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707.423
The Role of Electron-electron Interactions in Graphene ARPES Spectra
We report on a theoretical study of the influence of electron-electron interactions on ARPES spectra in graphene that is based on the random-phase-approximation and on graphene's massless Dirac equation continuum model. We find that level repulsion between quasiparticle and plasmaron resonances gives rise to a gap-like feature at small k. ARPES spectra are sensitive to the electron-electron interaction coupling strength $\alpha_{\rm gr}$ and might enable an experimental determination of this material parameter.
cond-mat.mes-hall
we report on a theoretical study of the influence of electronelectron interactions on arpes spectra in graphene that is based on the randomphaseapproximation and on graphenes massless dirac equation continuum model we find that level repulsion between quasiparticle and plasmaron resonances gives rise to a gaplike feature at small k arpes spectra are sensitive to the electronelectron interaction coupling strength alpha_rm gr and might enable an experimental determination of this material parameter
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707.4231
Energy of harmonic functions and Gromov's proof of Stallings' theorem
We provide the details for Gromov's proof of Stallings' theorem on groups with infinitely many ends using harmonic functions. The main technical result of the paper is a compactness theorem for a certain family of harmonic functions.
math.GR math.DG math.GT
we provide the details for gromovs proof of stallings theorem on groups with infinitely many ends using harmonic functions the main technical result of the paper is a compactness theorem for a certain family of harmonic functions
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707.4232
Performances of a Newly High Sensitive Trilayer F/Cu/F GMI Sensor
We have selected stress-annealed nanocrystalline Fe-based ribbons for ferromagnetic/copper/ferromagnetic sensors exhibiting high magneto-impedance ratio. Longitudinal magneto-impedance reaches 400% at 60 kHz and longitudinal magneto-resistance increases up to 1300% around 200 kHz.
cond-mat.mtrl-sci
we have selected stressannealed nanocrystalline febased ribbons for ferromagneticcopperferromagnetic sensors exhibiting high magnetoimpedance ratio longitudinal magnetoimpedance reaches 400 at 60 khz and longitudinal magnetoresistance increases up to 1300 around 200 khz
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707.4233
On the Synthesis of Sequential Reversible Circuit
Reversible circuits for SR flip flop, JK flip flop, D flip flop, T flip flop, Master Slave D flip flop and Master Slave JK flip flop have been provided with three different logical approaches. All the circuits have been optimized with the help of existing local optimization algorithms (e.g. template matching, moving rule and deletion rule) and the optimized sequential circuits have been compared with the earlier proposals for the same. It has been shown that the present proposals have lower gate complexities and lower number of garbage bits compared to the earlier proposals. It has also been shown that the advantage in gate count obtained in some of the earlier proposals by introduction of New gates is an \textcolor{black}{artifact} and if it is allowed then every circuit block (unless there is a measurement) can be reduced to a single gate. Further, it is shown that a reversible flip flop can be constructed even without a feedback. In this context, some important conceptual issues related to the designing and optimization of sequential reversible circuits have also been addressed.
quant-ph
reversible circuits for sr flip flop jk flip flop d flip flop t flip flop master slave d flip flop and master slave jk flip flop have been provided with three different logical approaches all the circuits have been optimized with the help of existing local optimization algorithms eg template matching moving rule and deletion rule and the optimized sequential circuits have been compared with the earlier proposals for the same it has been shown that the present proposals have lower gate complexities and lower number of garbage bits compared to the earlier proposals it has also been shown that the advantage in gate count obtained in some of the earlier proposals by introduction of new gates is an textcolorblackartifact and if it is allowed then every circuit block unless there is a measurement can be reduced to a single gate further it is shown that a reversible flip flop can be constructed even without a feedback in this context some important conceptual issues related to the designing and optimization of sequential reversible circuits have also been addressed
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707.4234
Molecular clouds in the center of M81
We investigate the molecular gas content and the excitation and fragmentation properties in the central region of the spiral galaxy Messier 81 in both the ^{12}CO(1-0) and ^{12}CO(2-1) transitions. We have recently observed the two transitions of CO in the M~81 center with A, B, and HERA receivers of the IRAM 30-m telescope. We find no CO emission in the inner $\sim$ 300 pc and a weak molecular gas clump structure at a distance of around 460 pc from the nucleus. Observations of the first two CO transitions allowed us to compute the line ratio, and the average I_{21}/I_{10} ratio is 0.68 for the M~81 center. This low value, atypical both of the galactic nuclei of spiral galaxies and of interacting systems, is probably associated to diffuse gas with molecular hydrogen density that is not high enough to excite the CO molecules. After analyzing the clumping properties of the molecular gas in detail, we identify very massive giant molecular associations (GMAs) in CO(2-1) emission with masses of $\sim$ 10$^{5}$ M$_\odot$ and diameters of $\sim$ 250 pc. The deduced N(H_{2})/I_{CO} ratio for the individually resolved GMAs, assumed to be virialized, is a factor of $\sim$ 15 higher than the \textit{standard} Galactic value, showing - as suspected - that the X ratio departs significantly from the mean for galaxies with an unusual physics of the molecular gas.
astro-ph
we investigate the molecular gas content and the excitation and fragmentation properties in the central region of the spiral galaxy messier 81 in both the 12co10 and 12co21 transitions we have recently observed the two transitions of co in the m81 center with a b and hera receivers of the iram 30m telescope we find no co emission in the inner sim 300 pc and a weak molecular gas clump structure at a distance of around 460 pc from the nucleus observations of the first two co transitions allowed us to compute the line ratio and the average i_21i_10 ratio is 068 for the m81 center this low value atypical both of the galactic nuclei of spiral galaxies and of interacting systems is probably associated to diffuse gas with molecular hydrogen density that is not high enough to excite the co molecules after analyzing the clumping properties of the molecular gas in detail we identify very massive giant molecular associations gmas in co21 emission with masses of sim 105 m_odot and diameters of sim 250 pc the deduced nh_2i_co ratio for the individually resolved gmas assumed to be virialized is a factor of sim 15 higher than the textitstandard galactic value showing as suspected that the x ratio departs significantly from the mean for galaxies with an unusual physics of the molecular gas
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707.4235
Analysis of atomic depth profiles directly extracted from Rutherford backscattering data for co-sputtered and ion irradiated Au-Ni films
Co-sputtered Au-Ni thin films having thickness of 30 nm were deposited on Si(100) substrates and irradiated with 160 keV ^{40}Ar^{+} under ambient condition at a number of fluences and analyzed using Rutherford backscattering spectrometry (RBS). The variation of Au signal counts in the RBS spectra with ion dose has been investigated. The distribution of Au, Ni and Si atoms over various depths within the as deposited and irradiated samples have been computed using the backscattering data by means of a direct analytical method. Au and Si profiles have been fitted with error function and the relative changes in variance for various ion fluences compared to that of as deposited profiles have been studied. The spreading rates of different constituents across the interface due to Ar ion impact have also been discussed.
cond-mat.mtrl-sci
cosputtered auni thin films having thickness of 30 nm were deposited on si100 substrates and irradiated with 160 kev 40ar under ambient condition at a number of fluences and analyzed using rutherford backscattering spectrometry rbs the variation of au signal counts in the rbs spectra with ion dose has been investigated the distribution of au ni and si atoms over various depths within the as deposited and irradiated samples have been computed using the backscattering data by means of a direct analytical method au and si profiles have been fitted with error function and the relative changes in variance for various ion fluences compared to that of as deposited profiles have been studied the spreading rates of different constituents across the interface due to ar ion impact have also been discussed
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707.4236
Quantum detection of electronic flying qubits
We consider a model of a detector of ballistic electrons at the edge of a two-dimensional electron gas in the integer quantum Hall regime. The electron is detected by capacitive coupling to a gate which is also coupled to a passive RC circuit. Using a quantum description of this circuit, we determine the signal over noise ratio of the detector in term of the detector characteristics. The back-action of the detector on the incident wavepacket is then computed using a Feynman-Vernon influence functional approach. Using information theory, we define the appropriate notion of quantum limit for such an "on the fly" detector. We show that our particular detector can approach the quantum limit up to logarithms in the ratio of the measurement time over the RC relaxation time. We argue that such a weak logarithmic effect is of no practical significance. Finally we show that a two-electron interference experiment can be used to probe the detector induced decoherence.
cond-mat.mes-hall
we consider a model of a detector of ballistic electrons at the edge of a twodimensional electron gas in the integer quantum hall regime the electron is detected by capacitive coupling to a gate which is also coupled to a passive rc circuit using a quantum description of this circuit we determine the signal over noise ratio of the detector in term of the detector characteristics the backaction of the detector on the incident wavepacket is then computed using a feynmanvernon influence functional approach using information theory we define the appropriate notion of quantum limit for such an on the fly detector we show that our particular detector can approach the quantum limit up to logarithms in the ratio of the measurement time over the rc relaxation time we argue that such a weak logarithmic effect is of no practical significance finally we show that a twoelectron interference experiment can be used to probe the detector induced decoherence
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707.4237
Fluctuation spectroscopy of granularity in superconducting structures
We suggest to use `fluctuation spectroscopy' as a method to detect granularity in a disordered metal close to a superconducting transition. We show that with lowering temperature $T$ the resistance $R(T)$ of a system of relatively large grains initially grows due to the fluctuation suppression of the one-electron tunneling but decreases with further lowering $T$ due to the coherent charge transfer of the fluctuation Cooper pairs. Under certain conditions, such a maximum in $R(T)$ turns out to be sensitive to weak magnetic fields due to a novel Maki -- Thompson type mechanism.
cond-mat.supr-con cond-mat.mes-hall
we suggest to use fluctuation spectroscopy as a method to detect granularity in a disordered metal close to a superconducting transition we show that with lowering temperature t the resistance rt of a system of relatively large grains initially grows due to the fluctuation suppression of the oneelectron tunneling but decreases with further lowering t due to the coherent charge transfer of the fluctuation cooper pairs under certain conditions such a maximum in rt turns out to be sensitive to weak magnetic fields due to a novel maki thompson type mechanism
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707.4238
Regularized braneworlds of arbitrary codimension
We consider a thick p-brane embedded in an n-dimensional spacetime possessing radial symmetry in the directions orthogonal to the brane. We first consider a static brane, and find a general fine tuning relationship between the brane and bulk parameters required for the brane to be flat. We then consider the cosmology of a time dependent brane in a static bulk, and find the Friedmann equation for the brane scale factor a(t). The singularities that would ordinarily arise when considering arbitrary codimensions are avoided by regularizing the brane, giving it a finite profile in the transverse dimensions. However, since we consider the brane to be a strictly local defect, we find that the transverse dimensions must have infinite volume, and hence gravity cannot be localized on the brane without resorting to some infra-red cutoff.
hep-ph hep-th
we consider a thick pbrane embedded in an ndimensional spacetime possessing radial symmetry in the directions orthogonal to the brane we first consider a static brane and find a general fine tuning relationship between the brane and bulk parameters required for the brane to be flat we then consider the cosmology of a time dependent brane in a static bulk and find the friedmann equation for the brane scale factor at the singularities that would ordinarily arise when considering arbitrary codimensions are avoided by regularizing the brane giving it a finite profile in the transverse dimensions however since we consider the brane to be a strictly local defect we find that the transverse dimensions must have infinite volume and hence gravity cannot be localized on the brane without resorting to some infrared cutoff
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707.4239
Tracial gauge norms on finite von Neumann algebras satisfying the weak Dixmier property
In this paper we set up a representation theorem for tracial gauge norms on finite von Neumann algebras satisfying the weak Dixmier property in terms of Ky Fan norms. Examples of tracial gauge norms on finite von Neumann algebras satisfying the weak Dixmier property include unitarily invariant norms on finite factors (type ${\rm II}\sb 1$ factors and $M_n(\cc)$) and symmetric gauge norms on $L^\infty[0,1]$ and $\cc^n$. As the first application, we obtain that the class of unitarily invariant norms on a type ${\rm II}\sb 1$ factor coincides with the class of symmetric gauge norms on $L^\infty[0,1]$ and von Neumann's classical result \cite{vN} on unitarily invariant norms on $M_n(\cc)$. As the second application, Ky Fan's dominance theorem \cite{Fan} is obtained for finite von Neumann algebras satisfying the weak Dixmier property. As the third application, some classical results in non-commutative $L^p$-theory (e.g., non-commutative H$\ddot{\text{o}}$lder's inequality, duality and reflexivity of non-commutative $L^p$-spaces) are obtained for general unitarily invariant norms on finite factors. We also investigate the extreme points of $\NN(\M)$, the convex compact set (in the pointwise weak topology) of normalized unitarily invariant norms (the norm of the identity operator is 1) on a finite factor $\M$. We obtain all extreme points of $\NN(M_2(\cc))$ and many extreme points of $\NN(M_n(\cc))$ ($n\geq 3$). For a type ${\rm II}\sb 1$ factor $\M$, we prove that if $t$ ($0\leq t\leq 1$) is a rational number then the Ky Fan $t$-th norm is an extreme point of $\NN(\M)$.
math.OA math.FA
in this paper we set up a representation theorem for tracial gauge norms on finite von neumann algebras satisfying the weak dixmier property in terms of ky fan norms examples of tracial gauge norms on finite von neumann algebras satisfying the weak dixmier property include unitarily invariant norms on finite factors type rm iisb 1 factors and m_ncc and symmetric gauge norms on linfty01 and ccn as the first application we obtain that the class of unitarily invariant norms on a type rm iisb 1 factor coincides with the class of symmetric gauge norms on linfty01 and von neumanns classical result citevn on unitarily invariant norms on m_ncc as the second application ky fans dominance theorem citefan is obtained for finite von neumann algebras satisfying the weak dixmier property as the third application some classical results in noncommutative lptheory eg noncommutative hddottextolders inequality duality and reflexivity of noncommutative lpspaces are obtained for general unitarily invariant norms on finite factors we also investigate the extreme points of nnm the convex compact set in the pointwise weak topology of normalized unitarily invariant norms the norm of the identity operator is 1 on a finite factor m we obtain all extreme points of nnm_2cc and many extreme points of nnm_ncc ngeq 3 for a type rm iisb 1 factor m we prove that if t 0leq tleq 1 is a rational number then the ky fan tth norm is an extreme point of nnm
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707.424
Unitarily invariant norms related to factors
Let $\M$ be a semi-finite factor and let $\J(\M)$ be the set of operators $T$ in $\M$ such that $T=ETE$ for some finite projection $E$. In this paper we obtain a representation theorem for unitarily invariant norms on $\J(\M)$ in terms of Ky Fan norms. As an application, we prove that the class of unitarily invariant norms on $\J(\M)$ coincides with the class of symmetric gauge norms on a classical abelian algebra, which generalizes von Neumann's classical result \cite{vN} on unitarily invariant norms on $M_n(\cc)$. As another application, Ky Fan's dominance theorem \cite{Fan} is obtained for semi-finite factors. Some classical results in non-commutative $L^p$-theory (e.g., non-commutative H$\ddot{\text{o}}$lder's inequality, duality and reflexivity of non-commutative $L^p$-spaces) are extended to general unitarily invariant norms related to semi-finite factors. We also prove that up to a scale the operator norm is the unique unitarily invariant norm associated to a type ${\rm III}$ factor.
math.OA math.FA
let m be a semifinite factor and let jm be the set of operators t in m such that tete for some finite projection e in this paper we obtain a representation theorem for unitarily invariant norms on jm in terms of ky fan norms as an application we prove that the class of unitarily invariant norms on jm coincides with the class of symmetric gauge norms on a classical abelian algebra which generalizes von neumanns classical result citevn on unitarily invariant norms on m_ncc as another application ky fans dominance theorem citefan is obtained for semifinite factors some classical results in noncommutative lptheory eg noncommutative hddottextolders inequality duality and reflexivity of noncommutative lpspaces are extended to general unitarily invariant norms related to semifinite factors we also prove that up to a scale the operator norm is the unique unitarily invariant norm associated to a type rm iii factor
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707.4241
Thermal rectification in carbon nanotube intramolecular junctions: Molecular dynamics calculations
We study heat conduction in (n, 0)/(2n, 0) intramolecular junctions by using molecular dynamics method. It is found that the heat conduction is asymmetric, namely, heat transports preferably in one direction. This phenomenon is also called thermal rectification. The rectification is weakly dependent on the detailed structure of connection part, but is strongly dependent on the temperature gradient. We also study the effect of the tube radius and intramolecular junction length on the rectification. Our study shows that the tensile stress can increase rectification. The physical mechanism of the rectification is explained.
