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708.3449
On Local Behavior of Holomorphic Functions Along Complex Submanifolds of C^N
In this paper we establish some general results on local behavior of holomorphic functions along complex submanifolds of $\Co^{N}$. As a corollary, we present multi-dimensional generalizations of an important result of Coman and Poletsky on Bernstein type inequalities on transcendental curves in $\Co^{2}$.
math.CV math.FA
in this paper we establish some general results on local behavior of holomorphic functions along complex submanifolds of con as a corollary we present multidimensional generalizations of an important result of coman and poletsky on bernstein type inequalities on transcendental curves in co2
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708.345
Mediation of Long-Range Attraction Selectively between Negatively-Charged Colloids on Surfaces by Solvation
We propose a mean-field analytical model to account for the observed asymmetry in the ability to form long-range attraction by the negatively charged colloidal particles and not their equivalently charged positive counterpart. We conjecture that this asymmetry is due to solvation effects, and we phenomenologically capture its physics by considering the relative strength of this water-induced short-range repulsion between the different charge species. We then apply our model to the colloidal system of negatively charged disks that are neutralized by a sea of counterions and strongly absorbed to an interface in a compressible binary system. We demonstrate the resulting coexistence between a dilute isotropic ionic phase and a condensed hexagonal lattice phase as a function of density and interaction strength.
cond-mat.soft cond-mat.mtrl-sci
we propose a meanfield analytical model to account for the observed asymmetry in the ability to form longrange attraction by the negatively charged colloidal particles and not their equivalently charged positive counterpart we conjecture that this asymmetry is due to solvation effects and we phenomenologically capture its physics by considering the relative strength of this waterinduced shortrange repulsion between the different charge species we then apply our model to the colloidal system of negatively charged disks that are neutralized by a sea of counterions and strongly absorbed to an interface in a compressible binary system we demonstrate the resulting coexistence between a dilute isotropic ionic phase and a condensed hexagonal lattice phase as a function of density and interaction strength
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708.3451
Diophantine subsets of function fields of curves
We consider diophantine subsets of function fields of curves and show, roughly speaking, that they are either very small or very large. In particular, this implies that the ring of polynomials $k[t]$ is a not a diophantine subset of the field of rational functions $k(t)$ for many fields $k$.
math.NT math.AG
we consider diophantine subsets of function fields of curves and show roughly speaking that they are either very small or very large in particular this implies that the ring of polynomials kt is a not a diophantine subset of the field of rational functions kt for many fields k
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708.3452
Scattering on D3-branes
In a direct open string approach we analyze scattering of massless states on a stack of D3-branes. First we construct vertex operators on the D-branes. The 4+6 splitting for the fermionic part is made possible by inserting appropriately defined projection operators. With the vertex operators constructed we compute various tree amplitudes. The results are then compared with the corresponding field theory computations of the $\N=4$ SYM with $\a'$-corrections: agreements are found. We comment on applications to AdS/CFT.
hep-th
in a direct open string approach we analyze scattering of massless states on a stack of d3branes first we construct vertex operators on the dbranes the 46 splitting for the fermionic part is made possible by inserting appropriately defined projection operators with the vertex operators constructed we compute various tree amplitudes the results are then compared with the corresponding field theory computations of the n4 sym with acorrections agreements are found we comment on applications to adscft
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708.3453
Asymptotic behavior of the rate of adaptation
We consider the accumulation of beneficial and deleterious mutations in large asexual populations. The rate of adaptation is affected by the total mutation rate, proportion of beneficial mutations and population size $N$. We show that regardless of mutation rates, as long as the proportion of beneficial mutations is strictly positive, the adaptation rate is at least $\mathcal{O}(\log^{1-\delta}N)$ where $\delta$ can be any small positive number, if the population size is sufficiently large. This shows that if the genome is modeled as continuous, there is no limit to natural selection, that is, the rate of adaptation grows in $N$ without bound.
math.PR
we consider the accumulation of beneficial and deleterious mutations in large asexual populations the rate of adaptation is affected by the total mutation rate proportion of beneficial mutations and population size n we show that regardless of mutation rates as long as the proportion of beneficial mutations is strictly positive the adaptation rate is at least mathcalolog1deltan where delta can be any small positive number if the population size is sufficiently large this shows that if the genome is modeled as continuous there is no limit to natural selection that is the rate of adaptation grows in n without bound
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708.3454
First-person visualizations of the special and general theory of relativity
Visualizations that adopt a first-person point of view allow observation and, in the case of interactive simulations, experimentation with relativistic scenes. This paper gives examples of three types of first-person visualizations: watching objects that move at nearly the speed of light, being a high-speed observer looking at a static environment and having a look-around near a compact object. I illustrate and explain the main aspects of the visual observations, outline their use in teaching relativity and report on teaching experiences. For teaching purposes, our visualization work is available on the web site http://www.spacetimetravel.org and its German counterpart http://www.tempolimit-lichtgeschwindigkeit.de . This paper assumes some basic knowledge about relativity on the part of the reader. It addresses instructors of physics at the undergraduate and advanced secondary school level as well as their students.
physics.ed-ph
visualizations that adopt a firstperson point of view allow observation and in the case of interactive simulations experimentation with relativistic scenes this paper gives examples of three types of firstperson visualizations watching objects that move at nearly the speed of light being a highspeed observer looking at a static environment and having a lookaround near a compact object i illustrate and explain the main aspects of the visual observations outline their use in teaching relativity and report on teaching experiences for teaching purposes our visualization work is available on the web site httpwwwspacetimetravelorg and its german counterpart httpwwwtempolimitlichtgeschwindigkeitde this paper assumes some basic knowledge about relativity on the part of the reader it addresses instructors of physics at the undergraduate and advanced secondary school level as well as their students
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708.3455
On the Range of Validity of the Dipole Picture
We derive correlated bounds on ratios of deep inelastic structure functions from the dipole picture of photon-hadron scattering at high energies. In particular we consider ratios of the longitudinal structure function, the total structure function and the charm part of the latter. We also consider ratios of total structure functions taken at the same energy but at three different photon virtualities. It is shown that by confronting these bounds with experimental data we can significantly constrain the range of validity of the dipole picture.
hep-ph hep-ex
we derive correlated bounds on ratios of deep inelastic structure functions from the dipole picture of photonhadron scattering at high energies in particular we consider ratios of the longitudinal structure function the total structure function and the charm part of the latter we also consider ratios of total structure functions taken at the same energy but at three different photon virtualities it is shown that by confronting these bounds with experimental data we can significantly constrain the range of validity of the dipole picture
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708.3456
Index theorems for quantum graphs
In geometric analysis, an index theorem relates the difference of the numbers of solutions of two differential equations to the topological structure of the manifold or bundle concerned, sometimes using the heat kernels of two higher-order differential operators as an intermediary. In this paper, the case of quantum graphs is addressed. A quantum graph is a graph considered as a (singular) one-dimensional variety and equipped with a second-order differential Hamiltonian H (a "Laplacian") with suitable conditions at vertices. For the case of scale-invariant vertex conditions (i.e., conditions that do not mix the values of functions and of their derivatives), the constant term of the heat-kernel expansion is shown to be proportional to the trace of the internal scattering matrix of the graph. This observation is placed into the index-theory context by factoring the Laplacian into two first-order operators, H =A*A, and relating the constant term to the index of A. An independent consideration provides an index formula for any differential operator on a finite quantum graph in terms of the vertex conditions. It is found also that the algebraic multiplicity of 0 as a root of the secular determinant of H is the sum of the nullities of A and A*.
