (QSOs). As a tracer of HI, we propose to use the Ly-alpha radiation produced by quasar ionization fronts (I-fronts) that expand in the partially ionized intergalactic medium (IGM) before reionization is complete. These Ly-alpha photons are mainly generated by collisional excitations of hydrogen atoms in the boundary of the rapidly expanding HII region. The observable signal is produced by the part of the I-front that lies behind the QSO with respect to the observer. Combining two radiative transfer models (one for the QSO ionizing radiation and one for the Ly-alpha photons), we estimate the expected Ly-alpha spectral shape and surface brightness (SB) for a large number of configurations where we varied both the properties of the ionizing QSO and of the surrounding medium. We find that the expected signal is observable as a single (broad) emission line with a characteristic width of 100-200 km/s. The expected SB produced at redshift z~6.5 within a fully neutral region (at mean density) by a typical QSO I-front lies in the range $10^{-21}-10^{-20}$ erg s$^{-1}$ cm$^{-2}$ arcsec$^{-2}$ and decreases proportionally to $(1+z)^2$ for a given QSO age. QSOs with harder spectra may produce a significantly brighter emission at early phases. The signal may cover up to a few hundred square arcmin on the sky and should be already detectable with current facilities by means of moderate/high resolution spectroscopy. The detection of this Ly-alpha emission can shed new light on the reionization history, the age and the emission properties of the highest-redshift QSOs. (abridged)
astro-ph
we present a new method to directly map the neutralhydrogen distribution during the reionization epoch and to constrain the emission properties of the highestredshift quasars qsos as a tracer of hi we propose to use the lyalpha radiation produced by quasar ionization fronts ifronts that expand in the partially ionized intergalactic medium igm before reionization is complete these lyalpha photons are mainly generated by collisional excitations of hydrogen atoms in the boundary of the rapidly expanding hii region the observable signal is produced by the part of the ifront that lies behind the qso with respect to the observer combining two radiative transfer models one for the qso ionizing radiation and one for the lyalpha photons we estimate the expected lyalpha spectral shape and surface brightness sb for a large number of configurations where we varied both the properties of the ionizing qso and of the surrounding medium we find that the expected signal is observable as a single broad emission line with a characteristic width of 100200 kms the expected sb produced at redshift z65 within a fully neutral region at mean density by a typical qso ifront lies in the range 10211020 erg s1 cm2 arcsec2 and decreases proportionally to 1z2 for a given qso age qsos with harder spectra may produce a significantly brighter emission at early phases the signal may cover up to a few hundred square arcmin on the sky and should be already detectable with current facilities by means of moderatehigh resolution spectroscopy the detection of this lyalpha emission can shed new light on the reionization history the age and the emission properties of the highestredshift qsos abridged
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709.0655
Colored Spin Systems, BKP Evolution and finite N_c effects
Even within the framework of the leading logarithmic approximation the eigenvalues of the BKP kernel for states of more than three reggeized gluons are unknown in general, contrary to the planar limit case where the problem becomes integrable. We consider a 4-gluon kernel for a finite number of colors and define some simple toy models for the configuration space dynamics, which are directly solvable with group theoretical methods. Then we study the dependence of the spectrum of these models with respect to the number of colors and make comparisons with the large limit case.
hep-th
even within the framework of the leading logarithmic approximation the eigenvalues of the bkp kernel for states of more than three reggeized gluons are unknown in general contrary to the planar limit case where the problem becomes integrable we consider a 4gluon kernel for a finite number of colors and define some simple toy models for the configuration space dynamics which are directly solvable with group theoretical methods then we study the dependence of the spectrum of these models with respect to the number of colors and make comparisons with the large limit case
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709.0656
Hidden Fermi Liquid: The Secret of High Tc Cuprates
I present a formalism for dealing directly with the effects of the Gutzwiller projection, which is implicit in the t-J model widely believed to underly the phenomenology of the high-Tc cuprates. I suggest that a true BCS condensation from a Fermi liquid state takes place, but in the unphysical space prior to projection. The theory which results upon projection does not follow conventional rules of diagram theory and in fact in the normal state is a Z=0 non-Fermi liquid. Anomalous properties of this strange metal normal state are predicted and compared to experiments.
cond-mat.str-el cond-mat.supr-con
i present a formalism for dealing directly with the effects of the gutzwiller projection which is implicit in the tj model widely believed to underly the phenomenology of the hightc cuprates i suggest that a true bcs condensation from a fermi liquid state takes place but in the unphysical space prior to projection the theory which results upon projection does not follow conventional rules of diagram theory and in fact in the normal state is a z0 nonfermi liquid anomalous properties of this strange metal normal state are predicted and compared to experiments
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709.0657
Quasi-Normal Modes and Gravitational Wave Astronomy
We review the main results obtained in the literature on quasi-normal modes of compact stars and black holes, in the light of recent exciting developments of gravitational wave detectors. Quasi-normal modes are a fundamental feature of the gravitational signal emitted by compact objects in many astrophysical processes; we will show that their eigenfrequencies encode interesting information on the nature and on the inner structure of the emitting source and we will discuss whether we are ready for a gravitational wave asteroseismology.
gr-qc astro-ph
we review the main results obtained in the literature on quasinormal modes of compact stars and black holes in the light of recent exciting developments of gravitational wave detectors quasinormal modes are a fundamental feature of the gravitational signal emitted by compact objects in many astrophysical processes we will show that their eigenfrequencies encode interesting information on the nature and on the inner structure of the emitting source and we will discuss whether we are ready for a gravitational wave asteroseismology
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709.0658
Chemical evolution of bulges at high redshift
We present a new class of hydrodynamical models for the formation of bulges (either massive elliptical galaxies or classical bulges in spirals) in which we implement detailed prescriptions for the chemical evolution of H, He, O and Fe. Our results hint toward an outside-in formation in the context of the supernovae-driven wind scenario. The build-up of the chemical properties of the stellar populations inhabiting the galactic core is very fast. Therefore we predict a non significant evolution of both the mass-metallicity and the mass-[alpha/Fe] relations after the first 0.5 - 1 Gyr. In this framework we explain how the observed slopes, either positive or negative, in the radial gradient of the mean stellar [alpha/Fe], and their apparent lack of any correlation with all the other observables, can arise as a consequence of the interplay between star formation and metal-enhanced internal gas flows.
astro-ph
we present a new class of hydrodynamical models for the formation of bulges either massive elliptical galaxies or classical bulges in spirals in which we implement detailed prescriptions for the chemical evolution of h he o and fe our results hint toward an outsidein formation in the context of the supernovaedriven wind scenario the buildup of the chemical properties of the stellar populations inhabiting the galactic core is very fast therefore we predict a non significant evolution of both the massmetallicity and the massalphafe relations after the first 05 1 gyr in this framework we explain how the observed slopes either positive or negative in the radial gradient of the mean stellar alphafe and their apparent lack of any correlation with all the other observables can arise as a consequence of the interplay between star formation and metalenhanced internal gas flows
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709.0659
Statistical Properties of the IntraCluster Light from SDSS Image Stacking
The presence of a diffuse stellar component in galaxy clusters has been established by a number of observational works in recent years. In this contribution I summarize our results (Zibetti et al. 2005) obtained by stacking SDSS images of 683 clusters, selected with the maxBCG algorithm at 0.2< z <0.3. Thanks to our large sample and the advantages of image stacking applied to SDSS images, we are able to measure the systematic properties of the intracluster light (ICL) with very high accuracy. We find that the average surface brightness of the ICL ranges between 26 and 32 mag/arcsec^2, and constantly declines from 70 kpc cluster-centric distance (i.e. distance from the BCG) to 700 kpc. The fraction of diffuse light over the total light (including galaxies), monotonically declines from ~50 to <~5% over the same range of distances, thus showing that the ICL is more easily produced close to the bottom of a cluster's potential well. Clusters lacking a bright BCG hardly build up a large amount of intracluster stellar component. The link between the growth of the BCG and the ICL is also suggested by the strong degree of alignment between these two components which is observed in clusters where the BCG displays a significant elongation. With the additional fact that the colors of the ICL are consistent with those of galaxies, all this appears to be evidence for IC stars being stripped from galaxies that suffer very strong tidal interactions in the center of clusters and eventually merge into the BCG. Our measurements also show that IC stars are a minor component of a cluster's baryonic budget, representing only ~10% of the total optical emission within 500 kpc. Finally, we discuss some open issues that emerge from a comparison of the present results with other observations and recent theoretical modeling.
astro-ph
the presence of a diffuse stellar component in galaxy clusters has been established by a number of observational works in recent years in this contribution i summarize our results zibetti et al 2005 obtained by stacking sdss images of 683 clusters selected with the maxbcg algorithm at 02 z 03 thanks to our large sample and the advantages of image stacking applied to sdss images we are able to measure the systematic properties of the intracluster light icl with very high accuracy we find that the average surface brightness of the icl ranges between 26 and 32 magarcsec2 and constantly declines from 70 kpc clustercentric distance ie distance from the bcg to 700 kpc the fraction of diffuse light over the total light including galaxies monotonically declines from 50 to 5 over the same range of distances thus showing that the icl is more easily produced close to the bottom of a clusters potential well clusters lacking a bright bcg hardly build up a large amount of intracluster stellar component the link between the growth of the bcg and the icl is also suggested by the strong degree of alignment between these two components which is observed in clusters where the bcg displays a significant elongation with the additional fact that the colors of the icl are consistent with those of galaxies all this appears to be evidence for ic stars being stripped from galaxies that suffer very strong tidal interactions in the center of clusters and eventually merge into the bcg our measurements also show that ic stars are a minor component of a clusters baryonic budget representing only 10 of the total optical emission within 500 kpc finally we discuss some open issues that emerge from a comparison of the present results with other observations and recent theoretical modeling
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709.066
Oscillations of General Relativistic Multi-fluid/Multi-layer Compact Stars
We develop the formalism for determining the quasinormal modes of general relativistic multi-fluid compact stars in such a way that the impact of superfluid gap data can be assessed. Our results represent the first attempt to study true multi-layer dynamics, an important step towards considering realistic superfluid/superconducting compact stars. We combine a relativistic model for entrainment with model equations of state that explicity incorporate the symmetry energy. Our analysis emphasises the many different parameters that are required for this kind of modelling, and the fact that standard tabulated equations of state are grossly incomplete in this respect. To make progress, future equations of state need to provide the energy density as a function of the various nucleon number densities, the temperature (i.e. entropy), and the entrainment among the various components.
gr-qc astro-ph
we develop the formalism for determining the quasinormal modes of general relativistic multifluid compact stars in such a way that the impact of superfluid gap data can be assessed our results represent the first attempt to study true multilayer dynamics an important step towards considering realistic superfluidsuperconducting compact stars we combine a relativistic model for entrainment with model equations of state that explicity incorporate the symmetry energy our analysis emphasises the many different parameters that are required for this kind of modelling and the fact that standard tabulated equations of state are grossly incomplete in this respect to make progress future equations of state need to provide the energy density as a function of the various nucleon number densities the temperature ie entropy and the entrainment among the various components
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709.0661
Unresolved Classical Electromagnetic Aspects of the Aharonov-Bohm Phase Shift
The long-standing controversy regarding the Aharonov-Bohm phase shift is reviewed. The shifts of both optical and particle interference patterns are summarized. It is pointed out that a line of electric dipoles and a line of magnetic dipoles (a long solenoid) both produce experimentally observed phase shifts similar to that produced by introducing a rectangular block of glass behind one slit of a double-slit interference pattern; the double-slit pattern is shifted while the single-slit envelope remains undisplaced. The quantum explanation for the magnetic interference pattern shift introduced by Aharonov and Bohm in 1959 involves completely different ideas from those suggested by a semiclassical analysis. Experiments planned by Caprez, Barwick, and Batelaan should clarify the connections between classical and quantum theories in connection with the Ahronov-Bohm phase shift.
physics.atom-ph
the longstanding controversy regarding the aharonovbohm phase shift is reviewed the shifts of both optical and particle interference patterns are summarized it is pointed out that a line of electric dipoles and a line of magnetic dipoles a long solenoid both produce experimentally observed phase shifts similar to that produced by introducing a rectangular block of glass behind one slit of a doubleslit interference pattern the doubleslit pattern is shifted while the singleslit envelope remains undisplaced the quantum explanation for the magnetic interference pattern shift introduced by aharonov and bohm in 1959 involves completely different ideas from those suggested by a semiclassical analysis experiments planned by caprez barwick and batelaan should clarify the connections between classical and quantum theories in connection with the ahronovbohm phase shift
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709.0662
Structure of BSCCO supermodulation from ab initio calculations
We present results of density functional theory (DFT) calculation of the structural supermodulation in BSCCO-2212 structure, and show that the supermodulation is indeed a spontaneous symmetry breaking of the nominal crystal symmetry, rather than a phenomenon driven by interstitial O dopants. The structure obtained is in excellent quantitative agreement with recent x-ray studies, and reproduces several qualitative aspects of scanning tunnelling microscopy (STM) experiments as well. The primary structural modulation affecting the CuO_2 plane is found to be a buckling wave of tilted CuO_5 half-octahedra, with maximum tilt angle near the phase of the supermodulation where recent STM experiments have discovered an enhancement of the superconducting gap. We argue that the tilting of the half-octahedra and concommitant planar buckling are directly modulating the superconducting pair interaction.
cond-mat.supr-con cond-mat.mtrl-sci
we present results of density functional theory dft calculation of the structural supermodulation in bscco2212 structure and show that the supermodulation is indeed a spontaneous symmetry breaking of the nominal crystal symmetry rather than a phenomenon driven by interstitial o dopants the structure obtained is in excellent quantitative agreement with recent xray studies and reproduces several qualitative aspects of scanning tunnelling microscopy stm experiments as well the primary structural modulation affecting the cuo_2 plane is found to be a buckling wave of tilted cuo_5 halfoctahedra with maximum tilt angle near the phase of the supermodulation where recent stm experiments have discovered an enhancement of the superconducting gap we argue that the tilting of the halfoctahedra and concommitant planar buckling are directly modulating the superconducting pair interaction
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709.0663
K3 surfaces, rational curves, and rational points
We prove that for any of a wide class of elliptic surfaces $X$ defined over a number field $k$, if there is an algebraic point on $X$ that lies on only finitely many rational curves, then there is an algebraic point on $X$ that lies on no rational curves. In particular, our theorem applies to a large class of elliptic $K3$ surfaces, which relates to a question posed by Bogomolov in 1981. We apply our results to construct an explicit algebraic point on a $K3$ surface that does not lie on any smooth rational curves.