cond-mat.mes-hall cond-mat.mtrl-sci
we study heat conduction in n 02n 0 intramolecular junctions by using molecular dynamics method it is found that the heat conduction is asymmetric namely heat transports preferably in one direction this phenomenon is also called thermal rectification the rectification is weakly dependent on the detailed structure of connection part but is strongly dependent on the temperature gradient we also study the effect of the tube radius and intramolecular junction length on the rectification our study shows that the tensile stress can increase rectification the physical mechanism of the rectification is explained
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707.4242
Importance Tempering
Simulated tempering (ST) is an established Markov chain Monte Carlo (MCMC) method for sampling from a multimodal density $\pi(\theta)$. Typically, ST involves introducing an auxiliary variable $k$ taking values in a finite subset of $[0,1]$ and indexing a set of tempered distributions, say $\pi_k(\theta) \propto \pi(\theta)^k$. In this case, small values of $k$ encourage better mixing, but samples from $\pi$ are only obtained when the joint chain for $(\theta,k)$ reaches $k=1$. However, the entire chain can be used to estimate expectations under $\pi$ of functions of interest, provided that importance sampling (IS) weights are calculated. Unfortunately this method, which we call importance tempering (IT), can disappoint. This is partly because the most immediately obvious implementation is na\"ive and can lead to high variance estimators. We derive a new optimal method for combining multiple IS estimators and prove that the resulting estimator has a highly desirable property related to the notion of effective sample size. We briefly report on the success of the optimal combination in two modelling scenarios requiring reversible-jump MCMC, where the na\"ive approach fails.
stat.CO stat.AP
simulated tempering st is an established markov chain monte carlo mcmc method for sampling from a multimodal density pitheta typically st involves introducing an auxiliary variable k taking values in a finite subset of 01 and indexing a set of tempered distributions say pi_ktheta propto pithetak in this case small values of k encourage better mixing but samples from pi are only obtained when the joint chain for thetak reaches k1 however the entire chain can be used to estimate expectations under pi of functions of interest provided that importance sampling is weights are calculated unfortunately this method which we call importance tempering it can disappoint this is partly because the most immediately obvious implementation is naive and can lead to high variance estimators we derive a new optimal method for combining multiple is estimators and prove that the resulting estimator has a highly desirable property related to the notion of effective sample size we briefly report on the success of the optimal combination in two modelling scenarios requiring reversiblejump mcmc where the naive approach fails
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707.4243
Deep optical observations of the interaction of the SS 433 microquasar jet with the W 50 radio continuum shell
Four mosaics of deep, continuum-subtracted, CCD images have been obtained over the extensive galactic radio continuum shell, W 50, which surrounds the remarkable stellar system SS 433. Two of these mosaics in the Halpha+[N II] and [O III] 5007 A emission lines respectively cover a field of ~2.3 x 2.5 degr^2 which contains all of W 50 but at a low angular resolution of 5 arcsec. The third and fourth mosaics cover the eastern (in [O III] 5007 A) and western (in Halpha+[N II]) filamentary nebulosity respectively but at an angular resolution of 1 arcsec. These observations are supplemented by new low dispersion spectra and longslit, spatially resolved echelle spectra. The [O III] 5007 A images show for the first time the distribution of this emission in both the eastern and western filaments while new Halpha+[N II] emission features are also found in both of these regions. Approaching flows of faintly emitting material from the bright eastern filaments of up 100 km/s in radial velocity are detected. The present observations also suggest that the heliocentric systemic radial velocity of the whole system is 56+-2 km/s. Furthermore, very deep imagery and high resolution spectroscopy of a small part of the northern radio ridge of W 50 has revealed for the first time the very faint optical nebulosity associated with this edge. It is suggested that patchy foreground dust along the ~5 kpc sightline is inhibiting the detection of all of the optical nebulosity associated with W 50. The interaction of the microquasar jets of SS 433 with the W 50 shell is discussed.
astro-ph
four mosaics of deep continuumsubtracted ccd images have been obtained over the extensive galactic radio continuum shell w 50 which surrounds the remarkable stellar system ss 433 two of these mosaics in the halphan ii and o iii 5007 a emission lines respectively cover a field of 23 x 25 degr2 which contains all of w 50 but at a low angular resolution of 5 arcsec the third and fourth mosaics cover the eastern in o iii 5007 a and western in halphan ii filamentary nebulosity respectively but at an angular resolution of 1 arcsec these observations are supplemented by new low dispersion spectra and longslit spatially resolved echelle spectra the o iii 5007 a images show for the first time the distribution of this emission in both the eastern and western filaments while new halphan ii emission features are also found in both of these regions approaching flows of faintly emitting material from the bright eastern filaments of up 100 kms in radial velocity are detected the present observations also suggest that the heliocentric systemic radial velocity of the whole system is 562 kms furthermore very deep imagery and high resolution spectroscopy of a small part of the northern radio ridge of w 50 has revealed for the first time the very faint optical nebulosity associated with this edge it is suggested that patchy foreground dust along the 5 kpc sightline is inhibiting the detection of all of the optical nebulosity associated with w 50 the interaction of the microquasar jets of ss 433 with the w 50 shell is discussed
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707.4244
Distinguishing cancerous from non-cancerous cells through analysis of electrical noise
Since 1984, electric cell-substrate impedance sensing (ECIS) has been used to monitor cell behavior in tissue culture and has proven sensitive to cell morphological changes and cell motility. We have taken ECIS measurements on several cultures of non-cancerous (HOSE) and cancerous (SKOV) human ovarian surface epithelial cells. By analyzing the noise in real and imaginary electrical impedance, we demonstrate that it is possible to distinguish the two cell types purely from signatures of their electrical noise. Our measures include power-spectral exponents, Hurst and detrended fluctuation analysis, and estimates of correlation time; principal-component analysis combines all the measures. The noise from both cancerous and non-cancerous cultures shows correlations on many time scales, but these correlations are stronger for the non-cancerous cells.
q-bio.CB q-bio.QM
since 1984 electric cellsubstrate impedance sensing ecis has been used to monitor cell behavior in tissue culture and has proven sensitive to cell morphological changes and cell motility we have taken ecis measurements on several cultures of noncancerous hose and cancerous skov human ovarian surface epithelial cells by analyzing the noise in real and imaginary electrical impedance we demonstrate that it is possible to distinguish the two cell types purely from signatures of their electrical noise our measures include powerspectral exponents hurst and detrended fluctuation analysis and estimates of correlation time principalcomponent analysis combines all the measures the noise from both cancerous and noncancerous cultures shows correlations on many time scales but these correlations are stronger for the noncancerous cells
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707.4245
On the Brauer groups of quasilocal fields and the norm groups of their finite Galois extensions
This paper shows that divisible abelian torsion groups are realizable as Brauer groups of quasilocal fields. It describes the isomorphism classes of Brauer groups of primarily quasilocal fields and solves the analogous problem concerning the reduced components of the Brauer groups of two basic types of Henselian valued absolutely stable fields. For a quasilocal field E and a finite separable extension R/E, we find two sufficient conditions for validity of the norm group equality $N(R/E) = N(R_{0}/E)$, where R_{0} is the maximal abelian extension of E in R. This is used for deriving information on the arising specific relations between Galois groups and norm groups of finite Galois extensions of E.
math.RA
this paper shows that divisible abelian torsion groups are realizable as brauer groups of quasilocal fields it describes the isomorphism classes of brauer groups of primarily quasilocal fields and solves the analogous problem concerning the reduced components of the brauer groups of two basic types of henselian valued absolutely stable fields for a quasilocal field e and a finite separable extension re we find two sufficient conditions for validity of the norm group equality nre nr_0e where r_0 is the maximal abelian extension of e in r this is used for deriving information on the arising specific relations between galois groups and norm groups of finite galois extensions of e
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707.4246
Balanced Superprojective Varieties
We first review the definition of superprojective spaces from the functor-of-points perspective. We derive the relation between superprojective spaces and supercosets in the framework of the theory of sheaves. As an application of the geometry of superprojective spaces, we extend Donaldson's definition of balanced manifolds to supermanifolds and we derive the new conditions of a balanced supermanifold. We apply the construction to superpoints viewed as submanifolds of superprojective spaces. We conclude with a list of open issues and interesting problems that can be addressed in the present context.
math-ph hep-th math.MP
we first review the definition of superprojective spaces from the functorofpoints perspective we derive the relation between superprojective spaces and supercosets in the framework of the theory of sheaves as an application of the geometry of superprojective spaces we extend donaldsons definition of balanced manifolds to supermanifolds and we derive the new conditions of a balanced supermanifold we apply the construction to superpoints viewed as submanifolds of superprojective spaces we conclude with a list of open issues and interesting problems that can be addressed in the present context
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707.4247
ISW effect in Unified Dark Matter Scalar Field Cosmologies: an analytical approach
We perform an analytical study of the Integrated Sachs-Wolfe (ISW) effect within the framework of Unified Dark Matter models based on a scalar field which aim at a unified description of dark energy and dark matter. Computing the temperature power spectrum of the Cosmic Microwave Background anisotropies we are able to isolate those contributions that can potentially lead to strong deviations from the usual ISW effect occurring in a $\Lambda$CDM universe. This helps to highlight the crucial role played by the sound speed in the Unified Dark Matter models. Our treatment is completely general in that all the results depend only on the speed of sound of the dark component and thus it can be applied to a variety of unified models, including those which are not described by a scalar field but relies on a single dark fluid.
astro-ph gr-qc hep-ph hep-th
we perform an analytical study of the integrated sachswolfe isw effect within the framework of unified dark matter models based on a scalar field which aim at a unified description of dark energy and dark matter computing the temperature power spectrum of the cosmic microwave background anisotropies we are able to isolate those contributions that can potentially lead to strong deviations from the usual isw effect occurring in a lambdacdm universe this helps to highlight the crucial role played by the sound speed in the unified dark matter models our treatment is completely general in that all the results depend only on the speed of sound of the dark component and thus it can be applied to a variety of unified models including those which are not described by a scalar field but relies on a single dark fluid
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707.4248
Effect of Holstein phonons on the electronic properties of graphene
We obtain the self-energy of the electronic propagator due to the presence of Holstein polarons within the first Born approximation. This leads to a renormalization of the Fermi velocity of one percent. We further compute the optical conductivity of the system at the Dirac point and at finite doping within the Kubo-formula. We argue that the effects due to Holstein phonons are negligible and that the Boltzmann approach which does not include inter-band transition and can thus not treat optical phonons due to their high energy of $\hbar\omega_0\sim0.1-0.2$eV, remains valid.
cond-mat.mes-hall
we obtain the selfenergy of the electronic propagator due to the presence of holstein polarons within the first born approximation this leads to a renormalization of the fermi velocity of one percent we further compute the optical conductivity of the system at the dirac point and at finite doping within the kuboformula we argue that the effects due to holstein phonons are negligible and that the boltzmann approach which does not include interband transition and can thus not treat optical phonons due to their high energy of hbaromega_0sim0102ev remains valid
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707.4249
Temperature of a Hamiltonian system given as the effective temperature of a non-equilibrium steady state Langevin thermostat
In non-equilibrium steady states (NESS) far from equilibrium, it is known that the Einstein relation is violated. Then, the ratio of the diffusion coefficient to the mobility is called an effective temperature, and the physical relevance of this effective temperature has been studied in several works. Although the physical relevance is not yet completely clear, it has been found that the role of an effective temperature in NESS is indeed analogous to that of the temperature in equilibrium systems in a number of respects. In this paper, we find further evidence establishing this analogy. We employ a non-equilibrium Langevin system as a thermostat for a Hamiltonian system and find that the kinetic temperature of this Hamiltonian system is equal to the effective temperature of the thermostat.
cond-mat.stat-mech
in nonequilibrium steady states ness far from equilibrium it is known that the einstein relation is violated then the ratio of the diffusion coefficient to the mobility is called an effective temperature and the physical relevance of this effective temperature has been studied in several works although the physical relevance is not yet completely clear it has been found that the role of an effective temperature in ness is indeed analogous to that of the temperature in equilibrium systems in a number of respects in this paper we find further evidence establishing this analogy we employ a nonequilibrium langevin system as a thermostat for a hamiltonian system and find that the kinetic temperature of this hamiltonian system is equal to the effective temperature of the thermostat
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707.425
Opening Remarks at Chiral Dynamics 2006:Experimental Tests of Chiral Symmetry Breaking
A physical introduction to the basics of chiral dynamics is presented. Emphasis is placed on experimental tests which have generally demonstrated a strong confirmation of the predictions of chiral perturbation theory, a low energy effective field theory of QCD. Special attention is paid to a few cases where discrepancies exist, requiring further work. Some desirable future tests are also recommended.
hep-ph
a physical introduction to the basics of chiral dynamics is presented emphasis is placed on experimental tests which have generally demonstrated a strong confirmation of the predictions of chiral perturbation theory a low energy effective field theory of qcd special attention is paid to a few cases where discrepancies exist requiring further work some desirable future tests are also recommended
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707.4251
Jet Geometrical Objects Produced by Linear ODEs Systems and Superior Order ODEs
The aim of this paper is to construct a Riemann-Lagrange geometry on 1-jet spaces, in the sense of d-connections, d-torsions, d-curvatures, electromagnetic d-field and geometric electromagnetic Yang-Mills energy, starting from a given linear ODEs system or a given superior order ODE. The case of a non-homogenous linear ODE of superior order is disscused.
math.DG math.DS
the aim of this paper is to construct a riemannlagrange geometry on 1jet spaces in the sense of dconnections dtorsions dcurvatures electromagnetic dfield and geometric electromagnetic yangmills energy starting from a given linear odes system or a given superior order ode the case of a nonhomogenous linear ode of superior order is disscused
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707.4252
Fluorine in a Carbon-Enhanced Metal-Poor Star
The fluorine abundance of the Carbon-Enhanced Metal-Poor (CEMP) star HE 1305+0132 has been derived by analysis of the molecular HF (1-0) R9 line at 2.3357 microns in a high-resolution (R = 50,000) spectrum obtained with the Phoenix spectrometer and Gemini-South telescope. Our abundance analysis makes use of a CNO-enhanced ATLAS12 model atmosphere characterized by a metallicity and CNO enhancements determined utilizing medium-resolution (R = 3,000) optical and near-IR spectra. The effective iron abundance is found to be [Fe/H] = -2.5, making HE 1305+0132 the most Fe-deficient star, by more than an order of magnitude, for which the abundance of fluorine has been measured. Using spectral synthesis, we derive a super-solar fluorine abundance of A(19F) = 4.96 +/- 0.21, corresponding to a relative abundance of [F/Fe] = 2.90. A single line of the Phillips C_2 system is identified in our Phoenix spectrum, and along with multiple lines of the first-overtone vibration-rotation CO (3-1) band head, C and O abundances of A(12C) = 8.57 +/- 0.11 and A(16O) = 7.04 +/- 0.14 are derived. We consider the striking fluorine overabundance in the framework of the nucleosynthetic processes thought to be responsible for the C-enhancement of CEMP stars and conclude that the atmosphere of HE 1305+0132 was polluted via mass transfer by a primary companion during its asymptotic giant branch phase. This is the first study of fluorine in a CEMP star, and it demonstrates that this rare nuclide can be a key diagnostic of nucleosynthetic processes in the early Galaxy.
