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706.2914
Comment on "Infrared freezing of Euclidean QCD observables"
Recently, P. M. Brooks and C.J. Maxwell [Phys. Rev. D{\bf 74} 065012 (2006)] claimed that the Landau pole of the one-loop coupling at $Q^2=\Lambda^2$ is absent from the leading one-chain term in a skeleton expansion of the Euclidean Adler ${\cal D}$ function. Moreover, in this approximation one has continuity along the Euclidean axis and a smooth infrared freezing, properties known to be satisfied by the "true" Adler function. We show that crucial in the derivation of these results is the use of a modified Borel summation, which leads simultaneously to the loss of another fundamental property of the true Adler function: the analyticity implied by the K\"allen-Lehmann representation.
hep-ph
recently p m brooks and cj maxwell phys rev dbf 74 065012 2006 claimed that the landau pole of the oneloop coupling at q2lambda2 is absent from the leading onechain term in a skeleton expansion of the euclidean adler cal d function moreover in this approximation one has continuity along the euclidean axis and a smooth infrared freezing properties known to be satisfied by the true adler function we show that crucial in the derivation of these results is the use of a modified borel summation which leads simultaneously to the loss of another fundamental property of the true adler function the analyticity implied by the kallenlehmann representation
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706.2915
Interplay between structure and density anomaly for an isotropic core-softened ramp-like potential
Using molecular dynamics simulations and integral equations we investigate the structure, the thermodynamics and the dynamics of a system of particles interacting through a continuous core- softened ramp-like interparticle potential. We found density, dynamic and structural anomalies similar to that found in water. Analysis of the radial distribution function for several temperatures at fixed densities show a pattern that may be related to the origin of density anomaly.
cond-mat.stat-mech cond-mat.soft
using molecular dynamics simulations and integral equations we investigate the structure the thermodynamics and the dynamics of a system of particles interacting through a continuous core softened ramplike interparticle potential we found density dynamic and structural anomalies similar to that found in water analysis of the radial distribution function for several temperatures at fixed densities show a pattern that may be related to the origin of density anomaly
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706.2916
Factor Two Discrepancy of Hawking Radiation Temperature
The possibility of an alternative way to formulate the Hawking radiation in a static Schwarzschild spacetime has been explored. To calculate the Hawking radiation, there can be two possible choices of the spacetime wedge pairs in the Krucal-Szekeres coordinates. One is the wedge pair consists of exterior spacetime of a black hole and the exterior spacetime of a white hole, and the other is that of exterior and interior spacetimes of one black hole. The radiation from the former is the Hawking's original one. Though the the latter has been often regarded as the same phenomena as the former, the result here suggests it is not; its radiation has a temperature twice as high as the Hawking temperature.
hep-th
the possibility of an alternative way to formulate the hawking radiation in a static schwarzschild spacetime has been explored to calculate the hawking radiation there can be two possible choices of the spacetime wedge pairs in the krucalszekeres coordinates one is the wedge pair consists of exterior spacetime of a black hole and the exterior spacetime of a white hole and the other is that of exterior and interior spacetimes of one black hole the radiation from the former is the hawkings original one though the the latter has been often regarded as the same phenomena as the former the result here suggests it is not its radiation has a temperature twice as high as the hawking temperature
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706.2917
A variational theory for point defects in patterns
We derive a rigorous scaling law for minimizers in a natural version of the regularized Cross-Newell model for pattern formation far from threshold. These energy-minimizing solutions support defects having the same character as what is seen in experimental studies of the corresponding physical systems and in numerical simulations of the microscopic equations that describe these systems.
math.AP nlin.PS
we derive a rigorous scaling law for minimizers in a natural version of the regularized crossnewell model for pattern formation far from threshold these energyminimizing solutions support defects having the same character as what is seen in experimental studies of the corresponding physical systems and in numerical simulations of the microscopic equations that describe these systems
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706.2918
Enumerative properties of Ferrers graphs
We define a class of bipartite graphs that correspond naturally with Ferrers diagrams. We give expressions for the number of spanning trees, the number of Hamiltonian paths when applicable, the chromatic polynomial, and the chromatic symmetric function. We show that the linear coefficient of the chromatic polynomial is given by the excedance set statistic.
math.CO
we define a class of bipartite graphs that correspond naturally with ferrers diagrams we give expressions for the number of spanning trees the number of hamiltonian paths when applicable the chromatic polynomial and the chromatic symmetric function we show that the linear coefficient of the chromatic polynomial is given by the excedance set statistic
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706.2919
The statistics of LCDM Halo Concentrations
We use the Millennium Simulation (MS) to study the statistics of LCDM halo concentrations at z = 0. Our results confirm that the average halo concentration declines monotonically with mass; a power-law fits well the concentration-mass relation for over 3 decades in mass, up to the most massive objects to form in a LCDM universe (~ 10^15 h^-1 Msol). This is in clear disagreement with the predictions of the model proposed by Bullock et al. for these rare objects, and agrees better with the original predictions of Navarro, Frenk, & White. The large volume surveyed, together with the unprecedented numerical resolution of the MS, allow us to estimate with confidence the distribution of concentrations and, consequently, the abundance of systems with unusual properties. About one in a hundred cluster haloes (M200 >~ 3x10^14 h^-1 Msol) have concentrations exceeding c200 = 7.5, a result that may be used to interpret the likelihood of unusually strong massive gravitational lenses, such as Abell 1689, in the LCDM cosmogony. A similar fraction (1 in 100) of galaxy-sized haloes (M200 ~ 10^12 h^-1 Msol) have c200 < 4.5, an important constraint on models that attempt to reconcile the rotation curves of low surface-brightness galaxies by appealing to haloes of unexpectedly low concentration. We find that halo concentrations are independent of spin once haloes manifestly out of equilibrium are removed from the sample. Compared to their relaxed brethren, the concentrations of out-of-equilibrium haloes tend to be lower and to have more scatter, while their spins tend to be higher... (continue)
astro-ph
we use the millennium simulation ms to study the statistics of lcdm halo concentrations at z 0 our results confirm that the average halo concentration declines monotonically with mass a powerlaw fits well the concentrationmass relation for over 3 decades in mass up to the most massive objects to form in a lcdm universe 1015 h1 msol this is in clear disagreement with the predictions of the model proposed by bullock et al for these rare objects and agrees better with the original predictions of navarro frenk white the large volume surveyed together with the unprecedented numerical resolution of the ms allow us to estimate with confidence the distribution of concentrations and consequently the abundance of systems with unusual properties about one in a hundred cluster haloes m200 3x1014 h1 msol have concentrations exceeding c200 75 a result that may be used to interpret the likelihood of unusually strong massive gravitational lenses such as abell 1689 in the lcdm cosmogony a similar fraction 1 in 100 of galaxysized haloes m200 1012 h1 msol have c200 45 an important constraint on models that attempt to reconcile the rotation curves of low surfacebrightness galaxies by appealing to haloes of unexpectedly low concentration we find that halo concentrations are independent of spin once haloes manifestly out of equilibrium are removed from the sample compared to their relaxed brethren the concentrations of outofequilibrium haloes tend to be lower and to have more scatter while their spins tend to be higher continue
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706.292
Tropical hyperplane arrangements and oriented matroids
We study the combinatorial properties of a tropical hyperplane arrangement. We define tropical oriented matroids, and prove that they share many of the properties of ordinary oriented matroids. We show that a tropical oriented matroid determines a subdivision of a product of two simplices, and conjecture that this correspondence is a bijection.
math.CO
we study the combinatorial properties of a tropical hyperplane arrangement we define tropical oriented matroids and prove that they share many of the properties of ordinary oriented matroids we show that a tropical oriented matroid determines a subdivision of a product of two simplices and conjecture that this correspondence is a bijection
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706.2921
Herwig++
We describe the recent development of the Herwig++ event generator.
hep-ph
we describe the recent development of the herwig event generator
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706.2922
Mackey functors on compact closed categories
We develop and extend the theory of Mackey functors as an application of enriched category theory. We define Mackey functors on a lextensive category $\E$ and investigate the properties of the category of Mackey functors on $\E$. We show that it is a monoidal category and the monoids are Green functors. Mackey functors are seen as providing a setting in which mere numerical equations occurring in the theory of groups can be given a structural foundation. We obtain an explicit description of the objects of the Cauchy completion of a monoidal functor and apply this to examine Morita equivalence of Green functors.
math.CT
we develop and extend the theory of mackey functors as an application of enriched category theory we define mackey functors on a lextensive category e and investigate the properties of the category of mackey functors on e we show that it is a monoidal category and the monoids are green functors mackey functors are seen as providing a setting in which mere numerical equations occurring in the theory of groups can be given a structural foundation we obtain an explicit description of the objects of the cauchy completion of a monoidal functor and apply this to examine morita equivalence of green functors
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706.2923
Representations of Truncated Current Lie Algebras
Let g denote a Lie algebra, and let T(g) denote the tensor product of g with a ring of truncated polynomials. The Lie algebra T(g) is called a truncated current Lie algebra. The highest-weight representation theory of T(g) is developed, and a reducibility criterion for the Verma modules is described.
math.RT math-ph math.MP
let g denote a lie algebra and let tg denote the tensor product of g with a ring of truncated polynomials the lie algebra tg is called a truncated current lie algebra the highestweight representation theory of tg is developed and a reducibility criterion for the verma modules is described
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706.2924
A scaling relation of anomalous Hall effect in ferromagnetic semiconductors and metals
A scaling relation of the anomalous Hall effect recently found in a ferromagnetic semiconductor (Ti,Co)O_2_ is compared with those of various ferromagnetic semiconductors and metals. Many of these compounds with relatively low conductivity sigma_xx_ < 10^4 ohm^-1 cm^-1 are also found to exhibit similar relation: anomalous Hall conductivity sigma_AH_ approximately scales as sigma_AH_ proportional to sigma_xx_^1.6, that is coincident with a recent theory. This relation is valid over five decades of sigma_xx_ irrespective of metallic or hopping conduction.
cond-mat.mtrl-sci cond-mat.str-el
a scaling relation of the anomalous hall effect recently found in a ferromagnetic semiconductor ticoo_2_ is compared with those of various ferromagnetic semiconductors and metals many of these compounds with relatively low conductivity sigma_xx_ 104 ohm1 cm1 are also found to exhibit similar relation anomalous hall conductivity sigma_ah_ approximately scales as sigma_ah_ proportional to sigma_xx_16 that is coincident with a recent theory this relation is valid over five decades of sigma_xx_ irrespective of metallic or hopping conduction
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706.2925
Non-Markovian dynamics in the theory of full counting statistics
We consider the theoretical description of real-time counting of electrons tunneling through a Coulomb-blockade quantum dot using a detector with finite bandwidth. By tracing out the quantum dot we find that the dynamics of the detector effectively is non-Markovian. We calculate the cumulant generating function corresponding to the resulting non-Markovian rate equation and find that the measured current cumulants behave significantly differently compared to those of a Markovian transport process. Our findings provide a novel interpretation of noise suppression found in a number of systems.
cond-mat.mes-hall
we consider the theoretical description of realtime counting of electrons tunneling through a coulombblockade quantum dot using a detector with finite bandwidth by tracing out the quantum dot we find that the dynamics of the detector effectively is nonmarkovian we calculate the cumulant generating function corresponding to the resulting nonmarkovian rate equation and find that the measured current cumulants behave significantly differently compared to those of a markovian transport process our findings provide a novel interpretation of noise suppression found in a number of systems
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706.2926
Reducing the Error Floor
We discuss how the loop calculus approach of [Chertkov, Chernyak '06], enhanced by the pseudo-codeword search algorithm of [Chertkov, Stepanov '06] and the facet-guessing idea from [Dimakis, Wainwright '06], improves decoding of graph based codes in the error-floor domain. The utility of the new, Linear Programming based, decoding is demonstrated via analysis and simulations of the model $[155,64,20]$ code.
cs.IT math.IT
we discuss how the loop calculus approach of chertkov chernyak 06 enhanced by the pseudocodeword search algorithm of chertkov stepanov 06 and the facetguessing idea from dimakis wainwright 06 improves decoding of graph based codes in the errorfloor domain the utility of the new linear programming based decoding is demonstrated via analysis and simulations of the model 1556420 code
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706.2927
Green's function approach to transport through a gate-all-around Si nanowire under impurity scattering
We investigate transport properties of gate-all-around Si nanowires using non-equilibrium Green's function technique. By taking into account of the ionized impurity scattering we calculate Green's functions self-consistently and examine the effects of ionized impurity scattering on electron densities and currents. For nano-scale Si wires, it is found that, due to the impurity scattering, the local density of state profiles loose it's interference oscillations as well as is broaden and shifted. In addition, the impurity scattering gives rise to a different transconductance as functions of temperature and impurity scattering strength when compared with the transconductance without impurity scattering.
cond-mat.mes-hall
we investigate transport properties of gateallaround si nanowires using nonequilibrium greens function technique by taking into account of the ionized impurity scattering we calculate greens functions selfconsistently and examine the effects of ionized impurity scattering on electron densities and currents for nanoscale si wires it is found that due to the impurity scattering the local density of state profiles loose its interference oscillations as well as is broaden and shifted in addition the impurity scattering gives rise to a different transconductance as functions of temperature and impurity scattering strength when compared with the transconductance without impurity scattering
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706.2928
Strong effect of weak diffusion on scalar turbulence at large scales
Passive scalar turbulence forced steadily is characterized by the velocity correlation scale, $L$, injection scale, $l$, and diffusive scale, $r_d$. The scales are well separated if the diffusivity is small, $r_d\ll l,L$, and one normally says that effects of diffusion are confined to smaller scales, $r\ll r_d$. However, if the velocity is single scale one finds that a weak dependence of the scalar correlations on the molecular diffusivity persists to even larger scales, e.g. $l\gg r\gg r_d$ \cite{95BCKL}. We consider the case of $L\gg l$ and report a counter-intuitive result -- the emergence of a new range of large scales, $L\gg r\gg l^2/r_d$, where the diffusivity shows a strong effect on scalar correlations.
nlin.CD
passive scalar turbulence forced steadily is characterized by the velocity correlation scale l injection scale l and diffusive scale r_d the scales are well separated if the diffusivity is small r_dll ll and one normally says that effects of diffusion are confined to smaller scales rll r_d however if the velocity is single scale one finds that a weak dependence of the scalar correlations on the molecular diffusivity persists to even larger scales eg lgg rgg r_d cite95bckl we consider the case of lgg l and report a counterintuitive result the emergence of a new range of large scales lgg rgg l2r_d where the diffusivity shows a strong effect on scalar correlations
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706.2929
Noncompact sigma-models: Large N expansion and thermodynamic limit
Noncompact SO(1,N) sigma-models are studied in terms of their large N expansion in a lattice formulation in dimensions d \geq 2. Explicit results for the spin and current two-point functions as well as for the Binder cumulant are presented to next to leading order on a finite lattice. The dynamically generated gap is negative and serves as a coupling-dependent infrared regulator which vanishes in the limit of infinite lattice size. The cancellation of infrared divergences in invariant correlation functions in this limit is nontrivial and is in d=2 demonstrated by explicit computation for the above quantities. For the Binder cumulant the thermodynamic limit is finite and is given by 2/(N+1) in the order considered. Monte Carlo simulations suggest that the remainder is small or zero. The potential implications for ``criticality'' and ``triviality'' of the theories in the SO(1,N) invariant sector are discussed.