math.AG math.NT
we prove that for any of a wide class of elliptic surfaces x defined over a number field k if there is an algebraic point on x that lies on only finitely many rational curves then there is an algebraic point on x that lies on no rational curves in particular our theorem applies to a large class of elliptic k3 surfaces which relates to a question posed by bogomolov in 1981 we apply our results to construct an explicit algebraic point on a k3 surface that does not lie on any smooth rational curves
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709.0664
Excited mesons on dynamical clover-Wilson lattices
We present results for masses of excited mesons from dynamical clover-Wilson lattices provided by the CP-PACS collaboration at pion masses down to 500 MeV. Our analysis of the data is based on using a matrix of correlators from various source and sink operators. The spectroscopy results are discussed and compared to experimental values.
hep-lat
we present results for masses of excited mesons from dynamical cloverwilson lattices provided by the cppacs collaboration at pion masses down to 500 mev our analysis of the data is based on using a matrix of correlators from various source and sink operators the spectroscopy results are discussed and compared to experimental values
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709.0665
Multiplicity fluctuations in relativistic nuclear collisions
Multiplicity distributions of hadrons produced in central nucleus-nucleus collisions are studied within the hadron-resonance gas model in the large volume limit. In the canonical ensemble conservation of three charges (baryon number, electric charge, and strangeness) is enforced. In addition, in the micro-canonical ensemble energy conservation is included. An analytical method is used to account for resonance decays. Multiplicity distributions and scaled variances for negatively charged hadrons are presented along the chemical freeze-out line of central Pb+Pb (Au+Au) collisions from SIS to LHC energies. Predictions obtained within different statistical ensembles are compared with preliminary NA49 experimental results on central Pb+Pb collisions in the SPS energy range. The measured fluctuations are significantly narrower than a Poisson reference distribution, and clearly favor expectations for the micro-canonical ensemble.
nucl-th
multiplicity distributions of hadrons produced in central nucleusnucleus collisions are studied within the hadronresonance gas model in the large volume limit in the canonical ensemble conservation of three charges baryon number electric charge and strangeness is enforced in addition in the microcanonical ensemble energy conservation is included an analytical method is used to account for resonance decays multiplicity distributions and scaled variances for negatively charged hadrons are presented along the chemical freezeout line of central pbpb auau collisions from sis to lhc energies predictions obtained within different statistical ensembles are compared with preliminary na49 experimental results on central pbpb collisions in the sps energy range the measured fluctuations are significantly narrower than a poisson reference distribution and clearly favor expectations for the microcanonical ensemble
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709.0666
Lepton Flavour Violation in the Constrained MSSM with Constrained Sequential Dominance
We consider charged Lepton Flavour Violation (LFV) in the Constrained Minimal Supersymmetric Standard Model, extended to include the see-saw mechanism with Constrained Sequential Dominance (CSD), where CSD provides a natural see-saw explanation of tri-bimaximal neutrino mixing. When charged lepton corrections to tri-bimaximal neutrino mixing are included, we discover characteristic correlations among the LFV branching ratios, depending on the mass ordering of the right-handed neutrinos, with a pronounced dependence on the leptonic mixing angle $\theta_{13}$ (and in some cases also on the Dirac CP phase $\delta$).
hep-ph
we consider charged lepton flavour violation lfv in the constrained minimal supersymmetric standard model extended to include the seesaw mechanism with constrained sequential dominance csd where csd provides a natural seesaw explanation of tribimaximal neutrino mixing when charged lepton corrections to tribimaximal neutrino mixing are included we discover characteristic correlations among the lfv branching ratios depending on the mass ordering of the righthanded neutrinos with a pronounced dependence on the leptonic mixing angle theta_13 and in some cases also on the dirac cp phase delta
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709.0667
Computation of weight lattices of G-varieties
Let G be a connected reductive group. To any irreducible G-variety one assigns the lattice generated by all weights of B-semiinvariant rational functions on X, where B$ is a Borel subgroup of G. This lattice is called the weight lattice of X. We establish algorithms for computing weight lattices for homogeneous spaces and affine homogeneous vector bundles. For affine homogeneous spaces of rank rk(G) we present a more or less explicit computation.
math.AG math.RT
let g be a connected reductive group to any irreducible gvariety one assigns the lattice generated by all weights of bsemiinvariant rational functions on x where b is a borel subgroup of g this lattice is called the weight lattice of x we establish algorithms for computing weight lattices for homogeneous spaces and affine homogeneous vector bundles for affine homogeneous spaces of rank rkg we present a more or less explicit computation
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709.0668
Entropy and Uncertainty Analysis in Financial Markets
The investor is interested in the expected return and he is also concerned about the risk and the uncertainty assumed by the investment. One of the most popular concepts used to measure the risk and the uncertainty is the variance and/or the standard-deviation. In this paper we explore the following issues: Is the standard-deviation a good measure of risk and uncertainty? What are the potentialities of the entropy in this context? Can entropy present some advantages as a measure of uncertainty and simultaneously verify some basic assumptions of the portfolio management theory, namely the effect of diversification?
q-fin.ST physics.soc-ph
the investor is interested in the expected return and he is also concerned about the risk and the uncertainty assumed by the investment one of the most popular concepts used to measure the risk and the uncertainty is the variance andor the standarddeviation in this paper we explore the following issues is the standarddeviation a good measure of risk and uncertainty what are the potentialities of the entropy in this context can entropy present some advantages as a measure of uncertainty and simultaneously verify some basic assumptions of the portfolio management theory namely the effect of diversification
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709.0669
G_2 gauge theory at finite temperature
The gauge group being centreless, $G_2$ gauge theory is a good laboratory for studying the role of the centre of the group for colour confinement in Yang-Mills gauge theories. In this paper, we investigate $G_2$ pure gauge theory at finite temperature on the lattice. By studying the finite size scaling of the plaquette, the Polyakov loop and their susceptibilities, we show that a deconfinement phase transition takes place. The analysis of the pseudocritical exponents give strong evidence of the deconfinement transition being first order. Implications of our findings for scenarios of colour confinement are discussed.
hep-lat
the gauge group being centreless g_2 gauge theory is a good laboratory for studying the role of the centre of the group for colour confinement in yangmills gauge theories in this paper we investigate g_2 pure gauge theory at finite temperature on the lattice by studying the finite size scaling of the plaquette the polyakov loop and their susceptibilities we show that a deconfinement phase transition takes place the analysis of the pseudocritical exponents give strong evidence of the deconfinement transition being first order implications of our findings for scenarios of colour confinement are discussed
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709.067
Using Data Compressors to Construct Rank Tests
Nonparametric rank tests for homogeneity and component independence are proposed, which are based on data compressors. For homogeneity testing the idea is to compress the binary string obtained by ordering the two joint samples and writing 0 if the element is from the first sample and 1 if it is from the second sample and breaking ties by randomization (extension to the case of multiple samples is straightforward). $H_0$ should be rejected if the string is compressed (to a certain degree) and accepted otherwise. We show that such a test obtained from an ideal data compressor is valid against all alternatives. Component independence is reduced to homogeneity testing by constructing two samples, one of which is the first half of the original and the other is the second half with one of the components randomly permuted.
cs.DS cs.IT math.IT
nonparametric rank tests for homogeneity and component independence are proposed which are based on data compressors for homogeneity testing the idea is to compress the binary string obtained by ordering the two joint samples and writing 0 if the element is from the first sample and 1 if it is from the second sample and breaking ties by randomization extension to the case of multiple samples is straightforward h_0 should be rejected if the string is compressed to a certain degree and accepted otherwise we show that such a test obtained from an ideal data compressor is valid against all alternatives component independence is reduced to homogeneity testing by constructing two samples one of which is the first half of the original and the other is the second half with one of the components randomly permuted
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709.0671
Which Partial Sums of the Taylor Series for $e$ are Convergents to $e$? (and a Link to the Primes 2, 5, 13, 37, 463), II
This is an expanded version of our earlier paper. Let the $n$th partial sum of the Taylor series $e = \sum_{r=0}^{\infty} 1/r!$ be $A_n/n!$, and let $p_k/q_k$ be the $k$th convergent of the simple continued fraction for $e$. Using a recent measure of irrationality for $e$, we prove weak versions of our conjecture that only two of the partial sums are convergents to $e$. A related result about the denominators $q_k$ and powers of factorials is proved. We also show a surprising connection between the $A_n$ and the primes 2, 5, 13, 37, 463. In the Appendix, we give a conditional proof of the conjecture, assuming a second conjecture we make about the zeros of $A_n$ and $q_k$ modulo powers of 2. Tables supporting this Zeros Conjecture are presented and we discuss a 2-adic reformulation of it.
math.NT math.HO
this is an expanded version of our earlier paper let the nth partial sum of the taylor series e sum_r0infty 1r be a_nn and let p_kq_k be the kth convergent of the simple continued fraction for e using a recent measure of irrationality for e we prove weak versions of our conjecture that only two of the partial sums are convergents to e a related result about the denominators q_k and powers of factorials is proved we also show a surprising connection between the a_n and the primes 2 5 13 37 463 in the appendix we give a conditional proof of the conjecture assuming a second conjecture we make about the zeros of a_n and q_k modulo powers of 2 tables supporting this zeros conjecture are presented and we discuss a 2adic reformulation of it
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709.0672
Harmonic morphisms on heaven spaces
We prove that any (real or complex) analytic horizontally conformal submersion from a three-dimensional conformal manifold M to a two-dimensional conformal manifold N can be, locally, `extended' to a unique harmonic morphism from the heaven space of M to N.
math.DG
we prove that any real or complex analytic horizontally conformal submersion from a threedimensional conformal manifold m to a twodimensional conformal manifold n can be locally extended to a unique harmonic morphism from the heaven space of m to n
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709.0673
Excited Fermions at H1
We present a search for excited neutrinos and electrons using all data collected by the H1 experiment at HERA at a center-of-mass energy of 320 GeV with an integrated luminosity of up to 435 pb$^{-1}$. No evidence for excited neutrino or electron production is found. Mass dependent exclusion limits are determined for the ratio of the coupling to the compositeness scale, $f/{\Lambda}$. These limits greatly extend the excluded region to higher masses than has been possible in previous searches.
hep-ex
we present a search for excited neutrinos and electrons using all data collected by the h1 experiment at hera at a centerofmass energy of 320 gev with an integrated luminosity of up to 435 pb1 no evidence for excited neutrino or electron production is found mass dependent exclusion limits are determined for the ratio of the coupling to the compositeness scale flambda these limits greatly extend the excluded region to higher masses than has been possible in previous searches
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709.0674
Simple Algorithmic Principles of Discovery, Subjective Beauty, Selective Attention, Curiosity & Creativity
I postulate that human or other intelligent agents function or should function as follows. They store all sensory observations as they come - the data is holy. At any time, given some agent's current coding capabilities, part of the data is compressible by a short and hopefully fast program / description / explanation / world model. In the agent's subjective eyes, such data is more regular and more "beautiful" than other data. It is well-known that knowledge of regularity and repeatability may improve the agent's ability to plan actions leading to external rewards. In absence of such rewards, however, known beauty is boring. Then "interestingness" becomes the first derivative of subjective beauty: as the learning agent improves its compression algorithm, formerly apparently random data parts become subjectively more regular and beautiful. Such progress in compressibility is measured and maximized by the curiosity drive: create action sequences that extend the observation history and yield previously unknown / unpredictable but quickly learnable algorithmic regularity. We discuss how all of the above can be naturally implemented on computers, through an extension of passive unsupervised learning to the case of active data selection: we reward a general reinforcement learner (with access to the adaptive compressor) for actions that improve the subjective compressibility of the growing data. An unusually large breakthrough in compressibility deserves the name "discovery". The "creativity" of artists, dancers, musicians, pure mathematicians can be viewed as a by-product of this principle. Several qualitative examples support this hypothesis.
cs.AI cs.GR
i postulate that human or other intelligent agents function or should function as follows they store all sensory observations as they come the data is holy at any time given some agents current coding capabilities part of the data is compressible by a short and hopefully fast program description explanation world model in the agents subjective eyes such data is more regular and more beautiful than other data it is wellknown that knowledge of regularity and repeatability may improve the agents ability to plan actions leading to external rewards in absence of such rewards however known beauty is boring then interestingness becomes the first derivative of subjective beauty as the learning agent improves its compression algorithm formerly apparently random data parts become subjectively more regular and beautiful such progress in compressibility is measured and maximized by the curiosity drive create action sequences that extend the observation history and yield previously unknown unpredictable but quickly learnable algorithmic regularity we discuss how all of the above can be naturally implemented on computers through an extension of passive unsupervised learning to the case of active data selection we reward a general reinforcement learner with access to the adaptive compressor for actions that improve the subjective compressibility of the growing data an unusually large breakthrough in compressibility deserves the name discovery the creativity of artists dancers musicians pure mathematicians can be viewed as a byproduct of this principle several qualitative examples support this hypothesis
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709.0675
Magnetic field induced singlet - triplet phase transition in quasi one-dimensional organic superconductors
We propose a theoretical model of quasi-one-dimensional superconductors, with attractive electron-electron interactions dominant in the singlet d-wave channel and sub-dominant in the p-wave channel. We discuss, in the mean field approximation, the effect of a magnetic field applied perpendicularly to the direction of the lowest conductivity. The lowest free energy phase corresponds to a singlet d-wave symmetry in low fields, but to a triplet symmetry in high fields. A first order singlet-triplet phase transition is expected at moderate applied fields of a few teslas. We propose to ascribe the recent critical field and NMR experimental data, observed in superconducting (TMTSF)2ClO4 to such an effect.