astro-ph
the fluorine abundance of the carbonenhanced metalpoor cemp star he 13050132 has been derived by analysis of the molecular hf 10 r9 line at 23357 microns in a highresolution r 50000 spectrum obtained with the phoenix spectrometer and geminisouth telescope our abundance analysis makes use of a cnoenhanced atlas12 model atmosphere characterized by a metallicity and cno enhancements determined utilizing mediumresolution r 3000 optical and nearir spectra the effective iron abundance is found to be feh 25 making he 13050132 the most fedeficient star by more than an order of magnitude for which the abundance of fluorine has been measured using spectral synthesis we derive a supersolar fluorine abundance of a19f 496 021 corresponding to a relative abundance of ffe 290 a single line of the phillips c_2 system is identified in our phoenix spectrum and along with multiple lines of the firstovertone vibrationrotation co 31 band head c and o abundances of a12c 857 011 and a16o 704 014 are derived we consider the striking fluorine overabundance in the framework of the nucleosynthetic processes thought to be responsible for the cenhancement of cemp stars and conclude that the atmosphere of he 13050132 was polluted via mass transfer by a primary companion during its asymptotic giant branch phase this is the first study of fluorine in a cemp star and it demonstrates that this rare nuclide can be a key diagnostic of nucleosynthetic processes in the early galaxy
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707.4253
Holomorphic Poisson Manifolds and Holomorphic Lie Algebroids
We study holomorphic Poisson manifolds and holomorphic Lie algebroids from the viewpoint of real Poisson geometry. We give a characterization of holomorphic Poisson structures in terms of the Poisson Nijenhuis structures of Magri-Morosi and describe a double complex which computes the holomorphic Poisson cohomology. A holomorphic Lie algebroid structure on a vector bundle $A\to X$ is shown to be equivalent to a matched pair of complex Lie algebroids $(T^{0,1}X,A^{1,0})$, in the sense of Lu. The holomorphic Lie algebroid cohomology of $A$ is isomorphic to the cohomology of the elliptic Lie algebroid $T^{0,1}X\bowtie A^{1,0}$. In the case when $(X,\pi)$ is a holomorphic Poisson manifold and $A=(T^*X)_\pi$, such an elliptic Lie algebroid coincides with the Dirac structure corresponding to the associated generalized complex structure of the holomorphic Poisson manifold.
math.DG hep-th math-ph math.MP
we study holomorphic poisson manifolds and holomorphic lie algebroids from the viewpoint of real poisson geometry we give a characterization of holomorphic poisson structures in terms of the poisson nijenhuis structures of magrimorosi and describe a double complex which computes the holomorphic poisson cohomology a holomorphic lie algebroid structure on a vector bundle ato x is shown to be equivalent to a matched pair of complex lie algebroids t01xa10 in the sense of lu the holomorphic lie algebroid cohomology of a is isomorphic to the cohomology of the elliptic lie algebroid t01xbowtie a10 in the case when xpi is a holomorphic poisson manifold and atx_pi such an elliptic lie algebroid coincides with the dirac structure corresponding to the associated generalized complex structure of the holomorphic poisson manifold
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707.4254
Strong-coupling expansion of cusp anomaly and gluon amplitudes from quantum open strings in AdS_5 x S^5
An important ``observable'' of planar N=4 SYM theory is the scaling function f(lambda) that appears in the anomalous dimension of large spin twist 2 operators and also in the cusp anomaly of light-like Wilson loops. The non-trivial relation between the anomalous dimension and the Wilson interpretations of f(lambda) is well-understood on the perturbative gauge theory side of the AdS/CFT duality. In the first part of this paper we present the dual string-theory counterpart of this relation, to all orders in lambda^(-1/2) expansion. As a check, we explicitly compute the leading 1-loop string sigma model correction to the cusp Wilson loop, reproducing the same subleading coefficient in f(lambda) as found earlier in the spinning closed string case. The same function f(lambda) appears also in the resummed form of the 4-gluon amplitude as discussed at weak coupling by Bern, Dixon and Smirnov and recently found at the leading order at strong coupling by Alday and Maldacena (AM). Here we attempt to extend this approach to subleading order in lambda^(-1/2) by computing the IR singular part of 1-loop string correction to the corresponding T-dual Wilson loop. We discuss explicitly the 1-cusp case and comment on apparent problems with the dimensional regularization proposal of AM when directly applied order by order in strong coupling (inverse string tension) expansion.
hep-th
an important observable of planar n4 sym theory is the scaling function flambda that appears in the anomalous dimension of large spin twist 2 operators and also in the cusp anomaly of lightlike wilson loops the nontrivial relation between the anomalous dimension and the wilson interpretations of flambda is wellunderstood on the perturbative gauge theory side of the adscft duality in the first part of this paper we present the dual stringtheory counterpart of this relation to all orders in lambda12 expansion as a check we explicitly compute the leading 1loop string sigma model correction to the cusp wilson loop reproducing the same subleading coefficient in flambda as found earlier in the spinning closed string case the same function flambda appears also in the resummed form of the 4gluon amplitude as discussed at weak coupling by bern dixon and smirnov and recently found at the leading order at strong coupling by alday and maldacena am here we attempt to extend this approach to subleading order in lambda12 by computing the ir singular part of 1loop string correction to the corresponding tdual wilson loop we discuss explicitly the 1cusp case and comment on apparent problems with the dimensional regularization proposal of am when directly applied order by order in strong coupling inverse string tension expansion
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707.4255
Complexity of Propositional Proofs under a Promise
We study -- within the framework of propositional proof complexity -- the problem of certifying unsatisfiability of CNF formulas under the promise that any satisfiable formula has many satisfying assignments, where ``many'' stands for an explicitly specified function $\Lam$ in the number of variables $n$. To this end, we develop propositional proof systems under different measures of promises (that is, different $\Lam$) as extensions of resolution. This is done by augmenting resolution with axioms that, roughly, can eliminate sets of truth assignments defined by Boolean circuits. We then investigate the complexity of such systems, obtaining an exponential separation in the average-case between resolution under different size promises: 1. Resolution has polynomial-size refutations for all unsatisfiable 3CNF formulas when the promise is $\eps\cd2^n$, for any constant $0<\eps<1$. 2. There are no sub-exponential size resolution refutations for random 3CNF formulas, when the promise is $2^{\delta n}$ (and the number of clauses is $o(n^{3/2})$), for any constant $0<\delta<1$.
cs.CC cs.LO
we study within the framework of propositional proof complexity the problem of certifying unsatisfiability of cnf formulas under the promise that any satisfiable formula has many satisfying assignments where many stands for an explicitly specified function lam in the number of variables n to this end we develop propositional proof systems under different measures of promises that is different lam as extensions of resolution this is done by augmenting resolution with axioms that roughly can eliminate sets of truth assignments defined by boolean circuits we then investigate the complexity of such systems obtaining an exponential separation in the averagecase between resolution under different size promises 1 resolution has polynomialsize refutations for all unsatisfiable 3cnf formulas when the promise is epscd2n for any constant 0eps1 2 there are no subexponential size resolution refutations for random 3cnf formulas when the promise is 2delta n and the number of clauses is on32 for any constant 0delta1
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707.4256
Rubbling and Optimal Rubbling of Graphs
A pebbling move on a graph removes two pebbles at a vertex and adds one pebble at an adjacent vertex. Rubbling is a version of pebbling where an additional move is allowed. In this new move one pebble is removed at vertices v and w adjacent to a vertex u and an extra pebble is added at vertex u. A vertex is reachable from a pebble distribution if it is possible to move a pebble to that vertex using rubbling moves. The rubbling number of a graph is the smallest number m needed to guarantee that any vertex is reachable from any pebble distribution of m pebbles. The optimal rubbling number is the smallest number m needed to guarantee a pebble distribution of m pebbles from which any vertex is reachable. We determine the rubbling and optimal rubbling number of some families of graphs including cycles.
math.CO
a pebbling move on a graph removes two pebbles at a vertex and adds one pebble at an adjacent vertex rubbling is a version of pebbling where an additional move is allowed in this new move one pebble is removed at vertices v and w adjacent to a vertex u and an extra pebble is added at vertex u a vertex is reachable from a pebble distribution if it is possible to move a pebble to that vertex using rubbling moves the rubbling number of a graph is the smallest number m needed to guarantee that any vertex is reachable from any pebble distribution of m pebbles the optimal rubbling number is the smallest number m needed to guarantee a pebble distribution of m pebbles from which any vertex is reachable we determine the rubbling and optimal rubbling number of some families of graphs including cycles
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707.4257
Axiomatic quantum field theory. Jet formalism
Jet formalism provides the adequate mathematical formulation of classical field theory, reviewed in hep-th/0612182v1. A formulation of QFT compatible with this classical one is discussed. We are based on the fact that an algebra of Euclidean quantum fields is graded commutative, and there are homomorphisms of the graded commutative algebra of classical fields to this algebra. As a result, any variational symmetry of a classical Lagrangian yields the identities which Euclidean Green functions of quantum fields satisfy.
hep-th math-ph math.MP
jet formalism provides the adequate mathematical formulation of classical field theory reviewed in hepth0612182v1 a formulation of qft compatible with this classical one is discussed we are based on the fact that an algebra of euclidean quantum fields is graded commutative and there are homomorphisms of the graded commutative algebra of classical fields to this algebra as a result any variational symmetry of a classical lagrangian yields the identities which euclidean green functions of quantum fields satisfy
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707.4258
Star Unfolding Convex Polyhedra via Quasigeodesic Loops
We extend the notion of star unfolding to be based on a quasigeodesic loop Q rather than on a point. This gives a new general method to unfold the surface of any convex polyhedron P to a simple (non-overlapping), planar polygon: cut along one shortest path from each vertex of P to Q, and cut all but one segment of Q.
cs.CG cs.DM
we extend the notion of star unfolding to be based on a quasigeodesic loop q rather than on a point this gives a new general method to unfold the surface of any convex polyhedron p to a simple nonoverlapping planar polygon cut along one shortest path from each vertex of p to q and cut all but one segment of q
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707.4259
Fermi-Polaron: Diagrammatic Monte Carlo for Divergent Sign-Alternating Series
Diagrammatic Monte Carlo approach is applied to a problem of a single spin-down fermion resonantly interacting with the sea of ideal spin-up fermions. On one hand, we develop a generic, sign-problem tolerant, method of exact numerical solution of polaron-type models. On the other hand, our solution is important for understanding the phase diagram and properties of the BCS-BEC crossover in the strongly imbalanced regime. This is the first, and possibly characteristic, example of how the Monte Carlo approach can be applied to a divergent sign-alternating diagrammatic series.
cond-mat.stat-mech
diagrammatic monte carlo approach is applied to a problem of a single spindown fermion resonantly interacting with the sea of ideal spinup fermions on one hand we develop a generic signproblem tolerant method of exact numerical solution of polarontype models on the other hand our solution is important for understanding the phase diagram and properties of the bcsbec crossover in the strongly imbalanced regime this is the first and possibly characteristic example of how the monte carlo approach can be applied to a divergent signalternating diagrammatic series
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707.426
Orbit Determination with Topocentric Correction: Algorithms for the Next Generation Surveys
Given a set of astrometric observations of the same object, the problem of orbit determination is to compute the orbit and to assess its uncertainty and reliability. For the next generation surveys, with much larger number density of observed objects, new algorithms or substantial revisions of the classical ones are needed. The problem has three main steps, preliminary orbit, least squares orbit, and quality control. The classical theory of preliminary orbits was incomplete: the consequences of the topocentric correction had not been fully studied. We show that it is possible to account for this correction, possibly with an increase in the number of preliminary solutions, without impairing the overall orbit determination performance. We have developed modified least squares orbit determination algorithms that can be used to improve the reliability of the procedure. We have tested the complete procedure on two simulations with number densities comparable to that expected from the next generation surveys such as Pan-STARRS and LSST. To control the problem of false identifications we have introduced a quality control on the fit residuals based on an array of metrics and a procedure to remove duplications and contradictions in the output. The results confirm that large sets of discoveries can be obtained with good quality orbits and very high success rate losing only 0.6 to 1.3% of objects and a false identification rate in the range 0.02 to 0.06%.
astro-ph
given a set of astrometric observations of the same object the problem of orbit determination is to compute the orbit and to assess its uncertainty and reliability for the next generation surveys with much larger number density of observed objects new algorithms or substantial revisions of the classical ones are needed the problem has three main steps preliminary orbit least squares orbit and quality control the classical theory of preliminary orbits was incomplete the consequences of the topocentric correction had not been fully studied we show that it is possible to account for this correction possibly with an increase in the number of preliminary solutions without impairing the overall orbit determination performance we have developed modified least squares orbit determination algorithms that can be used to improve the reliability of the procedure we have tested the complete procedure on two simulations with number densities comparable to that expected from the next generation surveys such as panstarrs and lsst to control the problem of false identifications we have introduced a quality control on the fit residuals based on an array of metrics and a procedure to remove duplications and contradictions in the output the results confirm that large sets of discoveries can be obtained with good quality orbits and very high success rate losing only 06 to 13 of objects and a false identification rate in the range 002 to 006
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707.4261
Congruence obstructions to pseudomodularity of Fricke groups
A pseudomodular group is a finite coarea nonarithmetic Fuchsian group whose cusp set is exactly $\mathbb{P}^1(\mathbb{Q})$. Long and Reid constructed finitely many of these by considering Fricke groups, i.e., those that uniformize one-cusped tori. We prove that a zonal Fricke group with rational cusps is pseudomodular if and only if its cusp set is dense in the finite adeles of $\mathbb{Q}$. We then deduce that infinitely many such Fricke groups are not pseudomodular.
math.NT
a pseudomodular group is a finite coarea nonarithmetic fuchsian group whose cusp set is exactly mathbbp1mathbbq long and reid constructed finitely many of these by considering fricke groups ie those that uniformize onecusped tori we prove that a zonal fricke group with rational cusps is pseudomodular if and only if its cusp set is dense in the finite adeles of mathbbq we then deduce that infinitely many such fricke groups are not pseudomodular
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707.4262
Spin Hamiltonian for which the Chiral Spin Liquid is the Exact Ground State
We construct a Hamiltonian that singles out the chiral spin liquid on a square lattice with periodic boundary conditions as the exact and, apart from the two-fold topological degeneracy, unique ground state.
cond-mat.str-el cond-mat.mes-hall
we construct a hamiltonian that singles out the chiral spin liquid on a square lattice with periodic boundary conditions as the exact and apart from the twofold topological degeneracy unique ground state
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707.4263
Toward the Jamming Threshold of Sphere Packings: Tunneled Crystals
We have discovered a new family of three-dimensional crystal sphere packings that are strictly jammed (i.e., mechanically stable) and yet possess an anomalously low density. This family constitutes an uncountably infinite number of crystal packings that are subpackings of the densest crystal packings and are characterized by a high concentration of self-avoiding "tunnels" (chains of vacancies) that permeate the structures. The fundamental geometric characteristics of these tunneled crystals command interest in their own right and are described here in some detail. These include the lattice vectors (that specify the packing configurations), coordination structure, Voronoi cells, and density fluctuations. The tunneled crystals are not only candidate structures for achieving the jamming threshold (lowest-density rigid packing), but may have substantially broader significance for condensed matter physics and materials science.
cond-mat.soft cond-mat.stat-mech
we have discovered a new family of threedimensional crystal sphere packings that are strictly jammed ie mechanically stable and yet possess an anomalously low density this family constitutes an uncountably infinite number of crystal packings that are subpackings of the densest crystal packings and are characterized by a high concentration of selfavoiding tunnels chains of vacancies that permeate the structures the fundamental geometric characteristics of these tunneled crystals command interest in their own right and are described here in some detail these include the lattice vectors that specify the packing configurations coordination structure voronoi cells and density fluctuations the tunneled crystals are not only candidate structures for achieving the jamming threshold lowestdensity rigid packing but may have substantially broader significance for condensed matter physics and materials science
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707.4264
Thermodynamic properties of the Spin-1/2 Heisenberg Antiferromagnet with Anisotropic Exchange on the Kagome Lattice: Comparison with Volborthite
Thermodynamic properties such as magnetic susceptibility and specific heat have been computed for the Heisenberg Antiferromagnet with spatially anisotropic exchange on the kagome lattice on clusters up to N=24 spins from the full spectra obtained by exact diagonalization. This approach is shown to provide a good represention of these thermodynamic properties above temperatures of about $J_{\rm av}/5$ where $J_{\rm av}$ is an average of the coupling constants. Comparison with experimental Volborthite data obtained by Hiroi {\it {et al}} [J. Phys. Soc. Jpn. {\bf 70},3377 (2001)] shows that Volborthite is best described by a model with nearly isotropic exchanges in spite of the significant distortion of the kagom\'{e} lattice of magnetic sites in this compound and suggests that additional interactions are present. Comparison of the specific heat at low temperature raise the possibility that the density of states at low energy in Volborthite might be much lower than in the Heisenberg model. Magnetization curves under an applied field of the model are also investigated. The M=1/3 plateau is found to subsist in the anisotropic case and extend to lower field with increased anisotropy. For sufficient anisotropy, this plateau would then be observable for a field reasonably accessible to experiment. The absence of a plateau well below $\sim$ 70 Teslas would further support a nearly isotropic model.