math.SP math-ph math.MP
in geometric analysis an index theorem relates the difference of the numbers of solutions of two differential equations to the topological structure of the manifold or bundle concerned sometimes using the heat kernels of two higherorder differential operators as an intermediary in this paper the case of quantum graphs is addressed a quantum graph is a graph considered as a singular onedimensional variety and equipped with a secondorder differential hamiltonian h a laplacian with suitable conditions at vertices for the case of scaleinvariant vertex conditions ie conditions that do not mix the values of functions and of their derivatives the constant term of the heatkernel expansion is shown to be proportional to the trace of the internal scattering matrix of the graph this observation is placed into the indextheory context by factoring the laplacian into two firstorder operators h aa and relating the constant term to the index of a an independent consideration provides an index formula for any differential operator on a finite quantum graph in terms of the vertex conditions it is found also that the algebraic multiplicity of 0 as a root of the secular determinant of h is the sum of the nullities of a and a
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708.3457
Enhanced Group Analysis and Exact Solutions of Variable Coefficient Semilinear Diffusion Equations with a Power Source
A new approach to group classification problems and more general investigations on transformational properties of classes of differential equations is proposed. It is based on mappings between classes of differential equations, generated by families of point transformations. A class of variable coefficient (1+1)-dimensional semilinear reaction-diffusion equations of the general form $f(x)u_t=(g(x)u_x)_x+h(x)u^m$ ($m\ne0,1$) is studied from the symmetry point of view in the framework of the approach proposed. The singular subclass of the equations with $m=2$ is singled out. The group classifications of the entire class, the singular subclass and their images are performed with respect to both the corresponding (generalized extended) equivalence groups and all point transformations. The set of admissible transformations of the imaged class is exhaustively described in the general case $m\ne2$. The procedure of classification of nonclassical symmetries, which involves mappings between classes of differential equations, is discussed. Wide families of new exact solutions are also constructed for equations from the classes under consideration by the classical method of Lie reductions and by generation of new solutions from known ones for other equations with point transformations of different kinds (such as additional equivalence transformations and mappings between classes of equations).
math-ph math.MP nlin.SI
a new approach to group classification problems and more general investigations on transformational properties of classes of differential equations is proposed it is based on mappings between classes of differential equations generated by families of point transformations a class of variable coefficient 11dimensional semilinear reactiondiffusion equations of the general form fxu_tgxu_x_xhxum mne01 is studied from the symmetry point of view in the framework of the approach proposed the singular subclass of the equations with m2 is singled out the group classifications of the entire class the singular subclass and their images are performed with respect to both the corresponding generalized extended equivalence groups and all point transformations the set of admissible transformations of the imaged class is exhaustively described in the general case mne2 the procedure of classification of nonclassical symmetries which involves mappings between classes of differential equations is discussed wide families of new exact solutions are also constructed for equations from the classes under consideration by the classical method of lie reductions and by generation of new solutions from known ones for other equations with point transformations of different kinds such as additional equivalence transformations and mappings between classes of equations
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708.3458
First Law, Counterterms and Kerr-AdS_5 Black Holes
We apply the counterterm subtraction technique to calculate the action and other quantities for the Kerr--AdS black hole in five dimensions using two boundary metrics; the Einstein universe and rotating Einstein universe with arbitrary angular velocity. In both cases, the resulting thermodynamic quantities satisfy the first law of thermodynamics. We point out that the reason for the violation of the first law in previous calculations is that the rotating Einstein universe, used as a boundary metric, was rotating with an angular velocity that depends on the black hole rotation parameter. Using a new coordinate system with a boundary metric that has an arbitrary angular velocity, one can show that the resulting physical quantities satisfy the first law.
hep-th
we apply the counterterm subtraction technique to calculate the action and other quantities for the kerrads black hole in five dimensions using two boundary metrics the einstein universe and rotating einstein universe with arbitrary angular velocity in both cases the resulting thermodynamic quantities satisfy the first law of thermodynamics we point out that the reason for the violation of the first law in previous calculations is that the rotating einstein universe used as a boundary metric was rotating with an angular velocity that depends on the black hole rotation parameter using a new coordinate system with a boundary metric that has an arbitrary angular velocity one can show that the resulting physical quantities satisfy the first law
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708.3459
Bulk viscosity of gauge theory plasma at strong coupling
We propose a lower bound on bulk viscosity of strongly coupled gauge theory plasmas. Using explicit example of the N=2^* gauge theory plasma we show that the bulk viscosity remains finite at a critical point with a divergent specific heat. We present an estimate for the bulk viscosity of QGP plasma at RHIC.
hep-th
we propose a lower bound on bulk viscosity of strongly coupled gauge theory plasmas using explicit example of the n2 gauge theory plasma we show that the bulk viscosity remains finite at a critical point with a divergent specific heat we present an estimate for the bulk viscosity of qgp plasma at rhic
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708.346
First-principles study of a single-molecule magnet Mn_{12} monolayer on the Au(111) surface
The electronic structure of a monolayer of single-molecule magnets Mn$_{12}$ on a Au(111) surface is studied using spin-polarized density-functional theory. The Mn$_{12}$ molecules are oriented such that the magnetic easy axis is normal to the surface, and the terminating ligands in the Mn$_{12}$ are replaced by thiol groups (-SH) where the H atoms are lost upon adsorption onto the surface. This sulfur-terminated Mn$_{12}$ molecule has a total magnetic moment of 18 $\mu_B$ in the ground state, in contrast to 20$\mu_B$ for the standard Mn$_{12}$. The Mn$_{12}$ molecular orbitals broaden due to the interaction of the molecule with the gold surface and the broadening is of the order of 0.1 eV. It is an order of magnitude less than the single-electron charging energy of the molecule so the molecule is weakly bonded to the surface. Only electrons with majority spin can be transferred from the surface to the sulfur-terminated Mn$_{12}$ since the gold Fermi level is well above the majority lowest unoccupied molecular orbital (LUMO) but below the minority LUMO. The amount of the charge transfer is calculated to be 1.23 electrons, dominated by the tail in the electronic distribution of the gold surface. A calculation of level shift upon charging provides 0.28 electrons being transferred. The majority of the charge transfer occurs at the S, C, and O atoms close to the surface. The total magnetic moment also changes from 18 $\mu_B$ to 20 $\mu_B$, due to rearrangements of the magnetic moments on the S and Mn atoms upon adsorption onto the surface. The magnetic anisotropy barrier is computed including spin-orbit interaction self-consistently in density-functional theory. The barrier for the Mn$_{12}$ on the gold surface decreases by 6 K in comparison to that for an isolated Mn$_{12}$ molecule.
cond-mat.mtrl-sci
the electronic structure of a monolayer of singlemolecule magnets mn_12 on a au111 surface is studied using spinpolarized densityfunctional theory the mn_12 molecules are oriented such that the magnetic easy axis is normal to the surface and the terminating ligands in the mn_12 are replaced by thiol groups sh where the h atoms are lost upon adsorption onto the surface this sulfurterminated mn_12 molecule has a total magnetic moment of 18 mu_b in the ground state in contrast to 20mu_b for the standard mn_12 the mn_12 molecular orbitals broaden due to the interaction of the molecule with the gold surface and the broadening is of the order of 01 ev it is an order of magnitude less than the singleelectron charging energy of the molecule so the molecule is weakly bonded to the surface only electrons with majority spin can be transferred from the surface to the sulfurterminated mn_12 since the gold fermi level is well above the majority lowest unoccupied molecular orbital lumo but below the minority lumo the amount of the charge transfer is calculated to be 123 electrons dominated by the tail in the electronic distribution of the gold surface a calculation of level shift upon charging provides 028 electrons being transferred the majority of the charge transfer occurs at the s c and o atoms close to the surface the total magnetic moment also changes from 18 mu_b to 20 mu_b due to rearrangements of the magnetic moments on the s and mn atoms upon adsorption onto the surface the magnetic anisotropy barrier is computed including spinorbit interaction selfconsistently in densityfunctional theory the barrier for the mn_12 on the gold surface decreases by 6 k in comparison to that for an isolated mn_12 molecule
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708.3461
Quaternion-Octonion Analyticity for Abelian and Non-Abelian Gauge Theories of Dyons
Einstein- Schroedinger (ES) non-symmetric theory has been extended to accommodate the Abelian and non-Abelian gauge theories of dyons in terms of the quaternion-octonion metric realization. Corresponding covariant derivatives for complex, quaternion and octonion spaces in internal gauge groups are shown to describe the consistent field equations and generalized Dirac equation of dyons. It is also shown that quaternion and octonion representations extend the so-called unified theory of gravitation and electromagnetism to the Yang-Mill's fields leading to two SU(2) gauge theories of internal spaces due to the presence of electric and magnetic charges on dyons.
hep-th
einstein schroedinger es nonsymmetric theory has been extended to accommodate the abelian and nonabelian gauge theories of dyons in terms of the quaternionoctonion metric realization corresponding covariant derivatives for complex quaternion and octonion spaces in internal gauge groups are shown to describe the consistent field equations and generalized dirac equation of dyons it is also shown that quaternion and octonion representations extend the socalled unified theory of gravitation and electromagnetism to the yangmills fields leading to two su2 gauge theories of internal spaces due to the presence of electric and magnetic charges on dyons
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708.3462
Search for pulsed multi-TeV gamma rays from the Crab pulsar using the Tibet-III air shower array
We searched for pulsed gamma-ray emissions from the Crab pulsar using data of the Tibet-III air shower array from November 1999 through November 2005. No evidence for the pulsed emissions was found in our analysis. Upper limits at different energies were calculated for a $3 \sigma$ confidence level in the energy range of multi-TeV to several hundred TeV.