cond-mat.str-el cond-mat.supr-con
we propose a theoretical model of quasionedimensional superconductors with attractive electronelectron interactions dominant in the singlet dwave channel and subdominant in the pwave channel we discuss in the mean field approximation the effect of a magnetic field applied perpendicularly to the direction of the lowest conductivity the lowest free energy phase corresponds to a singlet dwave symmetry in low fields but to a triplet symmetry in high fields a first order singlettriplet phase transition is expected at moderate applied fields of a few teslas we propose to ascribe the recent critical field and nmr experimental data observed in superconducting tmtsf2clo4 to such an effect
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709.0676
The potential for Earth-mass planet formation around brown dwarfs
Recent observations point to the presence of structured dust grains in the discs surrounding young brown dwarfs, thus implying that the first stages of planet formation take place also in the sub-stellar regime. Here, we investigate the potential for planet formation around brown dwarfs and very low mass stars according to the sequential core accretion model of planet formation. We find that, for a brown dwarfs of mass 0.05M_{\odot}, our models predict a maximum planetary mass of ~5M_{\oplus}, orbiting with semi-major axis ~1AU. However, we note that the predictions for the mass - semi-major axis distribution are strongly dependent upon the models chosen for the disc surface density profiles and the assumed distribution of disc masses. In particular, if brown dwarf disc masses are of the order of a few Jupiter masses, Earth-mass planets might be relatively frequent, while if typical disc masses are only a fraction of Jupiter mass, we predict that planet formation would be extremely rare in the sub-stellar regime. As the observational constraints on disc profiles, mass dependencies and their distributions are poor in the brown dwarf regime, we advise caution in validating theoretical models only on stars similar to the Sun and emphasise the need for observational data on planetary systems around a wide range of stellar masses. We also find that, unlike the situation around solar-like stars, Type-II migration is totally absent from the planet formation process around brown dwarfs, suggesting that any future observations of planets around brown dwarfs would provide a direct measure of the role of other types of migration.
astro-ph
recent observations point to the presence of structured dust grains in the discs surrounding young brown dwarfs thus implying that the first stages of planet formation take place also in the substellar regime here we investigate the potential for planet formation around brown dwarfs and very low mass stars according to the sequential core accretion model of planet formation we find that for a brown dwarfs of mass 005m_odot our models predict a maximum planetary mass of 5m_oplus orbiting with semimajor axis 1au however we note that the predictions for the mass semimajor axis distribution are strongly dependent upon the models chosen for the disc surface density profiles and the assumed distribution of disc masses in particular if brown dwarf disc masses are of the order of a few jupiter masses earthmass planets might be relatively frequent while if typical disc masses are only a fraction of jupiter mass we predict that planet formation would be extremely rare in the substellar regime as the observational constraints on disc profiles mass dependencies and their distributions are poor in the brown dwarf regime we advise caution in validating theoretical models only on stars similar to the sun and emphasise the need for observational data on planetary systems around a wide range of stellar masses we also find that unlike the situation around solarlike stars typeii migration is totally absent from the planet formation process around brown dwarfs suggesting that any future observations of planets around brown dwarfs would provide a direct measure of the role of other types of migration
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709.0677
On the Complexity of Protein Local Structure Alignment Under the Discrete Fr\'echet Distance
We show that given $m$ proteins (or protein backbones, which are modeled as 3D polygonal chains each of length O(n)) the problem of protein local structure alignment under the discrete Fr\'{e}chet distance is as hard as Independent Set. So the problem does not admit any approximation of factor $n^{1-\epsilon}$. This is the strongest negative result regarding the protein local structure alignment problem. On the other hand, if $m$ is a constant, then the problem can be solved in polygnomial time.
cs.CC cs.DS
we show that given m proteins or protein backbones which are modeled as 3d polygonal chains each of length on the problem of protein local structure alignment under the discrete frechet distance is as hard as independent set so the problem does not admit any approximation of factor n1epsilon this is the strongest negative result regarding the protein local structure alignment problem on the other hand if m is a constant then the problem can be solved in polygnomial time
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709.0678
Constraints on Unparticle Physics from Solar and KamLAND Neutrinos
Interest has been directed recently towards low energy implications of a non-trivial conformal sector of an effective field theory with an IR fixed point (\Lambda), manifest in terms of ``unparticles'' with bizarre properties. We re-examine the implications of the limits on decay lifetimes of solar neutrinos for unparticle interactions. We study in detail the fundamental parameter space (\Lambda, M) and derive bounds on the energy scale M characterizing the new physics. We work strictly within the framework where conformal invariance holds down to low energies. We first assume that couplings of the unparticle sector to the Higgs field are suppressed and derive bounds with \Lambda in the TeV region from neutrino decay into scalar unparticles. These bounds are significant for values of the anomalous dimension of the unparticle operator 1.0 < d < 1.2. For a region of the parameter space, we show that the bounds are comparable to those arising from production rates at high energy colliders. We then relax our assumption, by considering a more natural framework which does not require a priori restrictions on couplings of Higgs-unparticle operators, and derive bounds with \Lambda in meV region from neutrino decay into vector unparticles. Such low scales for the IR fixed point are relevant in gauge theories with many flavors.
hep-ph
interest has been directed recently towards low energy implications of a nontrivial conformal sector of an effective field theory with an ir fixed point lambda manifest in terms of unparticles with bizarre properties we reexamine the implications of the limits on decay lifetimes of solar neutrinos for unparticle interactions we study in detail the fundamental parameter space lambda m and derive bounds on the energy scale m characterizing the new physics we work strictly within the framework where conformal invariance holds down to low energies we first assume that couplings of the unparticle sector to the higgs field are suppressed and derive bounds with lambda in the tev region from neutrino decay into scalar unparticles these bounds are significant for values of the anomalous dimension of the unparticle operator 10 d 12 for a region of the parameter space we show that the bounds are comparable to those arising from production rates at high energy colliders we then relax our assumption by considering a more natural framework which does not require a priori restrictions on couplings of higgsunparticle operators and derive bounds with lambda in mev region from neutrino decay into vector unparticles such low scales for the ir fixed point are relevant in gauge theories with many flavors
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709.0679
Curvature and torsion in growing actin networks
Intracellular pathogens such as Listeria monocytogenes and Rickettsia rickettsii move within a host cell by polymerizing a comet-tail of actin fibers that ultimately pushes the cell forward. This dense network of cross-linked actin polymers typically exhibits a striking curvature that causes bacteria to move in gently looping paths. Theoretically, tail curvature has been linked to details of motility by considering force and torque balances from a finite number of polymerizing filaments. Here we track beads coated with a prokaryotic activator of actin polymerization in three dimensions to directly quantify the curvature and torsion of bead motility paths. We find that bead paths are more likely to have low rather than high curvature at any given time. Furthermore, path curvature changes very slowly in time, with an autocorrelation decay time of 200 seconds. Paths with a small radius of curvature, therefore, remain so for an extended period resulting in loops when confined to two dimensions. When allowed to explore a 3D space, path loops are less evident. Finally, we quantify the torsion in the bead paths and show that beads do not exhibit a significant left- or right-handed bias to their motion in 3D. These results suggest that paths of actin-propelled objects may be attributed to slow changes in curvature rather than a fixed torque.
q-bio.BM physics.bio-ph q-bio.CB
intracellular pathogens such as listeria monocytogenes and rickettsia rickettsii move within a host cell by polymerizing a comettail of actin fibers that ultimately pushes the cell forward this dense network of crosslinked actin polymers typically exhibits a striking curvature that causes bacteria to move in gently looping paths theoretically tail curvature has been linked to details of motility by considering force and torque balances from a finite number of polymerizing filaments here we track beads coated with a prokaryotic activator of actin polymerization in three dimensions to directly quantify the curvature and torsion of bead motility paths we find that bead paths are more likely to have low rather than high curvature at any given time furthermore path curvature changes very slowly in time with an autocorrelation decay time of 200 seconds paths with a small radius of curvature therefore remain so for an extended period resulting in loops when confined to two dimensions when allowed to explore a 3d space path loops are less evident finally we quantify the torsion in the bead paths and show that beads do not exhibit a significant left or righthanded bias to their motion in 3d these results suggest that paths of actinpropelled objects may be attributed to slow changes in curvature rather than a fixed torque
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709.068
Designing a Virtual Manikin Animation Framework Aimed at Virtual Prototyping
In the industry, numerous commercial packages provide tools to introduce, and analyse human behaviour in the product's environment (for maintenance, ergonomics...), thanks to Virtual Humans. We will focus on control. Thanks to algorithms newly introduced in recent research papers, we think we can provide an implementation, which even widens, and simplifies the animation capacities of virtual manikins. In order to do so, we are going to express the industrial expectations as for Virtual Humans, without considering feasibility (not to bias the issue). The second part will show that no commercial application provides the tools that perfectly meet the needs. Thus we propose a new animation framework that better answers the problem. Our contribution is the integration - driven by need ~ of available new scientific techniques to animate Virtual Humans, in a new control scheme that better answers industrial expectations.
cs.RO
in the industry numerous commercial packages provide tools to introduce and analyse human behaviour in the products environment for maintenance ergonomics thanks to virtual humans we will focus on control thanks to algorithms newly introduced in recent research papers we think we can provide an implementation which even widens and simplifies the animation capacities of virtual manikins in order to do so we are going to express the industrial expectations as for virtual humans without considering feasibility not to bias the issue the second part will show that no commercial application provides the tools that perfectly meet the needs thus we propose a new animation framework that better answers the problem our contribution is the integration driven by need of available new scientific techniques to animate virtual humans in a new control scheme that better answers industrial expectations
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709.0681
Strong-coupling expansion of cusp anomaly from quantum superstring
We consider the world surface in AdS_5 that ends on two intersecting null lines at the boundary. The corresponding string partition function describes the expectation value of the Wilson line with a null cusp in dual large N maximally supersymmetric gauge theory and thus determines the cusp anomaly function f(\lambda) of the gauge coupling. The first two coefficients in its strong-coupling or string inverse tension expansion were determined in hep-th/0210115 (a_1=1) and in arXiv:0707.4254 (a_2=- 3 log 2). Here we find that the 2-loop coefficient is a_2 = - K where K is the Catalan's constant. This is in agreement (expected on general grounds) with the previous results for f(\lambda) as the coefficient of log(S) term in the energy of closed spinning string in AdS_5. The string theory value for a_2 is in agreement with the numerical result in hep-th/0611135 and the recent analytic result in arXiv:0708.3933 for the solution of the BES equation following from the asymptotic Bethe ansatz for the spectrum of the theory. We explicitly verify the cancellation of 2-loop 2d logarithmic divergences thus demonstrating the quantum consistency of the AdS_5 x S^5 superstring. We also discuss the structure of higher loop string corrections to the cusp anomaly giving a 2d QFT diagrammatic interpretation to the strong-coupling expansion of the cusp anomaly function as solution of the BES equation found in arXiv:0708.3933.
hep-th
we consider the world surface in ads_5 that ends on two intersecting null lines at the boundary the corresponding string partition function describes the expectation value of the wilson line with a null cusp in dual large n maximally supersymmetric gauge theory and thus determines the cusp anomaly function flambda of the gauge coupling the first two coefficients in its strongcoupling or string inverse tension expansion were determined in hepth0210115 a_11 and in arxiv07074254 a_2 3 log 2 here we find that the 2loop coefficient is a_2 k where k is the catalans constant this is in agreement expected on general grounds with the previous results for flambda as the coefficient of logs term in the energy of closed spinning string in ads_5 the string theory value for a_2 is in agreement with the numerical result in hepth0611135 and the recent analytic result in arxiv07083933 for the solution of the bes equation following from the asymptotic bethe ansatz for the spectrum of the theory we explicitly verify the cancellation of 2loop 2d logarithmic divergences thus demonstrating the quantum consistency of the ads_5 x s5 superstring we also discuss the structure of higher loop string corrections to the cusp anomaly giving a 2d qft diagrammatic interpretation to the strongcoupling expansion of the cusp anomaly function as solution of the bes equation found in arxiv07083933
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709.0682
Pressure sensor-based tongue-placed electrotactile biofeedback for balance improvement - Biomedical application to prevent pressure sores formation and falls
We introduce the innovative technologies, based on the concept of "sensory substitution", we are developing in the fields of biomedical engineering and human disability. Precisely, our goal is to design, develop and validate practical assistive biomedical and/or technical devices and/or rehabilitating procedures for persons with disabilities, using artificial tongue-placed tactile biofeedback systems. Proposed applications are dealing with: (1) pressure sores prevention in case of spinal cord injuries (persons with paraplegia, or tetraplegia); and (2) balance control improvement to prevent fall in older and/or disabled adults. This paper describes the architecture and the functioning principle of these biofeedback systems and presents preliminary results of two feasibility studies performed on young healthy adults.
physics.med-ph q-bio.NC
we introduce the innovative technologies based on the concept of sensory substitution we are developing in the fields of biomedical engineering and human disability precisely our goal is to design develop and validate practical assistive biomedical andor technical devices andor rehabilitating procedures for persons with disabilities using artificial tongueplaced tactile biofeedback systems proposed applications are dealing with 1 pressure sores prevention in case of spinal cord injuries persons with paraplegia or tetraplegia and 2 balance control improvement to prevent fall in older andor disabled adults this paper describes the architecture and the functioning principle of these biofeedback systems and presents preliminary results of two feasibility studies performed on young healthy adults
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709.0683
Framework for a low-cost intra-operative image-guided neuronavigator including brain shift compensation
In this paper we present a methodology to address the problem of brain tissue deformation referred to as 'brain-shift'. This deformation occurs throughout a neurosurgery intervention and strongly alters the accuracy of the neuronavigation systems used to date in clinical routine which rely solely on pre-operative patient imaging to locate the surgical target, such as a tumour or a functional area. After a general description of the framework of our intra-operative image-guided system, we describe a procedure to generate patient specific finite element meshes of the brain and propose a biomechanical model which can take into account tissue deformations and surgical procedures that modify the brain structure, like tumour or tissue resection.