hep-th hep-lat
noncompact so1n sigmamodels are studied in terms of their large n expansion in a lattice formulation in dimensions d geq 2 explicit results for the spin and current twopoint functions as well as for the binder cumulant are presented to next to leading order on a finite lattice the dynamically generated gap is negative and serves as a couplingdependent infrared regulator which vanishes in the limit of infinite lattice size the cancellation of infrared divergences in invariant correlation functions in this limit is nontrivial and is in d2 demonstrated by explicit computation for the above quantities for the binder cumulant the thermodynamic limit is finite and is given by 2n1 in the order considered monte carlo simulations suggest that the remainder is small or zero the potential implications for criticality and triviality of the theories in the so1n invariant sector are discussed
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706.293
Strong magnetic field enhancement of spin triplet pairing arising from coexisting $2k_F$ spin and $2k_F$ charge fluctuations
We study the effect of the magnetic field (Zeeman splitting) on the triplet pairing. We show generally that the enhancement of spin triplet pairing mediated by coexisting $2k_F$ spin and $2k_F$ charge fluctuations can be much larger than in the case of triplet pairing mediated by ferromagnetic spin fluctuations. We propose that this may be related to the recent experiment for (TMTSF)$_2$ClO$_4$, in which a possibility of singlet to triplet pairing transition has been suggested.
cond-mat.supr-con
we study the effect of the magnetic field zeeman splitting on the triplet pairing we show generally that the enhancement of spin triplet pairing mediated by coexisting 2k_f spin and 2k_f charge fluctuations can be much larger than in the case of triplet pairing mediated by ferromagnetic spin fluctuations we propose that this may be related to the recent experiment for tmtsf_2clo_4 in which a possibility of singlet to triplet pairing transition has been suggested
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706.2931
Markov Process of Muscle Motors
We study a Markov random process describing a muscle molecular motor behavior. Every motor is either bound up with a thin filament or unbound. In the bound state the motor creates a force proportional to its displacement from the neutral position. In both states the motor spend an exponential time depending on the state. The thin filament moves at its velocity proportional to average of all displacements of all motors. We assume that the time which a motor stays at the bound state does not depend on its displacement. Then one can find an exact solution of a non-linear equation appearing in the limit of infinite number of the motors.
math-ph math.MP
we study a markov random process describing a muscle molecular motor behavior every motor is either bound up with a thin filament or unbound in the bound state the motor creates a force proportional to its displacement from the neutral position in both states the motor spend an exponential time depending on the state the thin filament moves at its velocity proportional to average of all displacements of all motors we assume that the time which a motor stays at the bound state does not depend on its displacement then one can find an exact solution of a nonlinear equation appearing in the limit of infinite number of the motors
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706.2932
The formation of the [alpha/Fe] radial gradients in the stars of elliptical galaxies
The scope of this paper is two-fold: i) to test and improve our previous models of an outside-in formation for the majority of ellipticals in the context of the SN-driven wind scenario, by means of a careful study of gas inflows/outflows; ii) to explain 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. In order to pursue these goals we present a new class of hydrodynamical simulations for the formation of single elliptical galaxies in which we implement detailed prescriptions for the chemical evolution of H, He, O and Fe. We find that all the models which predict chemical properties (such as the central mass-weighted abundance ratios, the colours as well as the [<Fe/H>] gradient) within the observed ranges for a typical elliptical, also exhibit a variety of gradients in the [<alpha/Fe>] ratio, in agreement with the observations (namely positive, null or negative). All these models undergo an outside-in formation, in the sense that star formation stops earlier in the outermost than in the innermost regions, owing to the onset of a galactic wind. The typical [<Z/H>] gradients predicted by our models have a slope of -0.3 dex per decade variation in radius, consistent with the mean values of several observational samples. We can safely conclude that the history of star formation is fundamental for the creation of abundance gradients in ellipticals but that radial flows with different velocity in conjunction with the duration and efficiency of star formation in different galactic regions are responsible for the gradients in the [<alpha/Fe>] ratios.
astro-ph
the scope of this paper is twofold i to test and improve our previous models of an outsidein formation for the majority of ellipticals in the context of the sndriven wind scenario by means of a careful study of gas inflowsoutflows ii to explain 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 in order to pursue these goals we present a new class of hydrodynamical simulations for the formation of single elliptical galaxies in which we implement detailed prescriptions for the chemical evolution of h he o and fe we find that all the models which predict chemical properties such as the central massweighted abundance ratios the colours as well as the feh gradient within the observed ranges for a typical elliptical also exhibit a variety of gradients in the alphafe ratio in agreement with the observations namely positive null or negative all these models undergo an outsidein formation in the sense that star formation stops earlier in the outermost than in the innermost regions owing to the onset of a galactic wind the typical zh gradients predicted by our models have a slope of 03 dex per decade variation in radius consistent with the mean values of several observational samples we can safely conclude that the history of star formation is fundamental for the creation of abundance gradients in ellipticals but that radial flows with different velocity in conjunction with the duration and efficiency of star formation in different galactic regions are responsible for the gradients in the alphafe ratios
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706.2933
Electromagnetic quasinormal modes of D-dimensional black holes II
By using the sixth order WKB approximation we calculate for an electromagnetic field propagating in D-dimensional Schwarzschild and Schwarzschild de Sitter black holes its quasinormal frequencies for the fundamental mode and first overtones. We study the dependence of these QN frequencies on the value of the cosmological constant and the spacetime dimension. We also compare with the known results for the gravitational perturbations propagating in the same background. Moreover we exactly compute the QN frequencies of the electromagnetic field propagating in D-dimensional massless topological black hole and for charged D-dimensional Nariai spacetime we exactly calculate the QN frequencies of the coupled electromagnetic and gravitational perturbations.
gr-qc
by using the sixth order wkb approximation we calculate for an electromagnetic field propagating in ddimensional schwarzschild and schwarzschild de sitter black holes its quasinormal frequencies for the fundamental mode and first overtones we study the dependence of these qn frequencies on the value of the cosmological constant and the spacetime dimension we also compare with the known results for the gravitational perturbations propagating in the same background moreover we exactly compute the qn frequencies of the electromagnetic field propagating in ddimensional massless topological black hole and for charged ddimensional nariai spacetime we exactly calculate the qn frequencies of the coupled electromagnetic and gravitational perturbations
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706.2934
Recent heavy flavor results from STAR
We report on recent heavy flavor measurements from the STAR experiment at RHIC. The measured charm cross section in heavy-ion collisions scales with the number of binary collisions, which is an indication for exclusive charm production in the initial state of the collision. The observed strong suppression of non-photonic electrons at high $\pt$ in Au+Au collisions together with the azimuthal correlation measurements in p+p collisions imply a suppression of $B$ production in heavy-ion collisions. We also present recent measurements of the $\Upsilon$ cross section in p+p collisions.
nucl-ex
we report on recent heavy flavor measurements from the star experiment at rhic the measured charm cross section in heavyion collisions scales with the number of binary collisions which is an indication for exclusive charm production in the initial state of the collision the observed strong suppression of nonphotonic electrons at high pt in auau collisions together with the azimuthal correlation measurements in pp collisions imply a suppression of b production in heavyion collisions we also present recent measurements of the upsilon cross section in pp collisions
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706.2935
Preferential attachment during the evolution of a potential energy landscape
It has previously been shown that the network of connected minima on a potential energy landscape is scale-free, and that this reflects a power-law distribution for the areas of the basins of attraction surrounding the minima. Here, we set out to understand more about the physical origins of these puzzling properties by examining how the potential energy landscape of a 13-atom cluster evolves with the range of the potential. In particular, on decreasing the range of the potential the number of stationary points increases and thus the landscape becomes rougher and the network gets larger. Thus, we are able to follow the evolution of the potential energy landscape from one with just a single minimum to a complex landscape with many minima and a scale-free pattern of connections. We find that during this growth process, new edges in the network of connected minima preferentially attach to more highly-connected minima, thus leading to the scale-free character. Furthermore, minima that appear when the range of the potential is shorter and the network is larger have smaller basins of attraction. As there are many of these smaller basins because the network grows exponentially, the observed growth process thus also gives rise to a power-law distribution for the hyperareas of the basins.
cond-mat.stat-mech
it has previously been shown that the network of connected minima on a potential energy landscape is scalefree and that this reflects a powerlaw distribution for the areas of the basins of attraction surrounding the minima here we set out to understand more about the physical origins of these puzzling properties by examining how the potential energy landscape of a 13atom cluster evolves with the range of the potential in particular on decreasing the range of the potential the number of stationary points increases and thus the landscape becomes rougher and the network gets larger thus we are able to follow the evolution of the potential energy landscape from one with just a single minimum to a complex landscape with many minima and a scalefree pattern of connections we find that during this growth process new edges in the network of connected minima preferentially attach to more highlyconnected minima thus leading to the scalefree character furthermore minima that appear when the range of the potential is shorter and the network is larger have smaller basins of attraction as there are many of these smaller basins because the network grows exponentially the observed growth process thus also gives rise to a powerlaw distribution for the hyperareas of the basins
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706.2936
High-Resolution Spectra Observed for SPY. II. DB and DBA Stars
We present a detailed spectroscopic analysis of the stars with helium-dominated spectra in the ESO Supernova Ia Progenitor Survey (SPY). Atmospheric parameters, masses, and abundances of trace hydrogen are determined and discussed in the context of spectral evolution of white dwarfs. Our final sample contains 71 objects, of which 6 are new detections and 14 are reclassified from DB to DBA because of the presence of H lines. 55% of the DB sample show hydrogen and are thus DBA, a significantly higher fraction than found before. The large incidence of DBA, and the derived total hydrogen masses are compatible with the scenario that DBs ``reappear'' around 30000 K from the DB gap by mixing and diluting a thin hydrogen layer of the order of E-15 Msun. This hydrogen mass is then during the evolution continuously increased by interstellar accretion. There are indications that the accretion rate increases smoothly with age or decreasing temperature, a trend which continuous even below the current low temperature limit (Dufour 2006). A remaining mystery is the low accretion rate of H compared to that of Ca observed in the DBZA, but a stellar wind extending down to the lowest temperatures with decreasing strength might be part of the solution.
astro-ph
we present a detailed spectroscopic analysis of the stars with heliumdominated spectra in the eso supernova ia progenitor survey spy atmospheric parameters masses and abundances of trace hydrogen are determined and discussed in the context of spectral evolution of white dwarfs our final sample contains 71 objects of which 6 are new detections and 14 are reclassified from db to dba because of the presence of h lines 55 of the db sample show hydrogen and are thus dba a significantly higher fraction than found before the large incidence of dba and the derived total hydrogen masses are compatible with the scenario that dbs reappear around 30000 k from the db gap by mixing and diluting a thin hydrogen layer of the order of e15 msun this hydrogen mass is then during the evolution continuously increased by interstellar accretion there are indications that the accretion rate increases smoothly with age or decreasing temperature a trend which continuous even below the current low temperature limit dufour 2006 a remaining mystery is the low accretion rate of h compared to that of ca observed in the dbza but a stellar wind extending down to the lowest temperatures with decreasing strength might be part of the solution
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706.2937
On the dependence of the wave function of a bound nucleon on its momentum and the EMC effect
It is widely discussed in the literature that the wave function of the nucleon bound in a nucleus is modified due to the interaction with the surrounding medium. We argue that the modification should strongly depend on the momentum of the nucleon. We study such an effect in the case of the point-like configuration component of the wave function of a nucleon bound in a nucleus A, considering the case of arbitrary final state of the spectator A-1 system. We show that for non relativistic values of the nucleon momentum, the momentum dependence of the nucleon deformation appears to follow from rather general considerations and discuss the implications of our theoretical observation for two different phenomena: i) the search for medium induced modifications of the nucleon radius of a bound nucleon through the measurement of the electromagnetic nucleon form factors via the A(e,e'p)X process, and ii) the A-dependence of the EMC effect; in this latter case we also present a new method of estimating the fraction of the nucleus light-cone momentum carried by the photons and find that in a heavy nuclei protons loose about 2% of their momentum.
nucl-th hep-ph nucl-ex
it is widely discussed in the literature that the wave function of the nucleon bound in a nucleus is modified due to the interaction with the surrounding medium we argue that the modification should strongly depend on the momentum of the nucleon we study such an effect in the case of the pointlike configuration component of the wave function of a nucleon bound in a nucleus a considering the case of arbitrary final state of the spectator a1 system we show that for non relativistic values of the nucleon momentum the momentum dependence of the nucleon deformation appears to follow from rather general considerations and discuss the implications of our theoretical observation for two different phenomena i the search for medium induced modifications of the nucleon radius of a bound nucleon through the measurement of the electromagnetic nucleon form factors via the aeepx process and ii the adependence of the emc effect in this latter case we also present a new method of estimating the fraction of the nucleus lightcone momentum carried by the photons and find that in a heavy nuclei protons loose about 2 of their momentum
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706.2938
New Heavy Quark Baryons
During the past year many interesting results were published in heavy quark baryon spectroscopy. In addition to several refined measurements, new states were directly observed both in the charm and the bottom sector. In this paper we review recent results on heavy quark baryons from B-factories and Tevatron experiments.
hep-ex
during the past year many interesting results were published in heavy quark baryon spectroscopy in addition to several refined measurements new states were directly observed both in the charm and the bottom sector in this paper we review recent results on heavy quark baryons from bfactories and tevatron experiments
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706.2939
On the stabilization of the elasticity system by the boundary
We obtain free of resonances regions for the elasticity system in the exterior of a strictly convex body with dissipative boundary conditions under some natural assumptions on the behaviour of the geodesics on the boundary.
math.AP
we obtain free of resonances regions for the elasticity system in the exterior of a strictly convex body with dissipative boundary conditions under some natural assumptions on the behaviour of the geodesics on the boundary
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706.294
Early Electroweak and Top Quark Physics with CMS
The Large Hadron Collider is an ideal place for precision measurements of the properties of the electroweak gauge bosons W^\pm, Z^0, as well as of the top quark. In this article, a few highlights of the prospects for performing such measurements with the CMS detector are summarized, with an emphasis on the first few 1/fb of data.
hep-ex
the large hadron collider is an ideal place for precision measurements of the properties of the electroweak gauge bosons wpm z0 as well as of the top quark in this article a few highlights of the prospects for performing such measurements with the cms detector are summarized with an emphasis on the first few 1fb of data
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706.2941
A Common Origin for Quasar Extended Emission-Line Regions and Their Broad-Line Regions
We present a correlation between the presence of luminous extended emission-line regions (EELRs) and the metallicity of the broad-line regions (BLRs) of low-redshift quasars. The result is based on ground-based [O III] 5007 narrow-band imaging and Hubble Space Telescope UV spectra of 12 quasars at 0.20 < z < 0.45. Quasars showing luminous EELRs have low-metallicity BLRs (Z < 0.6 Z_Solar), while the remaining quasars show typical metal-rich gas (Z > Z_Solar). Previous studies have shown that EELRs themselves also have low metallicities (Z < 0.5 Z_Solar). The correlation between the occurrence of EELRs and the metallicity of the BLRs, strengthened by the sub-Solar metallicity in both regions, indicates a common external origin for the gas, almost certainly from the merger of a gas-rich galaxy. Our results provide the first direct observational evidence that the gas from a merger can indeed be driven down to the immediate vicinity (< 1 pc) of the central black hole.
astro-ph
we present a correlation between the presence of luminous extended emissionline regions eelrs and the metallicity of the broadline regions blrs of lowredshift quasars the result is based on groundbased o iii 5007 narrowband imaging and hubble space telescope uv spectra of 12 quasars at 020 z 045 quasars showing luminous eelrs have lowmetallicity blrs z 06 z_solar while the remaining quasars show typical metalrich gas z z_solar previous studies have shown that eelrs themselves also have low metallicities z 05 z_solar the correlation between the occurrence of eelrs and the metallicity of the blrs strengthened by the subsolar metallicity in both regions indicates a common external origin for the gas almost certainly from the merger of a gasrich galaxy our results provide the first direct observational evidence that the gas from a merger can indeed be driven down to the immediate vicinity 1 pc of the central black hole
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706.2942
Astrometric effects of solar-like magnetic activity in late-type stars and their relevance for the detection of extrasolar planets
Using a simple model based on the characteristics of sunspots and faculae in solar active regions, the effects of surface brightness inhomogeneities on the position of the photocentre of the disk of a solar-like, magnetically active star, are studied. A general law is introduced, giving the maximum amplitude of the photocentre excursion produced by a distribution of active regions with a given surface filling factor. The consequences for the detection of extrasolar planets by means of the astrometric method are investigated with some applications to forthcoming space missions, such as GAIA and SIM, as well as to ground-based interferometric measurements. Spurious detections of extrasolar planets can indeed be caused by activity-induced photocentre oscillations, requiring a simultaneous monitoring of the optical flux and a determination of the rotation period and of the level of activity of the target stars for an appropriate discrimination.