astro-ph
we searched for pulsed gammaray emissions from the crab pulsar using data of the tibetiii air shower array from november 1999 through november 2005 no evidence for the pulsed emissions was found in our analysis upper limits at different energies were calculated for a 3 sigma confidence level in the energy range of multitev to several hundred tev
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708.3463
A Neural Networks Model of the Venezuelan Economy
Besides an indicator of the GDP, the Central Bank of Venezuela generates the so called Monthly Economic Activity General Indicator. The a priori knowledge of this indicator, which represents and sometimes even anticipates the economy's fluctuations, could be helpful in developing public policies and in investment decision making. The purpose of this study is forecasting the IGAEM through non parametric methods, an approach that has proven effective in a wide variety of problems in economics and finance.
cs.CE cs.NE
besides an indicator of the gdp the central bank of venezuela generates the so called monthly economic activity general indicator the a priori knowledge of this indicator which represents and sometimes even anticipates the economys fluctuations could be helpful in developing public policies and in investment decision making the purpose of this study is forecasting the igaem through non parametric methods an approach that has proven effective in a wide variety of problems in economics and finance
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708.3464
A Non Parametric Study of the Volatility of the Economy as a Country Risk Predictor
This paper intends to explain Venezuela's country spread behavior through the Neural Networks analysis of a monthly economic activity general index of economic indicators constructed by the Central Bank of Venezuela, a measure of the shocks affecting country risk of emerging markets and the U.S. short term interest rate. The use of non parametric methods allowed the finding of non linear relationship between these inputs and the country risk. The networks performance was evaluated using the method of excess predictability.
cs.CE cs.NE
this paper intends to explain venezuelas country spread behavior through the neural networks analysis of a monthly economic activity general index of economic indicators constructed by the central bank of venezuela a measure of the shocks affecting country risk of emerging markets and the us short term interest rate the use of non parametric methods allowed the finding of non linear relationship between these inputs and the country risk the networks performance was evaluated using the method of excess predictability
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708.3465
An Early Warning System for Bankruptcy Prediction: lessons from the Venezuelan Bank Crisis
During 1993-94 Venezuela experienced a severe banking crisis which ended up with 18 commercial banks intervened by the government. Here we develop an early warning system for detecting credit related bankruptcy through discriminant functions developed on financial and macroeconomic data predating the crisis. A robustness test performed on these functions shows high precision in error estimation. The model calibrated on pre-crisis data could detect abnormal financial tension in the late Banco Capital many months before it was intervened and liquidated.
cs.CE
during 199394 venezuela experienced a severe banking crisis which ended up with 18 commercial banks intervened by the government here we develop an early warning system for detecting credit related bankruptcy through discriminant functions developed on financial and macroeconomic data predating the crisis a robustness test performed on these functions shows high precision in error estimation the model calibrated on precrisis data could detect abnormal financial tension in the late banco capital many months before it was intervened and liquidated
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708.3466
Photoionization of Clustered Halos by the First Stars
We present numerical simulations of the photoevaporation of cosmological halos clustered around a 120 M$_\odot$ primordial star, confining our study to structures capable of hosting Population III star formation. The calculations include self-consistent multifrequency conservative transfer of UV photons together with nine-species primordial chemistry and all relevant radiative processes. The ultimate fates of these halos varies with central density and proximity to the central source but generally fall into one of four categories. Diffuse halos with central densities below 2 - 3 cm$^{-3}$ are completely ionized and evaporated by the central star anywhere in the cluster. More evolved halo cores at densities above 2000 cm$^{-3}$ are impervious to both ionizing and Lyman-Werner flux at most distances from the star and collapse of their cores proceeds without delay. Radiative feedback in halos of intermediate density can be either positive or negative, depending on how the I-front remnant shock both compresses and deforms the core and enriches it with H$_2$. We find that the 120 M$_\odot$ star photodissociates H$_2$ in most halos within the cluster but that catalysis by H- rapidly restores molecular hydrogen within a few hundred Kyr after the death of the star, with little delay in star formation. Our models exhibit significant departures from previous one-dimensional spherically-symmetric simulations, which are prone to serious errors due to unphysical geometric focusing effects.
astro-ph
we present numerical simulations of the photoevaporation of cosmological halos clustered around a 120 m_odot primordial star confining our study to structures capable of hosting population iii star formation the calculations include selfconsistent multifrequency conservative transfer of uv photons together with ninespecies primordial chemistry and all relevant radiative processes the ultimate fates of these halos varies with central density and proximity to the central source but generally fall into one of four categories diffuse halos with central densities below 2 3 cm3 are completely ionized and evaporated by the central star anywhere in the cluster more evolved halo cores at densities above 2000 cm3 are impervious to both ionizing and lymanwerner flux at most distances from the star and collapse of their cores proceeds without delay radiative feedback in halos of intermediate density can be either positive or negative depending on how the ifront remnant shock both compresses and deforms the core and enriches it with h_2 we find that the 120 m_odot star photodissociates h_2 in most halos within the cluster but that catalysis by h rapidly restores molecular hydrogen within a few hundred kyr after the death of the star with little delay in star formation our models exhibit significant departures from previous onedimensional sphericallysymmetric simulations which are prone to serious errors due to unphysical geometric focusing effects
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708.3467
Analytical modelling of terminal properties in industrial growth
In this pedagogical study, carried out by adopting standard mathematical methods of nonlinear dynamics, we have presented some simple analytical models to understand terminal behaviour in industrial growth. This issue has also been addressed from a dynamical systems perspective, with especial emphasis on the concept of the Balanced Scorecard. Our study enables us to make the general claim that although the fortunes of an industrial organization can rise with exponential rapidity on relatively short time scales, its growth will ultimately and inevitably be saturated on long time scales by various factors which are nonlinear in character. We have mathematically demonstrated the likely occurrence of this feature under various possible circumstances, including the Red Ocean and the Blue Ocean. Finally and most importantly, our arguments and their associated mathematical modelling have received remarkable support from the growth pattern indicated by empirical data gathered from a well-recognized global company like IBM.
q-fin.GN physics.soc-ph
in this pedagogical study carried out by adopting standard mathematical methods of nonlinear dynamics we have presented some simple analytical models to understand terminal behaviour in industrial growth this issue has also been addressed from a dynamical systems perspective with especial emphasis on the concept of the balanced scorecard our study enables us to make the general claim that although the fortunes of an industrial organization can rise with exponential rapidity on relatively short time scales its growth will ultimately and inevitably be saturated on long time scales by various factors which are nonlinear in character we have mathematically demonstrated the likely occurrence of this feature under various possible circumstances including the red ocean and the blue ocean finally and most importantly our arguments and their associated mathematical modelling have received remarkable support from the growth pattern indicated by empirical data gathered from a wellrecognized global company like ibm
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708.3468
Weak ferromagnetism and spin glass state with nano-sized nickel carbide
Ni3C nanoparticles of about 40 nm have been studied experimentally to exhibit weak ferromagnetic (FM), spin-glass (SG) and paramagnetic (PM) properties. The freezing temperature of the SG phase at zero applied field is determined as, TF0 ~ 11.0 K. At T > TF0, a very weak ferromagnetism has been observed over a PM background. The Curie temperature, TC, is shown to exceed 300 K and the ferromagnetism at 300 K is determined as about 0.02 emu/g (~6.7*10^{-4}mu_B per Ni3C formula unit) by subtracting the background paramagnetism. An anomalous dip appears in the temperature dependent coercivity, HC(T), near the freezing temperature, TF0. It reflects a distortedly reduced coercivity in the M(H) hysteresis loop measured at T = TF0 with the applied sweeping field around H = 0. This is attributable to the exchange coupling effect between the SG and the weak FM phases. The possible origin of the magnetic moments that account for the observed FM, SG and PM properties is discussed.