physics.med-ph
in this paper we present a methodology to address the problem of brain tissue deformation referred to as brainshift this deformation occurs throughout a neurosurgery intervention and strongly alters the accuracy of the neuronavigation systems used to date in clinical routine which rely solely on preoperative patient imaging to locate the surgical target such as a tumour or a functional area after a general description of the framework of our intraoperative imageguided system we describe a procedure to generate patient specific finite element meshes of the brain and propose a biomechanical model which can take into account tissue deformations and surgical procedures that modify the brain structure like tumour or tissue resection
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709.0684
Muon spin rotation studies of spin dynamics at avoided level crossings in LiY0.998Ho0.002F4
We have studied the Ho3+ spin dynamics for LiY0.998Ho0.002F4 through the positive muon (mu+) transverse field depolarization rate lambda_TF as a function of temperature and magnetic field. We find sharp reductions in lambda_TF(H) at fields of 23, 46 and 69 mT, for which the Ho3+ ion system has field-induced (avoided) level crossings. The reduction scales with calculated level repulsions, suggesting that mu+ depolarization by slow fluctuations of non-resonant Ho3+ spin states is partially suppressed when resonant tunneling opens new fluctuation channels at frequencies much greater than the muon precession frequency.
cond-mat.mes-hall
we have studied the ho3 spin dynamics for liy0998ho0002f4 through the positive muon mu transverse field depolarization rate lambda_tf as a function of temperature and magnetic field we find sharp reductions in lambda_tfh at fields of 23 46 and 69 mt for which the ho3 ion system has fieldinduced avoided level crossings the reduction scales with calculated level repulsions suggesting that mu depolarization by slow fluctuations of nonresonant ho3 spin states is partially suppressed when resonant tunneling opens new fluctuation channels at frequencies much greater than the muon precession frequency
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709.0685
Not Only Because of Theory: Dyson, Eddington and the Competing Myths of the 1919 Eclipse Expedition
The 1919 Eclipse Expedition to test the light-bending prediction of General Relativity remains one of the most famous physics experiments of the 20th century. However, in recent decades it has been increasingly often alleged that the data-analysis of the expedition's leaders was faulty and biased in favor of Einstein's theory. Arthur Stanley Eddington is particularly alleged to have been prejudiced in favor of general relativity. Specifically it is claimed that some of the data, which would have favored the so-called Newtonian prediction, was thrown out on dubious grounds. This paper argues that a close examination of the views of the expedition's organizers, and of their data analysis, suggests that they had good grounds for acting as they did, and that the key people involved, in particular the astronomer Frank Watson Dyson, were not biased in favor of Einstein. It also draws attention to a modern re-analysis of the most important eclipse plates which, though overlooked until now, tends to strongly support the thesis of this paper.
physics.hist-ph astro-ph gr-qc
the 1919 eclipse expedition to test the lightbending prediction of general relativity remains one of the most famous physics experiments of the 20th century however in recent decades it has been increasingly often alleged that the dataanalysis of the expeditions leaders was faulty and biased in favor of einsteins theory arthur stanley eddington is particularly alleged to have been prejudiced in favor of general relativity specifically it is claimed that some of the data which would have favored the socalled newtonian prediction was thrown out on dubious grounds this paper argues that a close examination of the views of the expeditions organizers and of their data analysis suggests that they had good grounds for acting as they did and that the key people involved in particular the astronomer frank watson dyson were not biased in favor of einstein it also draws attention to a modern reanalysis of the most important eclipse plates which though overlooked until now tends to strongly support the thesis of this paper
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709.0686
Bio-Mechanical Model of the Brain for a Per-Operative Image-Guided Neuronavigator Compensating for "Brain-Shift" Deformations
In this paper we present a methodology to address the problem of brain tissue deformation referred to as 'brain-shift'. This deformation occurs throughout a neurosurgery intervention and strongly alters the accuracy of the neuronavigation systems used to date in clinical routine which rely solely on pre-operative patient imaging to locate the surgical target, such as a tumour or a functional area. After a general description of the framework of our intra-operative image-guided system, we describe a procedure to generate patient specific finite element meshes of the brain and propose a biomechanical model which can take into account tissue deformations and surgical procedures that modify the brain structure, like tumour or tissue resection.
physics.med-ph
in this paper we present a methodology to address the problem of brain tissue deformation referred to as brainshift this deformation occurs throughout a neurosurgery intervention and strongly alters the accuracy of the neuronavigation systems used to date in clinical routine which rely solely on preoperative patient imaging to locate the surgical target such as a tumour or a functional area after a general description of the framework of our intraoperative imageguided system we describe a procedure to generate patient specific finite element meshes of the brain and propose a biomechanical model which can take into account tissue deformations and surgical procedures that modify the brain structure like tumour or tissue resection
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709.0687
On the concept of relativistic mass
Within the past fifteen years the use of the concept of "relativistic mass" has been on the decline and has been replaced by the concept of "proper mass" (aka "rest mass") - ?simply referred to as "mass" and labeled "m" by its proponents. This decline in usage appears to be due to arguments presented in several journal articles over the last thirty-five years, as well as to standard practices in the field of particle physics. The aforementioned debate consists of arguments as to how the term "mass" should be defined to maximize logic as well as to be less confusing to the layman and people just starting to learn relativity. Lacking in the debate is a clear definition of all types of mass and all its usages in a wide variety of cases. The purpose in this article is to bring a unifying perspective to the subject. In doing so I will explore those things omitted from previous articles on this subject including the importance of point particles vs. extended objects; open vs. closed systems and gravitational mass. Although I argue for the usage of relativistic mass I do "not" argue that proper mass is not an important tool in relativistic dynamics.
physics.gen-ph
within the past fifteen years the use of the concept of relativistic mass has been on the decline and has been replaced by the concept of proper mass aka rest mass simply referred to as mass and labeled m by its proponents this decline in usage appears to be due to arguments presented in several journal articles over the last thirtyfive years as well as to standard practices in the field of particle physics the aforementioned debate consists of arguments as to how the term mass should be defined to maximize logic as well as to be less confusing to the layman and people just starting to learn relativity lacking in the debate is a clear definition of all types of mass and all its usages in a wide variety of cases the purpose in this article is to bring a unifying perspective to the subject in doing so i will explore those things omitted from previous articles on this subject including the importance of point particles vs extended objects open vs closed systems and gravitational mass although i argue for the usage of relativistic mass i do not argue that proper mass is not an important tool in relativistic dynamics
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709.0688
rho0(770)-f0(980) mixing and CPT violation in a non-unitary evolution of pion creation process pi(-)p->pi(-)pi(+)n on polarized target
Unitary evolution from pure initial states to pure final states in pi(-)p-> pi(-)pi(+)n imposes constraints on pion production amplitudes that are violated by CERN data on polarized target at 17.2 GeV/c. The pion creation is a non-unitary process arising from a unitary co-evolution of the pion creation process with a quantum environment. The purpose of this work is to identify the interacting degrees of freedom of the environment in a high resolution amplitude analysis of CERN data on polarized target for dipion masses 580-1080 MeV. The S-wave spectra |S|^2 show presence of rho0(770) while P-wave spectra |L|^2 show a dip at f0(980) mass. The observed rho0(770)-f0(980) mixing is encoded in all measured density matrix elements which also encode a level splitting of the spectra arising from the interaction of the pion creation process with the environment. The analytical form of the level splitting reveals the existence of a new quantum number characterizing the environment. We propose a model for the CPT violating interaction of the pion creation process with the environment in which non-diagonal transitions between resonant qqbar modes and pi(-)pi(+) states lead to vector-scalar mixing and a dynamic entanglement of the pi(-)pi(+) isospin states. The final states pi(-)p(+)n do not posses CPT cojugate states and the concept of CPT symmetry looses its meanining.
hep-ph hep-th
unitary evolution from pure initial states to pure final states in pip pipin imposes constraints on pion production amplitudes that are violated by cern data on polarized target at 172 gevc the pion creation is a nonunitary process arising from a unitary coevolution of the pion creation process with a quantum environment the purpose of this work is to identify the interacting degrees of freedom of the environment in a high resolution amplitude analysis of cern data on polarized target for dipion masses 5801080 mev the swave spectra s2 show presence of rho0770 while pwave spectra l2 show a dip at f0980 mass the observed rho0770f0980 mixing is encoded in all measured density matrix elements which also encode a level splitting of the spectra arising from the interaction of the pion creation process with the environment the analytical form of the level splitting reveals the existence of a new quantum number characterizing the environment we propose a model for the cpt violating interaction of the pion creation process with the environment in which nondiagonal transitions between resonant qqbar modes and pipi states lead to vectorscalar mixing and a dynamic entanglement of the pipi isospin states the final states pipn do not posses cpt cojugate states and the concept of cpt symmetry looses its meanining
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709.0689
A Plantar-pressure Based Tongue-placed Tactile Biofeedback System for Balance Improvement
Maintaining an upright stance represents a complex task, which is achieved by integrating sensory information from the visual, vestibular and somatosensory systems. When one of these sensory inputs becomes unavailable and/or inaccurate and/or unreliable, postural control generally is degraded. One way to solve this problem is to supplement and/or substitute limited/altered/missing sensory information by providing additional sensory information to the central nervous system via an alternative sensory modality. Along these lines, we developed an original biofeedback system [1] whose underlying principle consists in supplying the user with supplementary sensory information related to foot sole pressure distribution through a tongue-placed output device (Tongue Display Unit, "TDU" [2]). The purpose of the present experiment was to assess its effectiveness in improving balance in young healthy adults.
physics.med-ph q-bio.NC
maintaining an upright stance represents a complex task which is achieved by integrating sensory information from the visual vestibular and somatosensory systems when one of these sensory inputs becomes unavailable andor inaccurate andor unreliable postural control generally is degraded one way to solve this problem is to supplement andor substitute limitedalteredmissing sensory information by providing additional sensory information to the central nervous system via an alternative sensory modality along these lines we developed an original biofeedback system 1 whose underlying principle consists in supplying the user with supplementary sensory information related to foot sole pressure distribution through a tongueplaced output device tongue display unit tdu 2 the purpose of the present experiment was to assess its effectiveness in improving balance in young healthy adults
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709.069
Constructing presentations of subgroups of right-angled Artin groups
Let $G$ be the right-angled Artin group associated to the flag complex $\Sigma$ and let $\pi:G\to\Z$ be its canonical height function. We investigate the presentation theory of the groups $\Gamma_n=\pi^{-1}(n\Z)$ and construct an algorithm that, given $n$ and $\Sigma$, outputs a presentation of optimal deficiency on a minimal generating set, provided $\Sigma$ is triangle-free; the deficiency tends to infinity as $n\to\infty$ if and only if the corresponding Bestvina-Brady kernel $\bigcap_n\Gamma_n$ is not finitely presented, and the algorithm detects whether this is the case. We explain why there cannot exist an algorithm that constructs finite presentations with these properties in the absence of the triangle-free hypothesis. We explore what is possible in the general case, describing how to use the configuration of 2-simplices in $\Sigma$ to simplify presentations and giving conditions on $\Sigma$ that ensure that the deficiency goes to infinity with $n$. We also prove, for general $\Sigma$, that the abelianized deficiency of $\Gamma_n$ tends to infinity if and only if $\Sigma$ is 1-acyclic, and discuss connections with the relation gap problem.
math.GR
let g be the rightangled artin group associated to the flag complex sigma and let pigtoz be its canonical height function we investigate the presentation theory of the groups gamma_npi1nz and construct an algorithm that given n and sigma outputs a presentation of optimal deficiency on a minimal generating set provided sigma is trianglefree the deficiency tends to infinity as ntoinfty if and only if the corresponding bestvinabrady kernel bigcap_ngamma_n is not finitely presented and the algorithm detects whether this is the case we explain why there cannot exist an algorithm that constructs finite presentations with these properties in the absence of the trianglefree hypothesis we explore what is possible in the general case describing how to use the configuration of 2simplices in sigma to simplify presentations and giving conditions on sigma that ensure that the deficiency goes to infinity with n we also prove for general sigma that the abelianized deficiency of gamma_n tends to infinity if and only if sigma is 1acyclic and discuss connections with the relation gap problem
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709.0691
Dynamical modelling of luminous and dark matter in 17 Coma early-type galaxies
Dynamical models for 17 Coma early-type galaxies are presented. The galaxy sample consists of flattened, rotating as well as non-rotating early-types including cD and S0 galaxies with luminosities between M=-18.79 and M=-22.56. Kinematical long-slit observations cover at least the major and minor axis and extend to 1-4 effective radii. Axisymmetric Schwarzschild models are used to derive stellar mass-to-light ratios and dark halo parameters. In every galaxy models with a dark matter halo match the data better than models without. The statistical significance is over 95 percent for 8 galaxies, around 90 percent for 5 galaxies and for four galaxies it is not significant. For the highly significant cases systematic deviations between observed and modelled kinematics are clearly seen; for the remaining galaxies differences are more statistical in nature. Best-fit models contain 10-50 percent dark matter inside the half-light radius. The central dark matter density is at least one order of magnitude lower than the luminous mass density. The central phase-space density of dark matter is often orders of magnitude lower than in the luminous component, especially when the halo core radius is large. The orbital system of the stars along the major-axis is slightly dominated by radial motions. Some galaxies show tangential anisotropy along the minor-axis, which is correlated with the minor-axis Gauss-Hermite coefficient H4. Changing the balance between data-fit and regularisation constraints does not change the reconstructed mass structure significantly. Model anisotropies tend to strengthen if the weight on regularisation is reduced, but the general property of a galaxy to be radially or tangentially anisotropic, respectively, does not change. (abridged)
astro-ph
dynamical models for 17 coma earlytype galaxies are presented the galaxy sample consists of flattened rotating as well as nonrotating earlytypes including cd and s0 galaxies with luminosities between m1879 and m2256 kinematical longslit observations cover at least the major and minor axis and extend to 14 effective radii axisymmetric schwarzschild models are used to derive stellar masstolight ratios and dark halo parameters in every galaxy models with a dark matter halo match the data better than models without the statistical significance is over 95 percent for 8 galaxies around 90 percent for 5 galaxies and for four galaxies it is not significant for the highly significant cases systematic deviations between observed and modelled kinematics are clearly seen for the remaining galaxies differences are more statistical in nature bestfit models contain 1050 percent dark matter inside the halflight radius the central dark matter density is at least one order of magnitude lower than the luminous mass density the central phasespace density of dark matter is often orders of magnitude lower than in the luminous component especially when the halo core radius is large the orbital system of the stars along the majoraxis is slightly dominated by radial motions some galaxies show tangential anisotropy along the minoraxis which is correlated with the minoraxis gausshermite coefficient h4 changing the balance between datafit and regularisation constraints does not change the reconstructed mass structure significantly model anisotropies tend to strengthen if the weight on regularisation is reduced but the general property of a galaxy to be radially or tangentially anisotropic respectively does not change abridged
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709.0692
Thickness-dependence of the electronic properties in V2O3 thin films
High quality vanadium sesquioxide V2O3 films (170-1100 {\AA}) were grown using the pulsed laser deposition technique on (0001)-oriented sapphire substrates, and the effects of film thickness on the lattice strain and electronic properties were examined. X-ray diffraction indicates that there is an in-plane compressive lattice parameter (a), close to -3.5% with respect to the substrate and an out-of-plane tensile lattice parameter (c) . The thin film samples display metallic character between 2-300 K, and no metal-to-insulator transition is observed. At low temperature, the V2O3 films behave as a strongly correlated metal, and the resistivity (\rho) follows the equation \rho =\rho_0 + A T^2, where A is the transport coefficient in a Fermi liquid. Typical values of A have been calculated to be 0.14 \mu\Omega cm K^{-2}, which is in agreement with the coefficient reported for V2O3 single crystals under high pressure. Moreover, a strong temperature-dependence of the Hall resistance confirms the electronic correlations of these V2O3 thin films samples.