astro-ph
using a simple model based on the characteristics of sunspots and faculae in solar active regions the effects of surface brightness inhomogeneities on the position of the photocentre of the disk of a solarlike magnetically active star are studied a general law is introduced giving the maximum amplitude of the photocentre excursion produced by a distribution of active regions with a given surface filling factor the consequences for the detection of extrasolar planets by means of the astrometric method are investigated with some applications to forthcoming space missions such as gaia and sim as well as to groundbased interferometric measurements spurious detections of extrasolar planets can indeed be caused by activityinduced photocentre oscillations requiring a simultaneous monitoring of the optical flux and a determination of the rotation period and of the level of activity of the target stars for an appropriate discrimination
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706.2943
Kondo physics in the algebraic spin liquid
We study Kondo physics in the algebraic spin liquid, recently proposed to describe $ZnCu_{3}(OH)_{6}Cl_{2}$ [Phys. Rev. Lett. {\bf 98}, 117205 (2007)]. Although spin dynamics of the algebraic spin liquid is described by massless Dirac fermions, this problem differs from the Pseudogap Kondo model, because the bulk physics in the algebraic spin liquid is governed by an interacting fixed point where well-defined quasiparticle excitations are not allowed. Considering an effective bulk model characterized by an anomalous critical exponent, we derive an effective impurity action in the slave-boson context. Performing the large-$N_{\sigma}$ analysis with a spin index $N_{\sigma}$, we find an impurity quantum phase transition from a decoupled local-moment state to a Kondo-screened phase. We evaluate the impurity spin susceptibility and specific heat coefficient at zero temperature, and find that such responses follow power-law dependencies due to the anomalous exponent of the algebraic spin liquid. Our main finding is that the Wilson's ratio for the magnetic impurity depends strongly on the critical exponent in the zero temperature limit. We propose that the Wilson's ratio for the magnetic impurity may be one possible probe to reveal criticality of the bulk system.
cond-mat.str-el
we study kondo physics in the algebraic spin liquid recently proposed to describe zncu_3oh_6cl_2 phys rev lett bf 98 117205 2007 although spin dynamics of the algebraic spin liquid is described by massless dirac fermions this problem differs from the pseudogap kondo model because the bulk physics in the algebraic spin liquid is governed by an interacting fixed point where welldefined quasiparticle excitations are not allowed considering an effective bulk model characterized by an anomalous critical exponent we derive an effective impurity action in the slaveboson context performing the largen_sigma analysis with a spin index n_sigma we find an impurity quantum phase transition from a decoupled localmoment state to a kondoscreened phase we evaluate the impurity spin susceptibility and specific heat coefficient at zero temperature and find that such responses follow powerlaw dependencies due to the anomalous exponent of the algebraic spin liquid our main finding is that the wilsons ratio for the magnetic impurity depends strongly on the critical exponent in the zero temperature limit we propose that the wilsons ratio for the magnetic impurity may be one possible probe to reveal criticality of the bulk system
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706.2944
Summing Pomeron loops in the dipole approach
In this paper we argue that in the kinematic range given by $ 1 \ll \ln(1/\as^2) \ll \as Y \ll \frac{1}{\as}$, we can reduce the Pomeron calculus to the exchange of non-interacting Pomerons with the renormalized amplitude of their interaction with the target. Therefore, the summation of the Pomeron loops can be performed using the improved Mueller, Patel, Salam and Iancu approximation and this leads to the geometrical scaling solution. This solution is found for the simplified BFKL kernel. We reproduce the findings of Hatta and Mueller that there are overlapping singularities. We suggest a way of dealing with these singularities.
hep-ph
in this paper we argue that in the kinematic range given by 1 ll ln1as2 ll as y ll frac1as we can reduce the pomeron calculus to the exchange of noninteracting pomerons with the renormalized amplitude of their interaction with the target therefore the summation of the pomeron loops can be performed using the improved mueller patel salam and iancu approximation and this leads to the geometrical scaling solution this solution is found for the simplified bfkl kernel we reproduce the findings of hatta and mueller that there are overlapping singularities we suggest a way of dealing with these singularities
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706.2945
Atom capture by nanotube and scaling anomaly
The existence of bound state of the polarizable neutral atom in the inverse square potential created by the electric field of single walled charged carbon nanotube (SWNT) is shown to be theoretically possible. The consideration of inequivalent boundary conditions due to self-adjoint extensions lead to this nontrivial bound state solution. It is also shown that the scaling anomaly is responsible for the existence of bound state. Binding of the polarizable atoms in the coupling constant interval \eta^2\in[0,1) may be responsible for the smearing of the edge of steps in quantized conductance, which has not been considered so far in literature.
cond-mat.mtrl-sci hep-th
the existence of bound state of the polarizable neutral atom in the inverse square potential created by the electric field of single walled charged carbon nanotube swnt is shown to be theoretically possible the consideration of inequivalent boundary conditions due to selfadjoint extensions lead to this nontrivial bound state solution it is also shown that the scaling anomaly is responsible for the existence of bound state binding of the polarizable atoms in the coupling constant interval eta2in01 may be responsible for the smearing of the edge of steps in quantized conductance which has not been considered so far in literature
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706.2946
An Obstruction to Quantization of the Sphere
In the standard example of strict deformation quantization of the symplectic sphere $S^2$, the set of allowed values of the quantization parameter $\hbar$ is not connected; indeed, it is almost discrete. Li recently constructed a class of examples (including $S^2$) in which $\hbar$ can take any value in an interval, but these examples are badly behaved. Here, I identify a natural additional axiom for strict deformation quantization and prove that it implies that the parameter set for quantizing $S^2$ is never connected.
math-ph math.MP math.OA math.QA
in the standard example of strict deformation quantization of the symplectic sphere s2 the set of allowed values of the quantization parameter hbar is not connected indeed it is almost discrete li recently constructed a class of examples including s2 in which hbar can take any value in an interval but these examples are badly behaved here i identify a natural additional axiom for strict deformation quantization and prove that it implies that the parameter set for quantizing s2 is never connected
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706.2947
Quantum Coherence Engines
In a report published in Science, Scully et al propose to generate "phaseonium", and "extract work from a single heat bath via vanishing coherence" [1]. On the basis of the laws of physics, such a proposal is futile for at least two reasons.
quant-ph
in a report published in science scully et al propose to generate phaseonium and extract work from a single heat bath via vanishing coherence 1 on the basis of the laws of physics such a proposal is futile for at least two reasons
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706.2948
Do local analogs of Lyman Break Galaxies exist?
The optical properties of a number of supercompact ultraviolet luminous galaxies (UVLG), recently discovered in the local Universe matching GALEX and Sloan Digital Sky Survey (SDSS) data, are discussed. Detailed re-analysis of the SDSS data for these and other similar but nearer galaxies shows that their surface brightness radial profile in both R and u bands is in most cases well described by an extended disk plus a central unresolved component (possibly a bulge). Since the SDSS pipeline used a single disk component to derive the half light radius of these UVLGs their size was severely underestimated. Consequently, the average UV surface brightness is much lower that previously quoted casting doubts on the claim that UVLGs are the local analogs of high redshift Lyman break galaxies.
astro-ph
the optical properties of a number of supercompact ultraviolet luminous galaxies uvlg recently discovered in the local universe matching galex and sloan digital sky survey sdss data are discussed detailed reanalysis of the sdss data for these and other similar but nearer galaxies shows that their surface brightness radial profile in both r and u bands is in most cases well described by an extended disk plus a central unresolved component possibly a bulge since the sdss pipeline used a single disk component to derive the half light radius of these uvlgs their size was severely underestimated consequently the average uv surface brightness is much lower that previously quoted casting doubts on the claim that uvlgs are the local analogs of high redshift lyman break galaxies
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706.2949
AGN effect on cooling flow dynamics
We analyzed the feedback of AGN jets on cooling flow clusters using three-dimensional AMR hydrodynamic simulations. We studied the interaction of the jet with the intracluster medium and creation of low X-ray emission cavities (Bubbles) in cluster plasma. The distribution of energy input by the jet into the system was quantified in its different forms, i.e. internal, kinetic and potential. We find that the energy associated with the bubbles, (pV + gamma pV/(gamma-1)), accounts for less than 10 percent of the jet energy.
astro-ph
we analyzed the feedback of agn jets on cooling flow clusters using threedimensional amr hydrodynamic simulations we studied the interaction of the jet with the intracluster medium and creation of low xray emission cavities bubbles in cluster plasma the distribution of energy input by the jet into the system was quantified in its different forms ie internal kinetic and potential we find that the energy associated with the bubbles pv gamma pvgamma1 accounts for less than 10 percent of the jet energy
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706.295
Electron Bunching in Stacks of Coupled Quantum Dots
We study the transport properties of two double quantum dots in a parallel arrangement at temperatures of a few Kelvin. Thereby, we show that decoherence entailed by the substrate phonons affects the shot noise. For asymmetric coupling between the dots and the respective lead, the current noise is sub-Poissonian for resonant tunneling, but super-Poissonian in the vicinity of the resonances. Our results indicate that phonon emission and absorption is responsible for the shot noise enhancement. The observed asymmetry of the peaks at low temperatures stems from spontaneous emission.
cond-mat.mes-hall cond-mat.mtrl-sci
we study the transport properties of two double quantum dots in a parallel arrangement at temperatures of a few kelvin thereby we show that decoherence entailed by the substrate phonons affects the shot noise for asymmetric coupling between the dots and the respective lead the current noise is subpoissonian for resonant tunneling but superpoissonian in the vicinity of the resonances our results indicate that phonon emission and absorption is responsible for the shot noise enhancement the observed asymmetry of the peaks at low temperatures stems from spontaneous emission
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706.2951
Collinear versus non-collinear magnetic order in Pd atomic clusters: ab-initio calculations
We present a thorough theoretical assessment of the stability of non-collinear spin arrangements in small palladium clusters. We generally find that ferromagnetic order is always preferred, but that antiferromagnetic and non-collinear configurations of different sorts exist and compete for the first excited isomers. We also show that the ground state is insensitive to the choice of atomic configuration for the pseudopotential used and to the approximation taken for the exchange and correlation potential. Moreover, the existence and relative stability of the different excited configurations also depends weakly on the approximations employed. These results provide strong evidence on the transferability of pseudopotential and exchange and correlation functionals for palladium clusters as opposed to the situation found for the bulk phases of palladium.
cond-mat.mtrl-sci
we present a thorough theoretical assessment of the stability of noncollinear spin arrangements in small palladium clusters we generally find that ferromagnetic order is always preferred but that antiferromagnetic and noncollinear configurations of different sorts exist and compete for the first excited isomers we also show that the ground state is insensitive to the choice of atomic configuration for the pseudopotential used and to the approximation taken for the exchange and correlation potential moreover the existence and relative stability of the different excited configurations also depends weakly on the approximations employed these results provide strong evidence on the transferability of pseudopotential and exchange and correlation functionals for palladium clusters as opposed to the situation found for the bulk phases of palladium
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706.2952
Mass distributions for nuclear disintegration from fission to evaporation
By a proper choice of the excitation energy per nucleon we analyze the mass distributions of the nuclear fragmentation at various excitation energies. Starting from low energies (between 0.1 and 1 MeV/nucleon) up to higher energies about 12 MeV/n, we classified the mass yield characteristics for heavy nuclei (A>200) on the basis of Statistical Multifragmentation Model. The evaluation of fragment distribution with the excitation energy show that the present results exhibit the same trend as the experimental ones.
nucl-th
by a proper choice of the excitation energy per nucleon we analyze the mass distributions of the nuclear fragmentation at various excitation energies starting from low energies between 01 and 1 mevnucleon up to higher energies about 12 mevn we classified the mass yield characteristics for heavy nuclei a200 on the basis of statistical multifragmentation model the evaluation of fragment distribution with the excitation energy show that the present results exhibit the same trend as the experimental ones
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706.2953
Running of $\alpha_s$ and $m_b$ in the MSSM
A consistent evolution of the strong coupling constant $\alpha_s$ from $M_Z$ to the GUT scale is presented, involving three-loop running and two-loop decoupling. The two-loop transition from the MS- to the DR-scheme is properly taken into account. In the second part of the paper, the bottom quark mass in the DR-scheme at the electroweak/SUSY scale is evaluated with four-loop accuracy. We find that the three-loop effects are comparable to the experimental uncertainty both for $\alpha_s$ and $m_b$.
hep-ph
a consistent evolution of the strong coupling constant alpha_s from m_z to the gut scale is presented involving threeloop running and twoloop decoupling the twoloop transition from the ms to the drscheme is properly taken into account in the second part of the paper the bottom quark mass in the drscheme at the electroweaksusy scale is evaluated with fourloop accuracy we find that the threeloop effects are comparable to the experimental uncertainty both for alpha_s and m_b
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706.2954
Ergodicity properties of quantum expectation values in entangled states
Using a model Hamiltonian for a single-mode electromagnetic field interacting with a nonlinear medium, we show that quantum expectation values of subsystem observables can exhibit remarkably diverse ergodic properties even when the dynamics of the total system is regular. The time series of the mean photon number is studied over a range of values of the ratio of the strength $\gamma$ of the nonlinearity to that of the inter-mode coupling $g$. We obtain the power spectrum, estimate the embedding dimension of the reconstructed phase space and the maximal Liapunov exponent $\lambda_{\rm max}$, and find the recurrence-time distribution of the coarse-grained dynamics. The dynamical behavior ranges from quasiperiodicity (for $\gamma/g \ll 1$) to chaos as characterized by $\lambda_{\rm max} > 0$ (for $\gamma/g \gtrsim 1$), and is interpreted.
quant-ph
using a model hamiltonian for a singlemode electromagnetic field interacting with a nonlinear medium we show that quantum expectation values of subsystem observables can exhibit remarkably diverse ergodic properties even when the dynamics of the total system is regular the time series of the mean photon number is studied over a range of values of the ratio of the strength gamma of the nonlinearity to that of the intermode coupling g we obtain the power spectrum estimate the embedding dimension of the reconstructed phase space and the maximal liapunov exponent lambda_rm max and find the recurrencetime distribution of the coarsegrained dynamics the dynamical behavior ranges from quasiperiodicity for gammag ll 1 to chaos as characterized by lambda_rm max 0 for gammag gtrsim 1 and is interpreted
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706.2955
Thue equations and torsion groups of elliptic curves
A new characterization of rational torsion subgroups of elliptic curves is found, for points of order greater than 4, through the existence of solution for systems of Thue equations.
math.NT
a new characterization of rational torsion subgroups of elliptic curves is found for points of order greater than 4 through the existence of solution for systems of thue equations
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706.2956
Density-dependent interactions and structure of charged colloidal dispersions in the weak screening regime
We determine the structure of charge-stabilized colloidal suspensions at low ionic strength over an extended range of particle volume fractions using a combination of light and small angle neutron scattering experiments. The variation of the structure factor with concentration is analyzed within a one-component model of a colloidal suspension. We show that the observed structural behavior corresponds to a non-monotonic density dependence of the colloid effective charge and the mean interparticle interaction energy. Our findings are corroborated by similar observations from primitive model computer simulations of salt-free colloidal suspensions.