cond-mat.mtrl-sci
ni3c nanoparticles of about 40 nm have been studied experimentally to exhibit weak ferromagnetic fm spinglass sg and paramagnetic pm properties the freezing temperature of the sg phase at zero applied field is determined as tf0 110 k at t tf0 a very weak ferromagnetism has been observed over a pm background the curie temperature tc is shown to exceed 300 k and the ferromagnetism at 300 k is determined as about 002 emug 67104mu_b per ni3c formula unit by subtracting the background paramagnetism an anomalous dip appears in the temperature dependent coercivity hct near the freezing temperature tf0 it reflects a distortedly reduced coercivity in the mh hysteresis loop measured at t tf0 with the applied sweeping field around h 0 this is attributable to the exchange coupling effect between the sg and the weak fm phases the possible origin of the magnetic moments that account for the observed fm sg and pm properties is discussed
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708.3469
Electronic structure of self-assembled InAs/InP quantum dots: A Comparison with self-assembled InAs/GaAs quantum dots
We investigate the electronic structure of the InAs/InP quantum dots using an atomistic pseudopotential method and compare them to those of the InAs/GaAs QDs. We show that even though the InAs/InP and InAs/GaAs dots have the same dot material, their electronic structure differ significantly in certain aspects, especially for holes: (i) The hole levels have a much larger energy spacing in the InAs/InP dots than in the InAs/GaAs dots of corresponding size. (ii) Furthermore, in contrast with the InAs/GaAs dots, where the sizeable hole $p$, $d$ intra-shell level splitting smashes the energy level shell structure, the InAs/InP QDs have a well defined energy level shell structure with small $p$, $d$ level splitting, for holes. (iii) The fundamental exciton energies of the InAs/InP dots are calculated to be around 0.8 eV ($\sim$ 1.55 $\mu$m), about 200 meV lower than those of typical InAs/GaAs QDs, mainly due to the smaller lattice mismatch in the InAs/InP dots. (iii) The widths of the exciton $P$ shell and $D$ shell are much narrower in the InAs/InP dots than in the InAs/GaAs dots. (iv) The InAs/GaAs and InAs/InP dots have a reversed light polarization anisotropy along the [100] and [1$\bar{1}$0] directions.
cond-mat.mtrl-sci
we investigate the electronic structure of the inasinp quantum dots using an atomistic pseudopotential method and compare them to those of the inasgaas qds we show that even though the inasinp and inasgaas dots have the same dot material their electronic structure differ significantly in certain aspects especially for holes i the hole levels have a much larger energy spacing in the inasinp dots than in the inasgaas dots of corresponding size ii furthermore in contrast with the inasgaas dots where the sizeable hole p d intrashell level splitting smashes the energy level shell structure the inasinp qds have a well defined energy level shell structure with small p d level splitting for holes iii the fundamental exciton energies of the inasinp dots are calculated to be around 08 ev sim 155 mum about 200 mev lower than those of typical inasgaas qds mainly due to the smaller lattice mismatch in the inasinp dots iii the widths of the exciton p shell and d shell are much narrower in the inasinp dots than in the inasgaas dots iv the inasgaas and inasinp dots have a reversed light polarization anisotropy along the 100 and 1bar10 directions
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708.347
Effects of mode degeneracy in the LIGO Livingston Observatory recycling cavity
We analyze the electromagnetic fields in a Pound-Drever-Hall locked, marginally unstable, Fabry-Perot cavity as a function of small changes in the cavity length during resonance. More specifically, we compare the results of a detailed numerical model with the behavior of the recycling cavity of the Laser Interferometer Gravitational-wave Observatory (LIGO) detector that is located in Livingston, Louisiana. In the interferometer's normal mode of operation, the recycling cavity is stabilized by inducing a thermal lens in the cavity mirrors with an external CO2 laser. During the study described here, this thermal compensation system was not operating, causing the cavity to be marginally optically unstable and cavity modes to become degenerate. In contrast to stable optical cavities, the modal content of the resonating beam in the uncompensated recycling cavity is significantly altered by very small cavity length changes. This modifies the error signals used to control the cavity length in such a way that the zero crossing point is no longer the point of maximum power in the cavity nor is it the point where the input beam mode in the cavity is maximized.
gr-qc
we analyze the electromagnetic fields in a pounddreverhall locked marginally unstable fabryperot cavity as a function of small changes in the cavity length during resonance more specifically we compare the results of a detailed numerical model with the behavior of the recycling cavity of the laser interferometer gravitationalwave observatory ligo detector that is located in livingston louisiana in the interferometers normal mode of operation the recycling cavity is stabilized by inducing a thermal lens in the cavity mirrors with an external co2 laser during the study described here this thermal compensation system was not operating causing the cavity to be marginally optically unstable and cavity modes to become degenerate in contrast to stable optical cavities the modal content of the resonating beam in the uncompensated recycling cavity is significantly altered by very small cavity length changes this modifies the error signals used to control the cavity length in such a way that the zero crossing point is no longer the point of maximum power in the cavity nor is it the point where the input beam mode in the cavity is maximized
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708.3471
Structure of the Roper Resonance with Diquark Correlations
We study electromagnetic properties of the nucleon and Roper resonance in a chiral quark-diquark model including two kinds of diquarks needed to describe the nucleon: scalar and axial-vector diquarks. The nucleon and Roper resonance are described as superpositions of two quark-diquark bound states of a quark and a scalar diquark and of a quark and an axial-vector diquark. Electromagnetic form factors of the nucleon and Roper resonance are obtained from one-loop diagrams where the quark and diquarks are coupled by a photon. We include the effects of intrinsic properties of the diquarks: the intrinsic form factors both of the diquarks and the anomalous magnetic moment of the axial-vector diquark. The electric form factors of the proton and neutron reasonably agree with the experiments due to the inclusions of the diquark sizes, while the magnetic moments become smaller than the experimental values because of the scalar dominance in the nucleon. The charge radii of the Roper resonance are almost comparable with those of the nucleon.
hep-ph
we study electromagnetic properties of the nucleon and roper resonance in a chiral quarkdiquark model including two kinds of diquarks needed to describe the nucleon scalar and axialvector diquarks the nucleon and roper resonance are described as superpositions of two quarkdiquark bound states of a quark and a scalar diquark and of a quark and an axialvector diquark electromagnetic form factors of the nucleon and roper resonance are obtained from oneloop diagrams where the quark and diquarks are coupled by a photon we include the effects of intrinsic properties of the diquarks the intrinsic form factors both of the diquarks and the anomalous magnetic moment of the axialvector diquark the electric form factors of the proton and neutron reasonably agree with the experiments due to the inclusions of the diquark sizes while the magnetic moments become smaller than the experimental values because of the scalar dominance in the nucleon the charge radii of the roper resonance are almost comparable with those of the nucleon
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708.3472
Empirical distributions of Chinese stock returns at different microscopic timescales
We study the distributions of event-time returns and clock-time returns at different microscopic timescales using ultra-high-frequency data extracted from the limit-order books of 23 stocks traded in the Chinese stock market in 2003. We find that the returns at the one-trade timescale obey the inverse cubic law. For larger timescales (2-32 trades and 1-5 minutes), the returns follow the Student distribution with power-law tails. With the decrease of timescale, the tail becomes fatter, which is consistent with the vibrational theory.
q-fin.ST physics.soc-ph
we study the distributions of eventtime returns and clocktime returns at different microscopic timescales using ultrahighfrequency data extracted from the limitorder books of 23 stocks traded in the chinese stock market in 2003 we find that the returns at the onetrade timescale obey the inverse cubic law for larger timescales 232 trades and 15 minutes the returns follow the student distribution with powerlaw tails with the decrease of timescale the tail becomes fatter which is consistent with the vibrational theory
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708.3473
Geodesic plasma flows instabilities of Riemann twisted solar loops
Riemann and sectional curvatures of magnetic twisted flux tubes in Riemannian manifold are computed to investigate the stability of the plasma astrophysical tubes. The geodesic equations are used to show that in the case of thick magnetic tubes, the curvature of planar (Frenet torsion-free) tubes have the effect ct of damping the flow speed along the tube. Stability of geodesic flows in the Riemannian twisted thin tubes (almost filaments), against constant radial perturbations is investigated by using the method of negative sectional curvature for unstable flows. No special form of the flow like Beltrami flows is admitted, and the proof is general for the case of thin magnetic flux tubes. In the magnetic equilibrium state, the twist of the tube is shown to display also a damping effect on the toroidal velocity of the plasma flow. It is found that for positive perturbations and angular speed of the flow, instability is achieved, since the sectional Ricci curvature of the magnetic twisted tube metric is negative. Solar flare production may appear from these geometrical instabilities of the twisted solar loops.