cond-mat.str-el cond-mat.mtrl-sci
high quality vanadium sesquioxide v2o3 films 1701100 aa were grown using the pulsed laser deposition technique on 0001oriented sapphire substrates and the effects of film thickness on the lattice strain and electronic properties were examined xray diffraction indicates that there is an inplane compressive lattice parameter a close to 35 with respect to the substrate and an outofplane tensile lattice parameter c the thin film samples display metallic character between 2300 k and no metaltoinsulator transition is observed at low temperature the v2o3 films behave as a strongly correlated metal and the resistivity rho follows the equation rho rho_0 a t2 where a is the transport coefficient in a fermi liquid typical values of a have been calculated to be 014 muomega cm k2 which is in agreement with the coefficient reported for v2o3 single crystals under high pressure moreover a strong temperaturedependence of the hall resistance confirms the electronic correlations of these v2o3 thin films samples
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709.0693
The closed string spectrum of SU(N) gauge theories in 2+1 dimensions
We use lattice techniques to study the closed-string spectrum of SU(N) gauge theories in 2+1 dimensions. We calculate the energies of the lowest lying ~30 states for strings with lengths between l ~ 0.45 fm and l ~ 3 fm, and compare to different theoretical predictions. We obtain unambiguous evidence that the closed-strings are in the universality class of the Nambu-Goto free bosonic string. Moreover, we clearly see that our data can be described by a covariant string theory with a small/moderate correction down to very short distance scales, and possibly on all distance scales at large-N.
hep-lat hep-th
we use lattice techniques to study the closedstring spectrum of sun gauge theories in 21 dimensions we calculate the energies of the lowest lying 30 states for strings with lengths between l 045 fm and l 3 fm and compare to different theoretical predictions we obtain unambiguous evidence that the closedstrings are in the universality class of the nambugoto free bosonic string moreover we clearly see that our data can be described by a covariant string theory with a smallmoderate correction down to very short distance scales and possibly on all distance scales at largen
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709.0694
A Rigid-Field Hydrodynamics approach to modeling the magnetospheres of massive stars
We introduce a new Rigid-Field Hydrodynamics approach to modeling the magnetospheres of massive stars in the limit of very-strong magnetic fields. Treating the field lines as effectively rigid, we develop hydrodynamical equations describing the 1-dimensional flow along each, subject to pressure, radiative, gravitational, and centrifugal forces. We solve these equations numerically for a large ensemble of field lines, to build up a 3-dimensional time-dependent simulation of a model star with parameters similar to the archetypal Bp star sigma Ori E. Since the flow along each field line can be solved for independently of other field lines, the computational cost of this approach is a fraction of an equivalent magnetohydrodynamical treatment. The simulations confirm many of the predictions of previous analytical and numerical studies. Collisions between wind streams from opposing magnetic hemispheres lead to strong shock heating. The post-shock plasma cools initially via X-ray emission, and eventually accumulates into a warped, rigidly rotating disk defined by the locus of minima of the effective (gravitational plus centrifugal) potential. But a number of novel results also emerge. For field lines extending far from the star, the rapid area divergence enhances the radiative acceleration of the wind, resulting in high shock velocities (up to ~3,000 km/s) and hard X-rays. Moreover, the release of centrifugal potential energy continues to heat the wind plasma after the shocks, up to temperatures around twice those achieved at the shocks themselves. Finally, in some circumstances the cool plasma in the accumulating disk can oscillate about its equilibrium position, possibly due to radiative cooling instabilities in the adjacent post-shock regions.
astro-ph
we introduce a new rigidfield hydrodynamics approach to modeling the magnetospheres of massive stars in the limit of verystrong magnetic fields treating the field lines as effectively rigid we develop hydrodynamical equations describing the 1dimensional flow along each subject to pressure radiative gravitational and centrifugal forces we solve these equations numerically for a large ensemble of field lines to build up a 3dimensional timedependent simulation of a model star with parameters similar to the archetypal bp star sigma ori e since the flow along each field line can be solved for independently of other field lines the computational cost of this approach is a fraction of an equivalent magnetohydrodynamical treatment the simulations confirm many of the predictions of previous analytical and numerical studies collisions between wind streams from opposing magnetic hemispheres lead to strong shock heating the postshock plasma cools initially via xray emission and eventually accumulates into a warped rigidly rotating disk defined by the locus of minima of the effective gravitational plus centrifugal potential but a number of novel results also emerge for field lines extending far from the star the rapid area divergence enhances the radiative acceleration of the wind resulting in high shock velocities up to 3000 kms and hard xrays moreover the release of centrifugal potential energy continues to heat the wind plasma after the shocks up to temperatures around twice those achieved at the shocks themselves finally in some circumstances the cool plasma in the accumulating disk can oscillate about its equilibrium position possibly due to radiative cooling instabilities in the adjacent postshock regions
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709.0695
A Reformulation of the Hoop Conjecture
A reformulation of the Hoop Conjecture based on the concept of trapped circle is presented. The problems of severe compactness in every spatial direction, and of how to superpose the hoops with the surface of the black hole, are resolved. A new conjecture concerning "peeling" properties of dynamical/trapping horizons is propounded. A novel geometric Hoop inequality is put forward. The possibility of carrying over the results to arbitrary dimension is discussed.
gr-qc
a reformulation of the hoop conjecture based on the concept of trapped circle is presented the problems of severe compactness in every spatial direction and of how to superpose the hoops with the surface of the black hole are resolved a new conjecture concerning peeling properties of dynamicaltrapping horizons is propounded a novel geometric hoop inequality is put forward the possibility of carrying over the results to arbitrary dimension is discussed
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709.0696
Resonant x-ray scattering study of NpRhGa_5 and NpCoGa_5
We report a resonant x-ray scattering (RXS) study of antiferromagnetic neptunium compounds NpCoGa_5 and NpRhGa_5 at the Np M_4 and Ga K-edges. Large resonant signals of magnetic dipole character are observed below the Neel temperatures at both edges. The signals at the Np edges confirm the behaviour determined previously from neutron diffraction, i.e. the moments along [001] in NpCoGa_{5} and in NpRhGa_5 a reorientation of the moments from the c-axis direction to the ab plane. In the latter material, on application of magnetic field of 9 Tesla along the [010] direction we observe a change in the population of different [110]-type domains. We observe also a magnetic dipole signal at the Ga K-edge, similarly to the reported UGa_3 case, that can be interpreted within a semi-localized model as an orbital polarization of the Ga 4p states induced via strong hybridization with the Np 5f valence band. Quantitative analysis of the signal shows that the Ga dipole on the two different Ga sites follows closely the Np magnetic moment reorientation in NpRhGa_5. The ratios of the signals on the two inequivalent Ga sites are not the same for the different compounds.
cond-mat.str-el
we report a resonant xray scattering rxs study of antiferromagnetic neptunium compounds npcoga_5 and nprhga_5 at the np m_4 and ga kedges large resonant signals of magnetic dipole character are observed below the neel temperatures at both edges the signals at the np edges confirm the behaviour determined previously from neutron diffraction ie the moments along 001 in npcoga_5 and in nprhga_5 a reorientation of the moments from the caxis direction to the ab plane in the latter material on application of magnetic field of 9 tesla along the 010 direction we observe a change in the population of different 110type domains we observe also a magnetic dipole signal at the ga kedge similarly to the reported uga_3 case that can be interpreted within a semilocalized model as an orbital polarization of the ga 4p states induced via strong hybridization with the np 5f valence band quantitative analysis of the signal shows that the ga dipole on the two different ga sites follows closely the np magnetic moment reorientation in nprhga_5 the ratios of the signals on the two inequivalent ga sites are not the same for the different compounds
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709.0697
A Note on Gravitational Baryogenesis
The coupling between Ricci scalar curvature and the baryon number current dynamically breaks CPT in an expanding universe and leads to baryon asymmetry. We study the effect of time dependence of equation of state parameter of the FRW universe on this asymmetry.
gr-qc hep-th
the coupling between ricci scalar curvature and the baryon number current dynamically breaks cpt in an expanding universe and leads to baryon asymmetry we study the effect of time dependence of equation of state parameter of the frw universe on this asymmetry
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709.0698
Probing two-fluid hydrodynamics in a trapped Fermi superfluid at unitarity
We develop a variational approach to calculate the density response function at finite temperatures of the lowest-lying two-fluid modes in a trapped two-component Fermi superfluid close to a Feshbach resonance. The out-of-phase oscillations, which are the analogue in trapped gases of second sound in uniform superfluids, have so far not been observed in cold-atom experiments. At unitarity, we show that these modes are observable at finite temperatures via two-photon Bragg scattering, whose spectrum is related to the imaginary part of density response function. This provides direct evidence for superfluidity and a promising way to test microscopic results for thermodynamics at unitarity.
cond-mat.other
we develop a variational approach to calculate the density response function at finite temperatures of the lowestlying twofluid modes in a trapped twocomponent fermi superfluid close to a feshbach resonance the outofphase oscillations which are the analogue in trapped gases of second sound in uniform superfluids have so far not been observed in coldatom experiments at unitarity we show that these modes are observable at finite temperatures via twophoton bragg scattering whose spectrum is related to the imaginary part of density response function this provides direct evidence for superfluidity and a promising way to test microscopic results for thermodynamics at unitarity
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709.0699
Optical-approximation analysis of sidewall-spacing effects on the force between two squares with parallel sidewalls
Using the ray-optics approximation, we analyze the Casimir force in a two dimensional domain formed by two metallic blocks adjacent to parallel metallic sidewalls, which are separated from the blocks by a finite distance h. For h > 0, the ray-optics approach is not exact because diffraction effects are neglected. Nevertheless, we show that ray optics is able to qualitatively reproduce a surprising effect recently identified in an exact numerical calculation: the force between the blocks varies non-monotonically with h. In this sense, the ray-optics approach captures an essential part of the physics of multi-body interactions in this system, unlike simpler pairwise-interaction approximations such as PFA. Furthermore, by comparison to the exact numerical results, we are able to quantify the impact of diffraction on Casimir forces in this geometry.
quant-ph
using the rayoptics approximation we analyze the casimir force in a two dimensional domain formed by two metallic blocks adjacent to parallel metallic sidewalls which are separated from the blocks by a finite distance h for h 0 the rayoptics approach is not exact because diffraction effects are neglected nevertheless we show that ray optics is able to qualitatively reproduce a surprising effect recently identified in an exact numerical calculation the force between the blocks varies nonmonotonically with h in this sense the rayoptics approach captures an essential part of the physics of multibody interactions in this system unlike simpler pairwiseinteraction approximations such as pfa furthermore by comparison to the exact numerical results we are able to quantify the impact of diffraction on casimir forces in this geometry
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709.07
Abundance of elliptic dynamics on conservative 3-flows
We consider a compact 3-dimensional boundaryless Riemannian manifold M and the set of divergence-free (or zero divergence) vector fields without singularities, then we prove that this set has a C1-residual such that any vector field inside it is Anosov or else its elliptical orbits are dense in the manifold M.
math.DS
we consider a compact 3dimensional boundaryless riemannian manifold m and the set of divergencefree or zero divergence vector fields without singularities then we prove that this set has a c1residual such that any vector field inside it is anosov or else its elliptical orbits are dense in the manifold m
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709.0701
Statistical mechanics of non-hamiltonian systems: Traffic flow
Statistical mechanics of a small system of cars on a single-lane road is developed. The system is not characterized by a Hamiltonian but by a conditional probability of a velocity of a car for the given velocity and distance of the car ahead. Distribution of car velocities for various densities of a group of cars are derived as well as probabilities of density fluctuations of the group for different velocities. For high braking abilities of cars free-flow and congested phases are found. Platoons of cars are formed for system of cars with inefficient brakes. A first order phase transition between free-flow and congested phase is suggested.
physics.soc-ph
statistical mechanics of a small system of cars on a singlelane road is developed the system is not characterized by a hamiltonian but by a conditional probability of a velocity of a car for the given velocity and distance of the car ahead distribution of car velocities for various densities of a group of cars are derived as well as probabilities of density fluctuations of the group for different velocities for high braking abilities of cars freeflow and congested phases are found platoons of cars are formed for system of cars with inefficient brakes a first order phase transition between freeflow and congested phase is suggested
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709.0702
On two-component contact model in continuum with one independent component
Properties of a contact process in continuum for a system of two type particles one type of which is independent are considered. We study dynamics of the first and second order correlation functions, their asymptotics and dependence on parameters of the system.