cond-mat.soft
we determine the structure of chargestabilized colloidal suspensions at low ionic strength over an extended range of particle volume fractions using a combination of light and small angle neutron scattering experiments the variation of the structure factor with concentration is analyzed within a onecomponent model of a colloidal suspension we show that the observed structural behavior corresponds to a nonmonotonic density dependence of the colloid effective charge and the mean interparticle interaction energy our findings are corroborated by similar observations from primitive model computer simulations of saltfree colloidal suspensions
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706.2957
Reply to Comment on "A local realist model for correlations of the singlet state"
The general conclusion of Seevinck and Larsson is that our model exploits the so-called coincidence-time loophole and produces sinusoidal (quantum-like) correlations but does not model the singlet state because it does not violate the relevant Bell inequality derived by Larsson and Gill, since in order to obtain the sinusoidal correlations the probability of coincidences in our model goes to zero. In this reply, we refute their arguments that lead to this conclusion and demonstrate that our model can reproduce results of photon and ion-trap experiments with frequencies of coincidences that are not in conflict with the observations.
quant-ph
the general conclusion of seevinck and larsson is that our model exploits the socalled coincidencetime loophole and produces sinusoidal quantumlike correlations but does not model the singlet state because it does not violate the relevant bell inequality derived by larsson and gill since in order to obtain the sinusoidal correlations the probability of coincidences in our model goes to zero in this reply we refute their arguments that lead to this conclusion and demonstrate that our model can reproduce results of photon and iontrap experiments with frequencies of coincidences that are not in conflict with the observations
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706.2958
On the shadow boundary of a centrally symmetric convex body
We discuss the concept of the shadow boundary of a centrally symmetric convex ball $K$ (actually being the unit ball of a Minkowski normed space) with respect to a direction ${\bf x}$ of the Euclidean n-space $R^n$. We introduce the concept of general parameter spheres of $K$ corresponding to this direction and prove that the shadow boundary is a topological manifold if all of the non-degenerated general parameter spheres are, too. In this case, using the approximation theorem of cell-like maps we get that they are homeomorphic to the $(n-2)$-dimensional sphere $S^{(n-2)}$. We also prove that the bisector (equidistant set of the corresponding normed space) in the direction ${\bf x}$ is homeomorphic to $R^{(n-1)}$ iff all of the non-degenerated general parameter spheres are $(n-2)$-manifolds implying that if the bisector is a homeomorphic copy of $R^{(n-1)}$ then the corresponding shadow boundary is a topological $(n-2)$-sphere.
math.MG math.GT
we discuss the concept of the shadow boundary of a centrally symmetric convex ball k actually being the unit ball of a minkowski normed space with respect to a direction bf x of the euclidean nspace rn we introduce the concept of general parameter spheres of k corresponding to this direction and prove that the shadow boundary is a topological manifold if all of the nondegenerated general parameter spheres are too in this case using the approximation theorem of celllike maps we get that they are homeomorphic to the n2dimensional sphere sn2 we also prove that the bisector equidistant set of the corresponding normed space in the direction bf x is homeomorphic to rn1 iff all of the nondegenerated general parameter spheres are n2manifolds implying that if the bisector is a homeomorphic copy of rn1 then the corresponding shadow boundary is a topological n2sphere
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706.2959
The variability plane of accreting compact objects
Recently, it has been shown that soft-state black hole X-ray binaries and active galactic nuclei populate a plane in the space defined by the black hole mass, accretion rate and characteristic frequency. We show that this plane can be extended to hard-state objects if one allows a constant offset for the frequencies in the soft and the hard state. During a state transition the frequencies rapidly move from one scaling to the other depending on an additional parameter, possibly the disk-fraction. The relationship between frequency, mass and accretion rate can be further extended by including weakly accreting neutron stars. We explore if the lower kHz QPOs of neutron stars and the dwarf nova oscillations of white dwarfs can be included as well and discuss the physical implications of the found correlation.
astro-ph
recently it has been shown that softstate black hole xray binaries and active galactic nuclei populate a plane in the space defined by the black hole mass accretion rate and characteristic frequency we show that this plane can be extended to hardstate objects if one allows a constant offset for the frequencies in the soft and the hard state during a state transition the frequencies rapidly move from one scaling to the other depending on an additional parameter possibly the diskfraction the relationship between frequency mass and accretion rate can be further extended by including weakly accreting neutron stars we explore if the lower khz qpos of neutron stars and the dwarf nova oscillations of white dwarfs can be included as well and discuss the physical implications of the found correlation
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706.296
Constraints on top-down models for the origin of UHECRs from the Pierre Auger Observatory data
Taking into account the Pierre Auger Observatory limits on the photon fraction among the highest energy cosmic rays, we show that the models based on the decay of super-heavy dark matter in the halo of our Galaxy are essentially excluded from being the sources of UHECRs unless their contribution becomes significant only above 100 EeV. Some top-down models based on topological defects are however compatible with the current data and may be best constrained in the future by the high-energy neutrino flux limit.
astro-ph
taking into account the pierre auger observatory limits on the photon fraction among the highest energy cosmic rays we show that the models based on the decay of superheavy dark matter in the halo of our galaxy are essentially excluded from being the sources of uhecrs unless their contribution becomes significant only above 100 eev some topdown models based on topological defects are however compatible with the current data and may be best constrained in the future by the highenergy neutrino flux limit
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706.2961
Structure of glassy lithium sulfate films sputtered in nitrogen (LISON): Insight from Raman spectroscopy and ab initio calculations
Raman spectra of thin solid electrolyte films obtained by sputtering a lithium sulfate target in nitrogen plasma are measured and compared to ab initio electronic structure calculations for clusters composed of 28 atoms. Agreement between measured and calculated spectra is obtained when oxygen atoms are replaced by nitrogen atoms and when the nitrogen atoms form bonds with each other. This suggests that the incorporation of nitrogen during the sputtering process leads to structures in the film, which prevent crystallization of these thin film salt glasses.
cond-mat.mtrl-sci
raman spectra of thin solid electrolyte films obtained by sputtering a lithium sulfate target in nitrogen plasma are measured and compared to ab initio electronic structure calculations for clusters composed of 28 atoms agreement between measured and calculated spectra is obtained when oxygen atoms are replaced by nitrogen atoms and when the nitrogen atoms form bonds with each other this suggests that the incorporation of nitrogen during the sputtering process leads to structures in the film which prevent crystallization of these thin film salt glasses
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706.2962
Variable stars in the open cluster NGC 6791 and its surrounding field
Aims: This work presents a high--precision variability survey in the field of the old, super metal-rich open cluster NGC 6791. Methods: The data sample consists of more than 75,000 high-precision CCD time series measurements in the V band obtained mainly at the Canada-France-Hawaii Telescope, with additional data from S. Pedro Martir and Loiano observatories, over a time span of ten nights. The field covers an area of 42x28 arcmin^2. Results: We have discovered 260 new variables and re-determined periods and amplitudes of 70 known variable stars. By means of a photometric evaluation of the membership in NGC 6791, and a preliminary membership based on the proper motions, we give a full description of the variable content of the cluster and surrounding field in the range 16<V<23.5. Accurate periods can be given for the variables with P<4.0 d, while for ones with longer periods the limited time-baseline hampered precise determinations. We categorized the entire sample as follows: 6 pulsating, 3 irregular, 3 cataclysmic, 89 rotational variables and 61 eclipsing systems; moreover, we detected 168 candidate variables for which we cannot give a variability class since their periods are much longer than our time baseline. Conclusions: On the basis of photometric considerations, and of the positions of the stars with respect to the center of the cluster, we inferred that 11 new variable stars are likely members of the cluster, for 22 stars the membership is doubtful and 137 are likely non-members. We also detected an outburst of about 3 mag in the light curve of a very faint blue star belonging to the cluster and we suggest that this star could be a new U Gem (dwarf nova) cataclysmic variable.
astro-ph
aims this work presents a highprecision variability survey in the field of the old super metalrich open cluster ngc 6791 methods the data sample consists of more than 75000 highprecision ccd time series measurements in the v band obtained mainly at the canadafrancehawaii telescope with additional data from s pedro martir and loiano observatories over a time span of ten nights the field covers an area of 42x28 arcmin2 results we have discovered 260 new variables and redetermined periods and amplitudes of 70 known variable stars by means of a photometric evaluation of the membership in ngc 6791 and a preliminary membership based on the proper motions we give a full description of the variable content of the cluster and surrounding field in the range 16v235 accurate periods can be given for the variables with p40 d while for ones with longer periods the limited timebaseline hampered precise determinations we categorized the entire sample as follows 6 pulsating 3 irregular 3 cataclysmic 89 rotational variables and 61 eclipsing systems moreover we detected 168 candidate variables for which we cannot give a variability class since their periods are much longer than our time baseline conclusions on the basis of photometric considerations and of the positions of the stars with respect to the center of the cluster we inferred that 11 new variable stars are likely members of the cluster for 22 stars the membership is doubtful and 137 are likely nonmembers we also detected an outburst of about 3 mag in the light curve of a very faint blue star belonging to the cluster and we suggest that this star could be a new u gem dwarf nova cataclysmic variable
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706.2963
Outage Behavior of Discrete Memoryless Channels Under Channel Estimation Errors
Classically, communication systems are designed assuming perfect channel state information at the receiver and/or transmitter. However, in many practical situations, only an estimate of the channel is available that differs from the true channel. We address this channel mismatch scenario by using the notion of estimation-induced outage capacity, for which we provide an associated coding theorem and its strong converse, assuming a discrete memoryless channel. We illustrate our ideas via numerical simulations for transmissions over Ricean fading channels under a quality of service (QoS) constraint using rate-limited feedback channel and maximum likelihood (ML) channel estimation. Our results provide intuitive insights on the impact of the channel estimate and the channel characteristics (SNR, Ricean K-factor, training sequence length, feedback rate, etc.) on the mean outage capacity.
cs.IT math.IT
classically communication systems are designed assuming perfect channel state information at the receiver andor transmitter however in many practical situations only an estimate of the channel is available that differs from the true channel we address this channel mismatch scenario by using the notion of estimationinduced outage capacity for which we provide an associated coding theorem and its strong converse assuming a discrete memoryless channel we illustrate our ideas via numerical simulations for transmissions over ricean fading channels under a quality of service qos constraint using ratelimited feedback channel and maximum likelihood ml channel estimation our results provide intuitive insights on the impact of the channel estimate and the channel characteristics snr ricean kfactor training sequence length feedback rate etc on the mean outage capacity
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706.2964
Local models and EPR quantum correlations
A model for two entangled systems in an EPR setting is shown to reproduce the quantum-mechanical outcomes and expectation values. Each system is represented by a small sphere containing a point-like particle embedded in a field. A quantum state appears as an equivalence class of several possible particle-field configurations. Contrarily to Bell-type hidden variables models, the fields account for the non-commutative aspects of the measurements and deny the simultaneous reality of incompatible physical quantities, thereby allowing to escape EPR's ``completeness or locality'' dilemma.
quant-ph
a model for two entangled systems in an epr setting is shown to reproduce the quantummechanical outcomes and expectation values each system is represented by a small sphere containing a pointlike particle embedded in a field a quantum state appears as an equivalence class of several possible particlefield configurations contrarily to belltype hidden variables models the fields account for the noncommutative aspects of the measurements and deny the simultaneous reality of incompatible physical quantities thereby allowing to escape eprs completeness or locality dilemma
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706.2965
The two Josephson junction flux qubit with large tunneling amplitude
In this paper we discuss solid-state nanoelectronic realizations of Josephson flux qubits with large tunneling amplitude between the two macroscopic states. The latter can be controlled via the height and wells form of the potential barrier, which is determined by quantum-state engineering of the flux qubit circuit. The simplest circuit of the flux qubit is a superconducting loop interrupted by a Josephson nanoscale tunnel junction. The tunneling amplitude between two macroscopically different states can be essentially increased, by engineering of the qubit circuit, if tunnel junction is replaced by a ScS contact. However, only Josephson tunnel junctions are particularly suitable for large-scale integration circuits and quantum detectors with preset-day technology. To overcome this difficulty we consider here the flux qubit with high-level energy separation between "ground" and "excited" states, which consists of a superconducting loop with two low-capacitance Josephson tunnel junctions in series. We demonstrate that for real parameters of resonant superposition between the two macroscopic states the tunneling amplitude can reach values greater than 1K. Analytical results for the tunneling amplitude obtained within semiclassical approximation by instanton technique show good correlation with a numerical solution.
cond-mat.supr-con cond-mat.mes-hall
in this paper we discuss solidstate nanoelectronic realizations of josephson flux qubits with large tunneling amplitude between the two macroscopic states the latter can be controlled via the height and wells form of the potential barrier which is determined by quantumstate engineering of the flux qubit circuit the simplest circuit of the flux qubit is a superconducting loop interrupted by a josephson nanoscale tunnel junction the tunneling amplitude between two macroscopically different states can be essentially increased by engineering of the qubit circuit if tunnel junction is replaced by a scs contact however only josephson tunnel junctions are particularly suitable for largescale integration circuits and quantum detectors with presetday technology to overcome this difficulty we consider here the flux qubit with highlevel energy separation between ground and excited states which consists of a superconducting loop with two lowcapacitance josephson tunnel junctions in series we demonstrate that for real parameters of resonant superposition between the two macroscopic states the tunneling amplitude can reach values greater than 1k analytical results for the tunneling amplitude obtained within semiclassical approximation by instanton technique show good correlation with a numerical solution
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706.2966
Surface melting of nanoscopic epitaxial films
By introducing finite size surface and interfacial excess quantities, interactions between interfaces are shown to modify the usual surface premelting phenomenon. It is the case of surface melting of a thin solid film s deposited on a planar solid substrate S. More precisely to the usual wetting condition of the solid s by its own melt l, necessary for premelting (wetting factor F<0), is adjoined a new quantity G describing the interactions of the l/s interface with the s/S interface. When G>0 this interface attraction boosts the premelting so that a two stage boosted surface premelting is foreseen: a continuous premelting, up to roughly half the deposited film, is followed by an abrupt first order premelting. When G<0 these interfaces repell each other so that premelting is refrained and the film remains partly solid above the bulk melting point (overheating) what is called astride melting. Elastic stress modifies both types of melting curves. Bulk and surface stresses have to be distinguished.
cond-mat.mtrl-sci
by introducing finite size surface and interfacial excess quantities interactions between interfaces are shown to modify the usual surface premelting phenomenon it is the case of surface melting of a thin solid film s deposited on a planar solid substrate s more precisely to the usual wetting condition of the solid s by its own melt l necessary for premelting wetting factor f0 is adjoined a new quantity g describing the interactions of the ls interface with the ss interface when g0 this interface attraction boosts the premelting so that a two stage boosted surface premelting is foreseen a continuous premelting up to roughly half the deposited film is followed by an abrupt first order premelting when g0 these interfaces repell each other so that premelting is refrained and the film remains partly solid above the bulk melting point overheating what is called astride melting elastic stress modifies both types of melting curves bulk and surface stresses have to be distinguished
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706.2967
Terahertz Parametric Gain in Semiconductor Superlattices
We consider a high-frequency response of electrons in a single miniband of superlattice subject to dc and ac electric fields. Action of ac electric field causes oscillations of electron's effective mass in miniband, which result in a parametric resonance. We have established a theoretical feasibility of phase-sensitive parametric amplification at the resonance. The parametric amplification does not require operation in conditions of negative differential conductance. Therefore a formation of destructive domains of high electric field inside the superlattice can be prevented. Here we concentrate on the parametric up- and down-conversion of electromagnetic radiation from available frequencies to desirable THz frequency range.
cond-mat.mes-hall cond-mat.stat-mech
we consider a highfrequency response of electrons in a single miniband of superlattice subject to dc and ac electric fields action of ac electric field causes oscillations of electrons effective mass in miniband which result in a parametric resonance we have established a theoretical feasibility of phasesensitive parametric amplification at the resonance the parametric amplification does not require operation in conditions of negative differential conductance therefore a formation of destructive domains of high electric field inside the superlattice can be prevented here we concentrate on the parametric up and downconversion of electromagnetic radiation from available frequencies to desirable thz frequency range
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706.2968
Random resistor network model of minimal conductivity in graphene
Transport in undoped graphene is related to percolating current patterns in the networks of {\em N-} and {\em P}-type regions reflecting the strong bipolar charge density fluctuations. Transmissions of the {\em P-N} junctions, though small, are vital in establishing the macroscopic conductivity. We propose a random resistor network model to analyze scaling dependencies of the conductance on the doping and disorder, the quantum magnetoresistance and the corresponding dephasing rate.