cond-mat.str-el
thermodynamic properties such as magnetic susceptibility and specific heat have been computed for the heisenberg antiferromagnet with spatially anisotropic exchange on the kagome lattice on clusters up to n24 spins from the full spectra obtained by exact diagonalization this approach is shown to provide a good represention of these thermodynamic properties above temperatures of about j_rm av5 where j_rm av is an average of the coupling constants comparison with experimental volborthite data obtained by hiroi it et al j phys soc jpn bf 703377 2001 shows that volborthite is best described by a model with nearly isotropic exchanges in spite of the significant distortion of the kagome lattice of magnetic sites in this compound and suggests that additional interactions are present comparison of the specific heat at low temperature raise the possibility that the density of states at low energy in volborthite might be much lower than in the heisenberg model magnetization curves under an applied field of the model are also investigated the m13 plateau is found to subsist in the anisotropic case and extend to lower field with increased anisotropy for sufficient anisotropy this plateau would then be observable for a field reasonably accessible to experiment the absence of a plateau well below sim 70 teslas would further support a nearly isotropic model
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707.4265
Traces on pseudodifferential operators and sums of commutators
The aim of this paper is to show that various known characterizations of traces on classical pseudodifferentials operators (PsiDOs) can actually be obtained by very elementary considerations on PsiDOs, using only basic properties of these operators. Thereby, we give a unified treatment of the determinations of the space of traces (i) on PsiDOs of noninteger orders or of regular parity-class, (ii) on integer order PsiDOs, (iii) on nonpositive order PsiDOs in dimension greather than or equal to 2, and (iv) on nonpositive order PsiDOs in dimension 1.
math.AP math.OA
the aim of this paper is to show that various known characterizations of traces on classical pseudodifferentials operators psidos can actually be obtained by very elementary considerations on psidos using only basic properties of these operators thereby we give a unified treatment of the determinations of the space of traces i on psidos of noninteger orders or of regular parityclass ii on integer order psidos iii on nonpositive order psidos in dimension greather than or equal to 2 and iv on nonpositive order psidos in dimension 1
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707.4266
Representation of Integral Dispersion Relations by Local Forms
The representation of the usual integral dispersion relations (IDR) of scattering theory through series of derivatives of the amplitudes is discussed, extended, simplified, and confirmed as mathematical identities. Forms of derivative dispersion relations (DDR) valid for the whole energy interval, recently obtained and presented as double infinite series, are simplified through the use of new sum rules of the incomplete $\Gamma$ functions, being reduced to single summations, where the usual convergence criteria are easily applied. For the forms of the imaginary amplitude used in phenomenology of hadronic scattering, we show that expressions for the DDR can represent, with absolute accuracy, the IDR of scattering theory, as true mathematical identities. Besides the fact that the algebraic manipulation can be easily understood, numerical examples show the accuracy of these representations up to the maximum available machine precision. As consequence of our work, it is concluded that the standard simplified forms sDDR, originally intended for the high energy limits, are an inconvenient and incomplete separation of terms of the full expression, leading to wrong evaluations. Since the correspondence between IDR and the DDR expansions is linear, our results have wide applicability, covering more general functions, built as combinations of well studied basic forms.
hep-ph
the representation of the usual integral dispersion relations idr of scattering theory through series of derivatives of the amplitudes is discussed extended simplified and confirmed as mathematical identities forms of derivative dispersion relations ddr valid for the whole energy interval recently obtained and presented as double infinite series are simplified through the use of new sum rules of the incomplete gamma functions being reduced to single summations where the usual convergence criteria are easily applied for the forms of the imaginary amplitude used in phenomenology of hadronic scattering we show that expressions for the ddr can represent with absolute accuracy the idr of scattering theory as true mathematical identities besides the fact that the algebraic manipulation can be easily understood numerical examples show the accuracy of these representations up to the maximum available machine precision as consequence of our work it is concluded that the standard simplified forms sddr originally intended for the high energy limits are an inconvenient and incomplete separation of terms of the full expression leading to wrong evaluations since the correspondence between idr and the ddr expansions is linear our results have wide applicability covering more general functions built as combinations of well studied basic forms
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707.4267
An Explicit Construction of Type A Demazure Atoms
Demazure characters of type A, which are equivalent to key polynomials, have been decomposed by Lascoux and Sch\"{u}tzenberger into standard bases. We prove that the resulting polynomials, which we call Demazure atoms, can be obtained from a certain specialization of nonsymmetric Macdonald polynomials. This combinatorial interpretation for Demazure atoms accelerates the computation of the right key associated to a semi-standard Young tableau. Utilizing a related construction, we provide a new combinatorial description for the key polynomials.
math.CO math.RT
demazure characters of type a which are equivalent to key polynomials have been decomposed by lascoux and schutzenberger into standard bases we prove that the resulting polynomials which we call demazure atoms can be obtained from a certain specialization of nonsymmetric macdonald polynomials this combinatorial interpretation for demazure atoms accelerates the computation of the right key associated to a semistandard young tableau utilizing a related construction we provide a new combinatorial description for the key polynomials
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707.4268
HAT-P-3b: A heavy-element rich planet transiting a K dwarf star
We report the discovery of a Jupiter-size planet transiting a relatively bright (V = 11.56) and metal-rich early K dwarf star with a period of about 2.9 days. On the basis of follow-up photometry and spectroscopy we determine the mass and radius of the planet, HAT-P-3b, to be M_p = 0.599 +/- 0.026 M_Jup and R_p = 0.890 +/- 0.046 R_Jup. The relatively small size of the object for its mass implies the presence of about 75 Earth masses worth of heavy elements (1/3 of the total mass) based on current theories of irradiated extrasolar giant planets, similar to the mass of the core inferred for the transiting planet HD 149026b. The bulk density of HAT-P-3b is found to be rho_p = 1.06 +/- 0.17 g/cm^3, and the planet orbits the star at a distance of 0.03894 AU. Ephemerides for the transit centers are T_c = 2,454,218.7594 +/- 0.0029 + N (2.899703 +/- 0.000054) (HJD).
astro-ph
we report the discovery of a jupitersize planet transiting a relatively bright v 1156 and metalrich early k dwarf star with a period of about 29 days on the basis of followup photometry and spectroscopy we determine the mass and radius of the planet hatp3b to be m_p 0599 0026 m_jup and r_p 0890 0046 r_jup the relatively small size of the object for its mass implies the presence of about 75 earth masses worth of heavy elements 13 of the total mass based on current theories of irradiated extrasolar giant planets similar to the mass of the core inferred for the transiting planet hd 149026b the bulk density of hatp3b is found to be rho_p 106 017 gcm3 and the planet orbits the star at a distance of 003894 au ephemerides for the transit centers are t_c 24542187594 00029 n 2899703 0000054 hjd
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707.4269
Structure and randomness in combinatorics
Combinatorics, like computer science, often has to deal with large objects of unspecified (or unusable) structure. One powerful way to deal with such an arbitrary object is to decompose it into more usable components. In particular, it has proven profitable to decompose such objects into a \emph{structured} component, a \emph{pseudo-random} component, and a \emph{small} component (i.e. an error term); in many cases it is the structured component which then dominates. We illustrate this philosophy in a number of model cases.
math.CO
combinatorics like computer science often has to deal with large objects of unspecified or unusable structure one powerful way to deal with such an arbitrary object is to decompose it into more usable components in particular it has proven profitable to decompose such objects into a emphstructured component a emphpseudorandom component and a emphsmall component ie an error term in many cases it is the structured component which then dominates we illustrate this philosophy in a number of model cases
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707.427
AdS4 flux vacua in type II superstrings and their domain-wall solutions
We investigate the emergence of supersymmetric negative-vacuum-energy ground states in four dimensions. First, we rely on the analysis of the effective superpotential, which depends on the background fluxes of the internal manifold, or equivalently has its origin in the underlying gauged supergravity. Four-dimensional, supersymmetric anti-de Sitter vacua with all moduli stabilized appear when appropriate Ramond and Neveu--Schwarz fluxes are introduced in IIA. Geometric fluxes are not necessary. Then the whole setup is analyzed from the perspective of the sources, namely D/NS-branes or Kaluza--Klein monopoles. Orientifold planes are also required for tadpole cancellation. The solutions found in four dimensions correspond to domain walls interpolating between AdS4 and flat spacetime. The various consistency conditions (equations of motion, Bianchi identities and tadpole cancellation conditions) are always satisfied, albeit with source terms. We also speculate on the possibility of assigning (formal) entropies to AdS4 flux vacua via the corresponding dual brane systems.
hep-th
we investigate the emergence of supersymmetric negativevacuumenergy ground states in four dimensions first we rely on the analysis of the effective superpotential which depends on the background fluxes of the internal manifold or equivalently has its origin in the underlying gauged supergravity fourdimensional supersymmetric antide sitter vacua with all moduli stabilized appear when appropriate ramond and neveuschwarz fluxes are introduced in iia geometric fluxes are not necessary then the whole setup is analyzed from the perspective of the sources namely dnsbranes or kaluzaklein monopoles orientifold planes are also required for tadpole cancellation the solutions found in four dimensions correspond to domain walls interpolating between ads4 and flat spacetime the various consistency conditions equations of motion bianchi identities and tadpole cancellation conditions are always satisfied albeit with source terms we also speculate on the possibility of assigning formal entropies to ads4 flux vacua via the corresponding dual brane systems
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707.4271
Many-body excitations in tunneling current spectra of a few-electron quantum dot
Inherent asymmetry in the tunneling barriers of few-electron quantum dots induces intrinsically different tunneling currents for forward and reverse source-drain biases in the non-linear transport regime. Here we show that in addition to spin selection rules, overlap matrix elements between many-body states are crucial for the correct description of tunneling transmission through quantum dots at large magnetic fields. Signatures of excited (N-1)-electron states in the transport process through the N-electron system are clearly identified in the measured transconductances. Our analysis clearly confirms the validity of single-electron quantum transport theory in quantum dots.
cond-mat.mes-hall
inherent asymmetry in the tunneling barriers of fewelectron quantum dots induces intrinsically different tunneling currents for forward and reverse sourcedrain biases in the nonlinear transport regime here we show that in addition to spin selection rules overlap matrix elements between manybody states are crucial for the correct description of tunneling transmission through quantum dots at large magnetic fields signatures of excited n1electron states in the transport process through the nelectron system are clearly identified in the measured transconductances our analysis clearly confirms the validity of singleelectron quantum transport theory in quantum dots
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707.4272
Vacuum Fluctuation (1): the Same Basis of the Relativity and the Quantum Mechanics
The aim of this paper is to reveal the deep relationship between matter and vacuum, and to seek for the same physical basis of the relativity and the quantum mechanics. In doing this, three postulates of vacuum fluctuation are proposed first, the basic premises of the relativity and the quantum mechanics including the velocity limit, the energy-frequency relation and the de Broglie wavelength expression of any matter particles are deduced then. As applications, the idea is used to analyze the Compton effect and the electron-positron annihilation. It is found that the calculation becomes simple, and the physical meaning gets clear. The simplicity comes from the power of the three postulates. To illustrate this, the basic conclusions of the special theory of relativity such as the relations of mass-velocity, mass-energy, energy-momentum, time dilation and length contraction are further deduced. In addition, the significance of the investigation of vacuum fluctuation in the unification of the physical theories is pointed out.
physics.gen-ph
the aim of this paper is to reveal the deep relationship between matter and vacuum and to seek for the same physical basis of the relativity and the quantum mechanics in doing this three postulates of vacuum fluctuation are proposed first the basic premises of the relativity and the quantum mechanics including the velocity limit the energyfrequency relation and the de broglie wavelength expression of any matter particles are deduced then as applications the idea is used to analyze the compton effect and the electronpositron annihilation it is found that the calculation becomes simple and the physical meaning gets clear the simplicity comes from the power of the three postulates to illustrate this the basic conclusions of the special theory of relativity such as the relations of massvelocity massenergy energymomentum time dilation and length contraction are further deduced in addition the significance of the investigation of vacuum fluctuation in the unification of the physical theories is pointed out
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707.4273
A convexity property of expectations under exponential weights
Take a random variable X with some finite exponential moments. Define an exponentially weighted expectation by E^t(f) = E(e^{tX}f)/E(e^{tX}) for admissible values of the parameter t. Denote the weighted expectation of X itself by r(t) = E^t(X), with inverse function t(r). We prove that for a convex function f the expectation E^{t(r)}(f) is a convex function of the parameter r. Along the way we develop correlation inequalities for convex functions. Motivation for this result comes from equilibrium investigations of some stochastic interacting systems with stationary product distributions. In particular, convexity of the hydrodynamic flux function follows in some cases.
math.PR
take a random variable x with some finite exponential moments define an exponentially weighted expectation by etf eetxfeetx for admissible values of the parameter t denote the weighted expectation of x itself by rt etx with inverse function tr we prove that for a convex function f the expectation etrf is a convex function of the parameter r along the way we develop correlation inequalities for convex functions motivation for this result comes from equilibrium investigations of some stochastic interacting systems with stationary product distributions in particular convexity of the hydrodynamic flux function follows in some cases
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707.4274
On dynamical tunneling and classical resonances
This work establishes a firm relationship between classical nonlinear resonances and the phenomenon of dynamical tunneling. It is shown that the classical phase space with its hierarchy of resonance islands completely characterizes dynamical tunneling and explicit forms of the dynamical barriers can be obtained only by identifying the key resonances. Relationship between the phase space viewpoint and the quantum mechanical superexchange approach is discussed in near-integrable and mixed regular-chaotic situations. For near-integrable systems with sufficient anharmonicity the effect of multiple resonances {\it i.e.,} resonance-assisted tunneling can be incorporated approximately. It is also argued that the, presumed, relation of avoided crossings to nonlinear resonances does not have to be invoked in order to understand dynamical tunneling. For molecules with low density of states the resonance-assisted mechanism is expected to be dominant.
nlin.CD
this work establishes a firm relationship between classical nonlinear resonances and the phenomenon of dynamical tunneling it is shown that the classical phase space with its hierarchy of resonance islands completely characterizes dynamical tunneling and explicit forms of the dynamical barriers can be obtained only by identifying the key resonances relationship between the phase space viewpoint and the quantum mechanical superexchange approach is discussed in nearintegrable and mixed regularchaotic situations for nearintegrable systems with sufficient anharmonicity the effect of multiple resonances it ie resonanceassisted tunneling can be incorporated approximately it is also argued that the presumed relation of avoided crossings to nonlinear resonances does not have to be invoked in order to understand dynamical tunneling for molecules with low density of states the resonanceassisted mechanism is expected to be dominant
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707.4275
Sums of the error term function in the mean square for $\zeta(s)$
Sums of the form $\sum_{n\le x}E^k(n) (k\in{\bf N}$ fixed) are investigated, where $$ E(T) = \int_0^T|\zeta(1/2+it)|^2 dt - T\Bigl(\log {T\over2\pi} + 2\gamma -1\Bigr)$$ is the error term in the mean square formula for $|\zeta(1/2+it)|$. The emphasis is on the case k=1, which is more difficult than the corresponding sum for the divisor problem. The analysis requires bounds for the irrationality measure of ${\rm e}^{2\pi m}$ and for the partial quotients in its continued fraction expansion.
math.NT
sums of the form sum_nle xekn kinbf n fixed are investigated where et int_0tzeta12it2 dt tbigllog tover2pi 2gamma 1bigr is the error term in the mean square formula for zeta12it the emphasis is on the case k1 which is more difficult than the corresponding sum for the divisor problem the analysis requires bounds for the irrationality measure of rm e2pi m and for the partial quotients in its continued fraction expansion
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707.4276
Towards precision determination of uPDFs
The unintegrated Parton Density Function of the gluon is obtained from a fit to dijet production in DIS as measured at HERA. Reasonable descriptions of the measurements are obtained, and a first attempt to constrain the intrinsic transverse momentum distribution at small kt is presented
hep-ph
the unintegrated parton density function of the gluon is obtained from a fit to dijet production in dis as measured at hera reasonable descriptions of the measurements are obtained and a first attempt to constrain the intrinsic transverse momentum distribution at small kt is presented
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707.4277
Effects of the CP Odd Dipole Operators on Gluino-Squark Production
We analyze effects of the CP violating interactions on associated gluino-squark production in the MSSM at hadron colliders. Depending on the sparticle masses, the hadronic cross sections can be enhanced up to 9.5 % for a 500 GeV gluino at the LHC energies.