physics.plasm-ph physics.flu-dyn
riemann and sectional curvatures of magnetic twisted flux tubes in riemannian manifold are computed to investigate the stability of the plasma astrophysical tubes the geodesic equations are used to show that in the case of thick magnetic tubes the curvature of planar frenet torsionfree tubes have the effect ct of damping the flow speed along the tube stability of geodesic flows in the riemannian twisted thin tubes almost filaments against constant radial perturbations is investigated by using the method of negative sectional curvature for unstable flows no special form of the flow like beltrami flows is admitted and the proof is general for the case of thin magnetic flux tubes in the magnetic equilibrium state the twist of the tube is shown to display also a damping effect on the toroidal velocity of the plasma flow it is found that for positive perturbations and angular speed of the flow instability is achieved since the sectional ricci curvature of the magnetic twisted tube metric is negative solar flare production may appear from these geometrical instabilities of the twisted solar loops
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708.3474
Nonlinear control of chaotic walking of atoms in an optical lattice
Centre-of-mass atomic motion in an optical lattice near the resonance is shown to be a chaotic walking due to the interplay between coherent internal atomic dynamics and spontaneous emission. Statistical properties of chaotic atomic motion can be controlled by the single parameter, the detuning between the atomic transition frequency and the laser frequency. We derive a Fokker-Planck equation in the energetic space to describe the atomic transport near the resonance and demonstrate numerically how to manipulate the atomic motion varying the detuning.
quant-ph
centreofmass atomic motion in an optical lattice near the resonance is shown to be a chaotic walking due to the interplay between coherent internal atomic dynamics and spontaneous emission statistical properties of chaotic atomic motion can be controlled by the single parameter the detuning between the atomic transition frequency and the laser frequency we derive a fokkerplanck equation in the energetic space to describe the atomic transport near the resonance and demonstrate numerically how to manipulate the atomic motion varying the detuning
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708.3475
Optical sum rule anomalies in the cuprates: interplay between strong correlation and electronic bandstructures
We theoretically analyze some of the anomalies of the optical sumrules in the high-temperature superconductors. In particular we address the particularly strong dependence on temperature of the sumrule in the normal state. Both electron-electron correlations and the presence of a Van-Hove singularity have been shown to enhance such a dependence. Here we consider both effects simultaneously by means of Dynamical Mean-Field Theory for a two dimensional Hubbard model with realistic parameters for different cuprates, and we find that the two effects are not cooperative, as they appear to compete one another in the region of parameters relevant for the experiments.
cond-mat.str-el
we theoretically analyze some of the anomalies of the optical sumrules in the hightemperature superconductors in particular we address the particularly strong dependence on temperature of the sumrule in the normal state both electronelectron correlations and the presence of a vanhove singularity have been shown to enhance such a dependence here we consider both effects simultaneously by means of dynamical meanfield theory for a two dimensional hubbard model with realistic parameters for different cuprates and we find that the two effects are not cooperative as they appear to compete one another in the region of parameters relevant for the experiments
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708.3476
Mean Field Theory for Pedestrian Outflow through an Exit
An average pedestrian flow through an exit is one of the most important index in evaluating pedestrian dynamics. In order to study the flow in detail, the floor field model, which is a crowd model by using cellular automaton, is extended by taking into account a realistic behavior of pedestrians around the exit. The model is studied by both numerical simulations and cluster analysis to obtain a theoretical expression of an average pedestrian flow through the exit. It is found quantitatively that the effect of exit door width, a wall, and pedestrian's mood of competition or cooperation significantly influence the average flow. The results show that there is suitable width of the exit and position according to pedestrian's mood.
cond-mat.stat-mech physics.soc-ph
an average pedestrian flow through an exit is one of the most important index in evaluating pedestrian dynamics in order to study the flow in detail the floor field model which is a crowd model by using cellular automaton is extended by taking into account a realistic behavior of pedestrians around the exit the model is studied by both numerical simulations and cluster analysis to obtain a theoretical expression of an average pedestrian flow through the exit it is found quantitatively that the effect of exit door width a wall and pedestrians mood of competition or cooperation significantly influence the average flow the results show that there is suitable width of the exit and position according to pedestrians mood
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708.3477
The Church Synthesis Problem with Parameters
For a two-variable formula &psi;(X,Y) of Monadic Logic of Order (MLO) the Church Synthesis Problem concerns the existence and construction of an operator Y=F(X) such that &psi;(X,F(X)) is universally valid over Nat. B\"{u}chi and Landweber proved that the Church synthesis problem is decidable; moreover, they showed that if there is an operator F that solves the Church Synthesis Problem, then it can also be solved by an operator defined by a finite state automaton or equivalently by an MLO formula. We investigate a parameterized version of the Church synthesis problem. In this version &psi; might contain as a parameter a unary predicate P. We show that the Church synthesis problem for P is computable if and only if the monadic theory of <Nat,<,P> is decidable. We prove that the B\"{u}chi-Landweber theorem can be extended only to ultimately periodic parameters. However, the MLO-definability part of the B\"{u}chi-Landweber theorem holds for the parameterized version of the Church synthesis problem.
cs.LO
for a twovariable formula psixy of monadic logic of order mlo the church synthesis problem concerns the existence and construction of an operator yfx such that psixfx is universally valid over nat buchi and landweber proved that the church synthesis problem is decidable moreover they showed that if there is an operator f that solves the church synthesis problem then it can also be solved by an operator defined by a finite state automaton or equivalently by an mlo formula we investigate a parameterized version of the church synthesis problem in this version psi might contain as a parameter a unary predicate p we show that the church synthesis problem for p is computable if and only if the monadic theory of natp is decidable we prove that the buchilandweber theorem can be extended only to ultimately periodic parameters however the mlodefinability part of the buchilandweber theorem holds for the parameterized version of the church synthesis problem
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708.3478
Feedback from Multiple Supernova Explosions inside a Wind-Blown Bubble
We study the evolution of multiple supernova (SN) explosions inside a pre-exiting cavity blown by winds from massive progenitor stars. Hydrodynamic simulations in one-dimensional spherical geometry, including radiative cooling and thermal conduction, are carried out to follow first the development of the wind-blown bubble during the main sequence and then the evolution of the SN-driven bubble. We find the size and mass of the SN-driven bubble shell depend on the structure of the pre-existing wind bubble as well as the SN explosion energy E_{SN} (= N_{SN} 10^{51} ergs). The hot cavity inside the bubble is 2-3 times bigger in volume and hotter than that of a bubble created by SNe exploded in a uniform interstellar medium (ISM). For an association with 10 massive stars in the average ISM, the SN-driven shell has an outer radius of R_{ss} ~ (85 pc) N_{SN}^{0.1} and a mass of M_{ss} ~ (10^{4.8} Msun) N_{SN}^{0.3}at 10^6 years after the explosion. By that time most of the explosion energy is lost via radiative cooling, while ~10% remains as kinetic energy and ~10% as thermal energy. We also calculate the total integrated spectrum of diffuse radiation emitted by the shock-heated gas of the SN bubble. For the models with 0.1 solar metalicity, the radiative energy loss is smaller and the fraction of non-ionizing photons is larger, compared to those with solar metalicity. We conclude the photoionization/heating by diffuse radiation is the most dominant form of feedback from SN explosions into the surrounding medium.
astro-ph
we study the evolution of multiple supernova sn explosions inside a preexiting cavity blown by winds from massive progenitor stars hydrodynamic simulations in onedimensional spherical geometry including radiative cooling and thermal conduction are carried out to follow first the development of the windblown bubble during the main sequence and then the evolution of the sndriven bubble we find the size and mass of the sndriven bubble shell depend on the structure of the preexisting wind bubble as well as the sn explosion energy e_sn n_sn 1051 ergs the hot cavity inside the bubble is 23 times bigger in volume and hotter than that of a bubble created by sne exploded in a uniform interstellar medium ism for an association with 10 massive stars in the average ism the sndriven shell has an outer radius of r_ss 85 pc n_sn01 and a mass of m_ss 1048 msun n_sn03at 106 years after the explosion by that time most of the explosion energy is lost via radiative cooling while 10 remains as kinetic energy and 10 as thermal energy we also calculate the total integrated spectrum of diffuse radiation emitted by the shockheated gas of the sn bubble for the models with 01 solar metalicity the radiative energy loss is smaller and the fraction of nonionizing photons is larger compared to those with solar metalicity we conclude the photoionizationheating by diffuse radiation is the most dominant form of feedback from sn explosions into the surrounding medium
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708.3479
Possible nodeless superconductivity in the noncentrosymmetric superconductor Mg_(12-delta)Ir_19B_16
We measured the resistivity, diamagnetization, and low-temperature specific heat of the newly discovered noncentrosymmetric superconductor Mg_(12-delta)Ir_19B_16. The temperature dependence of specific heat is consistent with the model of an isotropic s-wave gap with value Delta_0 = 0.94 meV for the sample Tc = 5.7 K, and the ratio Delta_0/k_BTc = 1.91 indicates a slightly moderate coupling for the superconductivity. The correlations among the normal state Sommerfeld constant gamma_n, the slope -dHc2(T)/dT near Tc, and the condensation energy Ec are all consistent with the slightly moderate coupling picture. Based on the data of phonon contribution, Tc and the McMillan formula, we obtained an electron-phonon coupling strength lambda_(e-ph) = 0.66, which suggests that the superconductivity here is induced by the electron-phonon coupling.