cond-mat.mes-hall cond-mat.dis-nn
transport in undoped graphene is related to percolating current patterns in the networks of em n and em ptype regions reflecting the strong bipolar charge density fluctuations transmissions of the em pn junctions though small are vital in establishing the macroscopic conductivity we propose a random resistor network model to analyze scaling dependencies of the conductance on the doping and disorder the quantum magnetoresistance and the corresponding dephasing rate
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706.2969
Optical spectroscopy of RU Cam, a pulsating carbon star
We analysed the high resolution spectra of a RU Cam, classified as W Vir type star. The atmospheric parameters of RU Cam were estimated Teff=5250K and log g=1.0. The hydrogen deficiency of RU Cam was not confirmed. The iron abundance, [Fe/H]=-0.37, is close to the solar one. Abundances of most other elements are also close to normal. We found considerable excesses of carbon and nitrogen: [C/Fe]=+0.98, [N/Fe]=+0.60. The carbon to oxygen ratio is C/O$\ge$1. The carbon isotopic abundance ratio is equal to C^12/C^13=4.5. For sodium a moderate overabundance Na/Fe=+0.55 was obtained. For two moments of observations we found close heliocentric velocity values, Vr=-21.7+/-0.8 and -23.1+/-1.0 km/s. Both spectra contain a peculiar feature - an emission component of NaI doublet which location agrees with the radial velocity from the bulk of metallic lines. For our two observing moments we found no dependence of radial velocities on the formation depth or on excitation energy for metallic lines.
astro-ph
we analysed the high resolution spectra of a ru cam classified as w vir type star the atmospheric parameters of ru cam were estimated teff5250k and log g10 the hydrogen deficiency of ru cam was not confirmed the iron abundance feh037 is close to the solar one abundances of most other elements are also close to normal we found considerable excesses of carbon and nitrogen cfe098 nfe060 the carbon to oxygen ratio is coge1 the carbon isotopic abundance ratio is equal to c12c1345 for sodium a moderate overabundance nafe055 was obtained for two moments of observations we found close heliocentric velocity values vr21708 and 23110 kms both spectra contain a peculiar feature an emission component of nai doublet which location agrees with the radial velocity from the bulk of metallic lines for our two observing moments we found no dependence of radial velocities on the formation depth or on excitation energy for metallic lines
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706.297
On Scattering for CMV Matrices
Adamjan-Arov (Lax--Phillips) model space is considered as a scattering representation space for a CMV matrix in context of an extended Marchenko--Faddeev scattering theory. That is, there exists a basis in which the multiplication by independent variable is a CMV matrix. This basis as well as Verblunski coefficients are computed explicitly in terms of Nehari interpolation. Asymptotically the Verblynski coefficients go to zero. Moreover, relations between the basis and wandering subspaces are established. Transformation from scattering representation to spectral representation is given.
math.SP math.FA
adamjanarov laxphillips model space is considered as a scattering representation space for a cmv matrix in context of an extended marchenkofaddeev scattering theory that is there exists a basis in which the multiplication by independent variable is a cmv matrix this basis as well as verblunski coefficients are computed explicitly in terms of nehari interpolation asymptotically the verblynski coefficients go to zero moreover relations between the basis and wandering subspaces are established transformation from scattering representation to spectral representation is given
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706.2971
Entropy profiles in X-ray luminous galaxy clusters at z>0.1
[Abridged] The entropy distribution of the intracluster gas reflects both accretion history of the gas and processes of feedback which provide a further non-gravitational energy besides the potential one. In this work, we study the profiles and the scaling properties of the gas entropy in 24 hot (kT_{gas} > 6 keV) galaxy clusters observed with Chandra in the redshift range 0.14-0.82 and showing different states of relaxation. We recover the gas density, temperature and entropy profiles in a non-parametric way. Adding the hydrostatic equilibrium hypothesis, radial profiles are also obtained from the deprojection of the surface brightness, allowing to verify whether the hydrostatic equilibrium is a tenable hypothesis by comparison with the spectral measurements. We confirm that this is the case on scales larger than 100 kpc and discuss the deviations observed in few non-cooling core clusters in the inner regions. We show that the entropy profiles are remarkably similar outside the core and can be described by simple power-laws with slope of 1.0-1.2. We measure an entropy level at 0.1 R_{200} of 100-500 keV cm^2 and a central plateau which spans a wide range of value (~ a few-200 keV cm^2) depending on the state of relaxation of the source. To characterize the energetic of the central regions, we compare the radial behaviour of the temperature of the gas with the temperature of the dark matter T_{DM} by estimating the excess of energy Delta E = 3/2 k(T_{gas}- T_{DM}). We point out that Delta E ranges from ~ 0 in typical cooling-core clusters to few keV within 100 kpc in non-cooling core systems. We also measure a significant correlation between the total iron mass and the entropy outside the cooling region,whereas in the inner regions they anti-correlate strongly.
astro-ph
abridged the entropy distribution of the intracluster gas reflects both accretion history of the gas and processes of feedback which provide a further nongravitational energy besides the potential one in this work we study the profiles and the scaling properties of the gas entropy in 24 hot kt_gas 6 kev galaxy clusters observed with chandra in the redshift range 014082 and showing different states of relaxation we recover the gas density temperature and entropy profiles in a nonparametric way adding the hydrostatic equilibrium hypothesis radial profiles are also obtained from the deprojection of the surface brightness allowing to verify whether the hydrostatic equilibrium is a tenable hypothesis by comparison with the spectral measurements we confirm that this is the case on scales larger than 100 kpc and discuss the deviations observed in few noncooling core clusters in the inner regions we show that the entropy profiles are remarkably similar outside the core and can be described by simple powerlaws with slope of 1012 we measure an entropy level at 01 r_200 of 100500 kev cm2 and a central plateau which spans a wide range of value a few200 kev cm2 depending on the state of relaxation of the source to characterize the energetic of the central regions we compare the radial behaviour of the temperature of the gas with the temperature of the dark matter t_dm by estimating the excess of energy delta e 32 kt_gas t_dm we point out that delta e ranges from 0 in typical coolingcore clusters to few kev within 100 kpc in noncooling core systems we also measure a significant correlation between the total iron mass and the entropy outside the cooling regionwhereas in the inner regions they anticorrelate strongly
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706.2972
Electron-positron annihilation into phi f_{0}(980) and clues for a new 1^{--} resonance
We study the e^{+}e^{-} to phi pi pi reaction for pions in an isoscalar s-wave which is dominated by loop mechanisms. For kaon loops we start from the conventional RCHPT, but use the unitarized amplitude for KbarK-pipi scattering and the full kaon form factor instead of the lowest order terms. We study also effects of vector mesons using RCHPT supplemented with the conventional anomalous term for VVP interactions and taking into account the effects of heavy vector mesons in the K*K transition form factor. We find a peak in the dipion invariant mass around the f_{0}(980) as in the experiment. Selecting the phi f_{0}(980) contribution as a function of the e^{+}e^{-} energy we also reproduce the experimental data except for a narrow peak, yielding support to the existence of a 1^{--} resonance above the phi f_{0}(980) threshold, coupling strongly to this state.
hep-ph
we study the ee to phi pi pi reaction for pions in an isoscalar swave which is dominated by loop mechanisms for kaon loops we start from the conventional rchpt but use the unitarized amplitude for kbarkpipi scattering and the full kaon form factor instead of the lowest order terms we study also effects of vector mesons using rchpt supplemented with the conventional anomalous term for vvp interactions and taking into account the effects of heavy vector mesons in the kk transition form factor we find a peak in the dipion invariant mass around the f_0980 as in the experiment selecting the phi f_0980 contribution as a function of the ee energy we also reproduce the experimental data except for a narrow peak yielding support to the existence of a 1 resonance above the phi f_0980 threshold coupling strongly to this state
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706.2973
Nontrivial critical crossover between directed percolation models: Effect of infinitely many absorbing states
At non-equilibrium phase transitions into absorbing (trapped) states, it is well known that the directed percolation (DP) critical scaling is shared by two classes of models with a single (S) absorbing state and with infinitely many (IM) absorbing states. We study the crossover behavior in one dimension, arising from a considerable reduction of the number of absorbing states (typically from the IM-type to the S-type DP models), by following two different (excitatory or inhibitory) routes which make the auxiliary field density abruptly jump at the crossover. Along the excitatory route, the system becomes overly activated even for an infinitesimal perturbation and its crossover becomes discontinuous. Along the inhibitory route, we find continuous crossover with the universal crossover exponent $\phi\simeq 1.78(6)$, which is argued to be equal to $\nu_\|$, the relaxation time exponent of the DP universality class on a general footing. This conjecture is also confirmed in the case of the directed Ising (parity-conserving) class. Finally, we discuss the effect of diffusion to the IM-type models and suggest an argument why diffusive models with some hybrid-type reactions should belong to the DP class.
cond-mat.stat-mech
at nonequilibrium phase transitions into absorbing trapped states it is well known that the directed percolation dp critical scaling is shared by two classes of models with a single s absorbing state and with infinitely many im absorbing states we study the crossover behavior in one dimension arising from a considerable reduction of the number of absorbing states typically from the imtype to the stype dp models by following two different excitatory or inhibitory routes which make the auxiliary field density abruptly jump at the crossover along the excitatory route the system becomes overly activated even for an infinitesimal perturbation and its crossover becomes discontinuous along the inhibitory route we find continuous crossover with the universal crossover exponent phisimeq 1786 which is argued to be equal to nu_ the relaxation time exponent of the dp universality class on a general footing this conjecture is also confirmed in the case of the directed ising parityconserving class finally we discuss the effect of diffusion to the imtype models and suggest an argument why diffusive models with some hybridtype reactions should belong to the dp class
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706.2974
Remote laboratories: new technology and standard based architecture
E-Laboratories are important components of e- learning environments, especially in scientific and technical disciplines. First widespread E-Labs consisted in proposing simulations of real systems (virtual labs), as building remote labs (remote control of real systems) was difficult by lack of industrial standards and common protocols. Nowadays, robotics and automation technologies make easier the interfacing of systems with computers. In this frame, many researchers (such as those mentioned in [1]) focus on how to set up such a remote control. But, only a few of them deal with the educational point of view of the problem. This paper outlines our current research and reflection about remote laboratory modelling.
cs.OH
elaboratories are important components of e learning environments especially in scientific and technical disciplines first widespread elabs consisted in proposing simulations of real systems virtual labs as building remote labs remote control of real systems was difficult by lack of industrial standards and common protocols nowadays robotics and automation technologies make easier the interfacing of systems with computers in this frame many researchers such as those mentioned in 1 focus on how to set up such a remote control but only a few of them deal with the educational point of view of the problem this paper outlines our current research and reflection about remote laboratory modelling
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706.2975
U_{PMNS} = U_ell^dagger U_nu
We consider corrections to vanishing U_{e3} and maximal atmospheric neutrino mixing originating from the relation U = U_ell^dagger U_nu, where U is the PMNS mixing matrix and U_ell (U_nu) is associated with the diagonalization of the charged lepton (neutrino) mass matrix. We assume that in the limit of U_ell or U_nu being the unit matrix, one has U_{e3} = 0 and theta_{23} = pi/4, while the solar neutrino mixing angle is a free parameter. Well-known special cases of the indicated scenario are the bimaximal and tri-bimaximal mixing schemes. If U_{e3} \neq 0 and theta_{23} \neq pi/4 due to corrections from the charged leptons, |U_{e3}| can be sizable (close to the existing upper limit) and we find that the value of the solar neutrino mixing angle is linked to the magnitude of CP violation in neutrino oscillations. In the alternative case of the neutrino sector correcting U_{e3} = 0 and theta_{23} = pi/4, we obtain a generically smaller |U_{e3}| than in the first case. Now the magnitude of CP violation in neutrino oscillations is connected to the value of the atmospheric neutrino mixing angle theta_{23}. We find that both cases are in agreement with present observations. We also introduce parametrization independent "sum-rules" for the oscillation parameters.
hep-ph
we consider corrections to vanishing u_e3 and maximal atmospheric neutrino mixing originating from the relation u u_elldagger u_nu where u is the pmns mixing matrix and u_ell u_nu is associated with the diagonalization of the charged lepton neutrino mass matrix we assume that in the limit of u_ell or u_nu being the unit matrix one has u_e3 0 and theta_23 pi4 while the solar neutrino mixing angle is a free parameter wellknown special cases of the indicated scenario are the bimaximal and tribimaximal mixing schemes if u_e3 neq 0 and theta_23 neq pi4 due to corrections from the charged leptons u_e3 can be sizable close to the existing upper limit and we find that the value of the solar neutrino mixing angle is linked to the magnitude of cp violation in neutrino oscillations in the alternative case of the neutrino sector correcting u_e3 0 and theta_23 pi4 we obtain a generically smaller u_e3 than in the first case now the magnitude of cp violation in neutrino oscillations is connected to the value of the atmospheric neutrino mixing angle theta_23 we find that both cases are in agreement with present observations we also introduce parametrization independent sumrules for the oscillation parameters
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706.2976
The Interaction Of Multiple Convection Zones In A-type Stars
A-type stars have a complex internal structure with the possibility of multiple convection zones. If not sufficiently separated, such zones will interact through the convectively stable regions that lie between them. It is therefore of interest to ask whether the typical conditions that exist within such stars are such that these convections zones can ever be considered as disjoint. In this paper we present results from numerical simulations that help in understanding how increasing the distance between the convectively unstable regions are likely to interact through the stable region that separates them. This has profound implications for mixing and transport within these stars.
astro-ph
atype stars have a complex internal structure with the possibility of multiple convection zones if not sufficiently separated such zones will interact through the convectively stable regions that lie between them it is therefore of interest to ask whether the typical conditions that exist within such stars are such that these convections zones can ever be considered as disjoint in this paper we present results from numerical simulations that help in understanding how increasing the distance between the convectively unstable regions are likely to interact through the stable region that separates them this has profound implications for mixing and transport within these stars
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706.2977
Rational formality of function spaces
Let $X$ be a nilpotent space such that there exists $N\geq 1$ with $H^N(X,\mathbb Q) \ne 0$ and $H^n(X,\mathbb Q)=0$ if $n>N$. Let $Y$ be a m-connected space with $m\geq N+1$ and $H^*(Y,\mathbb Q)$ is finitely generated as algebra. We assume that the odd part of the rational Hurewicz homomorphism: $\pi_{odd}(X)\otimes \mathbb Q\to H_{odd}(X,\mathbb Q)$ is non-zero. We prove that if the space $\mathcal F(X,Y)$ of continuous maps from $X$ to $Y$ is rationally formal, then $Y$ has the rational homotopy type of a finite product of Eilenberg Mac Lane spaces. At the opposite, we exhibit an example of a rationally formal space $\mathcal F(S^2,Y)$ where $Y$ is not rationally equivalent to a product of Eilenberg Mac Lane spaces.