hep-ph
we analyze effects of the cp violating interactions on associated gluinosquark production in the mssm at hadron colliders depending on the sparticle masses the hadronic cross sections can be enhanced up to 95 for a 500 gev gluino at the lhc energies
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707.4278
Rheology of dilute suspensions of vesicles and red blood cells
We present rheology experiments on dilute solutions of vesicles and red blood cells (RBC). Varying the viscosity ratio $\lambda$ between internal and external fluids, the microscopic dynamics of suspended objects can be qualitatively changed from tank-treading ($tt$) to tumbling ($tb$). We find that in the tt regime the viscosity $\eta$, decreases when $\lambda$ increases, in contrast with droplet emulsions and elastic capsule theories which are sometimes invoked to model RBC dynamics. At a critical $\lambda$ (close to the tt-tb transition) $\eta$ exhibits a minimum before it increases in the tb regime. This is consistent with a recent theory for vesicles. This points to the nontrivial fact that the cytoskeleton in RBC does not alter the qualitative evolution of $\eta$ and that, as far as rheology is concerned, vesicle models might be a better description.
cond-mat.soft cond-mat.mtrl-sci
we present rheology experiments on dilute solutions of vesicles and red blood cells rbc varying the viscosity ratio lambda between internal and external fluids the microscopic dynamics of suspended objects can be qualitatively changed from tanktreading tt to tumbling tb we find that in the tt regime the viscosity eta decreases when lambda increases in contrast with droplet emulsions and elastic capsule theories which are sometimes invoked to model rbc dynamics at a critical lambda close to the tttb transition eta exhibits a minimum before it increases in the tb regime this is consistent with a recent theory for vesicles this points to the nontrivial fact that the cytoskeleton in rbc does not alter the qualitative evolution of eta and that as far as rheology is concerned vesicle models might be a better description
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707.4279
Non-Thermal X-ray Properties of Rotation Powered Pulsars and Their Wind Nebulae
We present a statistical study of the non-thermal X-ray emission of 27 young rotation powered pulsars (RPPs) and 24 pulsar wind nebulae (PWNe) by using the Chandra and the XMM-Newton observations, which with the high spatial resolutions enable us to spatially resolve pulsars from their surrounding PWNe. We obtain the X-ray luminosities and spectra separately for RPPs and PWNe, and then investigate their distribution and relation to each other as well as the relation with the pulsar rotational parameters. In the pair-correlation analysis we find that: (1) the X-ray (2-10 keV) luminosities of both pulsar and PWN (L_{psr} and L_{pwn}) display a strong correlation with pulsar spin down power Edot and characteristic age, and the scalings resulting from a simple linear fit to the data are L_{psr} \propto Edot^{0.92 \pm 0.04} and L_{pwn} \propto Edot^{1.45 \pm 0.08} (68% confidence level), respectively, however, both the fits are not statistically acceptable; (2) L_{psr} also shows a possible weak correlation with pulsar period P and period derivative Pdot, whereas L_{pwn} manifests a similar weak correlation with Pdot only; (3) The PWN photon index Gamma_{pwn} is positively correlated with L_{pwn} and L_{pwn}/Edot. We also found that the PWN X-ray luminosity is typically 1 to 10 times larger than that from the underlying pulsar, and the PWN photon indices span a range of ~1.5 to ~2. The statistic study of PWN spectral properties supports the particle wind model in which the X-ray emitting electrons are accelerated by the termination shock of the wind.
astro-ph
we present a statistical study of the nonthermal xray emission of 27 young rotation powered pulsars rpps and 24 pulsar wind nebulae pwne by using the chandra and the xmmnewton observations which with the high spatial resolutions enable us to spatially resolve pulsars from their surrounding pwne we obtain the xray luminosities and spectra separately for rpps and pwne and then investigate their distribution and relation to each other as well as the relation with the pulsar rotational parameters in the paircorrelation analysis we find that 1 the xray 210 kev luminosities of both pulsar and pwn l_psr and l_pwn display a strong correlation with pulsar spin down power edot and characteristic age and the scalings resulting from a simple linear fit to the data are l_psr propto edot092 pm 004 and l_pwn propto edot145 pm 008 68 confidence level respectively however both the fits are not statistically acceptable 2 l_psr also shows a possible weak correlation with pulsar period p and period derivative pdot whereas l_pwn manifests a similar weak correlation with pdot only 3 the pwn photon index gamma_pwn is positively correlated with l_pwn and l_pwnedot we also found that the pwn xray luminosity is typically 1 to 10 times larger than that from the underlying pulsar and the pwn photon indices span a range of 15 to 2 the statistic study of pwn spectral properties supports the particle wind model in which the xray emitting electrons are accelerated by the termination shock of the wind
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707.428
Fast ion diffusion, superionic conductivity and phase transitions of the nuclear materials UO2 and Li2O
Lattice dynamics and molecular dynamics studies of the oxides UO2 and Li2O in their normal as well as superionic phase are reported. Lattice dynamics calculations have been carried out using a shell model in the quasiharmonic approximation. The calculated elastic constants, phonon frequencies and specific heat are in good agreement with reported experimental data, which help validate the interatomic potentials required for undertaking molecular dynamics simulations. The calculated free energies reveal high pressure fluorite to cottunite phase transitions at 70 GPa for UO2 and anti-fluorite to anti-cotunnite phase transformation at 25 GPa for Li2O, in agreement with reported experiments. Molecular dynamics studies shed important insights into the mechanisms of diffusion and superionic behavior at high temperatures. The calculated superionic transition temperature of Li2O is 1000 K, while that of UO2 is 2300 K.
cond-mat.mtrl-sci cond-mat.other
lattice dynamics and molecular dynamics studies of the oxides uo2 and li2o in their normal as well as superionic phase are reported lattice dynamics calculations have been carried out using a shell model in the quasiharmonic approximation the calculated elastic constants phonon frequencies and specific heat are in good agreement with reported experimental data which help validate the interatomic potentials required for undertaking molecular dynamics simulations the calculated free energies reveal high pressure fluorite to cottunite phase transitions at 70 gpa for uo2 and antifluorite to anticotunnite phase transformation at 25 gpa for li2o in agreement with reported experiments molecular dynamics studies shed important insights into the mechanisms of diffusion and superionic behavior at high temperatures the calculated superionic transition temperature of li2o is 1000 k while that of uo2 is 2300 k
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707.4281
Central and Local Limit Theorems for RNA Structures
A k-noncrossing RNA pseudoknot structure is a graph over $\{1,...,n\}$ without 1-arcs, i.e. arcs of the form (i,i+1) and in which there exists no k-set of mutually intersecting arcs. In particular, RNA secondary structures are 2-noncrossing RNA structures. In this paper we prove a central and a local limit theorem for the distribution of the numbers of 3-noncrossing RNA structures over n nucleotides with exactly h bonds. We will build on the results of \cite{Reidys:07rna1} and \cite{Reidys:07rna2}, where the generating function of k-noncrossing RNA pseudoknot structures and the asymptotics for its coefficients have been derived. The results of this paper explain the findings on the numbers of arcs of RNA secondary structures obtained by molecular folding algorithms and predict the distributions for k-noncrossing RNA folding algorithms which are currently being developed.
math.CO q-bio.QM
a knoncrossing rna pseudoknot structure is a graph over 1n without 1arcs ie arcs of the form ii1 and in which there exists no kset of mutually intersecting arcs in particular rna secondary structures are 2noncrossing rna structures in this paper we prove a central and a local limit theorem for the distribution of the numbers of 3noncrossing rna structures over n nucleotides with exactly h bonds we will build on the results of citereidys07rna1 and citereidys07rna2 where the generating function of knoncrossing rna pseudoknot structures and the asymptotics for its coefficients have been derived the results of this paper explain the findings on the numbers of arcs of rna secondary structures obtained by molecular folding algorithms and predict the distributions for knoncrossing rna folding algorithms which are currently being developed
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707.4282
Matrix and vector models in the strong coupling limit
In this paper we consider matrix and vector models in the large N limit ($N \times N$ matrices and vectors with N^{2} components). For the case of zero-dimensional model (D=0) it is proved that in the strong coupling limit $g \to \infty$ statistical sums of both models coincide up to a coefficient. This is also true for D=1.
hep-th
in this paper we consider matrix and vector models in the large n limit n times n matrices and vectors with n2 components for the case of zerodimensional model d0 it is proved that in the strong coupling limit g to infty statistical sums of both models coincide up to a coefficient this is also true for d1
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707.4283
Voids in the SDSS Galaxy Survey
Using the method of searching for arbitrary shaped voids in the distribution of volume-limited samples of galaxies from the DR5 SDSS survey, we have identified voids and investigated their characteristics and the change in these characteristics with decreasing Mlim - the upper limit on the absolute magnitude of the galaxies involved in the construction of voids. The total volume of the 50 largest voids increases with decreasing Mlim with a break near Mr* = -20.44 for SDSS galaxies. The mean density contrast in voids increases with decreasing Mlim also with a weak break near M*. The exponent of the dependence of the volume of a void on its rank increases significantly with decreasing Mlim starting from Mlim ~ -20.4 in the characteristic range of volumes, which reflects the tendency for greater clustering of brighter galaxies. The galaxies mostly tend to concentrate toward the void boundaries and to avoid the central void regions. The axial ratios of the ellipsoids equivalent to the voids are, on average, retained with changing Mlim and correspond to elongated and nonoblate void shapes, but some of the voids can change their shape significantly. The void centers show correlations reflecting the correlations of the galaxy distribution on scales (35-70)/h Mpc. The galaxy distribution in the identified voids is nonrandom - groups and filaments can be identified. We have compared the properties of the galaxies in voids and galaxies in structures identified using the minimum spanning tree. A noticeable difference is observed in the mean color indices and star formation rates per unit stellar mass of the galaxies in dense regions (structures) - as expected, the galaxies in voids are, on average, bluer and have higher log(SFR/M_star). These tendencies become stronger toward the central void regions.
astro-ph
using the method of searching for arbitrary shaped voids in the distribution of volumelimited samples of galaxies from the dr5 sdss survey we have identified voids and investigated their characteristics and the change in these characteristics with decreasing mlim the upper limit on the absolute magnitude of the galaxies involved in the construction of voids the total volume of the 50 largest voids increases with decreasing mlim with a break near mr 2044 for sdss galaxies the mean density contrast in voids increases with decreasing mlim also with a weak break near m the exponent of the dependence of the volume of a void on its rank increases significantly with decreasing mlim starting from mlim 204 in the characteristic range of volumes which reflects the tendency for greater clustering of brighter galaxies the galaxies mostly tend to concentrate toward the void boundaries and to avoid the central void regions the axial ratios of the ellipsoids equivalent to the voids are on average retained with changing mlim and correspond to elongated and nonoblate void shapes but some of the voids can change their shape significantly the void centers show correlations reflecting the correlations of the galaxy distribution on scales 3570h mpc the galaxy distribution in the identified voids is nonrandom groups and filaments can be identified we have compared the properties of the galaxies in voids and galaxies in structures identified using the minimum spanning tree a noticeable difference is observed in the mean color indices and star formation rates per unit stellar mass of the galaxies in dense regions structures as expected the galaxies in voids are on average bluer and have higher logsfrm_star these tendencies become stronger toward the central void regions
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707.4284
Structure Functions and Low-x
We summarize recent experimental and theoretical results, which were reported in the working group on Structure Functions and Low-x at the DIS 2007 workshop.
hep-ph
we summarize recent experimental and theoretical results which were reported in the working group on structure functions and lowx at the dis 2007 workshop
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707.4285
Spectroscopy of two PN candidates in IC10
We present the results of the first spectroscopic observations of two planetary nebula (PN) candidates in the Local Group dwarf irregular galaxy IC10. Using several spectral classification diagrams we show that the brightest PN candidate (PN7) is not a PN, but rather a compact HII region consisting of two components with low electron number densities. After the rejection of this PN candidate, the IC10 planetary nebula luminosity function cutoff becomes very close to the standard value. With the compiled spectroscopic data for a large number of extragalactic PNe, we analyse a series of diagnostic diagrams to generate quantitative criteria for separating PNe from unresolved HII regions. We show that, with the help of the diagnostic diagrams and the derived set of criteria, PNe can be distinguished from HII regions with an efficiency of ~99.6%. With the obtained spectroscopic data we confirm that another, 1.7 mag fainter PN candidate (PN9) is a genuine PN. We argue that, based on all currently available PNe data, IC10 is located at a distance 725+63-33 kpc (distance modulus (m-M) = 24.30+0.18-0.10).
astro-ph
we present the results of the first spectroscopic observations of two planetary nebula pn candidates in the local group dwarf irregular galaxy ic10 using several spectral classification diagrams we show that the brightest pn candidate pn7 is not a pn but rather a compact hii region consisting of two components with low electron number densities after the rejection of this pn candidate the ic10 planetary nebula luminosity function cutoff becomes very close to the standard value with the compiled spectroscopic data for a large number of extragalactic pne we analyse a series of diagnostic diagrams to generate quantitative criteria for separating pne from unresolved hii regions we show that with the help of the diagnostic diagrams and the derived set of criteria pne can be distinguished from hii regions with an efficiency of 996 with the obtained spectroscopic data we confirm that another 17 mag fainter pn candidate pn9 is a genuine pn we argue that based on all currently available pne data ic10 is located at a distance 7256333 kpc distance modulus mm 2430018010
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707.4286
Symmetry Supporting a Transition to Zero Cosmological Constant State
In a number of previous publications we demonstrated that the Two Measures Field Theory (TMT) enables to resolve the old cosmological constant (CC) problem avoiding the Weinberg's no-go CC theorem and together with this TMT agrees with all tests of the Einstein's general relativity and allows inflationary scenarios. Analysis performed in the present paper shows that there exists an intrinsic symmetry of TMT which emerges in the $\Lambda =0$ ground state. This symmetry contains a subgroup of reflections of the metric $g_{\mu\nu}\to -g_{\mu\nu}$ studied recently by a number of authors as the symmetry imposing zero CC. We show that realization of this idea in TMT is free of fine tuning and has no problems typical to other approaches.
hep-th astro-ph gr-qc
in a number of previous publications we demonstrated that the two measures field theory tmt enables to resolve the old cosmological constant cc problem avoiding the weinbergs nogo cc theorem and together with this tmt agrees with all tests of the einsteins general relativity and allows inflationary scenarios analysis performed in the present paper shows that there exists an intrinsic symmetry of tmt which emerges in the lambda 0 ground state this symmetry contains a subgroup of reflections of the metric g_munuto g_munu studied recently by a number of authors as the symmetry imposing zero cc we show that realization of this idea in tmt is free of fine tuning and has no problems typical to other approaches
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707.4287
Effective Iitaka fibrations
We show that the M-canonical map of an n-dimensional complex projective manifold X of Kodaira dimension two is birational to an Iitaka fibration for a computable positive integer M. M depends on the index b of a general fibre F of the Iitaka fibration and on the Betti number of the canonical covering of F, In particular, M is a universal constant if the dimension n is smaller than or equal to 4.
math.AG math.CV
we show that the mcanonical map of an ndimensional complex projective manifold x of kodaira dimension two is birational to an iitaka fibration for a computable positive integer m m depends on the index b of a general fibre f of the iitaka fibration and on the betti number of the canonical covering of f in particular m is a universal constant if the dimension n is smaller than or equal to 4
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707.4288
The metallicity extremes of the Sagittarius dSph using SALT spectroscopy of PNe
In this work we present the first spectroscopic results obtained with the Southern African Large Telescope (SALT) telescope during its perfomance-verification phase. We find that the Sagittarius dwarf spheroidal galaxy (Sgr) Sgr contains a youngest stellar population with [O/H] -0.2 and age t>1 Gyr, and an oldest population with [O/H]=-2.0. The values are based on spectra of two planetary nebulae (PNe), using empirical abundance determinations. We calculated abundances for O, N, Ne, Ar, S, Cl, Fe, C and He. We confirm the high abundances of PN StWr2-21 with 12+log(O/H) = 8.57+/-0.02 dex. The other PN studied, BoBn1, is an extraordinary object in that the neon abundance exceeds that of oxygen. The abundances of S, Ar and Cl in BoBn1 yield the original stellar metallicity, corresponding to 12+log(O/H) = 6.72+/-0.16 dex which is 1/110 of the solar value. The actual [O/H] is much higher: third dredge-up enriched the material by a factor of ~12 in oxygen, ~240 in nitrogen and ~70 in neon. Neon as well as nitrogen and oxygen content may have been produced in the intershell of low-mass AGB stars. Well defined broad WR lines are present in the spectrum of StWr2-21 and absent in the spectrum of BoBn1. This puts the fraction of [WR]-type central PNe stars to 67% for dSph galaxies.