cond-mat.supr-con
we measured the resistivity diamagnetization and lowtemperature specific heat of the newly discovered noncentrosymmetric superconductor mg_12deltair_19b_16 the temperature dependence of specific heat is consistent with the model of an isotropic swave gap with value delta_0 094 mev for the sample tc 57 k and the ratio delta_0k_btc 191 indicates a slightly moderate coupling for the superconductivity the correlations among the normal state sommerfeld constant gamma_n the slope dhc2tdt near tc and the condensation energy ec are all consistent with the slightly moderate coupling picture based on the data of phonon contribution tc and the mcmillan formula we obtained an electronphonon coupling strength lambda_eph 066 which suggests that the superconductivity here is induced by the electronphonon coupling
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708.348
On the Theory of Surfaces in the Four-dimensional Euclidean Space
For a two-dimensional surface in the four-dimensional Euclidean space we introduce an invariant linear map of Weingarten type in the tangent space of the surface, which generates two invariants k and kappa. The condition k = kappa = 0 characterizes the surfaces consisting of flat points. The minimal surfaces are characterized by the equality kappa^2=k. The class of the surfaces with flat normal connection is characterized by the condition kappa = 0. For the surfaces of general type we obtain a geometrically determined orthonormal frame field at each point and derive Frenet-type derivative formulas. We apply our theory to the class of the rotational surfaces, which prove to be surfaces with flat normal connection, and describe the rotational surfaces with constant invariants.
math.DG
for a twodimensional surface in the fourdimensional euclidean space we introduce an invariant linear map of weingarten type in the tangent space of the surface which generates two invariants k and kappa the condition k kappa 0 characterizes the surfaces consisting of flat points the minimal surfaces are characterized by the equality kappa2k the class of the surfaces with flat normal connection is characterized by the condition kappa 0 for the surfaces of general type we obtain a geometrically determined orthonormal frame field at each point and derive frenettype derivative formulas we apply our theory to the class of the rotational surfaces which prove to be surfaces with flat normal connection and describe the rotational surfaces with constant invariants
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708.3481
Formation of Multipartite Entanglement Using Random Quantum Gates
The formation of multipartite quantum entanglement by repeated operation of one and two qubit gates is examined. The resulting entanglement is evaluated using two measures: the average bipartite entanglement and the Groverian measure. A comparison is made between two geometries of the quantum register: a one dimensional chain in which two-qubit gates apply only locally between nearest neighbors and a non-local geometry in which such gates may apply between any pair of qubits. More specifically, we use a combination of random single qubit rotations and a fixed two-qubit gate such as the controlled-phase gate. It is found that in the non-local geometry the entanglement is generated at a higher rate. In both geometries, the Groverian measure converges to its asymptotic value more slowly than the average bipartite entanglement. These results are expected to have implications on different proposed geometries of future quantum computers with local and non-local interactions between the qubits.
quant-ph
the formation of multipartite quantum entanglement by repeated operation of one and two qubit gates is examined the resulting entanglement is evaluated using two measures the average bipartite entanglement and the groverian measure a comparison is made between two geometries of the quantum register a one dimensional chain in which twoqubit gates apply only locally between nearest neighbors and a nonlocal geometry in which such gates may apply between any pair of qubits more specifically we use a combination of random single qubit rotations and a fixed twoqubit gate such as the controlledphase gate it is found that in the nonlocal geometry the entanglement is generated at a higher rate in both geometries the groverian measure converges to its asymptotic value more slowly than the average bipartite entanglement these results are expected to have implications on different proposed geometries of future quantum computers with local and nonlocal interactions between the qubits
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708.3482
Designing a Spin Channel for Perfect Quantum Communication
We propose a scheme for using a spin chain with fixed symmetry interaction as a channel for perfect quantum communication. The perfect quantum communication is determined by the eigenvalues that form a special arithmetical progression, the concrete interaction parameter $J_i$ is obtained as a function of integer and perfect transmission time $t_p$. There are infinite choices of $J_i$ for perfect transmission and one can design the channel according to the requirement of $t_p$. This scheme will provide more choices of spin chain for future experiment in quantum communication.
quant-ph
we propose a scheme for using a spin chain with fixed symmetry interaction as a channel for perfect quantum communication the perfect quantum communication is determined by the eigenvalues that form a special arithmetical progression the concrete interaction parameter j_i is obtained as a function of integer and perfect transmission time t_p there are infinite choices of j_i for perfect transmission and one can design the channel according to the requirement of t_p this scheme will provide more choices of spin chain for future experiment in quantum communication
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708.3483
An Ideal Channel of Long Distance Entanglement in Spin Systems
We propose a scheme for using spin chain to realize an ideal channel of long distance entanglement. The results show that there has different entanglement in different Hilbert subspace, the anisotropic parameter $\Delta$ will frustrate the entanglement and the magnetic field affect the entanglement through changing the ground state, the boundary entanglement $C_{1N}$ has the simplest expression in the simplest subspace and it only depend on the first item of the ground state, that item can be increased when a local magnetic field is introduced. Our propose can be handled easily because it only needs a uniform XX open chain initialized in the simplest Hilbert subspace and a bulk magnetic field that absent for the boundary qubits.
quant-ph
we propose a scheme for using spin chain to realize an ideal channel of long distance entanglement the results show that there has different entanglement in different hilbert subspace the anisotropic parameter delta will frustrate the entanglement and the magnetic field affect the entanglement through changing the ground state the boundary entanglement c_1n has the simplest expression in the simplest subspace and it only depend on the first item of the ground state that item can be increased when a local magnetic field is introduced our propose can be handled easily because it only needs a uniform xx open chain initialized in the simplest hilbert subspace and a bulk magnetic field that absent for the boundary qubits
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708.3484
(p,q)-string in matrix-regularized membrane and type IIB duality
We consider a lightcone wrapped supermembrane compactified on 2-torus in the matrix regularization. We examine the double dimensional reduction technique and deduce the free matrix string of (p,q)-string in type IIB superstring theory explicitly from the matrix-regularized wrapped supermembrane. In addition we obtain the (2+1)-dimensional super Yang-Mills action in curved background. We also examine the duality.
hep-th
we consider a lightcone wrapped supermembrane compactified on 2torus in the matrix regularization we examine the double dimensional reduction technique and deduce the free matrix string of pqstring in type iib superstring theory explicitly from the matrixregularized wrapped supermembrane in addition we obtain the 21dimensional super yangmills action in curved background we also examine the duality
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708.3485
Unparticle decay of neutrinos and it's effect on ultra high energy neutrinos
The unparticle is proposed by Georgi as a conceptual new physics beyond the standard model to describe the low energy sector of a nontrivial scale invariant sector of an effective theory. We consider the neutrino decay in unparticle scenario and investigate the effect of such decay for the case of ultra high energy neutrinos from GRB. The effect on the detection yield of these neutrinos are also probed for a kilometer scale ice-Cerenkov detector.
hep-ph
the unparticle is proposed by georgi as a conceptual new physics beyond the standard model to describe the low energy sector of a nontrivial scale invariant sector of an effective theory we consider the neutrino decay in unparticle scenario and investigate the effect of such decay for the case of ultra high energy neutrinos from grb the effect on the detection yield of these neutrinos are also probed for a kilometer scale icecerenkov detector
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708.3486
On topological spaces possessing uniformly distributed sequences
Two classes of topological spaces are introduced on which every probability Radon measure possesses a uniformly distributed sequence or a uniformly tight uniformly distributed sequence. It is shown that these classes are stable under multiplication by completely regular Souslin spaces
math.GN math.PR
two classes of topological spaces are introduced on which every probability radon measure possesses a uniformly distributed sequence or a uniformly tight uniformly distributed sequence it is shown that these classes are stable under multiplication by completely regular souslin spaces
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708.3487
Threadbare Parallel Port DAQ Card
A very simple Data acquisition card was developed in our under-graduate class for interfacing with the parallel port of a standard computer. It was developed with the intention to enable students to do various physics experiments with the computer sparing them from knowing the details of the electronics required. The article is a summary of our experience and ends with a request for suggestions to improve the circuit without losing its simplicity.