math.AT
let x be a nilpotent space such that there exists ngeq 1 with hnxmathbb q ne 0 and hnxmathbb q0 if nn let y be a mconnected space with mgeq n1 and hymathbb q is finitely generated as algebra we assume that the odd part of the rational hurewicz homomorphism pi_oddxotimes mathbb qto h_oddxmathbb q is nonzero we prove that if the space mathcal fxy of continuous maps from x to y is rationally formal then y has the rational homotopy type of a finite product of eilenberg mac lane spaces at the opposite we exhibit an example of a rationally formal space mathcal fs2y where y is not rationally equivalent to a product of eilenberg mac lane spaces
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706.2978
Quantum and semiclassical phase functions for the quantization of symmetric oscillators
We investigate symmetric oscillators, and in particular their quantization, by employing semiclassical and quantum phase functions introduced in the context of Liouville-Green transformations of the Schr\"{o}dinger equation. For anharmonic oscillators, first order semiclassical quantization is seldom accurate and the higher order expansions eventually break down given the asymptotic nature of the series. A quantum phase that allows in principle to retrieve the exact quantum mechanical quantization condition and wavefunctions is given along with an iterative scheme to compute it. The arbitrariness surrounding quantum phase functions is lifted by supplementing the phase with boundary conditions involving high order semiclassical expansions. This allows to extend the definition of oscillation numbers, that determine the quantization of the harmonic oscillator, to the anharmonic case. Several illustrations involving homogeneous as well as coupling constant dependant anharmonic oscillators are given.
quant-ph hep-th math-ph math.MP
we investigate symmetric oscillators and in particular their quantization by employing semiclassical and quantum phase functions introduced in the context of liouvillegreen transformations of the schrodinger equation for anharmonic oscillators first order semiclassical quantization is seldom accurate and the higher order expansions eventually break down given the asymptotic nature of the series a quantum phase that allows in principle to retrieve the exact quantum mechanical quantization condition and wavefunctions is given along with an iterative scheme to compute it the arbitrariness surrounding quantum phase functions is lifted by supplementing the phase with boundary conditions involving high order semiclassical expansions this allows to extend the definition of oscillation numbers that determine the quantization of the harmonic oscillator to the anharmonic case several illustrations involving homogeneous as well as coupling constant dependant anharmonic oscillators are given
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706.2979
Security problems with a SC-CNN-based Chaotic Masking Secure Communication System
This paper studies the security of a chaotic cryptosystem based on the Chua circuit and implemented with State Controlled Cellular Neural Networks. It is shown that the plaintext can be retrieved by ciphertext band-pass filtering after an imperfect decoding with wrong receiver parameters. It is also shown that the key space of the system can be notably reduced easing a brute force attack. The system parameters were determined with high precision through the analysis of the decoding error produced by the mismatch between receiver and transmitter parameters.
nlin.CD
this paper studies the security of a chaotic cryptosystem based on the chua circuit and implemented with state controlled cellular neural networks it is shown that the plaintext can be retrieved by ciphertext bandpass filtering after an imperfect decoding with wrong receiver parameters it is also shown that the key space of the system can be notably reduced easing a brute force attack the system parameters were determined with high precision through the analysis of the decoding error produced by the mismatch between receiver and transmitter parameters
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706.298
Kinetics of cell division in epidermal maintenance
The rules governing cell division and differentiation are central to understanding the mechanisms of development, aging and cancer. By utilising inducible genetic labelling, recent studies have shown that the clonal population in transgenic mouse epidermis can be tracked in vivo. Drawing on these results, we explain how clonal fate data may be used to infer the rules of cell division and differentiation underlying the maintenance of adult murine tail-skin. We show that the rates of cell division and differentiation may be evaluated by considering the long-time and short-time clone fate data, and that the data is consistent with cells dividing independently rather than synchronously. Motivated by these findings, we consider a mechanism for cancer onset based closely on the model for normal adult skin. By analysing the expected changes to clonal fate in cancer emerging from a simple two-stage mutation, we propose that clonal fate data may provide a novel method for studying the earliest stages of the disease.
physics.bio-ph cond-mat.stat-mech q-bio.CB
the rules governing cell division and differentiation are central to understanding the mechanisms of development aging and cancer by utilising inducible genetic labelling recent studies have shown that the clonal population in transgenic mouse epidermis can be tracked in vivo drawing on these results we explain how clonal fate data may be used to infer the rules of cell division and differentiation underlying the maintenance of adult murine tailskin we show that the rates of cell division and differentiation may be evaluated by considering the longtime and shorttime clone fate data and that the data is consistent with cells dividing independently rather than synchronously motivated by these findings we consider a mechanism for cancer onset based closely on the model for normal adult skin by analysing the expected changes to clonal fate in cancer emerging from a simple twostage mutation we propose that clonal fate data may provide a novel method for studying the earliest stages of the disease
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706.2981
Moduli space of Brody curves, energy and mean dimension
We study the mean dimension of the moduli space of Brody curves. We introduce the notion of "mean energy" and show that this can be used to estimate the mean dimension.
math.DG math.CV
we study the mean dimension of the moduli space of brody curves we introduce the notion of mean energy and show that this can be used to estimate the mean dimension
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706.2982
Dimensional Reduction applied to QCD at higher orders
Recent developments in higher order calculations within the framework of Dimensional Reduction, the preferred regularization scheme for supersymmetric theories, are reported on. Special emphasis is put on the treatment of evanescent couplings, the equivalence to Dimensional Regularization, and the evaluation of $\alpha_s(M_GUT)$ from $\alpha_s(M_Z)$.
hep-ph
recent developments in higher order calculations within the framework of dimensional reduction the preferred regularization scheme for supersymmetric theories are reported on special emphasis is put on the treatment of evanescent couplings the equivalence to dimensional regularization and the evaluation of alpha_sm_gut from alpha_sm_z
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706.2983
Real Forms of Complex Higher Spin Field Equations and New Exact Solutions
We formulate four dimensional higher spin gauge theories in spacetimes with signature (4-p,p) and nonvanishing cosmological constant. Among them are chiral models in Euclidean (4,0) and Kleinian (2,2) signature involving half-flat gauge fields. Apart from the maximally symmetric solutions, including de Sitter spacetime, we find: (a) SO(4-p,p) invariant deformations, depending on a continuous and infinitely many discrete parameters, including a degenerate metric of rank one; (b) non-maximally symmetric solutions with vanishing Weyl tensors and higher spin gauge fields, that differ from the maximally symmetric solutions in the auxiliary field sector; and (c) solutions of the chiral models furnishing higher spin generalizations of Type D gravitational instantons, with an infinite tower of Weyl tensors proportional to totally symmetric products of two principal spinors. These are apparently the first exact 4D solutions with non-vanishing massless higher spin fields.
hep-th
we formulate four dimensional higher spin gauge theories in spacetimes with signature 4pp and nonvanishing cosmological constant among them are chiral models in euclidean 40 and kleinian 22 signature involving halfflat gauge fields apart from the maximally symmetric solutions including de sitter spacetime we find a so4pp invariant deformations depending on a continuous and infinitely many discrete parameters including a degenerate metric of rank one b nonmaximally symmetric solutions with vanishing weyl tensors and higher spin gauge fields that differ from the maximally symmetric solutions in the auxiliary field sector and c solutions of the chiral models furnishing higher spin generalizations of type d gravitational instantons with an infinite tower of weyl tensors proportional to totally symmetric products of two principal spinors these are apparently the first exact 4d solutions with nonvanishing massless higher spin fields
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706.2984
QED collinear radiation factors in the next-to-leading logarithmic approximation
The effect of the collinear photon radiation by charged particles is considered in the second order of the perturbation theory. Double and single photon radiation is evaluated. The corresponding radiation factors are obtained. The QED renormalization group approach is exploited in the next-to-leading order. The results are suited to perform a systematic treatment of the second order next-to-leading logarithmic radiative corrections to various processes either analytically or numerically.
hep-ph
the effect of the collinear photon radiation by charged particles is considered in the second order of the perturbation theory double and single photon radiation is evaluated the corresponding radiation factors are obtained the qed renormalization group approach is exploited in the nexttoleading order the results are suited to perform a systematic treatment of the second order nexttoleading logarithmic radiative corrections to various processes either analytically or numerically
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706.2985
Characterization of an asynchronous source of heralded single photons generated at a wavelength of 1550 nm
We make a thorough analysis of heralded single photon sources regarding how factors such as the detector gate-period, the photon rates, the fiber coupling efficiencies, and the system losses affect the performance of the source. In the course of this we give a detailed description of how to determine fiber coupling efficiencies from experimentally measurable quantities. We show that asynchronous sources perform, under most conditions, better than synchronous sources with respect to multiphoton events, but only for nearly perfect coupling efficiencies. We apply the theory to an asynchronous source of heralded single photons based on spontaneous parametric downconversion in a periodically poled, bulk, KTiOPO4 crystal. The source generates light with highly non-degenerate wavelengths of 810 nm and 1550 nm, where the 810 nm photons are used to announce the presence of the 1550 nm photons inside a single-mode optical fiber. For our setup we find the probability of having a 1550 nm photon present in the single-mode fiber, as announced by the 810 nm photon, to be 48%. The probability of multiphoton events is strongly suppressed compared to a Poissonian light source, giving highly sub-Poisson photon statistics.
quant-ph
we make a thorough analysis of heralded single photon sources regarding how factors such as the detector gateperiod the photon rates the fiber coupling efficiencies and the system losses affect the performance of the source in the course of this we give a detailed description of how to determine fiber coupling efficiencies from experimentally measurable quantities we show that asynchronous sources perform under most conditions better than synchronous sources with respect to multiphoton events but only for nearly perfect coupling efficiencies we apply the theory to an asynchronous source of heralded single photons based on spontaneous parametric downconversion in a periodically poled bulk ktiopo4 crystal the source generates light with highly nondegenerate wavelengths of 810 nm and 1550 nm where the 810 nm photons are used to announce the presence of the 1550 nm photons inside a singlemode optical fiber for our setup we find the probability of having a 1550 nm photon present in the singlemode fiber as announced by the 810 nm photon to be 48 the probability of multiphoton events is strongly suppressed compared to a poissonian light source giving highly subpoisson photon statistics
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706.2986
Dark Matter and Dark Energy
This is a short review, aimed at a general audience, of several current subjects of research in cosmology. The topics discussed include the cosmic microwave background (CMB), with particular emphasis on its relevance for testing inflation; dark matter, with a brief review of astrophysical evidence and more emphasis on particle candidates; and cosmic acceleration and some of the ideas that have been put forward to explain it. A glossary of technical terms and acronyms is provided.
astro-ph
this is a short review aimed at a general audience of several current subjects of research in cosmology the topics discussed include the cosmic microwave background cmb with particular emphasis on its relevance for testing inflation dark matter with a brief review of astrophysical evidence and more emphasis on particle candidates and cosmic acceleration and some of the ideas that have been put forward to explain it a glossary of technical terms and acronyms is provided
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706.2987
Explicit birational geometry of threefolds of general type
Let $V$ be a complex nonsingular projective 3-fold of general type. We prove $P_{12}(V)>0$ and $P_{24}(V)>1$ (which answers an open problem of J. Kollar and S. Mori). We also prove that the canonical volume has an universal lower bound $\text{Vol}(V) \geq 1/2660$ and that the pluri-canonical map $\Phi_m$ is birational onto its image for all $m\geq 77$. As an application of our method, we prove Fletcher's conjecture on weighted hyper-surface 3-folds with terminal quotient singularities. Another featured result is the optimal lower bound $\text{Vol}(V)\geq {1/420}$ among all those 3-folds $V$ with $\chi({\mathcal O}_V)\leq 1$.
math.AG
let v be a complex nonsingular projective 3fold of general type we prove p_12v0 and p_24v1 which answers an open problem of j kollar and s mori we also prove that the canonical volume has an universal lower bound textvolv geq 12660 and that the pluricanonical map phi_m is birational onto its image for all mgeq 77 as an application of our method we prove fletchers conjecture on weighted hypersurface 3folds with terminal quotient singularities another featured result is the optimal lower bound textvolvgeq 1420 among all those 3folds v with chimathcal o_vleq 1
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706.2988
Parton distribution functions and quark orbital motion
Covariant version of the quark-parton model is studied. Dependence of the structure functions and parton distributions on the 3D quark intrinsic motion is discussed. The important role of the quark orbital momentum, which is a particular case of intrinsic motion, appears as a direct consequence of the covariant description. Effect of orbital motion is substantial especially for polarized structure functions. At the same time, the procedure for obtaining the quark momentum distributions of polarized quarks from the combination of polarized and unpolarized structure functions is suggested.
hep-ph
covariant version of the quarkparton model is studied dependence of the structure functions and parton distributions on the 3d quark intrinsic motion is discussed the important role of the quark orbital momentum which is a particular case of intrinsic motion appears as a direct consequence of the covariant description effect of orbital motion is substantial especially for polarized structure functions at the same time the procedure for obtaining the quark momentum distributions of polarized quarks from the combination of polarized and unpolarized structure functions is suggested
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706.2989
Low-energy Dipole Excitations in Nuclei at the N=50,82 and Z=50 Shell Closures as Signatures for a Neutron Skin
Low-energy dipole excitations have been investigated theoretically in N=50, several N=82 isotones and the Z=50 Sn isotopes. For this purpose a method incorporating both HFB and multi-phonon QPM theory is applied. A concentration of one-phonon dipole strength located below the neutron emission threshold has been calculated in these nuclei. The analysis of the corresponding neutron and proton dipole transition densities allows to assign a genuine pattern to the low-energy excitations and making them distinct from the conventional GDR modes. Analyzing also the QRPA wave functions of the states we can identify these excitations as Pygmy Dipole Resonance (PDR) modes, recently studied also in Sn and N=82 nuclei. The results for N=50 are exploratory for an experimental project designed for the bremsstrahlung facility at the ELBE accelerator.
nucl-th
lowenergy dipole excitations have been investigated theoretically in n50 several n82 isotones and the z50 sn isotopes for this purpose a method incorporating both hfb and multiphonon qpm theory is applied a concentration of onephonon dipole strength located below the neutron emission threshold has been calculated in these nuclei the analysis of the corresponding neutron and proton dipole transition densities allows to assign a genuine pattern to the lowenergy excitations and making them distinct from the conventional gdr modes analyzing also the qrpa wave functions of the states we can identify these excitations as pygmy dipole resonance pdr modes recently studied also in sn and n82 nuclei the results for n50 are exploratory for an experimental project designed for the bremsstrahlung facility at the elbe accelerator
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706.299
QCD dynamics at low x in ep collisions at HERA
Forward jet and multijet production has been measured at low Bjorken x at HERA. The measured cross sections and correlations were compared to predictions from DGLAP-based fixed-order calculations. Further comparisons were made to DGLAP-based and CCFM-based leading-order Monte Carlo predictions, as well as to Colour-Dipole model predictions. For the majority of the phase space covered in the HERA kinematic region, fixed-order calculations describe the data well, while the leading-order models provide an inconsistent description of the data.
hep-ex
forward jet and multijet production has been measured at low bjorken x at hera the measured cross sections and correlations were compared to predictions from dglapbased fixedorder calculations further comparisons were made to dglapbased and ccfmbased leadingorder monte carlo predictions as well as to colourdipole model predictions for the majority of the phase space covered in the hera kinematic region fixedorder calculations describe the data well while the leadingorder models provide an inconsistent description of the data
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706.2991
Wave propagation in axion electrodynamics
In this paper, the axion contribution to the electromagnetic wave propagation is studied. First we show how the axion electrodynamics model can be embedded into a premetric formalism of Maxwell electrodynamics. In this formalism, the axion field is not an arbitrary added Chern-Simon term of the Lagrangian, but emerges in a natural way as an irreducible part of a general constitutive tensor.We show that in order to represent the axion contribution to the wave propagation it is necessary to go beyond the geometric approximation, which is usually used in the premetric formalism. We derive a covariant dispersion relation for the axion modified electrodynamics. The wave propagation in this model is studied for an axion field with timelike, spacelike and null derivative covectors. The birefringence effect emerges in all these classes as a signal of Lorentz violation. This effect is however completely different from the ordinary birefringence appearing in classical optics and in premetric electrodynamics. The axion field does not simple double the ordinary light cone structure. In fact, it modifies the global topological structure of light cones surfaces. In CFJ-electrodynamics, such a modification results in violation of causality. In addition, the optical metrics in axion electrodynamics are not pseudo-Riemannian. In fact, for all types of the axion field, they are even non-Finslerian.