math-ph math.CA math.DS math.MP
properties of a contact process in continuum for a system of two type particles one type of which is independent are considered we study dynamics of the first and second order correlation functions their asymptotics and dependence on parameters of the system
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709.0703
Modules of covariants in modular invariant theory
Let the finite group $G$ act linearly on the vector space $V$ over the field $k$ of arbitrary characteristic. If $H<G$ is a subgroup the extension of invariant rings $k[V]^G\subset k[V]^H$ is studied using modules of covariants. An example of our results is the following. Let $W$ be the subgroup of $G$ generated by the reflections in $G$. A classical theorem due to Serre says that if $k[V]$ is a free $k[V]^G$-module then $G=W$. We generalize this result as follows. If $k[V]^H$ is a free $k[V]^G$-module then $G$ is generated by $H$ and $W$, and the invariant ring $k[V]^{H\cap W}$ is free over $k[V]^W$ and generated as an algebra by $H$-invariants and $W$-invariants.
math.AC
let the finite group g act linearly on the vector space v over the field k of arbitrary characteristic if hg is a subgroup the extension of invariant rings kvgsubset kvh is studied using modules of covariants an example of our results is the following let w be the subgroup of g generated by the reflections in g a classical theorem due to serre says that if kv is a free kvgmodule then gw we generalize this result as follows if kvh is a free kvgmodule then g is generated by h and w and the invariant ring kvhcap w is free over kvw and generated as an algebra by hinvariants and winvariants
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709.0704
White Paper on the Status and Future of Ground-based Gamma-ray Astronomy
In recent years, ground-based gamma-ray observatories have made a number of important astrophysical discoveries which have attracted the attention of the wider scientific community. The Division of Astrophysics of the American Physical Society has requested the preparation of a white paper on the status and future of ground-based gamma-ray astronomy to define the science goals of the future observatory, to determine the performance specifications, and to identify the areas of necessary technology development. In this contribution we give a brief overview of the activities of the current white paper team and invite the international community to contribute to the white paper.
astro-ph
in recent years groundbased gammaray observatories have made a number of important astrophysical discoveries which have attracted the attention of the wider scientific community the division of astrophysics of the american physical society has requested the preparation of a white paper on the status and future of groundbased gammaray astronomy to define the science goals of the future observatory to determine the performance specifications and to identify the areas of necessary technology development in this contribution we give a brief overview of the activities of the current white paper team and invite the international community to contribute to the white paper
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709.0705
Search for resonant ttbar production in ppbar collisions at sqrt{s}=1.96 TeV
We report on a search for narrow-width particles decaying to a top and antitop quark pair. The data set used in the analysis corresponds to an integrated luminosity of 680 pb^{-1} collected with the Collider Detector at Fermilab in Run II. We present 95% confidence level upper limits on the cross section times branching ratio. Assuming a specific topcolor-assisted technicolor production model, the leptophobic Z' with width \Gamma_{Z'}=0.012M_{Z'}, we exclude the mass range M_{Z'} < 725 GeV/c^2 at the 95% confidence level.
hep-ex
we report on a search for narrowwidth particles decaying to a top and antitop quark pair the data set used in the analysis corresponds to an integrated luminosity of 680 pb1 collected with the collider detector at fermilab in run ii we present 95 confidence level upper limits on the cross section times branching ratio assuming a specific topcolorassisted technicolor production model the leptophobic z with width gamma_z0012m_z we exclude the mass range m_z 725 gevc2 at the 95 confidence level
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709.0706
Leading Order QED Electrical Conductivity from the 3PI Effective Action
In this article we study the electrical conductivity in QED using the resummed 3PI effective action. We work to 3-loop order in the effective action. We show that the resulting expression for the conductivity is explicitly gauge invariant, and that the integral equations that resum the pinching and colinear contributions are produced naturally by the formalism. All leading order terms are included, without the need for any kind of power counting arguments.
hep-ph
in this article we study the electrical conductivity in qed using the resummed 3pi effective action we work to 3loop order in the effective action we show that the resulting expression for the conductivity is explicitly gauge invariant and that the integral equations that resum the pinching and colinear contributions are produced naturally by the formalism all leading order terms are included without the need for any kind of power counting arguments
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709.0707
The extremal volume ellipsoids of convex bodies, their symmetry properties, and their determination in some special cases
A convex body K has associated with it a unique circumscribed ellipsoid CE(K) with minimum volume, and a unique inscribed ellipsoid IE(K) with maximum volume. We first give a unified, modern exposition of the basic theory of these extremal ellipsoids using the semi-infinite programming approach pioneered by Fritz John in his seminal 1948 paper. We then investigate the automorphism groups of convex bodies and their extremal ellipsoids. We show that if the automorphism group of a convex body K is large enough, then it is possible to determine the extremal ellipsoids CE(K) and IE(K) exactly, using either semi-infinite programming or nonlinear programming. As examples, we compute the extremal ellipsoids when the convex body K is the part of a given ellipsoid between two parallel hyperplanes, and when K is a truncated second order cone or an ellipsoidal cylinder.
math.MG math.FA
a convex body k has associated with it a unique circumscribed ellipsoid cek with minimum volume and a unique inscribed ellipsoid iek with maximum volume we first give a unified modern exposition of the basic theory of these extremal ellipsoids using the semiinfinite programming approach pioneered by fritz john in his seminal 1948 paper we then investigate the automorphism groups of convex bodies and their extremal ellipsoids we show that if the automorphism group of a convex body k is large enough then it is possible to determine the extremal ellipsoids cek and iek exactly using either semiinfinite programming or nonlinear programming as examples we compute the extremal ellipsoids when the convex body k is the part of a given ellipsoid between two parallel hyperplanes and when k is a truncated second order cone or an ellipsoidal cylinder
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709.0708
Pion Production in Neutrino-Nucleon Reactions
We construct a model for the weak pion production off the nucleon, which in addition to the weak excitation of the $\Delta(1232)$ resonance and its subsequent decay into $N\pi$, it includes also some background terms required by chiral symmetry. We re-fit the $C_5^A(q^2)$ form factor to the flux averaged $\nu_\mu p \to \mu^-p\pi^+$ ANL $q^2-$differential cross section data, finding a substantially smaller contribution of the $\Delta$ pole mechanism than traditionally assumed in the literature. We also show that the interference between the Delta pole and the background terms produces parity-violating contributions to the pion angular differential cross section.
nucl-th
we construct a model for the weak pion production off the nucleon which in addition to the weak excitation of the delta1232 resonance and its subsequent decay into npi it includes also some background terms required by chiral symmetry we refit the c_5aq2 form factor to the flux averaged nu_mu p to muppi anl q2differential cross section data finding a substantially smaller contribution of the delta pole mechanism than traditionally assumed in the literature we also show that the interference between the delta pole and the background terms produces parityviolating contributions to the pion angular differential cross section
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709.0709
One-dimensional resistive states in quasi-two-dimensional superconductors
We investigate competition between one- and two-dimensional topological excitations - phase slips and vortices - in formation of resistive states in quasi-two-dimensional superconductors in a wide temperature range below the mean-field transition temperature $T_{C0}$. The widths $w$ = 100 nm of our ultrathin NbN samples is substantially larger than the Ginzburg-Landau coherence length $\xi$ = 4nm and the fluctuation resistivity above $T_{C0}$ has a two-dimensional character. However, our data shows that the resistivity below $T_{C0}$ is produced by one-dimensional excitations, - thermally activated phase slip strips (PSSs) overlapping the sample cross-section. We also determine the scaling phase diagram, which shows that even in wider samples the PSS contribution dominates over vortices in a substantial region of current/temperature variations. Measuring the resistivity within seven orders of magnitude, we find that the quantum phase slips can only be essential below this level.
cond-mat.supr-con cond-mat.dis-nn
we investigate competition between one and twodimensional topological excitations phase slips and vortices in formation of resistive states in quasitwodimensional superconductors in a wide temperature range below the meanfield transition temperature t_c0 the widths w 100 nm of our ultrathin nbn samples is substantially larger than the ginzburglandau coherence length xi 4nm and the fluctuation resistivity above t_c0 has a twodimensional character however our data shows that the resistivity below t_c0 is produced by onedimensional excitations thermally activated phase slip strips psss overlapping the sample crosssection we also determine the scaling phase diagram which shows that even in wider samples the pss contribution dominates over vortices in a substantial region of currenttemperature variations measuring the resistivity within seven orders of magnitude we find that the quantum phase slips can only be essential below this level
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709.071
Combinatorically Prescribed Packings and Applications to Conformal and Quasiconformal Maps
The Andreev-Thurston Circle Packing Theorem is generalized to packings of convex bodies in planar simply connected domains. This turns out to be a useful tool for constructing conformal and quasiconformal mappings with interesting geometric properties. We attempt to illustrate this with a few results about uniformizations of finitely connected planar domains. For example, the following variation of a theorem by Courant, Manel and Shiffman is proved and generalized. If $G$ is an $n+1$-connected bounded planar domain, $H$ is a simply connected bounded planar domain, and $P_1,P_2,...,P_n$ are (compact) planar convex bodies, then sets $P_j'$ can be found so that $G$ is conformally equivalent to $H-\cup_{j=1}^n P_j'$, and each $P_j'$ is either a point, or is positively homothetic to $P_j$.
math.CV math.CO math.MG
the andreevthurston circle packing theorem is generalized to packings of convex bodies in planar simply connected domains this turns out to be a useful tool for constructing conformal and quasiconformal mappings with interesting geometric properties we attempt to illustrate this with a few results about uniformizations of finitely connected planar domains for example the following variation of a theorem by courant manel and shiffman is proved and generalized if g is an n1connected bounded planar domain h is a simply connected bounded planar domain and p_1p_2p_n are compact planar convex bodies then sets p_j can be found so that g is conformally equivalent to hcup_j1n p_j and each p_j is either a point or is positively homothetic to p_j
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709.0711
Bayesian posterior classification of planetary nebulae according to the Peimbert types
In this paper we present a re-analysis of the criteria used to characterize the Peimbert classes I, IIa, IIb, III and IV, through a statistical study of a large sample of planetary nebulae previously classified according to these groups. In the original classification, it is usual to find planetary nebulae that cannot be associated with a single type; these most likely have dubious classifications into two or three types. Statistical methods can greatly contribute in providing a better characterization of planetary nebulae groups. We use the Bayes Theorem to calculate the posterior probabilities for an object to be member of each of the types I, IIa, IIb, III and IV. This calculation is particularly important for planetary nebulae that are ambiguously classified in the traditional method. The posterior probabilities are defined from the probability density function of classificatory parameters of a well-defined sample, composed only by planetary nebulae unambiguously fitted into the Peimbert types. Because the probabilities depend on the available observational data, they are conditional probabilities, and, as new observational data are added to the sample, the classification of the nebula can be improved, to take into account this new information. This method differs from the original classificatory scheme, because it provides a quantitative result of the representativity of the object within its group. Also, through the use of marginal distributions it is possible to extend the Peimbert classification even to those objects for which only a few classificatory parameters are known.
astro-ph
in this paper we present a reanalysis of the criteria used to characterize the peimbert classes i iia iib iii and iv through a statistical study of a large sample of planetary nebulae previously classified according to these groups in the original classification it is usual to find planetary nebulae that cannot be associated with a single type these most likely have dubious classifications into two or three types statistical methods can greatly contribute in providing a better characterization of planetary nebulae groups we use the bayes theorem to calculate the posterior probabilities for an object to be member of each of the types i iia iib iii and iv this calculation is particularly important for planetary nebulae that are ambiguously classified in the traditional method the posterior probabilities are defined from the probability density function of classificatory parameters of a welldefined sample composed only by planetary nebulae unambiguously fitted into the peimbert types because the probabilities depend on the available observational data they are conditional probabilities and as new observational data are added to the sample the classification of the nebula can be improved to take into account this new information this method differs from the original classificatory scheme because it provides a quantitative result of the representativity of the object within its group also through the use of marginal distributions it is possible to extend the peimbert classification even to those objects for which only a few classificatory parameters are known
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709.0712
Invariant theory of abelian transvection groups
Let $G$ be a finite group acting linearly on the vector space $V$ over a field of arbitrary characteristic. The action is called {\em coregular} if the invariant ring is generated by algebraically independent homogeneous invariants and the {\em direct summand property} holds if there is a surjective $k[V]^G$-linear map $\pi:k[V]\to k[V]^G$. The following Chevalley--Shephard--Todd type theorem is proved. Suppose $G$ is abelian, then the action is coregular if and only if $G$ is generated by pseudo-reflections and the direct summand property holds.
math.AC
let g be a finite group acting linearly on the vector space v over a field of arbitrary characteristic the action is called em coregular if the invariant ring is generated by algebraically independent homogeneous invariants and the em direct summand property holds if there is a surjective kvglinear map pikvto kvg the following chevalleyshephardtodd type theorem is proved suppose g is abelian then the action is coregular if and only if g is generated by pseudoreflections and the direct summand property holds
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709.0713
The geometrically-averaged density of states calculated from the local Green's function as a measure of localization
With the goal of measuring localization in disordered interacting systems, we examine the finite-size scaling of the geometrically-averaged density of states calculated from the local Green's function with finite energy resolution. Our results show that, unlike in a simple energy binning procedure, there is no limit in which the finite energy resolution is irrelevant.