astro-ph
in this work we present the first spectroscopic results obtained with the southern african large telescope salt telescope during its perfomanceverification phase we find that the sagittarius dwarf spheroidal galaxy sgr sgr contains a youngest stellar population with oh 02 and age t1 gyr and an oldest population with oh20 the values are based on spectra of two planetary nebulae pne using empirical abundance determinations we calculated abundances for o n ne ar s cl fe c and he we confirm the high abundances of pn stwr221 with 12logoh 857002 dex the other pn studied bobn1 is an extraordinary object in that the neon abundance exceeds that of oxygen the abundances of s ar and cl in bobn1 yield the original stellar metallicity corresponding to 12logoh 672016 dex which is 1110 of the solar value the actual oh is much higher third dredgeup enriched the material by a factor of 12 in oxygen 240 in nitrogen and 70 in neon neon as well as nitrogen and oxygen content may have been produced in the intershell of lowmass agb stars well defined broad wr lines are present in the spectrum of stwr221 and absent in the spectrum of bobn1 this puts the fraction of wrtype central pne stars to 67 for dsph galaxies
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707.4289
A Leaf Recognition Algorithm for Plant Classification Using Probabilistic Neural Network
In this paper, we employ Probabilistic Neural Network (PNN) with image and data processing techniques to implement a general purpose automated leaf recognition algorithm. 12 leaf features are extracted and orthogonalized into 5 principal variables which consist the input vector of the PNN. The PNN is trained by 1800 leaves to classify 32 kinds of plants with an accuracy greater than 90%. Compared with other approaches, our algorithm is an accurate artificial intelligence approach which is fast in execution and easy in implementation.
cs.AI
in this paper we employ probabilistic neural network pnn with image and data processing techniques to implement a general purpose automated leaf recognition algorithm 12 leaf features are extracted and orthogonalized into 5 principal variables which consist the input vector of the pnn the pnn is trained by 1800 leaves to classify 32 kinds of plants with an accuracy greater than 90 compared with other approaches our algorithm is an accurate artificial intelligence approach which is fast in execution and easy in implementation
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707.429
On deformations of maps and curve singularities
We study several deformation functors associated to the normalization of a reduced curve singularity $(X,0) \subset (\c^n,0)$. The main new results are explicit formulas, in terms of classical invariants of (X,0), for the cotangent cohomology groups $T^i, i = 0,1,2,$ of these functors. Thus we obtain precise statements about smoothness and dimension of the corresponding local moduli spaces. We apply the results to obtain explicit formulas resp. estimates for the $\hoa{A}_e$-codimension of a parametrized curve singularity, where $\hoa{A}_e$ denotes the Mather-Wall group of left-right equivalence.
math.AG math.AC
we study several deformation functors associated to the normalization of a reduced curve singularity x0 subset cn0 the main new results are explicit formulas in terms of classical invariants of x0 for the cotangent cohomology groups ti i 012 of these functors thus we obtain precise statements about smoothness and dimension of the corresponding local moduli spaces we apply the results to obtain explicit formulas resp estimates for the hoaa_ecodimension of a parametrized curve singularity where hoaa_e denotes the matherwall group of leftright equivalence
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707.4291
Specific Density Of Binding Enerfy Of Core In Beta - Stable Nuclei is 2.57 MeV/fm^3
Recently an alpha-cluster model based on the pn-pair interactions with using the isospin invariance of nuclear force has been proposed. According to the model the excess neutron pairs fill out the free space in the core determined by the difference in the charge and matter radii of the alpha-clusters. Then the number of excess neutrons in beta-stable nuclei depends on the number of the core alpha-clusters. In such a representation the specific density of binding energy of core is the only parameter to fit the experimental binding energies of beta-stable nuclei and it turned out to be a constant value equal to 2.57 MeV/fm^3. Knowing the value allows one to estimate the size of a nucleus from its experimental binding energy.
nucl-th
recently an alphacluster model based on the pnpair interactions with using the isospin invariance of nuclear force has been proposed according to the model the excess neutron pairs fill out the free space in the core determined by the difference in the charge and matter radii of the alphaclusters then the number of excess neutrons in betastable nuclei depends on the number of the core alphaclusters in such a representation the specific density of binding energy of core is the only parameter to fit the experimental binding energies of betastable nuclei and it turned out to be a constant value equal to 257 mevfm3 knowing the value allows one to estimate the size of a nucleus from its experimental binding energy
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707.4292
Spectral asymptotics of percolation Hamiltonians on amenable Cayley graphs
In this paper we study spectral properties of adjacency and Laplace operators on percolation subgraphs of Cayley graphs of amenable, finitely generated groups. In particular we describe the asymptotic behaviour of the integrated density of states (spectral distribution function) of these random Hamiltonians near the spectral minimum. The first part of the note discusses various aspects of the quantum percolation model, subsequently we formulate a series of new results, and finally we outline the strategy used to prove our main theorem.
math.SP math-ph math.GR math.MP
in this paper we study spectral properties of adjacency and laplace operators on percolation subgraphs of cayley graphs of amenable finitely generated groups in particular we describe the asymptotic behaviour of the integrated density of states spectral distribution function of these random hamiltonians near the spectral minimum the first part of the note discusses various aspects of the quantum percolation model subsequently we formulate a series of new results and finally we outline the strategy used to prove our main theorem
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707.4293
Modeling Dense Stellar Systems
Black holes and neutron stars present extreme forms of matter that cannot be created as such in a laboratory on Earth. Instead, we have to observe and analyze the experiments that are ongoing in the Universe. The most telling observations of black holes and neutron stars come from dense stellar systems, where stars are crowded close enough to each other to undergo frequent interactions. It is the interplay between black holes, neutron stars and other objects in a dense environment that allows us to use observations to draw firm conclusions about the properties of these extreme forms of matter, through comparisons with simulations. The art of modeling dense stellar systems through computer simulations forms the main topic of this review.
astro-ph
black holes and neutron stars present extreme forms of matter that cannot be created as such in a laboratory on earth instead we have to observe and analyze the experiments that are ongoing in the universe the most telling observations of black holes and neutron stars come from dense stellar systems where stars are crowded close enough to each other to undergo frequent interactions it is the interplay between black holes neutron stars and other objects in a dense environment that allows us to use observations to draw firm conclusions about the properties of these extreme forms of matter through comparisons with simulations the art of modeling dense stellar systems through computer simulations forms the main topic of this review
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707.4294
Spin coherence of a two-dimensional electron gas induced by resonant excitation of trions and excitons in CdTe/(Cd,Mg)Te quantum wells
The mechanisms for generation of long-lived spin coherence in a two-dimensional electron gas (2DEG) have been studied experimentally by means of a picosecond pump-probe Kerr rotation technique. CdTe/(Cd,Mg)Te quantum wells with a diluted 2DEG were investigated. The strong Coulomb interaction between electrons and holes, which results in large binding energies of neutral excitons and negatively charged excitons (trions), allows one to address selectively the exciton or trion states by resonant optical excitation. Different scenarios of spin coherence generation were analyzed theoretically, among them the direct trion photocreation, the formation of trions from photogenerated excitons and the electron-exciton exchange scattering. Good agreement between experiment and theory is found.
cond-mat.mes-hall cond-mat.mtrl-sci cond-mat.other
the mechanisms for generation of longlived spin coherence in a twodimensional electron gas 2deg have been studied experimentally by means of a picosecond pumpprobe kerr rotation technique cdtecdmgte quantum wells with a diluted 2deg were investigated the strong coulomb interaction between electrons and holes which results in large binding energies of neutral excitons and negatively charged excitons trions allows one to address selectively the exciton or trion states by resonant optical excitation different scenarios of spin coherence generation were analyzed theoretically among them the direct trion photocreation the formation of trions from photogenerated excitons and the electronexciton exchange scattering good agreement between experiment and theory is found
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707.4295
Task-Oriented Maximally Entangled States
We introduce the notion of a task-oriented maximally entangled state (TMES). This notion depends on the tasks for which a quantum state is used as the resource. This concept may be more fruitful than that of a general maximally entangled state in the case of a multipartite system. We illustrate this idea by giving an operational definition of maximally entangled states on the basis of communication tasks of teleportation and superdense coding. We also give examples and a procedure to obtain such TMESs for {\em n}-qubit systems.
quant-ph
we introduce the notion of a taskoriented maximally entangled state tmes this notion depends on the tasks for which a quantum state is used as the resource this concept may be more fruitful than that of a general maximally entangled state in the case of a multipartite system we illustrate this idea by giving an operational definition of maximally entangled states on the basis of communication tasks of teleportation and superdense coding we also give examples and a procedure to obtain such tmess for em nqubit systems
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707.4296
Infrared renormalization of two-loop integrals and the chiral expansion of the nucleon mass
We describe details of the renormalization of two-loop integrals relevant to the calculation of the nucleon mass in the framework of manifestly Lorentz-invariant chiral perturbation theory using infrared renormalization. It is shown that the renormalization can be performed while preserving all relevant symmetries, in particular chiral symmetry, and that renormalized diagrams respect the standard power counting rules. As an application we calculate the chiral expansion of the nucleon mass to order O(q^6).
hep-ph
we describe details of the renormalization of twoloop integrals relevant to the calculation of the nucleon mass in the framework of manifestly lorentzinvariant chiral perturbation theory using infrared renormalization it is shown that the renormalization can be performed while preserving all relevant symmetries in particular chiral symmetry and that renormalized diagrams respect the standard power counting rules as an application we calculate the chiral expansion of the nucleon mass to order oq6
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707.4297
Eigenvalue clusters of the Landau Hamiltonian in the exterior of a compact domain
We consider the Schrodinger operator with a constant magnetic field in the exterior of a compact domain on the plane. The spectrum of this operator consists of clusters of eigenvalues around the Landau levels. We discuss the rate of accumulation of eigenvalues in a fixed cluster.
math.SP math-ph math.MP
we consider the schrodinger operator with a constant magnetic field in the exterior of a compact domain on the plane the spectrum of this operator consists of clusters of eigenvalues around the landau levels we discuss the rate of accumulation of eigenvalues in a fixed cluster
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707.4298
A note on equipartition
The problem of the existence of an equi-partition of a curve in $\R^n$ has recently been raised in the context of computational geometry. The problem is to show that for a (continuous) curve $\Gamma : [0,1] \to \R^n$ and for any positive integer N, there exist points $t_0=0<t_1<...<t_{N-1}<1=t_N$, such that $d(\Gamma(t_{i-1}),\Gamma(t_i))=d(\Gamma(t_{i}),\Gamma(t_{i+1}))$ for all $i=1,...,N$, where d is a metric or even a semi-metric (a weaker notion) on $\R^n$. We show here that the existence of such points, in a broader context, is a consequence of Brower's fixed point theorem.
cs.CG math.FA
the problem of the existence of an equipartition of a curve in rn has recently been raised in the context of computational geometry the problem is to show that for a continuous curve gamma 01 to rn and for any positive integer n there exist points t_00t_1t_n11t_n such that dgammat_i1gammat_idgammat_igammat_i1 for all i1n where d is a metric or even a semimetric a weaker notion on rn we show here that the existence of such points in a broader context is a consequence of browers fixed point theorem
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707.4299
Neumann Heat kernel monotonicity
We prove that the diagonal of the transition probabilities for the d-dimensional Bessel processes on (0, 1], reflected at 1, which we denote by $p_R^N(t, r,r)$, is an increasing function of r for d>2 and that this is false for d=2.
math.PR
we prove that the diagonal of the transition probabilities for the ddimensional bessel processes on 0 1 reflected at 1 which we denote by p_rnt rr is an increasing function of r for d2 and that this is false for d2
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707.43
Volume and homology of one-cusped hyperbolic 3-manifolds
Let M be a complete, finite-volume, orientable hyperbolic manifold having exactly one cusp. If we assume that pi_1(M) has no subgroup isomorphic to a genus-2 surface group, and that either (a) H_1(M;Z_p) has dimension at least 5 for some prime p, or (b) H_1(M;Z_2) has dimension at least 4, and the subspace of H^2(M;Z_2) spanned by the image of the cup product has dimension at most 1, then vol M > 5.06 If we assume that H_1(M;Z_2) has dimension at least 7, and that the compact core of M does not contain a genus-2 closed incompressible surface, then vol M > 5.06.
math.GT
let m be a complete finitevolume orientable hyperbolic manifold having exactly one cusp if we assume that pi_1m has no subgroup isomorphic to a genus2 surface group and that either a h_1mz_p has dimension at least 5 for some prime p or b h_1mz_2 has dimension at least 4 and the subspace of h2mz_2 spanned by the image of the cup product has dimension at most 1 then vol m 506 if we assume that h_1mz_2 has dimension at least 7 and that the compact core of m does not contain a genus2 closed incompressible surface then vol m 506
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707.4301
Resonance sticking in the scattered disk
We investigate the dynamical evolution of trans-Neptunian objects (TNOs) in typical scattered disk orbits (scattered TNOs) by performing simulations using several thousand particles lying initially on Neptune-encountering orbits. We explore the role of resonance sticking in the scattered disk, a phenomenon characterized by multiple temporary resonance captures ('resonances' refers to external mean motion resonances with Neptune, which can be described in the form r:s, where the arguments r and s are integers). First, all scattered TNOs evolve through intermittent temporary resonance capture events and gravitational scattering by Neptune. Each scattered TNO experiences tens to hundreds of resonance captures over a period of 4 Gyr, which represents about 38% of the object's lifetime (mean value). Second, resonance sticking plays an important role at semimajor axes a < 250 AU, where the great majority of such captures occurred. It is noteworthy that the stickiest (i.e., dominant) resonances in the scattered disk are located within this distance range and are those possessing the lowest argument s. This was evinced by r:1, r:2 and r:3 resonances, which played the greatest role during resonance sticking evolution, often leading to captures in several of their neighboring resonances. Finally, the timescales and likelihood of temporary resonance captures are roughly proportional to resonance strength. The dominance of low s resonances is also related to the latter. In sum, resonance sticking has an important impact on the evolution of scattered TNOs, contributing significantly to the longevity of these objects.
astro-ph physics.comp-ph
we investigate the dynamical evolution of transneptunian objects tnos in typical scattered disk orbits scattered tnos by performing simulations using several thousand particles lying initially on neptuneencountering orbits we explore the role of resonance sticking in the scattered disk a phenomenon characterized by multiple temporary resonance captures resonances refers to external mean motion resonances with neptune which can be described in the form rs where the arguments r and s are integers first all scattered tnos evolve through intermittent temporary resonance capture events and gravitational scattering by neptune each scattered tno experiences tens to hundreds of resonance captures over a period of 4 gyr which represents about 38 of the objects lifetime mean value second resonance sticking plays an important role at semimajor axes a 250 au where the great majority of such captures occurred it is noteworthy that the stickiest ie dominant resonances in the scattered disk are located within this distance range and are those possessing the lowest argument s this was evinced by r1 r2 and r3 resonances which played the greatest role during resonance sticking evolution often leading to captures in several of their neighboring resonances finally the timescales and likelihood of temporary resonance captures are roughly proportional to resonance strength the dominance of low s resonances is also related to the latter in sum resonance sticking has an important impact on the evolution of scattered tnos contributing significantly to the longevity of these objects
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707.4302
Quenching of high-pT hadrons: Alternative scenario
A new scenario, alternative to energy loss, for the observed suppression of high-pT hadrons observed at RHIC is proposed. In the limit of a very dense medium crated in nuclear collisions the mean free-path of the produced (pre)hadron vanishes, and and the nuclear suppression, R_{AA} is completely controlled by the production length. The RHIC data are well explained in a parameter free way, and predictions for LHC are provided.