hep-th
in this paper the axion contribution to the electromagnetic wave propagation is studied first we show how the axion electrodynamics model can be embedded into a premetric formalism of maxwell electrodynamics in this formalism the axion field is not an arbitrary added chernsimon term of the lagrangian but emerges in a natural way as an irreducible part of a general constitutive tensorwe show that in order to represent the axion contribution to the wave propagation it is necessary to go beyond the geometric approximation which is usually used in the premetric formalism we derive a covariant dispersion relation for the axion modified electrodynamics the wave propagation in this model is studied for an axion field with timelike spacelike and null derivative covectors the birefringence effect emerges in all these classes as a signal of lorentz violation this effect is however completely different from the ordinary birefringence appearing in classical optics and in premetric electrodynamics the axion field does not simple double the ordinary light cone structure in fact it modifies the global topological structure of light cones surfaces in cfjelectrodynamics such a modification results in violation of causality in addition the optical metrics in axion electrodynamics are not pseudoriemannian in fact for all types of the axion field they are even nonfinslerian
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706.2992
Strong Lensing Analysis of the Cluster RCS0224-0002 at $z=0.77$
We present a detailed mass reconstruction of the cluster RCS0224-0002 at $z=0.773$ from the strong lensing features observed with HST/WFPC2. The mass profile is reconstructed using a parametric approach. We introduce a novel method to fit extended multiple images based on the Modified Hausdorff Distance between observed arcs and the arcs reproduced by the model. We perform the detailed error analysis of the model parameter using the MCMC method. Our model reproduces all the observed strong lensing features of the RCS0224-0002 and predicts the redshift of one of the arcs systems to be $z\approx 2.65$ (the other system has an spectroscopic redshift of $z=4.87$). The reconstructed inner mass profile is well fitted by a non-singular isothermal sphere, rather than with an NFW model. Dark matter substructure, derived from the light distribution of the most luminous cluster members, is crucial for reproducing the complexity of the quadrupole image system, which could not be achieved otherwise. The reconstructed mass distribution closely follows the light, however it is significantly shifted from the X-ray emission of the gas. The mass of RCS0224-0002 derived from the lensing model, $\approx 2\times10^{14} M_\odot$ is in a very good agreement with the one obtained from the X-ray temperature measured with deep Chandra observations.
astro-ph
we present a detailed mass reconstruction of the cluster rcs02240002 at z0773 from the strong lensing features observed with hstwfpc2 the mass profile is reconstructed using a parametric approach we introduce a novel method to fit extended multiple images based on the modified hausdorff distance between observed arcs and the arcs reproduced by the model we perform the detailed error analysis of the model parameter using the mcmc method our model reproduces all the observed strong lensing features of the rcs02240002 and predicts the redshift of one of the arcs systems to be zapprox 265 the other system has an spectroscopic redshift of z487 the reconstructed inner mass profile is well fitted by a nonsingular isothermal sphere rather than with an nfw model dark matter substructure derived from the light distribution of the most luminous cluster members is crucial for reproducing the complexity of the quadrupole image system which could not be achieved otherwise the reconstructed mass distribution closely follows the light however it is significantly shifted from the xray emission of the gas the mass of rcs02240002 derived from the lensing model approx 2times1014 m_odot is in a very good agreement with the one obtained from the xray temperature measured with deep chandra observations
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706.2993
Sensitivity of the NEMO detector to galactic microquasars
We present the results of Monte Carlo simulation studies of the capability of the proposed NEMO km$^3$ telescope to detect TeV muon neutrinos from Galactic microquasars. In particular we determined the detector sensitivity to each known microquasar, optimizing the event selection in order to reject the atmospheric background. We also determined the expected number of source and background events surviving the selection.
astro-ph
we present the results of monte carlo simulation studies of the capability of the proposed nemo km3 telescope to detect tev muon neutrinos from galactic microquasars in particular we determined the detector sensitivity to each known microquasar optimizing the event selection in order to reject the atmospheric background we also determined the expected number of source and background events surviving the selection
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706.2994
The cluster galaxy luminosity function at $z=0.3$: a recent origin for the faint-end upturn ?
We derive deep luminosity functions (to $M_z=-15$) for galaxies in Abell 1835 ($z=0.25$) and AC 114 ($z=0.31$) and compare these with the local $z'$ luminosity function for 69 clusters. The data show that the faint-end upturn, the excess of galaxies above a single Schechter function at $M_z < -17$, does not exist in the higher redshift clusters. This suggests that the faint-end upturn galaxies have been created recently, by infall into clusters of star-forming field populations or via tidal disruption of brighter objects.^M
astro-ph
we derive deep luminosity functions to m_z15 for galaxies in abell 1835 z025 and ac 114 z031 and compare these with the local z luminosity function for 69 clusters the data show that the faintend upturn the excess of galaxies above a single schechter function at m_z 17 does not exist in the higher redshift clusters this suggests that the faintend upturn galaxies have been created recently by infall into clusters of starforming field populations or via tidal disruption of brighter objectsm
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706.2995
Injectivity and Projectivity in Analysis and Topology
We give new proofs for many injectivity results in analysis that make more careful use of the duality between unital abelian C*-algebras and compact Hausdorff spaces. We then extend many of these results to incorporate group actions. Our approach uses only elementary topological constructions and eliminates the need for results from the theory of Boolean algebras and AW*-algebras that were used in earlier proofs.
math.OA
we give new proofs for many injectivity results in analysis that make more careful use of the duality between unital abelian calgebras and compact hausdorff spaces we then extend many of these results to incorporate group actions our approach uses only elementary topological constructions and eliminates the need for results from the theory of boolean algebras and awalgebras that were used in earlier proofs
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706.2996
The forgotten monoid
We study properties of the forgotten monoid which appeared in work of Lascoux and Schutzenberger and recently resurfaced in the construction of dual equivalence graphs by Assaf. In particular, we provide an explicit characterization of the forgotten classes in terms of inversion numbers and show that there are n^2-3n+4 forgotten classes in the symmetric group S_n. Each forgotten class contains a canonical element that can be characterized by pattern avoidance. We also show that the sum of Gessel's quasi-symmetric functions over a forgotten class is a 0-1 sum of ribbon-Schur functions.
math.CO
we study properties of the forgotten monoid which appeared in work of lascoux and schutzenberger and recently resurfaced in the construction of dual equivalence graphs by assaf in particular we provide an explicit characterization of the forgotten classes in terms of inversion numbers and show that there are n23n4 forgotten classes in the symmetric group s_n each forgotten class contains a canonical element that can be characterized by pattern avoidance we also show that the sum of gessels quasisymmetric functions over a forgotten class is a 01 sum of ribbonschur functions
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706.2997
Constraining the Two-Higgs-Doublet-Model parameter space
We confront the Two-Higgs-Doublet Model with a variety of experimental constraints as well as theoretical consistency conditions. The most constraining data are the \bar B\to X_s\gamma decay rate (at low values of M_{H^\pm}), and \Delta\rho (at both low and high M_{H^\pm}). We also take into account the B\bar B oscillation rate and R_b, or the width \Gamma(Z\to b\bar b) (both of which restrict the model at low values of \tan\beta), and the B^-\to\tau\nu_\tau decay rate, which restricts the model at high \tan\beta and low M_{H^\pm}. Furthermore, the LEP2 non-discovery of a light, neutral Higgs boson is considered, as well as the muon anomalous magnetic moment. Since perturbative unitarity excludes high values of \tan\beta, the model turns out to be very constrained. We outline the remaining allowed regions in the \tan\beta-M_{H^\pm} plane for different values of the masses of the two lightest neutral Higgs bosons, and describe some of their properties.
hep-ph
we confront the twohiggsdoublet model with a variety of experimental constraints as well as theoretical consistency conditions the most constraining data are the bar bto x_sgamma decay rate at low values of m_hpm and deltarho at both low and high m_hpm we also take into account the bbar b oscillation rate and r_b or the width gammazto bbar b both of which restrict the model at low values of tanbeta and the btotaunu_tau decay rate which restricts the model at high tanbeta and low m_hpm furthermore the lep2 nondiscovery of a light neutral higgs boson is considered as well as the muon anomalous magnetic moment since perturbative unitarity excludes high values of tanbeta the model turns out to be very constrained we outline the remaining allowed regions in the tanbetam_hpm plane for different values of the masses of the two lightest neutral higgs bosons and describe some of their properties
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706.2998
Conformal oxide coating of Carbon Nanotubes
The International Roadmap for Ferroelectric Memories requires three-dimensional integration of high-dielectric materials onto metal interconnects or bottom electrodes by 2010. We report the first integration of high-dielectric oxide films onto carbon nanotube electrodes with an aim of ultra-high integration density of FeRAMs (Tb/in2).
cond-mat.mtrl-sci
the international roadmap for ferroelectric memories requires threedimensional integration of highdielectric materials onto metal interconnects or bottom electrodes by 2010 we report the first integration of highdielectric oxide films onto carbon nanotube electrodes with an aim of ultrahigh integration density of ferams tbin2
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706.2999
Searches in Photon and Jet States
We present recent results from the Collider Detector at Fermilab (CDF) and D0 experiments using data from proton-antiproton collisions with sqrt(s) = 1.96 TeV at Run II of the Fermilab Tevatron. New physics may appear in events with high transverse momentum objects, including photons and quark or gluon jets. The results described here are of signature-based searches and model-based searches probing supersymmetry, leptoquarks, 4th generation quarks, and large extra dimensions.
hep-ex
we present recent results from the collider detector at fermilab cdf and d0 experiments using data from protonantiproton collisions with sqrts 196 tev at run ii of the fermilab tevatron new physics may appear in events with high transverse momentum objects including photons and quark or gluon jets the results described here are of signaturebased searches and modelbased searches probing supersymmetry leptoquarks 4th generation quarks and large extra dimensions
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706.3
Discovery of diffuse radio emission at the center of the most X-ray-luminous cluster RX J1347.5-1145
We report on new VLA radio observations of the distant cluster RX J1347.5-1145, which is the most luminous in X-rays. We aim at investigating the possible presence of diffuse and extended radio emission in this very peculiar system which shows both a massive cooling flow and merging signatures. New low resolution (~18 arcsec) VLA radio observations of this cluster are combined with higher resolution (~2 arcsec) data available in the VLA archive. We discover the presence of a diffuse and extended (~500 kpc) radio source centered on the cluster, unrelated to the radio emission of the central AGN. The properties of the radio source, in particular a) its occurrence at the center of a massive cooling flow cluster, b) its total size comparable to that of the cooling region, c) its agreement with the observational trend between radio luminosity and cooling flow power, indicate that RX J1347.5-1145 hosts a radio mini-halo. We suggest that the radio emission of this mini-halo, which is the most distant object of its class discovered up to now, is due to electron re-acceleration triggered by the central cooling flow. However, we also note that the morphology of the diffuse radio emission shows an elongation coincident with the position of a hot subclump detected in X-rays, thus suggesting that additional energy for the electron re-acceleration might be provided by the submerger event.
astro-ph
we report on new vla radio observations of the distant cluster rx j134751145 which is the most luminous in xrays we aim at investigating the possible presence of diffuse and extended radio emission in this very peculiar system which shows both a massive cooling flow and merging signatures new low resolution 18 arcsec vla radio observations of this cluster are combined with higher resolution 2 arcsec data available in the vla archive we discover the presence of a diffuse and extended 500 kpc radio source centered on the cluster unrelated to the radio emission of the central agn the properties of the radio source in particular a its occurrence at the center of a massive cooling flow cluster b its total size comparable to that of the cooling region c its agreement with the observational trend between radio luminosity and cooling flow power indicate that rx j134751145 hosts a radio minihalo we suggest that the radio emission of this minihalo which is the most distant object of its class discovered up to now is due to electron reacceleration triggered by the central cooling flow however we also note that the morphology of the diffuse radio emission shows an elongation coincident with the position of a hot subclump detected in xrays thus suggesting that additional energy for the electron reacceleration might be provided by the submerger event
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706.3001
Mass distribution in the most X-ray-luminous galaxy cluster RX J1347.5-1145 studied with XMM-Newton
We report on the analysis of XMM-Newton observations of RX J1347.5-1145 (z=0.451), the most X-ray-luminous galaxy cluster. We present a detailed total and gas mass determination up to large distances (~1.7 Mpc), study the scaling properties of the cluster, and explore the role of AGN heating in the cluster cool core. By means of spatially resolved spectroscopy we derive density, temperature, entropy, and cooling time profiles of the intra-cluster medium. We compute the total mass profile of the cluster in the assumption of hydrostatic equilibrium. If the disturbed south-east region of the cluster is excluded from the analysis, our results on shape, normalization, scaling properties of density, temperature, entropy, and cooling time profiles are fully consistent with those of relaxed, cool core clusters. We compare our total and gas mass estimates with previous X-ray, lensing, dynamical, and SZ studies. We find good agreement with other X-ray results, dynamical mass measurements, weak lensing masses and SZ results. We confirm a discrepancy of a factor ~2 between strong lensing and X-ray mass determinations and find a gross mismatch between our total mass estimate and the mass reconstructed through the combination of both strong and weak lensing. We explore the effervescent heating scenario in the core of RX J1347.5-1145 and find support to the picture that AGN outflows and heat conduction are able to quenching radiative cooling.
astro-ph
we report on the analysis of xmmnewton observations of rx j134751145 z0451 the most xrayluminous galaxy cluster we present a detailed total and gas mass determination up to large distances 17 mpc study the scaling properties of the cluster and explore the role of agn heating in the cluster cool core by means of spatially resolved spectroscopy we derive density temperature entropy and cooling time profiles of the intracluster medium we compute the total mass profile of the cluster in the assumption of hydrostatic equilibrium if the disturbed southeast region of the cluster is excluded from the analysis our results on shape normalization scaling properties of density temperature entropy and cooling time profiles are fully consistent with those of relaxed cool core clusters we compare our total and gas mass estimates with previous xray lensing dynamical and sz studies we find good agreement with other xray results dynamical mass measurements weak lensing masses and sz results we confirm a discrepancy of a factor 2 between strong lensing and xray mass determinations and find a gross mismatch between our total mass estimate and the mass reconstructed through the combination of both strong and weak lensing we explore the effervescent heating scenario in the core of rx j134751145 and find support to the picture that agn outflows and heat conduction are able to quenching radiative cooling
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706.3002
Potential energy curves and transition moments for the excimer states 0u+ (3P1) and 1u (3P2) of Ar2
Exactly solvable rererence potentials of several smoothly joined Morse-type components were constructed for the lowest two excimer states of Ar2 molecule. The parameters of the potentials have been ascertained by fitting to the experimental data, and they are reliable in a wide range of nuclear separations. A large number of quantum mechanical Franck-Condon factors for bound-free and bound-bound transitions have been calculated and compared with the observed spectroscopic features. The fitting procedure also involved dipole transition moments, which have been adjusted to the known radiative lifetimes of the vibrational levels. The resulting potential energy curves accurately reproduce the first and the second emission continua of Ar2* as well as the oscillatory spectrum related to their inner turning point region. The numbering and the positions of the vibrational levels reported by Herman et al. [P. R. Herman, P. E. LaRocque, and B. P. Stoicheff, J. Chem. Phys. 89, 4535 (1988)] have been confirmed.
physics.chem-ph
exactly solvable rererence potentials of several smoothly joined morsetype components were constructed for the lowest two excimer states of ar2 molecule the parameters of the potentials have been ascertained by fitting to the experimental data and they are reliable in a wide range of nuclear separations a large number of quantum mechanical franckcondon factors for boundfree and boundbound transitions have been calculated and compared with the observed spectroscopic features the fitting procedure also involved dipole transition moments which have been adjusted to the known radiative lifetimes of the vibrational levels the resulting potential energy curves accurately reproduce the first and the second emission continua of ar2 as well as the oscillatory spectrum related to their inner turning point region the numbering and the positions of the vibrational levels reported by herman et al p r herman p e larocque and b p stoicheff j chem phys 89 4535 1988 have been confirmed
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706.3003
Connections between real polynomial solutions of hypergeometric-type differential equations with Rodrigues formula
Starting from the Rodrigues representation of polynomial solutions of the general hypergeometric-type differential equation complementary polynomials are constructed using a natural method. Among the key results is a generating function in closed form leading to short and transparent derivations of recursion relations and an addition theorem. The complementary polynomials satisfy a hypergeometric-type differential equation themselves, have a three-term recursion among others and obey Rodrigues formulas. Applications to the classical polynomials are given.