cond-mat.str-el cond-mat.dis-nn
with the goal of measuring localization in disordered interacting systems we examine the finitesize scaling of the geometricallyaveraged density of states calculated from the local greens function with finite energy resolution our results show that unlike in a simple energy binning procedure there is no limit in which the finite energy resolution is irrelevant
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709.0714
The permutation group S_N and large Nc excited baryons
We study the excited baryon states for an arbitrary number of colors Nc from the perspective of the permutation group S_N of N objects. Classifying the transformation properties of states and quark-quark interaction operators under S_N allows a general analysis of the spin-flavor structure of the mass operator of these states, in terms of a few unknown constants parameterizing the unknown spatial structure. We explain how to perform the matching calculation of a general two-body quark-quark interaction onto the operators of the 1/Nc expansion. The inclusion of core and excited quark operators is shown to be necessary. Considering the case of the negative parity L=1 states transforming in the MS of S_N, we discuss the matching of the one-gluon and the Goldstone-boson exchange interactions.
hep-ph hep-th nucl-th
we study the excited baryon states for an arbitrary number of colors nc from the perspective of the permutation group s_n of n objects classifying the transformation properties of states and quarkquark interaction operators under s_n allows a general analysis of the spinflavor structure of the mass operator of these states in terms of a few unknown constants parameterizing the unknown spatial structure we explain how to perform the matching calculation of a general twobody quarkquark interaction onto the operators of the 1nc expansion the inclusion of core and excited quark operators is shown to be necessary considering the case of the negative parity l1 states transforming in the ms of s_n we discuss the matching of the onegluon and the goldstoneboson exchange interactions
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709.0715
On Chevalley-Shephard-Todd's theorem in positive characteristic
Let $G$ be a finite group acting linearly on the vector space $V$ over a field of arbitrary characteristic. The action is called coregular if the invariant ring is generated by algebraically independent homogeneous invariants and the direct summand property holds if there is a surjective $k[V]^G$-linear map $\pi:k[V]\to k[V]^G$. The following Chevalley-Shephard-Todd type theorem is proved. Suppose $V$ is an irreducible $kG$-representation, then the action is coregular if and only if $G$ is generated by pseudo-reflections and the direct summand property holds.
math.AC
let g be a finite group acting linearly on the vector space v over a field of arbitrary characteristic the action is called coregular if the invariant ring is generated by algebraically independent homogeneous invariants and the direct summand property holds if there is a surjective kvglinear map pikvto kvg the following chevalleyshephardtodd type theorem is proved suppose v is an irreducible kgrepresentation then the action is coregular if and only if g is generated by pseudoreflections and the direct summand property holds
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709.0716
Maximum Entanglement in Squeezed Boson and Fermion States
A class of squeezed boson and fermion states is studied with particular emphasis on the nature of entanglement. We first investigate the case of bosons, considering two-mode squeezed states. Then we construct the fermion version to show that such states are maximum entangled, for both bosons and fermions. To achieve these results, we demonstrate some relations involving squeezed boson states. The generalization to the case of fermions is made by using Grassmann variables.
quant-ph
a class of squeezed boson and fermion states is studied with particular emphasis on the nature of entanglement we first investigate the case of bosons considering twomode squeezed states then we construct the fermion version to show that such states are maximum entangled for both bosons and fermions to achieve these results we demonstrate some relations involving squeezed boson states the generalization to the case of fermions is made by using grassmann variables
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709.0717
Representation functions of bases for binary linear forms
Let F(x_1,...,x_m) = u_1 x_1 + ... + u_m x_m be a linear form with nonzero, relatively prime integer coefficients u_1,..., u_m. For any set A of integers, let F(A) = {F(a_1,...,a_m) : a_i in A for i=1,...,m}. The representation function associated with the form F is R_{A,F}(n) = card {(a_1,...,a_m) in A^m: F(a_1,..., a_m) = n}. The set A is a basis with respect to F for almost all integers the set Z\F(A) has asymptotic density zero. Equivalently, the representation function of an asymptotic basis is a function f:Z -> N_0 U {\infty} such that f^{-1}(0) has density zero. Given such a function, the inverse problem for bases is to construct a set A whose representation function is f. In this paper the inverse problem is solved for binary linear forms.
math.NT math.CO
let fx_1x_m u_1 x_1 u_m x_m be a linear form with nonzero relatively prime integer coefficients u_1 u_m for any set a of integers let fa fa_1a_m a_i in a for i1m the representation function associated with the form f is r_afn card a_1a_m in am fa_1 a_m n the set a is a basis with respect to f for almost all integers the set zfa has asymptotic density zero equivalently the representation function of an asymptotic basis is a function fz n_0 u infty such that f10 has density zero given such a function the inverse problem for bases is to construct a set a whose representation function is f in this paper the inverse problem is solved for binary linear forms
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709.0718
Evidence for a finite temperature phase transition in a bilayer quantum Hall system
We study the Josephson-like interlayer tunneling signature of the strongly correlated $\nu_T = 1$ quantum Hall phase in bilayer two-dimensional electron systems as a function of the layer separation, temperature and interlayer charge imbalance. Our results offer strong evidence that a finite temperature phase transition separates the interlayer coherent phase from incoherent phases which lack strong interlayer correlations. The transition temperature is dependent on both the layer spacing and charge imbalance between the layers.
cond-mat.mes-hall cond-mat.str-el
we study the josephsonlike interlayer tunneling signature of the strongly correlated nu_t 1 quantum hall phase in bilayer twodimensional electron systems as a function of the layer separation temperature and interlayer charge imbalance our results offer strong evidence that a finite temperature phase transition separates the interlayer coherent phase from incoherent phases which lack strong interlayer correlations the transition temperature is dependent on both the layer spacing and charge imbalance between the layers
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709.0719
Estimation of Possible Selectivity and Sensitivity of a Cooperative System to Low-Intensive Microwave Radiation
Recently, origins of non-deterministic behavior and free will in living systems obtain growing interest (see, e.g. Maye A, Hsieh C, Sugihara G, Brembs B (2007) Order in Spontaneous Behavior. PLoS ONE 2(5): e443. doi:10.1371/journal.pone.0000443). In this text, devoted to electromagnetic hypersensitivity, in n.2 and n.4, a possible physical mechanism of free will and consequent indeterminacy in behavior is discussed.
physics.bio-ph
recently origins of nondeterministic behavior and free will in living systems obtain growing interest see eg maye a hsieh c sugihara g brembs b 2007 order in spontaneous behavior plos one 25 e443 doi101371journalpone0000443 in this text devoted to electromagnetic hypersensitivity in n2 and n4 a possible physical mechanism of free will and consequent indeterminacy in behavior is discussed
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709.072
On knot Floer width and Turaev genus
To each knot $K\subset S^3$ one can associated its knot Floer homology $\hat{HFK}(K)$, a finitely generated bigraded abelian group. In general, the nonzero ranks of these homology groups lie on a finite number of slope one lines with respect to the bigrading. The width of the homology is, in essence, the largest horizontal distance between two such lines. Also, for each diagram $D$ of $K$ there is an associated Turaev surface, and the Turaev genus is the minimum genus of all Turaev surfaces for $K$. We show that the width of knot Floer homology is bounded by Turaev genus plus one. Skein relations for genus of the Turaev surface and width of a complex that generates knot Floer homology are given.
math.GT math.AT
to each knot ksubset s3 one can associated its knot floer homology hathfkk a finitely generated bigraded abelian group in general the nonzero ranks of these homology groups lie on a finite number of slope one lines with respect to the bigrading the width of the homology is in essence the largest horizontal distance between two such lines also for each diagram d of k there is an associated turaev surface and the turaev genus is the minimum genus of all turaev surfaces for k we show that the width of knot floer homology is bounded by turaev genus plus one skein relations for genus of the turaev surface and width of a complex that generates knot floer homology are given
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709.0721
A remark on degenerate singularity in three dimensional Ricci flow
We show that a rescale limit at any degenerate singularity of Ricci flow in dimension 3 is a steady gradient soliton. In particular, we give a geometric description of type I and type II singularities.
math.DG
we show that a rescale limit at any degenerate singularity of ricci flow in dimension 3 is a steady gradient soliton in particular we give a geometric description of type i and type ii singularities
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709.0722
Lattice Formulation of the N=4 D=3 Twisted Super Yang-Mills
A lattice formulation of a three dimensional super Yang-Mills model with a twisted N=4 supersymmetry is proposed. The extended supersymmetry algebra of all eight supercharges is fully and exactly realized on the lattice with a modified "Leibniz rule". The formulation we employ here is a three dimensional extension of the manifestly gauge covariant method which was developed in our previous proposal of Dirac-K\"ahler twisted N=2 super Yang-Mills on a two dimensional lattice. The twisted N=4 supersymmetry algebra is geometrically realized on a three dimensional lattice with link supercharges and the use of "shifted" (anti-)commutators. A possible solution to the recent critiques on the link formulation will be discussed.
hep-lat hep-th
a lattice formulation of a three dimensional super yangmills model with a twisted n4 supersymmetry is proposed the extended supersymmetry algebra of all eight supercharges is fully and exactly realized on the lattice with a modified leibniz rule the formulation we employ here is a three dimensional extension of the manifestly gauge covariant method which was developed in our previous proposal of dirackahler twisted n2 super yangmills on a two dimensional lattice the twisted n4 supersymmetry algebra is geometrically realized on a three dimensional lattice with link supercharges and the use of shifted anticommutators a possible solution to the recent critiques on the link formulation will be discussed
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709.0723
Viscous regularization and r-adaptive remeshing for finite element analysis of lipid membrane mechanics
As two-dimensional fluid shells, lipid bilayer membranes resist bending and stretching but are unable to sustain shear stresses. This property gives membranes the ability to adopt dramatic shape changes. In this paper, a finite element model is developed to study static equilibrium mechanics of membranes. In particular, a viscous regularization method is proposed to stabilize tangential mesh deformations and improve the convergence rate of nonlinear solvers. The Augmented Lagrangian method is used to enforce global constraints on area and volume during membrane deformations. As a validation of the method, equilibrium shapes for a shape-phase diagram of lipid bilayer vesicle are calculated. These numerical techniques are also shown to be useful for simulations of three-dimensional large-deformation problems: the formation of tethers (long tube-like exetensions); and Ginzburg-Landau phase separation of a two-lipid-component vesicle. To deal with the large mesh distortions of the two-phase model, modification of vicous regularization is explored to achieve r-adaptive mesh optimization.
physics.bio-ph physics.comp-ph
as twodimensional fluid shells lipid bilayer membranes resist bending and stretching but are unable to sustain shear stresses this property gives membranes the ability to adopt dramatic shape changes in this paper a finite element model is developed to study static equilibrium mechanics of membranes in particular a viscous regularization method is proposed to stabilize tangential mesh deformations and improve the convergence rate of nonlinear solvers the augmented lagrangian method is used to enforce global constraints on area and volume during membrane deformations as a validation of the method equilibrium shapes for a shapephase diagram of lipid bilayer vesicle are calculated these numerical techniques are also shown to be useful for simulations of threedimensional largedeformation problems the formation of tethers long tubelike exetensions and ginzburglandau phase separation of a twolipidcomponent vesicle to deal with the large mesh distortions of the twophase model modification of vicous regularization is explored to achieve radaptive mesh optimization
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709.0724
From Time-symmetric Microscopic Dynamics to Time-asymmetric Macroscopic Behavior: An Overview
Time-asymmetric behavior as embodied in the second law of thermodynamics is observed in {\it individual macroscopic} systems. It can be understood as arising naturally from time-symmetric microscopic laws when account is taken of a) the great disparity between microscopic and macroscopic scales, b) a low entropy state of the early universe, and c) the fact that what we observe is the behavior of systems coming from such an initial state--not all possible systems. The explanation of the origin of the second law based on these ingredients goes back to Maxwell, Thomson and particularly Boltzmann. Common alternate explanations, such as those based on the ergodic or mixing properties of probability distributions (ensembles) already present for chaotic dynamical systems having only a few degrees of freedom or on the impossibility of having a truly isolated system, are either unnecessary, misguided or misleading. Specific features of macroscopic evolution, such as the diffusion equation, do however depend on the dynamical instability (deterministic chaos) of trajectories of isolated macroscopic systems. The extensions of these classical notions to the quantum world is in many ways fairly direct. It does however also bring in some new problems. These will be discussed but not resolved.
cond-mat.stat-mech
timeasymmetric behavior as embodied in the second law of thermodynamics is observed in it individual macroscopic systems it can be understood as arising naturally from timesymmetric microscopic laws when account is taken of a the great disparity between microscopic and macroscopic scales b a low entropy state of the early universe and c the fact that what we observe is the behavior of systems coming from such an initial statenot all possible systems the explanation of the origin of the second law based on these ingredients goes back to maxwell thomson and particularly boltzmann common alternate explanations such as those based on the ergodic or mixing properties of probability distributions ensembles already present for chaotic dynamical systems having only a few degrees of freedom or on the impossibility of having a truly isolated system are either unnecessary misguided or misleading specific features of macroscopic evolution such as the diffusion equation do however depend on the dynamical instability deterministic chaos of trajectories of isolated macroscopic systems the extensions of these classical notions to the quantum world is in many ways fairly direct it does however also bring in some new problems these will be discussed but not resolved
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709.0725
Theory of spin Hall effect
An extension of Drude model is proposed that accounts for spin and spin-orbit interaction of charge carriers. Spin currents appear due to combined action of the external electric field, crystal field and scattering of charge carriers. The expression for spin Hall conductivity is derived for metals and semiconductors that is independent of the scattering mechanism. In cubic metals, spin Hall conductivity $\sigma_s$ and charge conductivity $\sigma_c$ are related through $\sigma_s = [2 \pi \hbar/(3mc^2)]\sigma_c^2$ with $m$ being the bare electron mass. Theoretically computed value is in agreement with experiment.
cond-mat.mes-hall
an extension of drude model is proposed that accounts for spin and spinorbit interaction of charge carriers spin currents appear due to combined action of the external electric field crystal field and scattering of charge carriers the expression for spin hall conductivity is derived for metals and semiconductors that is independent of the scattering mechanism in cubic metals spin hall conductivity sigma_s and charge conductivity sigma_c are related through sigma_s 2 pi hbar3mc2sigma_c2 with m being the bare electron mass theoretically computed value is in agreement with experiment
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709.0726
Inducing the Lovelock action
We re-analyze a possible ambiguity in the application of dimensional regularization to Einstein-Gauss-Bonnet gravity, arising from the way one treats the Gauss-Bonnet term. It is demonstrated that the addition of such a term to the action gives rise to a non-minimal graviton wave operator, but does not produce new on shell divergences at one loop order in d=4. However, from a d-dimensional perspective the Gauss-Bonnet term is shown to generate new divergences in the form of the six-dimensional Euler density. The conjecture that one would next produce the eight-dimensional Euler term is shown to be false.