nucl-th hep-ph
a new scenario alternative to energy loss for the observed suppression of highpt hadrons observed at rhic is proposed in the limit of a very dense medium crated in nuclear collisions the mean freepath of the produced prehadron vanishes and and the nuclear suppression r_aa is completely controlled by the production length the rhic data are well explained in a parameter free way and predictions for lhc are provided
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707.4303
Heterotic Coset Models of Microscopic Strings and Black Holes
Following a recent conjecture by Lapan, Simons and Strominger, we revisit and discuss an intrinsically heterotic class of conformal field theories, emphasizing their Lagrangian construction as asymmetrically gauged WZW models, which may be useful in several applications to the study of supersymmetric strings and black holes in heterotic and type II string theory compactified on T^6 and K3 X T^2 respectively. In these cases, the leading supergravity geometry is singular, but higher order corrections remove this singularity in a way that is consistent with, for example the non-zero entropy for the black holes that these strings form after wrapping on an additional circle. The conformal field theories have the right structure to capture the features of the supergravity analysis, and possess precisely the microscopic target spaces required. We describe in detail the model with AdS_3 X S^2 geometry, which is conjectured by Lapan et. al. to represent a fundamental heterotic string in five dimensions, and then propose conformal field theories which are potential candidates for the microscopic geometry of heterotic strings in $D$ dimensions, with target space AdS_3 X S^{D-3}. We also discuss some conformal field theories that give microscopic AdS target spaces in various dimensions.
hep-th
following a recent conjecture by lapan simons and strominger we revisit and discuss an intrinsically heterotic class of conformal field theories emphasizing their lagrangian construction as asymmetrically gauged wzw models which may be useful in several applications to the study of supersymmetric strings and black holes in heterotic and type ii string theory compactified on t6 and k3 x t2 respectively in these cases the leading supergravity geometry is singular but higher order corrections remove this singularity in a way that is consistent with for example the nonzero entropy for the black holes that these strings form after wrapping on an additional circle the conformal field theories have the right structure to capture the features of the supergravity analysis and possess precisely the microscopic target spaces required we describe in detail the model with ads_3 x s2 geometry which is conjectured by lapan et al to represent a fundamental heterotic string in five dimensions and then propose conformal field theories which are potential candidates for the microscopic geometry of heterotic strings in d dimensions with target space ads_3 x sd3 we also discuss some conformal field theories that give microscopic ads target spaces in various dimensions
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707.4304
Spatial Aggregation: Data Model and Implementation
Data aggregation in Geographic Information Systems (GIS) is only marginally present in commercial systems nowadays, mostly through ad-hoc solutions. In this paper, we first present a formal model for representing spatial data. This model integrates geographic data and information contained in data warehouses external to the GIS. We define the notion of geometric aggregation, a general framework for aggregate queries in a GIS setting. We also identify the class of summable queries, which can be efficiently evaluated by precomputing the overlay of two or more of the thematic layers involved in the query. We also sketch a language, denoted GISOLAP-QL, for expressing queries that involve GIS and OLAP features. In addition, we introduce Piet, an implementation of our proposal, that makes use of overlay precomputation for answering spatial queries (aggregate or not). Our experimental evaluation showed that for a certain class of geometric queries with or without aggregation, overlay precomputation outperforms R-tree-based techniques. Finally, as a particular application of our proposal, we study topological queries.
cs.DB
data aggregation in geographic information systems gis is only marginally present in commercial systems nowadays mostly through adhoc solutions in this paper we first present a formal model for representing spatial data this model integrates geographic data and information contained in data warehouses external to the gis we define the notion of geometric aggregation a general framework for aggregate queries in a gis setting we also identify the class of summable queries which can be efficiently evaluated by precomputing the overlay of two or more of the thematic layers involved in the query we also sketch a language denoted gisolapql for expressing queries that involve gis and olap features in addition we introduce piet an implementation of our proposal that makes use of overlay precomputation for answering spatial queries aggregate or not our experimental evaluation showed that for a certain class of geometric queries with or without aggregation overlay precomputation outperforms rtreebased techniques finally as a particular application of our proposal we study topological queries
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707.4305
On elements of prime order in the plane Cremona group over a perfect field
We show that the plane Cremona group over a perfect field $k$ of characteristic $p \ge 0$ contains an element of prime order $\ell\ge 7$ not equal to $p$ if and only if there exists a 2-dimensional algebraic torus $T$ over $k$ such that $T(k)$ contains an element of order $\ell$. If $p = 0$ and $k$ does not contain a primitive $\ell$-th root of unity, we show that there are no elements of prime order $\ell > 7$ in $\Cr_2(k)$ and all elements of order 7 are conjugate.
math.AG math.NT
we show that the plane cremona group over a perfect field k of characteristic p ge 0 contains an element of prime order ellge 7 not equal to p if and only if there exists a 2dimensional algebraic torus t over k such that tk contains an element of order ell if p 0 and k does not contain a primitive ellth root of unity we show that there are no elements of prime order ell 7 in cr_2k and all elements of order 7 are conjugate
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707.4306
Symplectic potentials and resolved Ricci-flat ACG metrics
We pursue the symplectic description of toric Kahler manifolds. There exists a general local classification of metrics on toric Kahler manifolds equipped with Hamiltonian two-forms due to Apostolov, Calderbank and Gauduchon(ACG). We derive the symplectic potential for these metrics. Using a method due to Abreu, we relate the symplectic potential to the canonical potential written by Guillemin. This enables us to recover the moment polytope associated with metrics and we thus obtain global information about the metric. We illustrate these general considerations by focusing on six-dimensional Ricci flat metrics and obtain Ricci flat metrics associated with real cones over L^{pqr} and Y^{pq} manifolds. The metrics associated with cones over Y^{pq} manifolds turn out to be partially resolved with two blowup parameters taking special (non-zero)values. For a fixed Y^{pq} manifold, we find explicit metrics for several inequivalent blow-ups parametrised by a natural number k in the range 0<k<p. We also show that all known examples of resolved metrics such as the resolved conifold and the resolution of C^3/Z_3 also fit the ACG classification.
hep-th math.DG
we pursue the symplectic description of toric kahler manifolds there exists a general local classification of metrics on toric kahler manifolds equipped with hamiltonian twoforms due to apostolov calderbank and gauduchonacg we derive the symplectic potential for these metrics using a method due to abreu we relate the symplectic potential to the canonical potential written by guillemin this enables us to recover the moment polytope associated with metrics and we thus obtain global information about the metric we illustrate these general considerations by focusing on sixdimensional ricci flat metrics and obtain ricci flat metrics associated with real cones over lpqr and ypq manifolds the metrics associated with cones over ypq manifolds turn out to be partially resolved with two blowup parameters taking special nonzerovalues for a fixed ypq manifold we find explicit metrics for several inequivalent blowups parametrised by a natural number k in the range 0kp we also show that all known examples of resolved metrics such as the resolved conifold and the resolution of c3z_3 also fit the acg classification
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707.4307
High speed single photon detection in the near-infrared
InGaAs avalanche photodiodes (APDs) are convenient for single photon detection in the near-infrared (NIR) including the fibre communication bands (1.31/1.55 $\mu$m). However, to suppress afterpulse noise due to trapped avalanche charge, they must be gated with MHz repetition frequencies, thereby severely limiting the count rate in NIR applications. Here we show gating frequencies for InGaAs-APDs well beyond 1 GHz. Using a self-differencing technique to sense much weaker avalanches, we reduce drastically afterpulse noise. At 1.25 GHz, we obtain a detection efficiency of 10.8% with an afterpulse probability of 6.16%. In addition, the detector features low jitter (55 ps) and a count rate of 100 MHz.
quant-ph physics.ins-det physics.optics
ingaas avalanche photodiodes apds are convenient for single photon detection in the nearinfrared nir including the fibre communication bands 131155 mum however to suppress afterpulse noise due to trapped avalanche charge they must be gated with mhz repetition frequencies thereby severely limiting the count rate in nir applications here we show gating frequencies for ingaasapds well beyond 1 ghz using a selfdifferencing technique to sense much weaker avalanches we reduce drastically afterpulse noise at 125 ghz we obtain a detection efficiency of 108 with an afterpulse probability of 616 in addition the detector features low jitter 55 ps and a count rate of 100 mhz
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707.4308
A Machian Solution of the Hierarchy Problem
The new interpretation of Mach's principle of mass of a particle being a measure of the interactions of this particle with all other gravitating particles inside its causal spheres is introduced. It is shown that within some alternative model of gravitation that incorporates this principle, the Machian influence of the universe can reduce Planck's scale to the electro-weak scale and the large number that is needed to explain the hierarchy between the scales is the amount of gravitating particles inside the universe horizon. Our model can lead to new observable effects at cosmological distances and close to the sources of a strong gravitational field.
hep-th gr-qc hep-ph
the new interpretation of machs principle of mass of a particle being a measure of the interactions of this particle with all other gravitating particles inside its causal spheres is introduced it is shown that within some alternative model of gravitation that incorporates this principle the machian influence of the universe can reduce plancks scale to the electroweak scale and the large number that is needed to explain the hierarchy between the scales is the amount of gravitating particles inside the universe horizon our model can lead to new observable effects at cosmological distances and close to the sources of a strong gravitational field
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707.4309
Unparticles-Higgs Interplay
We show that scalar unparticles coupled to the Standard Model Higgs at the renormalizable level can have a dramatic impact in the breaking of the electroweak symmetry already at tree level. In particular one can get the proper electroweak scale without the need of a Higgs mass term in the Lagrangian. By studying the mixed unparticle-Higgs propagator and spectral function we also show how unparticles can shift the Higgs mass away from its Standard Model value, \lambda v^2, and influence other Higgs boson properties. Conversely, we study in some detail how electroweak symmetry breaking affects the unparticle sector by breaking its conformal symmetry and generating a mass gap. We also show that, for Higgs masses above that gap, unparticles can increase quite significantly the Higgs width.
hep-ph
we show that scalar unparticles coupled to the standard model higgs at the renormalizable level can have a dramatic impact in the breaking of the electroweak symmetry already at tree level in particular one can get the proper electroweak scale without the need of a higgs mass term in the lagrangian by studying the mixed unparticlehiggs propagator and spectral function we also show how unparticles can shift the higgs mass away from its standard model value lambda v2 and influence other higgs boson properties conversely we study in some detail how electroweak symmetry breaking affects the unparticle sector by breaking its conformal symmetry and generating a mass gap we also show that for higgs masses above that gap unparticles can increase quite significantly the higgs width
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707.431
Cohomological characterizations of projective spaces and hyperquadrics
We confirm Beauville's conjecture that claims that if the p-th exterior power of the tangent bundle of a smooth projective variety contains the p-th power of an ample line bundle, then the variety is either the projective space or the p-dimensional quadric hypersurface.
math.AG
we confirm beauvilles conjecture that claims that if the pth exterior power of the tangent bundle of a smooth projective variety contains the pth power of an ample line bundle then the variety is either the projective space or the pdimensional quadric hypersurface
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707.4311
Embedded Rank Distance Codes for ISI channels
Designs for transmit alphabet constrained space-time codes naturally lead to questions about the design of rank distance codes. Recently, diversity embedded multi-level space-time codes for flat fading channels have been designed from sets of binary matrices with rank distance guarantees over the binary field by mapping them onto QAM and PSK constellations. In this paper we demonstrate that diversity embedded space-time codes for fading Inter-Symbol Interference (ISI) channels can be designed with provable rank distance guarantees. As a corollary we obtain an asymptotic characterization of the fixed transmit alphabet rate-diversity trade-off for multiple antenna fading ISI channels. The key idea is to construct and analyze properties of binary matrices with a particular structure induced by ISI channels.
cs.IT math.IT
designs for transmit alphabet constrained spacetime codes naturally lead to questions about the design of rank distance codes recently diversity embedded multilevel spacetime codes for flat fading channels have been designed from sets of binary matrices with rank distance guarantees over the binary field by mapping them onto qam and psk constellations in this paper we demonstrate that diversity embedded spacetime codes for fading intersymbol interference isi channels can be designed with provable rank distance guarantees as a corollary we obtain an asymptotic characterization of the fixed transmit alphabet ratediversity tradeoff for multiple antenna fading isi channels the key idea is to construct and analyze properties of binary matrices with a particular structure induced by isi channels
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707.4312
Evidence for a new light spin-zero boson from cosmological gamma-ray propagation?
Recent findings by Imaging Atmospheric Cherenkov Telescopes indicate a large transparency of the Universe to gamma rays, which can be hardly explained within the current models of extragalactic background light. We show that the observed transparency is naturally produced by an oscillation mechanism -- which can occur inside intergalactic magnetic fields -- whereby a photon can become a new spin-zero boson with mass m << 10^(-10) eV. Because the latter particle travels unimpeded throughout the Universe, photons can reach the observer even if the distance from the source considerably exceeds their mean free path. We compute the expected flux of gamma rays from blazar 3C279 at different energies. Our predictions can be tested in the near future by the gamma-ray telescopes H.E.S.S., MAGIC, CANGAROO and VERITAS. Moreover, our result provides an important observational test for models of dark energy wherein quintessence is coupled to the photon through an effective dimension-five operator.
astro-ph hep-ex hep-ph
recent findings by imaging atmospheric cherenkov telescopes indicate a large transparency of the universe to gamma rays which can be hardly explained within the current models of extragalactic background light we show that the observed transparency is naturally produced by an oscillation mechanism which can occur inside intergalactic magnetic fields whereby a photon can become a new spinzero boson with mass m 1010 ev because the latter particle travels unimpeded throughout the universe photons can reach the observer even if the distance from the source considerably exceeds their mean free path we compute the expected flux of gamma rays from blazar 3c279 at different energies our predictions can be tested in the near future by the gammaray telescopes hess magic cangaroo and veritas moreover our result provides an important observational test for models of dark energy wherein quintessence is coupled to the photon through an effective dimensionfive operator
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707.4313
Trace Estimates for Stable Processes
In this paper we study the behaviour in time of the trace (the partition function) of the heat semigroup associated with symmetric stable processes in domains of $\Rd$. In particular, we show that for domains with the so called {\it{$R$-smoothness}} property the second terms in the asymptotic as $t\to 0$ involves the surface area of the domain, just as in the case of Brownian motion.
math.SP math.PR
in this paper we study the behaviour in time of the trace the partition function of the heat semigroup associated with symmetric stable processes in domains of rd in particular we show that for domains with the so called itrsmoothness property the second terms in the asymptotic as tto 0 involves the surface area of the domain just as in the case of brownian motion
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707.4314
Spitzer/IRS spectroscopy of high mass precursors to planetary nebulae
We present Spitzer/IRS observations of a small sample of heavily obscured IRAS sources displaying both the infrared and OH maser emission characteristic of OH/IR stars on the asymptotic giant branch (AGB), but also radio continuum emission typical of ionized planetary nebulae (PNe), the so-called OHPNe. Our observations show that their mid-infrared spectra are dominated by the simultaneous presence of strong and broad amorphous silicate absorption features together with crystalline silicate features, originated in their O-rich circumstellar shells. Out of the five sources observed, three of them are clearly non-variable at infrared wavelengths, confirming their post-AGB status, while the remaining two still show strong photometric fluctuations, and may still have not yet departed from the AGB. One of the non-variable sources in the sample, IRAS 17393-2727, displays a strong [Ne II] nebular emission at 12.8 microns, indicating that the ionization of its central region has already started. This suggests a rapid evolution from the AGB to the PN stage. We propose that these heavily obscured OHPNe represent the population of high mass precursors to PNe in our Galaxy.
astro-ph
we present spitzerirs observations of a small sample of heavily obscured iras sources displaying both the infrared and oh maser emission characteristic of ohir stars on the asymptotic giant branch agb but also radio continuum emission typical of ionized planetary nebulae pne the socalled ohpne our observations show that their midinfrared spectra are dominated by the simultaneous presence of strong and broad amorphous silicate absorption features together with crystalline silicate features originated in their orich circumstellar shells out of the five sources observed three of them are clearly nonvariable at infrared wavelengths confirming their postagb status while the remaining two still show strong photometric fluctuations and may still have not yet departed from the agb one of the nonvariable sources in the sample iras 173932727 displays a strong ne ii nebular emission at 128 microns indicating that the ionization of its central region has already started this suggests a rapid evolution from the agb to the pn stage we propose that these heavily obscured ohpne represent the population of high mass precursors to pne in our galaxy
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707.4315
Beyond the standard entropic inequalities: stronger scalar separability criteria and their applications
Recently it was shown that if a given state fulfils the reduction criterion it must also satisfy the known entropic inequalities. Now the questions arises whether on the assumption that stronger criteria based on positive but not completely positive maps are satisfied, it is possible to derive some scalar inequalities stronger than the entropic ones. In this paper we show that under some assumptions the extended reduction criterion [H.-P. Breuer, Phys. Rev. Lett 97, 080501 (2006); W. Hall, J. Phys. A 40, 6183 (2007)] leads to some entropic--like inequalities which are much stronger than their entropic counterparts. The comparison of the derived inequalities with other separability criteria shows that such approach might lead to strong scalar criteria detecting both distillable and bound entanglement. In particular, in the case of SO(3)-invariant states it is shown that the present inequalities detect entanglement in regions in which entanglement witnesses based on extended reduction map fail. It should be also emphasized that in the case of $2\otimes N$ states the derived inequalities detect entanglement efficiently, while the extended reduction maps are useless when acting on the qubit subsystem. Moreover, there is a natural way to construct a many-copy entanglement witnesses based on the derived inequalities so, in principle, there is a possibility of experimental realization. Some open problems and possibilities for further studies are outlined.