math.CA
starting from the rodrigues representation of polynomial solutions of the general hypergeometrictype differential equation complementary polynomials are constructed using a natural method among the key results is a generating function in closed form leading to short and transparent derivations of recursion relations and an addition theorem the complementary polynomials satisfy a hypergeometrictype differential equation themselves have a threeterm recursion among others and obey rodrigues formulas applications to the classical polynomials are given
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706.3004
Strong extinction of a far-field laser beam by a single quantum dot
Through the utilization of index-matched GaAs immersion lens techniques we demonstrate a record extinction (12%) of a far-field focused laser by a single InAs/GaAs quantum dot. This contrast level enables us to report for the first time resonant laser transmission spectroscopy on a single InAs/GaAs quantum dot without the need for phase-sensitive lock-in detection.
cond-mat.other cond-mat.mes-hall quant-ph
through the utilization of indexmatched gaas immersion lens techniques we demonstrate a record extinction 12 of a farfield focused laser by a single inasgaas quantum dot this contrast level enables us to report for the first time resonant laser transmission spectroscopy on a single inasgaas quantum dot without the need for phasesensitive lockin detection
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706.3005
Two Stellar Components in the Halo of the Milky Way
The halo of the Milky Way provides unique elemental abundance and kinematic information on the first objects to form in the Universe, which can be used to tightly constrain models of galaxy formation and evolution. Although the halo was once considered a single component, evidence for its dichotomy has slowly emerged in recent years from inspection of small samples of halo objects. Here we show that the halo is indeed clearly divisible into two broadly overlapping structural components -- an inner and an outer halo -- that exhibit different spatial density profiles, stellar orbits and stellar metallicities (abundances of elements heavier than helium). The inner halo has a modest net prograde rotation, whereas the outer halo exhibits a net retrograde rotation and a peak metallicity one-third that of the inner halo. These properties indicate that the individual halo components probably formed in fundamentally different ways, through successive dissipational (inner) and dissipationless (outer) mergers and tidal disruption of proto-Galactic clumps.
astro-ph
the halo of the milky way provides unique elemental abundance and kinematic information on the first objects to form in the universe which can be used to tightly constrain models of galaxy formation and evolution although the halo was once considered a single component evidence for its dichotomy has slowly emerged in recent years from inspection of small samples of halo objects here we show that the halo is indeed clearly divisible into two broadly overlapping structural components an inner and an outer halo that exhibit different spatial density profiles stellar orbits and stellar metallicities abundances of elements heavier than helium the inner halo has a modest net prograde rotation whereas the outer halo exhibits a net retrograde rotation and a peak metallicity onethird that of the inner halo these properties indicate that the individual halo components probably formed in fundamentally different ways through successive dissipational inner and dissipationless outer mergers and tidal disruption of protogalactic clumps
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706.3006
Recollement of Deformed Preprojective Algebras and the Calogero-Moser Correspondence
The aim of this paper is to clarify the relation between the following objects: $ (a) $ rank 1 projective modules (ideals) over the first Weyl algebra $ A_1(\C)$; $ (b) $ simple modules over deformed preprojective algebras $ \Pi_{\lambda}(Q) $ introduced by Crawley-Boevey and Holland; and $ (c) $ simple modules over the rational Cherednik algebras $ H_{0,c}(S_n) $ associated to symmetric groups. The isomorphism classes of each type of these objects can be parametrized geometrically by the same space (namely, the Calogero-Moser algebraic varieties); however, no natural functors between the corresponding module categories seem to be known. We construct such functors by translating our earlier results on $\A$-modules over $ A_1 $ to a more familiar setting of representation theory. In the last section we extend our construction to the case of Kleinian singularities $ \C^2/\Gamma $, where $ \Gamma $ is a finite cyclic subgroup of $ \SL(2, \C) $.
math.RT math.QA
the aim of this paper is to clarify the relation between the following objects a rank 1 projective modules ideals over the first weyl algebra a_1c b simple modules over deformed preprojective algebras pi_lambdaq introduced by crawleyboevey and holland and c simple modules over the rational cherednik algebras h_0cs_n associated to symmetric groups the isomorphism classes of each type of these objects can be parametrized geometrically by the same space namely the calogeromoser algebraic varieties however no natural functors between the corresponding module categories seem to be known we construct such functors by translating our earlier results on amodules over a_1 to a more familiar setting of representation theory in the last section we extend our construction to the case of kleinian singularities c2gamma where gamma is a finite cyclic subgroup of sl2 c
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706.3007
Relations among Supersymmetric Lattice Gauge Theories via Orbifolding
We show how to derive Catterall's supersymmetric lattice gauge theories directly from the general principle of orbifolding followed by a variant of the usual deconstruction. These theories are forced to be complexified due to a clash between charge assignments under U(1)-symmetries and lattice assignments in terms of scalar, vector and tensor components for the fermions. Other prescriptions for how to discretize the theory follow automatically by orbifolding and deconstruction. We find that Catterall's complexified model for the two-dimensional N=(2,2) theory has two independent preserved supersymmetries. We comment on consistent truncations to lattice theories without this complexification and with the correct continuum limit. The construction of lattice theories this way is general, and can be used to derive new supersymmetric lattice theories through the orbifolding procedure. As an example, we apply the prescription to topologically twisted four-dimensional N=2 supersymmetric Yang-Mills theory. We show that a consistent truncation is closely related to the lattice formulation previously given by Sugino.
hep-lat hep-th
we show how to derive catteralls supersymmetric lattice gauge theories directly from the general principle of orbifolding followed by a variant of the usual deconstruction these theories are forced to be complexified due to a clash between charge assignments under u1symmetries and lattice assignments in terms of scalar vector and tensor components for the fermions other prescriptions for how to discretize the theory follow automatically by orbifolding and deconstruction we find that catteralls complexified model for the twodimensional n22 theory has two independent preserved supersymmetries we comment on consistent truncations to lattice theories without this complexification and with the correct continuum limit the construction of lattice theories this way is general and can be used to derive new supersymmetric lattice theories through the orbifolding procedure as an example we apply the prescription to topologically twisted fourdimensional n2 supersymmetric yangmills theory we show that a consistent truncation is closely related to the lattice formulation previously given by sugino
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706.3008
A Generic Deployment Framework for Grid Computing and Distributed Applications
Deployment of distributed applications on large systems, and especially on grid infrastructures, becomes a more and more complex task. Grid users spend a lot of time to prepare, install and configure middleware and application binaries on nodes, and eventually start their applications. The problem is that the deployment process is composed of many heterogeneous tasks that have to be orchestrated in a specific correct order. As a consequence, the automatization of the deployment process is currently very difficult to reach. To address this problem, we propose in this paper a generic deployment framework allowing to automatize the execution of heterogeneous tasks composing the whole deployment process. Our approach is based on a reification as software components of all required deployment mechanisms or existing tools. Grid users only have to describe the configuration to deploy in a simple natural language instead of programming or scripting how the deployment process is executed. As a toy example, this framework is used to deploy CORBA component-based applications and OpenCCM middleware on one thousand nodes of the French Grid5000 infrastructure.
cs.DC
deployment of distributed applications on large systems and especially on grid infrastructures becomes a more and more complex task grid users spend a lot of time to prepare install and configure middleware and application binaries on nodes and eventually start their applications the problem is that the deployment process is composed of many heterogeneous tasks that have to be orchestrated in a specific correct order as a consequence the automatization of the deployment process is currently very difficult to reach to address this problem we propose in this paper a generic deployment framework allowing to automatize the execution of heterogeneous tasks composing the whole deployment process our approach is based on a reification as software components of all required deployment mechanisms or existing tools grid users only have to describe the configuration to deploy in a simple natural language instead of programming or scripting how the deployment process is executed as a toy example this framework is used to deploy corba componentbased applications and openccm middleware on one thousand nodes of the french grid5000 infrastructure
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706.3009
Application of a design space exploration tool to enhance interleaver generation
This paper presents a methodology to efficiently explore the design space of communication adapters. In most digital signal processing (DSP) applications, the overall performance of the system is significantly affected by communication architectures, as a consequence the designers need specifically optimized adapters. By explicitly modeling these communications within an effective graph-theoretic model and analysis framework, we automatically generate an optimized architecture, named Space-Time AdapteR (STAR). Our design flow inputs a C description of Input/Output data scheduling, and user requirements (throughput, latency, parallelism...), and formalizes communication constraints through a Resource Constraints Graph (RCG). Design space exploration is then performed through associated tools, to synthesize a STAR component under time-to-market constraints. The proposed approach has been tested to design an industrial data mixing block example: an Ultra-Wideband interleaver.
cs.AR cs.IT math.IT
this paper presents a methodology to efficiently explore the design space of communication adapters in most digital signal processing dsp applications the overall performance of the system is significantly affected by communication architectures as a consequence the designers need specifically optimized adapters by explicitly modeling these communications within an effective graphtheoretic model and analysis framework we automatically generate an optimized architecture named spacetime adapter star our design flow inputs a c description of inputoutput data scheduling and user requirements throughput latency parallelism and formalizes communication constraints through a resource constraints graph rcg design space exploration is then performed through associated tools to synthesize a star component under timetomarket constraints the proposed approach has been tested to design an industrial data mixing block example an ultrawideband interleaver
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706.301
Quasi-invariance properties of a class of subordinators
We study absolute-continuity properties of a class of stochastic processes, including the gamma and the Dirichlet processes. We prove that the laws of a general class of non-linear transformations of such processes are locally equivalent to the law of the original process and we compute explicitly the associated Radon-Nikodym densities. This work unifies and generalizes to random non-linear transformations several previous results on quasi-invariance of gamma and Dirichlet processes.
math.PR
we study absolutecontinuity properties of a class of stochastic processes including the gamma and the dirichlet processes we prove that the laws of a general class of nonlinear transformations of such processes are locally equivalent to the law of the original process and we compute explicitly the associated radonnikodym densities this work unifies and generalizes to random nonlinear transformations several previous results on quasiinvariance of gamma and dirichlet processes
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706.3011
Axial Nucleon and Nucleon to Delta form fractors and the Goldberger-Treiman Relations from Lattice QCD
We evaluate the nucleon axial form factor, $G_A(q^2)$, and induced pseudoscalar form factor, $G_p(q^2)$, as well as the pion-nucleon form factor, $G_{\pi N N}(q^2)$, in lattice QCD. We also evaluate the corresponding nucleon to $\Delta$ transition form factors, $C_5^A(q^2)$ and $C_6^A(q^2)$, and the pion-nucleon-$\Delta$ form factor $G_{\pi N\Delta}(q^2)$. The nucleon form factors are evaluated in the quenched theory and with two degenerate flavors of dynamical Wilson fermions. The nucleon to $\Delta$ form factors, besides Wilson fermions, are evaluated using domain wall valence fermions with staggered sea quark configurations for pion masses as low as about 350 MeV. Using these form factors, together with an evaluation of the renormalized quark mass, we investigate the validity of the diagonal and non-diagonal Goldberger-Treiman relations. The ratios $G_{\pi N\Delta}(q^2)/G_{\pi NN}(q^2)$ and $2C_5^A(q^2)/G_A(q^2)$ are constant as a function of the momentum transfer squared and show almost no dependence on the quark mass. We confirm equality of these two ratios consistent with the Goldberger-Treiman relations extracting a mean value of $1.61(2)$.
hep-lat
we evaluate the nucleon axial form factor g_aq2 and induced pseudoscalar form factor g_pq2 as well as the pionnucleon form factor g_pi n nq2 in lattice qcd we also evaluate the corresponding nucleon to delta transition form factors c_5aq2 and c_6aq2 and the pionnucleondelta form factor g_pi ndeltaq2 the nucleon form factors are evaluated in the quenched theory and with two degenerate flavors of dynamical wilson fermions the nucleon to delta form factors besides wilson fermions are evaluated using domain wall valence fermions with staggered sea quark configurations for pion masses as low as about 350 mev using these form factors together with an evaluation of the renormalized quark mass we investigate the validity of the diagonal and nondiagonal goldbergertreiman relations the ratios g_pi ndeltaq2g_pi nnq2 and 2c_5aq2g_aq2 are constant as a function of the momentum transfer squared and show almost no dependence on the quark mass we confirm equality of these two ratios consistent with the goldbergertreiman relations extracting a mean value of 1612
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706.3012
Unbound exotic nuclei studied by projectile fragmentation
We call "projectile fragmentation" of neutron halo nuclei the elastic breakup (diffraction) reaction, when the observable studied is the neutron-core relative energy spectrum. This observable has been measured in relation to the Coulomb breakup on heavy target and recently also on light targets. Such data enlighten the effect of the neutron final state interaction with the core of origin. Projectile fragmentation is studied here by a time dependent model for the excitation of a nucleon from a bound state to a continuum resonant state in a neutron-core complex potential which acts as a final state interaction. The final state is described by an optical model S-matrix so that both resonant and non resonant states of any continuum energy can be studied as well as deeply bound initial states. It turns out that due to the coupling between the initial and final states, the neutron-core free particle phase shifts are modified, in the exit channel, by an additional phase. Some typical numerical calculations for the relevant observables are presented and compared to experimental data. It is suggest that the excitation energy spectra of an unbound nucleus might reflect the structure of the parent nucleus from whose fragmentation they are obtained.
nucl-th
we call projectile fragmentation of neutron halo nuclei the elastic breakup diffraction reaction when the observable studied is the neutroncore relative energy spectrum this observable has been measured in relation to the coulomb breakup on heavy target and recently also on light targets such data enlighten the effect of the neutron final state interaction with the core of origin projectile fragmentation is studied here by a time dependent model for the excitation of a nucleon from a bound state to a continuum resonant state in a neutroncore complex potential which acts as a final state interaction the final state is described by an optical model smatrix so that both resonant and non resonant states of any continuum energy can be studied as well as deeply bound initial states it turns out that due to the coupling between the initial and final states the neutroncore free particle phase shifts are modified in the exit channel by an additional phase some typical numerical calculations for the relevant observables are presented and compared to experimental data it is suggest that the excitation energy spectra of an unbound nucleus might reflect the structure of the parent nucleus from whose fragmentation they are obtained
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706.3013
Oscillation regimes of a solid-state ring laser with active beat note stabilization : from a chaotic device to a ring laser gyroscope
We report experimental and theoretical study of a rotating diode-pumped Nd-YAG ring laser with active beat note stabilization. Our experimental setup is described in the usual Maxwell-Bloch formalism. We analytically derive a stability condition and some frequency response characteristics for the solid-state ring laser gyroscope, illustrating the important role of mode coupling effects on the dynamics of such a device. Experimental data are presented and compared with the theory on the basis of realistic laser parameters, showing a very good agreement. Our results illustrate the duality between the very rich non linear dynamics of the diode-pumped solid-state ring laser (including chaotic behavior) and the possibility to obtain a very stable beat note, resulting in a potentially new kind of rotation sensor.
physics.optics
we report experimental and theoretical study of a rotating diodepumped ndyag ring laser with active beat note stabilization our experimental setup is described in the usual maxwellbloch formalism we analytically derive a stability condition and some frequency response characteristics for the solidstate ring laser gyroscope illustrating the important role of mode coupling effects on the dynamics of such a device experimental data are presented and compared with the theory on the basis of realistic laser parameters showing a very good agreement our results illustrate the duality between the very rich non linear dynamics of the diodepumped solidstate ring laser including chaotic behavior and the possibility to obtain a very stable beat note resulting in a potentially new kind of rotation sensor
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