physics.ed-ph
a very simple data acquisition card was developed in our undergraduate class for interfacing with the parallel port of a standard computer it was developed with the intention to enable students to do various physics experiments with the computer sparing them from knowing the details of the electronics required the article is a summary of our experience and ends with a request for suggestions to improve the circuit without losing its simplicity
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708.3488
Magnetometry Based on Nonlinear Magneto-Optical Rotation with Amplitude-Modulated Light
We report on an all-optical magnetometric technique based on nonlinear magneto-optical rotation with amplitude-modulated light. The method enables sensitive magnetic-field measurements in a broad dynamic range. We demonstrate the sensitivity of $4.3\times10^{-9}$ G/$\sqrt{\text{Hz}}$ at 10 mG and the magnetic field tracking in a range of 40 mG. The fundamental limits of the method sensitivity and factors determining current performance of the magnetometer are discussed.
physics.atom-ph physics.optics
we report on an alloptical magnetometric technique based on nonlinear magnetooptical rotation with amplitudemodulated light the method enables sensitive magneticfield measurements in a broad dynamic range we demonstrate the sensitivity of 43times109 gsqrttexthz at 10 mg and the magnetic field tracking in a range of 40 mg the fundamental limits of the method sensitivity and factors determining current performance of the magnetometer are discussed
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708.3489
Extrema of low eigenvalues of the Dirichlet-Neumann Laplacian on a disk
We study extrema of the first and the second mixed eigenvalues of the Laplacian on the disk among some families of Dirichlet-Neumann boundary conditions. We show that the minimizer of the second eigenvalue among all mixed boundary conditions lies in a compact 1-parameter family for which an explicit description is given. Moreover, we prove that among all partitions of the boundary with bounded number of parts on which Dirichlet and Neumann conditions are imposed alternately, the first eigenvalue is maximized by the uniformly distributed partition.
math.SP
we study extrema of the first and the second mixed eigenvalues of the laplacian on the disk among some families of dirichletneumann boundary conditions we show that the minimizer of the second eigenvalue among all mixed boundary conditions lies in a compact 1parameter family for which an explicit description is given moreover we prove that among all partitions of the boundary with bounded number of parts on which dirichlet and neumann conditions are imposed alternately the first eigenvalue is maximized by the uniformly distributed partition
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708.349
Two-Dimensional Spectroscopy of Photospheric Shear Flows in a Small delta Spot
In recent high-resolution observations of complex active regions, long-lasting and well-defined regions of strong flows were identified in major flares and associated with bright kernels of visible, near-infrared, and X-ray radiation. These flows, which occurred in the proximity of the magnetic neutral line, significantly contributed to the generation of magnetic shear. Signatures of these shear flows are strongly curved penumbral filaments, which are almost tangential to sunspot umbrae rather than exhibiting the typical radial filamentary structure. Solar active region NOAA 10756 was a moderately complex, beta-delta sunspot group, which provided an opportunity to extend previous studies of such shear flows to quieter settings. We conclude that shear flows are a common phenomenon in complex active regions and delta spots. However, they are not necessarily a prerequisite condition for flaring. Indeed, in the present observations, the photospheric shear flows along the magnetic neutral line are not related to any change of the local magnetic shear. We present high-resolution observations of NOAA 10756 obtained with the 65-cm vacuum reflector at Big Bear Solar Observatory (BBSO). Time series of speckle-reconstructed white-light images and two-dimensional spectroscopic data were combined to study the temporal evolution of the three-dimensional vector flow field in the beta-delta sunspot group. An hour-long data set of consistent high quality was obtained, which had a cadence of better than 30 seconds and sub-arcsecond spatial resolution.
astro-ph
in recent highresolution observations of complex active regions longlasting and welldefined regions of strong flows were identified in major flares and associated with bright kernels of visible nearinfrared and xray radiation these flows which occurred in the proximity of the magnetic neutral line significantly contributed to the generation of magnetic shear signatures of these shear flows are strongly curved penumbral filaments which are almost tangential to sunspot umbrae rather than exhibiting the typical radial filamentary structure solar active region noaa 10756 was a moderately complex betadelta sunspot group which provided an opportunity to extend previous studies of such shear flows to quieter settings we conclude that shear flows are a common phenomenon in complex active regions and delta spots however they are not necessarily a prerequisite condition for flaring indeed in the present observations the photospheric shear flows along the magnetic neutral line are not related to any change of the local magnetic shear we present highresolution observations of noaa 10756 obtained with the 65cm vacuum reflector at big bear solar observatory bbso time series of specklereconstructed whitelight images and twodimensional spectroscopic data were combined to study the temporal evolution of the threedimensional vector flow field in the betadelta sunspot group an hourlong data set of consistent high quality was obtained which had a cadence of better than 30 seconds and subarcsecond spatial resolution
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708.3491
Equation of State of Wet Granular Matter
A theory is derived for the nonequilibrium probability currents of the capillary interaction which determines the pair correlation function near contact. This yields an analytic expression for the equation of state, P = P(N/V,T), of wet granular matter for D=2 dimensions, valid in the complete density range from gas to jamming. Driven wet granular matter exhibits a van-der-Waals-like unstable branch at granular temperatures T<T_c corresponding to a first order segregation transition of clusters. For the realistic rupture length of the liquid bridge, s_crit=0.07 d, the critical point is located at T_c = 0.274 E_cb. While the critical temperature weakly depends on the rupture length, the critical density phi_c is shown to scale with s_crit according to s_crit = 4d (sqrt(phi_J / phi_c) -1). The segregation transition is closely related to the precipitation of granular droplets reported for the free cooling of one-dimensional wet granular matter [Phys. Rev. Lett. 97, 078001 (2006)], and extends the effect to higher dimensional systems. Since the limiting case of sticky bonds, E_cb >> T, is of relevance for aggregation in general, simulations have been performed which show very good agreement with the theoretically predicted coordination K of capillary bonds as a function of the bond length s_crit. This result implies that particles that stick at the surface, s_crit=0, form isostatic clusters.
cond-mat.soft
a theory is derived for the nonequilibrium probability currents of the capillary interaction which determines the pair correlation function near contact this yields an analytic expression for the equation of state p pnvt of wet granular matter for d2 dimensions valid in the complete density range from gas to jamming driven wet granular matter exhibits a vanderwaalslike unstable branch at granular temperatures tt_c corresponding to a first order segregation transition of clusters for the realistic rupture length of the liquid bridge s_crit007 d the critical point is located at t_c 0274 e_cb while the critical temperature weakly depends on the rupture length the critical density phi_c is shown to scale with s_crit according to s_crit 4d sqrtphi_j phi_c 1 the segregation transition is closely related to the precipitation of granular droplets reported for the free cooling of onedimensional wet granular matter phys rev lett 97 078001 2006 and extends the effect to higher dimensional systems since the limiting case of sticky bonds e_cb t is of relevance for aggregation in general simulations have been performed which show very good agreement with the theoretically predicted coordination k of capillary bonds as a function of the bond length s_crit this result implies that particles that stick at the surface s_crit0 form isostatic clusters
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708.3492
The Variability of Polarized Radiation from Sgr A*
Sgr A* is variable at radio and submillimeter wavelengths on hourly time scales showing time delays between the peaks of flare emission as well as linearly polarized emission at millimeter and sub-mm wavelengths. To determine the polarization characteristics of this variable source at radio frequencies, we present VLA observations of Sgr A* and report the detection of polarized emission at a level of 0.77\pm0.01% and 0.2\pm0.01% at 43 and 22 GHz, respectively. The change in the time averaged polarization angle between 22 and 43 GHz corresponds to a RM of -2.5\pm0.6 x10^3 rad m{-2} with no phase wrapping (or \sim 5x10^4 rad m^2 with 2\pi phase wrap). We also note a rise and fall time scale of 1.5 -- 2 hours in the total polarized intensity. The light curves of the degree of linearly polarized emission suggests a a correlation with the variability of the total intensity at 43 GHz. The available polarization data at radio and sub-mm wavelengths suggest that the rotation measure decreases with decreasing frequency. This frequency dependence, and observed changes in polarization angle during flare events, may be caused by the reduction in rotation measure associated with the expansion of synchrotron-emitting blobs.