quant-ph
recently it was shown that if a given state fulfils the reduction criterion it must also satisfy the known entropic inequalities now the questions arises whether on the assumption that stronger criteria based on positive but not completely positive maps are satisfied it is possible to derive some scalar inequalities stronger than the entropic ones in this paper we show that under some assumptions the extended reduction criterion hp breuer phys rev lett 97 080501 2006 w hall j phys a 40 6183 2007 leads to some entropiclike inequalities which are much stronger than their entropic counterparts the comparison of the derived inequalities with other separability criteria shows that such approach might lead to strong scalar criteria detecting both distillable and bound entanglement in particular in the case of so3invariant states it is shown that the present inequalities detect entanglement in regions in which entanglement witnesses based on extended reduction map fail it should be also emphasized that in the case of 2otimes n states the derived inequalities detect entanglement efficiently while the extended reduction maps are useless when acting on the qubit subsystem moreover there is a natural way to construct a manycopy entanglement witnesses based on the derived inequalities so in principle there is a possibility of experimental realization some open problems and possibilities for further studies are outlined
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707.4316
All CAT(0) Boundaries of a Group of the Form HxK are CE Equivalent
M. Bestvina has shown that for any given torsion-free CAT(0) group G, all of its boundaries are shape equivalent. He then posed the question of whether they satisfy the stronger condition of being cell-like equivalent. In this article we prove that the answer is "Yes" in the situation where the group in question splits as a direct product with infinite factors. We accomplish this by proving an interesting theorem in shape theory.
math.GT math.GR
m bestvina has shown that for any given torsionfree cat0 group g all of its boundaries are shape equivalent he then posed the question of whether they satisfy the stronger condition of being celllike equivalent in this article we prove that the answer is yes in the situation where the group in question splits as a direct product with infinite factors we accomplish this by proving an interesting theorem in shape theory
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707.4317
Optimalit\'e, congruences et calculs d'invariants des vari\'et\'es symplectiques r\'eelles de dimension quatre
This paper follows a previous one in which were introduced deformation invariants $\chi^d_r$, $d \in H_2 (X ; \Z)$, $r \in \N$, of closed real symplectic four-manifolds $(X, \omega, c_X)$, invariants which produced lower bounds in real enumerative geometry. We prove here using methods of symplectic field theory that the lower bounds are sharp when $r \leq 1$ and the real locus of the manifold contains a sphere, torus or real projective plane (under stronger assumptions in this last case). We also prove that a big power of two divides $\chi^d_r$ as soon as r is not too big and when the real locus contains a sphere or real projective plane (under the same stronger assumptions in this last case). We finally present some explicit computations in the case of the projective plane or quadric ellipsoid surface as well as the general formulas used to get them, formulas which involve some relative invariants that we first define.
math.SG math.AG
this paper follows a previous one in which were introduced deformation invariants chid_r d in h_2 x z r in n of closed real symplectic fourmanifolds x omega c_x invariants which produced lower bounds in real enumerative geometry we prove here using methods of symplectic field theory that the lower bounds are sharp when r leq 1 and the real locus of the manifold contains a sphere torus or real projective plane under stronger assumptions in this last case we also prove that a big power of two divides chid_r as soon as r is not too big and when the real locus contains a sphere or real projective plane under the same stronger assumptions in this last case we finally present some explicit computations in the case of the projective plane or quadric ellipsoid surface as well as the general formulas used to get them formulas which involve some relative invariants that we first define
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707.4318
Simple Mathematical Model Of Pathologic Microsatellite Expansions: When Self-Reparation Does Not Work
We propose a simple model of pathologic microsatellite expansion, and describe an inherent self-repairing mechanism working against expansion. We prove that if the probabilities of elementary expansions and contractions are equal, microsatellite expansions are always self-repairing. If these probabilities are different, self-reparation does not work. Mosaicism, anticipation and reverse mutation cases are discussed in the framework of the model. We explain these phenomena and provide some theoretical evidence for their properties, for example the rarity of reverse mutations.
q-bio.GN q-bio.CB
we propose a simple model of pathologic microsatellite expansion and describe an inherent selfrepairing mechanism working against expansion we prove that if the probabilities of elementary expansions and contractions are equal microsatellite expansions are always selfrepairing if these probabilities are different selfreparation does not work mosaicism anticipation and reverse mutation cases are discussed in the framework of the model we explain these phenomena and provide some theoretical evidence for their properties for example the rarity of reverse mutations
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707.4319
Improved limit on electron neutrino charge radius through a new evaluation of the weak mixing angle
We have obtained a new limit on the electron neutrino effective charge radius from a new evaluation of the weak mixing angle by a combined fit of all electron-(anti)neutrino electron elastic scattering measurements. Weak mixing angle is found to be sin^2 theta_W=0.259 \pm 0.025 in the low energy regime below 100 MeV. The electron neutrino charge radius squared is bounded to be in the range -0.13 10^-32 cm^2 < r^2 < 3.32 10^-32 cm^2 at 90 % C.L. Both results improve previously published analyses. We also discuss perspectives of future experiments to improve these constraints.
hep-ph hep-ex
we have obtained a new limit on the electron neutrino effective charge radius from a new evaluation of the weak mixing angle by a combined fit of all electronantineutrino electron elastic scattering measurements weak mixing angle is found to be sin2 theta_w0259 pm 0025 in the low energy regime below 100 mev the electron neutrino charge radius squared is bounded to be in the range 013 1032 cm2 r2 332 1032 cm2 at 90 cl both results improve previously published analyses we also discuss perspectives of future experiments to improve these constraints
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707.432
Tropical Nevanlinna theory and ultra-discrete equations
A tropical version of Nevanlinna theory is described in which the role of meromorphic functions is played by continuous piecewise linear functions of a real variable whose one-sided derivatives are integers at every point. These functions are naturally defined on the max-plus (or tropical) semi-ring. Analogues of the Nevanlinna characteristic, proximity and counting functions are defined and versions of Nevanlinna's first main theorem, the lemma on the logarithmic derivative and Clunie's lemma are proved. As well as providing another example of a tropical or dequantized analogue of an important area of complex analysis, this theory has applications to so-called ultra-discrete equations. Preliminary results are presented suggesting that the existence of finite-order max-plus meromorphic solutions can be considered to be an ultra-discrete analogue of the Painlev'e property.
nlin.SI nlin.CG
a tropical version of nevanlinna theory is described in which the role of meromorphic functions is played by continuous piecewise linear functions of a real variable whose onesided derivatives are integers at every point these functions are naturally defined on the maxplus or tropical semiring analogues of the nevanlinna characteristic proximity and counting functions are defined and versions of nevanlinnas first main theorem the lemma on the logarithmic derivative and clunies lemma are proved as well as providing another example of a tropical or dequantized analogue of an important area of complex analysis this theory has applications to socalled ultradiscrete equations preliminary results are presented suggesting that the existence of finiteorder maxplus meromorphic solutions can be considered to be an ultradiscrete analogue of the painleve property
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707.4321
The insulin superfamily of growth-promoting proteins
Recently, structural analysis of the human transferrin and growth hormone (GH) amino acid sequences has unravelled that they harbor a motif identical to a pattern found in viral oncoproteins known to bind the primarily nuclear tumor suppressor retinoblastoma protein (RB). Since related signatures had previously been identified also in insulin and the two insulin-like growth factors (IGFs), the aim of the current study has been to investigate whether further hints substantiating these reported homologies can be found in silico. Here, additional similarities are presented supporting the notion of an insulin superfamily of growth-promoting proteins with dual localization in the extracellular environment and the intracellular space, particularly in the nucleus, as well as characterized by a tropism for RB.
q-bio.BM q-bio.SC
recently structural analysis of the human transferrin and growth hormone gh amino acid sequences has unravelled that they harbor a motif identical to a pattern found in viral oncoproteins known to bind the primarily nuclear tumor suppressor retinoblastoma protein rb since related signatures had previously been identified also in insulin and the two insulinlike growth factors igfs the aim of the current study has been to investigate whether further hints substantiating these reported homologies can be found in silico here additional similarities are presented supporting the notion of an insulin superfamily of growthpromoting proteins with dual localization in the extracellular environment and the intracellular space particularly in the nucleus as well as characterized by a tropism for rb
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707.4322
Infinite topology of curve complexes and non-Poincare duality of Teichmueller modular groups
In this note, we fill in a gap in the literature by proving that the Teichmueller modular groups (mapping class groups) are not Poincare duality groups and the complexes of curves of surfaces have infinite homotopy type (i.e. are not homotopy equivalent to a finite CW-complex).
math.GT math.GR
in this note we fill in a gap in the literature by proving that the teichmueller modular groups mapping class groups are not poincare duality groups and the complexes of curves of surfaces have infinite homotopy type ie are not homotopy equivalent to a finite cwcomplex
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707.4323
Is the Mass Scale for Elementary Particles Classically Determined?
We investigate whether a mass scale for elementary particles can be derived from interactions of particles with distant matter in the Universe, the mechanism of the interaction being the classical vector potential, propagating in a space of negative curvature. A possible context for such a mass scale is conformal gravity. This theory may prove to be renormalizable, since all coupling constants are dimensionless; conversely, however, there is no coupling constant analogous to the conventional G to provide a starting point for a mass scale calculation. We obtain the equations for propagation of the vector potential of a charged particle moving in a plasma in a curved space. We then show that distant matter will contribute to A**2, and that this non-thermal part will eventually dominate the ordinary thermal part. At this point a symmetry breaking transition of the Coleman-Weinberg type is possible, and particle masses can be generated with m**2 of order A**2.
gr-qc
we investigate whether a mass scale for elementary particles can be derived from interactions of particles with distant matter in the universe the mechanism of the interaction being the classical vector potential propagating in a space of negative curvature a possible context for such a mass scale is conformal gravity this theory may prove to be renormalizable since all coupling constants are dimensionless conversely however there is no coupling constant analogous to the conventional g to provide a starting point for a mass scale calculation we obtain the equations for propagation of the vector potential of a charged particle moving in a plasma in a curved space we then show that distant matter will contribute to a2 and that this nonthermal part will eventually dominate the ordinary thermal part at this point a symmetry breaking transition of the colemanweinberg type is possible and particle masses can be generated with m2 of order a2
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707.4324
Additivity of effective quadrupole moments and angular momentum alignments in the A~130 nuclei
The additivity principle of the extreme shell model stipulates that an average value of a one-body operator be equal to the sum of the core contribution and effective contributions of valence (particle or hole) nucleons. For quadrupole moment and angular momentum operators, we test this principle for highly and superdeformed rotational bands in the A~130 nuclei. Calculations are done in the self-consistent cranked non-relativistic Hartree-Fock and relativistic Hartree mean-field approaches. Results indicate that the additivity principle is a valid concept that justifies the use of an extreme single-particle model in an unpaired regime typical of high angular momenta.
nucl-th
the additivity principle of the extreme shell model stipulates that an average value of a onebody operator be equal to the sum of the core contribution and effective contributions of valence particle or hole nucleons for quadrupole moment and angular momentum operators we test this principle for highly and superdeformed rotational bands in the a130 nuclei calculations are done in the selfconsistent cranked nonrelativistic hartreefock and relativistic hartree meanfield approaches results indicate that the additivity principle is a valid concept that justifies the use of an extreme singleparticle model in an unpaired regime typical of high angular momenta
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707.4325
Renormalization of Singular Potentials and Power Counting
We use a toy model to illustrate how to build effective theories for singular potentials. We consider a central attractive 1/r^2 potential perturbed by a 1/r^4 correction. The power-counting rule, an important ingredient of effective theory, is established by seeking the minimum set of short-range counterterms that renormalize the scattering amplitude. We show that leading-order counterterms are needed in all partial waves where the potential overcomes the centrifugal barrier, and that the additional counterterms at next-to-leading order are the ones expected on the basis of dimensional analysis.
quant-ph nucl-th physics.atom-ph
we use a toy model to illustrate how to build effective theories for singular potentials we consider a central attractive 1r2 potential perturbed by a 1r4 correction the powercounting rule an important ingredient of effective theory is established by seeking the minimum set of shortrange counterterms that renormalize the scattering amplitude we show that leadingorder counterterms are needed in all partial waves where the potential overcomes the centrifugal barrier and that the additional counterterms at nexttoleading order are the ones expected on the basis of dimensional analysis
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707.4326
Exponential peak and scaling of work fluctuations in modulated systems
We extend the stationary-state work fluctuation theorem to periodically modulated nonlinear systems. Such systems often have coexisting stable periodic states. We show that work fluctuations sharply increase near a kinetic phase transition where the state populations are close to each other. The work variance is proportional here to the reciprocal rate of interstate switching. We also show that the variance displays scaling with the distance to a bifurcation point and find the critical exponent for a saddle-node bifurcation.
cond-mat.stat-mech cond-mat.mes-hall
we extend the stationarystate work fluctuation theorem to periodically modulated nonlinear systems such systems often have coexisting stable periodic states we show that work fluctuations sharply increase near a kinetic phase transition where the state populations are close to each other the work variance is proportional here to the reciprocal rate of interstate switching we also show that the variance displays scaling with the distance to a bifurcation point and find the critical exponent for a saddlenode bifurcation
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707.4327
Stochastic background from extra-galactic double neutron stars
We present Monte Carlo simulations of the extra galactic population of inspiralling double neutron stars, and estimate its contribution to the astrophysical gravitational wave background, in the frequency range of ground based interferometers, corresponding to the last thousand seconds before the last stable orbit when more than 96 percent of the signal is released. We show that sources at redshift z>0.5 contribute to a truly continuous background which may be detected by correlating third generation interferometers.
gr-qc astro-ph
we present monte carlo simulations of the extra galactic population of inspiralling double neutron stars and estimate its contribution to the astrophysical gravitational wave background in the frequency range of ground based interferometers corresponding to the last thousand seconds before the last stable orbit when more than 96 percent of the signal is released we show that sources at redshift z05 contribute to a truly continuous background which may be detected by correlating third generation interferometers
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707.4328
Multiple extensions of a finite Euler's pentagonal number theorem and the Lucas formulas
Motivated by the resemblance of a multivariate series identity and a finite analogue of Euler's pentagonal number theorem, we study multiple extensions of the latter formula. In a different direction we derive a common extension of this multivariate series identity and two formulas of Lucas. Finally we give a combinatorial proof of Lucas' formulas.
math.CO
motivated by the resemblance of a multivariate series identity and a finite analogue of eulers pentagonal number theorem we study multiple extensions of the latter formula in a different direction we derive a common extension of this multivariate series identity and two formulas of lucas finally we give a combinatorial proof of lucas formulas
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707.4329
Cobordisms of maps with singularities of a given class
Let P be a connected smooth p-manifold. We describe the group of all cobordism classes of smooth maps of n-manifolds to P with singularities of a given $cal K$-invariant class in terms of certain stable homotopy groups by applying the relative homotopy principle on the existence level. We also deal with the oriented version and construct a classifying space to which this oriented cobordism group is represented as the set of homotopy classes of P in the codimension n<p and n\geqq p\geqq 2.
math.GT
let p be a connected smooth pmanifold we describe the group of all cobordism classes of smooth maps of nmanifolds to p with singularities of a given cal kinvariant class in terms of certain stable homotopy groups by applying the relative homotopy principle on the existence level we also deal with the oriented version and construct a classifying space to which this oriented cobordism group is represented as the set of homotopy classes of p in the codimension np and ngeqq pgeqq 2
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