gr-qc hep-th
we reanalyze a possible ambiguity in the application of dimensional regularization to einsteingaussbonnet gravity arising from the way one treats the gaussbonnet term it is demonstrated that the addition of such a term to the action gives rise to a nonminimal graviton wave operator but does not produce new on shell divergences at one loop order in d4 however from a ddimensional perspective the gaussbonnet term is shown to generate new divergences in the form of the sixdimensional euler density the conjecture that one would next produce the eightdimensional euler term is shown to be false
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709.0727
Probing the doping in metallic and semiconducting carbon nanotubes by Raman and transport measurements
In-situ Raman experiments together with transport measurements have been carried out on carbon nanotubes as a function of gate voltage. In metallic tubes, a large increase in the Raman frequency of the $G^-$ band, accompanied by a substantial decrease of its line-width, is observed with electron or hole doping. In addition, we see an increase in Raman frequency of the $G^+$ band in semiconducting tubes. These results are quantitatively explained using ab-initio calculations that take into account effects beyond the adiabatic approximation. Our results imply that Raman spectroscopy can be used as an accurate measure of the doping of both metallic and semiconducting nanotubes.
cond-mat.mes-hall cond-mat.str-el
insitu raman experiments together with transport measurements have been carried out on carbon nanotubes as a function of gate voltage in metallic tubes a large increase in the raman frequency of the g band accompanied by a substantial decrease of its linewidth is observed with electron or hole doping in addition we see an increase in raman frequency of the g band in semiconducting tubes these results are quantitatively explained using abinitio calculations that take into account effects beyond the adiabatic approximation our results imply that raman spectroscopy can be used as an accurate measure of the doping of both metallic and semiconducting nanotubes
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709.0728
Coherent pion production in neutrino-nucleus collisions
We have investigated the neutrino induced coherent pion production reaction at low and intermediate energies including pion, nucleon and Delta(1232) resonance. Medium effects in the production mechanism and the distortion of the pion wave function are included in the calculation. We find a strong reduction of the cross section due to these effects and also substantial modifications in the energy distributions of the final pion. The dependence on the atomic number is discussed.
nucl-th hep-ex nucl-ex
we have investigated the neutrino induced coherent pion production reaction at low and intermediate energies including pion nucleon and delta1232 resonance medium effects in the production mechanism and the distortion of the pion wave function are included in the calculation we find a strong reduction of the cross section due to these effects and also substantial modifications in the energy distributions of the final pion the dependence on the atomic number is discussed
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709.0729
Topological phases and topological entropy of two-dimensional systems with finite correlation length
We elucidate the topological features of the entanglement entropy of a region in two dimensional quantum systems in a topological phase with a finite correlation length $\xi$. Firstly, we suggest that simpler reduced quantities, related to the von Neumann entropy, could be defined to compute the topological entropy. We use our methods to compute the entanglement entropy for the ground state wave function of a quantum eight-vertex model in its topological phase, and show that a finite correlation length adds corrections of the same order as the topological entropy which come from sharp features of the boundary of the region under study. We also calculate the topological entropy for the ground state of the quantum dimer model on a triangular lattice by using a mapping to a loop model. The topological entropy of the state is determined by loop configurations with a non-trivial winding number around the region under study. Finally, we consider extensions of the Kitaev wave function, which incorporate the effects of electric and magnetic charge fluctuations, and use it to investigate the stability of the topological phase by calculating the topological entropy.
cond-mat.str-el
we elucidate the topological features of the entanglement entropy of a region in two dimensional quantum systems in a topological phase with a finite correlation length xi firstly we suggest that simpler reduced quantities related to the von neumann entropy could be defined to compute the topological entropy we use our methods to compute the entanglement entropy for the ground state wave function of a quantum eightvertex model in its topological phase and show that a finite correlation length adds corrections of the same order as the topological entropy which come from sharp features of the boundary of the region under study we also calculate the topological entropy for the ground state of the quantum dimer model on a triangular lattice by using a mapping to a loop model the topological entropy of the state is determined by loop configurations with a nontrivial winding number around the region under study finally we consider extensions of the kitaev wave function which incorporate the effects of electric and magnetic charge fluctuations and use it to investigate the stability of the topological phase by calculating the topological entropy
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709.073
The Star Formation and Extinction Co-Evolution of UV-Selected Galaxies over 0.05<z<1.2
We use a new stacking technique to obtain mean mid IR and far IR to far UV flux ratios over the rest near-UV/near-IR color-magnitude diagram. We employ COMBO-17 redshifts and COMBO-17 optical, GALEX far and near UV, Spitzer IRAC and MIPS Mid IR photometry. This technique permits us to probe infrared excess (IRX), the ratio of far IR to far UV luminosity, and specific star formation rate (SSFR) and their co-evolution over two orders of magnitude of stellar mass and redshift 0.1<z<1.2. We find that the SSFR and the characteristic mass (M_0) above which the SSFR drops increase with redshift (downsizing). At any given epoch, IRX is an increasing function of mass up to M_0. Above this mass IRX falls, suggesting gas exhaustion. In a given mass bin below M_0 IRX increases with time in a fashion consistent with enrichment. We interpret these trends using a simple model with a Schmidt-Kennicutt law and extinction that tracks gas density and enrichment. We find that the average IRX and SSFR follows a galaxy age parameter which is determined mainly by the galaxy mass and time since formation. We conclude that blue sequence galaxies have properties which show simple, systematic trends with mass and time such as the steady build-up of heavy elements in the interstellar media of evolving galaxies and the exhaustion of gas in galaxies that are evolving off the blue sequence. The IRX represents a tool for selecting galaxies at various stages of evolution.
astro-ph
we use a new stacking technique to obtain mean mid ir and far ir to far uv flux ratios over the rest nearuvnearir colormagnitude diagram we employ combo17 redshifts and combo17 optical galex far and near uv spitzer irac and mips mid ir photometry this technique permits us to probe infrared excess irx the ratio of far ir to far uv luminosity and specific star formation rate ssfr and their coevolution over two orders of magnitude of stellar mass and redshift 01z12 we find that the ssfr and the characteristic mass m_0 above which the ssfr drops increase with redshift downsizing at any given epoch irx is an increasing function of mass up to m_0 above this mass irx falls suggesting gas exhaustion in a given mass bin below m_0 irx increases with time in a fashion consistent with enrichment we interpret these trends using a simple model with a schmidtkennicutt law and extinction that tracks gas density and enrichment we find that the average irx and ssfr follows a galaxy age parameter which is determined mainly by the galaxy mass and time since formation we conclude that blue sequence galaxies have properties which show simple systematic trends with mass and time such as the steady buildup of heavy elements in the interstellar media of evolving galaxies and the exhaustion of gas in galaxies that are evolving off the blue sequence the irx represents a tool for selecting galaxies at various stages of evolution
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709.0731
The Geometric Phase in Supersymmetric Quantum Mechanics
We explore the geometric phase in N=(2,2) supersymmetric quantum mechanics. The Witten index ensures the existence of degenerate ground states, resulting in a non-Abelian Berry connection. We exhibit a non-renormalization theorem which prohibits the connection from receiving perturbative corrections. However, we show that it does receive corrections from BPS instantons. We compute the one-instanton contribution to the Berry connection for the massive CP^1 sigma-model as the potential is varied. This system has two ground states and the associated Berry connection is the smooth SU(2) 't Hooft-Polyakov monopole.
hep-th
we explore the geometric phase in n22 supersymmetric quantum mechanics the witten index ensures the existence of degenerate ground states resulting in a nonabelian berry connection we exhibit a nonrenormalization theorem which prohibits the connection from receiving perturbative corrections however we show that it does receive corrections from bps instantons we compute the oneinstanton contribution to the berry connection for the massive cp1 sigmamodel as the potential is varied this system has two ground states and the associated berry connection is the smooth su2 t hooftpolyakov monopole
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709.0732
Exact solution to the averaging problem in cosmology
The exact solution of a two-scale Buchert average of the Einstein equations is derived for an inhomogeneous universe which represents a close approximation to the observed universe. The two scales represent voids, and the bubble walls surrounding them within which clusters of galaxies are located. As described elsewhere [gr-qc/0702082], apparent cosmic acceleration can be recognised as a consequence of quasilocal gravitational energy gradients between observers in bound systems and the volume average position in freely expanding space. With this interpretation, the new solution presented here replaces the Friedmann solutions, in representing the average evolution of a matter-dominated universe without exotic dark energy, while being observationally viable.
gr-qc astro-ph hep-ph hep-th
the exact solution of a twoscale buchert average of the einstein equations is derived for an inhomogeneous universe which represents a close approximation to the observed universe the two scales represent voids and the bubble walls surrounding them within which clusters of galaxies are located as described elsewhere grqc0702082 apparent cosmic acceleration can be recognised as a consequence of quasilocal gravitational energy gradients between observers in bound systems and the volume average position in freely expanding space with this interpretation the new solution presented here replaces the friedmann solutions in representing the average evolution of a matterdominated universe without exotic dark energy while being observationally viable
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709.0733
Discovery of the Narrow-Line Seyfert 1 galaxy Mkn 335 in an historical low X-ray flux state
We report the discovery of the Narrow-Line Seyfert 1 galaxy Mkn 335 in an extremely low X-ray state. A comparison of Swift observations obtained in May and June/July 2007 with all previous X-ray observations between 1971 to 2006 show the AGN to have diminished in flux by a factor of more than 30, the lowest X-ray flux Mkn 335 has ever been observed in. The Swift observations show an extremely hard X-ray spectrum at energies above 2 keV. Possible interpretations include partial covering absorption or X-ray reflection from the disk. In this letter we consider the partial covering interpretation. The Swift observations can be well fit by a strong partial covering absorber with varying absorption column density N_H= 1-4 x 10^{23} cm-2 and a covering fraction f_c=0.9 - 1. When corrected for intrinsic absorption, the X-ray flux of Mkn 335 varies by only factors of 4-6. In the UV Mkn 335 shows variability in the order of 0.2 mag. We discuss the similarity of Mkn 335 with the highly variable NLS1 WPVS007, and speculate about a possible link between NLS1 galaxies and broad-absorption line quasars.
astro-ph
we report the discovery of the narrowline seyfert 1 galaxy mkn 335 in an extremely low xray state a comparison of swift observations obtained in may and junejuly 2007 with all previous xray observations between 1971 to 2006 show the agn to have diminished in flux by a factor of more than 30 the lowest xray flux mkn 335 has ever been observed in the swift observations show an extremely hard xray spectrum at energies above 2 kev possible interpretations include partial covering absorption or xray reflection from the disk in this letter we consider the partial covering interpretation the swift observations can be well fit by a strong partial covering absorber with varying absorption column density n_h 14 x 1023 cm2 and a covering fraction f_c09 1 when corrected for intrinsic absorption the xray flux of mkn 335 varies by only factors of 46 in the uv mkn 335 shows variability in the order of 02 mag we discuss the similarity of mkn 335 with the highly variable nls1 wpvs007 and speculate about a possible link between nls1 galaxies and broadabsorption line quasars
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709.0734
Predictions for the Cosmogenic Neutrino Flux in Light of New Data from the Pierre Auger Observatory
The Pierre Auger Observatory (PAO) has measured the spectrum and composition of the ultrahigh energy cosmic rays with unprecedented precision. We use these measurements to constrain their spectrum and composition as injected from their sources and, in turn, use these results to estimate the spectrum of cosmogenic neutrinos generated in their propagation through intergalactic space. We find that the PAO measurements can be well fit if the injected cosmic rays consist entirely of nuclei with masses in the intermediate (C, N, O) to heavy (Fe, Si) range. A mixture of protons and heavier species is also acceptable but (on the basis of existing hadronic interaction models) injection of pure light nuclei (p, He) results in unacceptable fits to the new elongation rate data. The expected spectrum of cosmogenic neutrinos can vary considerably, depending on the precise spectrum and chemical composition injected from the cosmic ray sources. In the models where heavy nuclei dominate the cosmic ray spectrum and few dissociated protons exceed GZK energies, the cosmogenic neutrino flux can be suppressed by up to two orders of magnitude relative to the all-proton prediction, making its detection beyond the reach of current and planned neutrino telescopes. Other models consistent with the data, however, are proton-dominated with only a small (1-10%) admixture of heavy nuclei and predict an associated cosmogenic flux within the reach of upcoming experiments. Thus a detection or non-detection of cosmogenic neutrinos can assist in discriminating between these possibilities.
astro-ph hep-ph
the pierre auger observatory pao has measured the spectrum and composition of the ultrahigh energy cosmic rays with unprecedented precision we use these measurements to constrain their spectrum and composition as injected from their sources and in turn use these results to estimate the spectrum of cosmogenic neutrinos generated in their propagation through intergalactic space we find that the pao measurements can be well fit if the injected cosmic rays consist entirely of nuclei with masses in the intermediate c n o to heavy fe si range a mixture of protons and heavier species is also acceptable but on the basis of existing hadronic interaction models injection of pure light nuclei p he results in unacceptable fits to the new elongation rate data the expected spectrum of cosmogenic neutrinos can vary considerably depending on the precise spectrum and chemical composition injected from the cosmic ray sources in the models where heavy nuclei dominate the cosmic ray spectrum and few dissociated protons exceed gzk energies the cosmogenic neutrino flux can be suppressed by up to two orders of magnitude relative to the allproton prediction making its detection beyond the reach of current and planned neutrino telescopes other models consistent with the data however are protondominated with only a small 110 admixture of heavy nuclei and predict an associated cosmogenic flux within the reach of upcoming experiments thus a detection or nondetection of cosmogenic neutrinos can assist in discriminating between these possibilities
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