astro-ph
sgr a is variable at radio and submillimeter wavelengths on hourly time scales showing time delays between the peaks of flare emission as well as linearly polarized emission at millimeter and submm wavelengths to determine the polarization characteristics of this variable source at radio frequencies we present vla observations of sgr a and report the detection of polarized emission at a level of 077pm001 and 02pm001 at 43 and 22 ghz respectively the change in the time averaged polarization angle between 22 and 43 ghz corresponds to a rm of 25pm06 x103 rad m2 with no phase wrapping or sim 5x104 rad m2 with 2pi phase wrap we also note a rise and fall time scale of 15 2 hours in the total polarized intensity the light curves of the degree of linearly polarized emission suggests a a correlation with the variability of the total intensity at 43 ghz the available polarization data at radio and submm wavelengths suggest that the rotation measure decreases with decreasing frequency this frequency dependence and observed changes in polarization angle during flare events may be caused by the reduction in rotation measure associated with the expansion of synchrotronemitting blobs
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708.3493
Best network chirplet-chain: Near-optimal coherent detection of unmodeled gravitation wave chirps with a network of detectors
The searches of impulsive gravitational waves (GW) in the data of the ground-based interferometers focus essentially on two types of waveforms: short unmodeled bursts and chirps from inspiralling compact binaries. There is room for other types of searches based on different models. Our objective is to fill this gap. More specifically, we are interested in GW chirps with an arbitrary phase/frequency vs. time evolution. These unmodeled GW chirps may be considered as the generic signature of orbiting/spinning sources. We expect quasi-periodic nature of the waveform to be preserved independent of the physics which governs the source motion. Several methods have been introduced to address the detection of unmodeled chirps using the data of a single detector. Those include the best chirplet chain (BCC) algorithm introduced by the authors. In the next years, several detectors will be in operation. The joint coherent analysis of GW by multiple detectors can improve the sight horizon, the estimation of the source location and the wave polarization angles. Here, we extend the BCC search to the multiple detector case. The method amounts to searching for salient paths in the combined time-frequency representation of two synthetic streams. The latter are time-series which combine the data from each detector linearly in such a way that all the GW signatures received are added constructively. We give a proof of principle for the full sky blind search in a simplified situation which shows that the joint estimation of the source sky location and chirp frequency is possible.
gr-qc
the searches of impulsive gravitational waves gw in the data of the groundbased interferometers focus essentially on two types of waveforms short unmodeled bursts and chirps from inspiralling compact binaries there is room for other types of searches based on different models our objective is to fill this gap more specifically we are interested in gw chirps with an arbitrary phasefrequency vs time evolution these unmodeled gw chirps may be considered as the generic signature of orbitingspinning sources we expect quasiperiodic nature of the waveform to be preserved independent of the physics which governs the source motion several methods have been introduced to address the detection of unmodeled chirps using the data of a single detector those include the best chirplet chain bcc algorithm introduced by the authors in the next years several detectors will be in operation the joint coherent analysis of gw by multiple detectors can improve the sight horizon the estimation of the source location and the wave polarization angles here we extend the bcc search to the multiple detector case the method amounts to searching for salient paths in the combined timefrequency representation of two synthetic streams the latter are timeseries which combine the data from each detector linearly in such a way that all the gw signatures received are added constructively we give a proof of principle for the full sky blind search in a simplified situation which shows that the joint estimation of the source sky location and chirp frequency is possible
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708.3494
Fidelity Between Partial States as Signature of Quantum Phase Transitions
We introduce a partial state fidelity approach to quantum phase transitions. We consider a superconducting lattice with a magnetic impurity inserted at its centre, and look at the fidelity between partial (either one-site or two-site) quantum states. In the vicinity of the point of the quantum phase transition, we observe a sudden drop of the fidelity between two one-site partial states corresponding to the impurity location and its close vicinity. In the case of two-site states, the fidelity reveals the transition point as long as one of the two electron sites is located at the impurity, while the other lies elsewhere in the lattice. We also determine the Uhlmann mixed state geometric phase, recently introduced in the study of the structural change of the system state eigenvectors in the vicinity of the lines of thermal phase transitions, and find it to be trivial, both for one- and two-site partial states, except when an electron site is at the impurity. This means that the system partial state eigenvectors do not contribute significantly to the enhanced state distinguishability around the point of this quantum phase transition. Finally, we use the fidelity to analyze the total amount of correlations contained within a composite system, showing that, even for the smallest two-site states, it features an abrupt quantitative change in the vicinity of the point of the quantum phase transition.
quant-ph cond-mat.str-el
we introduce a partial state fidelity approach to quantum phase transitions we consider a superconducting lattice with a magnetic impurity inserted at its centre and look at the fidelity between partial either onesite or twosite quantum states in the vicinity of the point of the quantum phase transition we observe a sudden drop of the fidelity between two onesite partial states corresponding to the impurity location and its close vicinity in the case of twosite states the fidelity reveals the transition point as long as one of the two electron sites is located at the impurity while the other lies elsewhere in the lattice we also determine the uhlmann mixed state geometric phase recently introduced in the study of the structural change of the system state eigenvectors in the vicinity of the lines of thermal phase transitions and find it to be trivial both for one and twosite partial states except when an electron site is at the impurity this means that the system partial state eigenvectors do not contribute significantly to the enhanced state distinguishability around the point of this quantum phase transition finally we use the fidelity to analyze the total amount of correlations contained within a composite system showing that even for the smallest twosite states it features an abrupt quantitative change in the vicinity of the point of the quantum phase transition
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708.3495
Study of the young stellar population of NGC 4214 using the Hubble Space Telescope
We present an original study of the dwarf starburst galaxy NGC 4214. We use archival optical and UV images obtained with WFPC2 and STIS on-board the Hubble Space Telescope. We explain the process followed to obtain high-quality photometry and astrometry of the stellar and cluster populations of this galaxy. We describe the procedure used to transform magnitudes and colours into physical parameters using spectral energy distributions. We analyze several aspects of the astrophysics of NGC 4214: we briefly describe the stellar populations in its inner structure with emphasis in the determination of the ratio of blue-to-red supergiants. We study the stellar extinction and we find it consistent with previous studies of the nebular extinction. The extinction associated to the stellar population is found to be rather low (E(B-V) < 0.1 mag). We make a complete research of the initial mass function (IMF) of the stars with masses between 20 and 100 Mo using a photometric method. We find that this dwarf galaxy has a steeper IMF than Salpeter. We analyze several extended structures distributed throughout the central regions of NGC 4214. We infer their properties, such as age, mass, and extinction. Some of the clusters that we study are likely to disappear because of "infant mortality". We discuss the interaction between massive stars and their environment. We argue that star formation in NGC 4214 could take place in several stages.
astro-ph
we present an original study of the dwarf starburst galaxy ngc 4214 we use archival optical and uv images obtained with wfpc2 and stis onboard the hubble space telescope we explain the process followed to obtain highquality photometry and astrometry of the stellar and cluster populations of this galaxy we describe the procedure used to transform magnitudes and colours into physical parameters using spectral energy distributions we analyze several aspects of the astrophysics of ngc 4214 we briefly describe the stellar populations in its inner structure with emphasis in the determination of the ratio of bluetored supergiants we study the stellar extinction and we find it consistent with previous studies of the nebular extinction the extinction associated to the stellar population is found to be rather low ebv 01 mag we make a complete research of the initial mass function imf of the stars with masses between 20 and 100 mo using a photometric method we find that this dwarf galaxy has a steeper imf than salpeter we analyze several extended structures distributed throughout the central regions of ngc 4214 we infer their properties such as age mass and extinction some of the clusters that we study are likely to disappear because of infant mortality we discuss the interaction between massive stars and their environment we argue that star formation in ngc 4214 could take place in several stages
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708.3496
Threshold effect and \pi^\pm \psi(2S) peak
A resonance-like structure in the $\pi^\pm \psi(2S)$ mass spectrum arising in $B \to K \pi^\pm \psi(2S)$ has recently been reported. It is noted that the mass of this structure, $4433 \pm 4 \pm 1$ MeV, is not far from the threshold for production of $D^* \bar{D}_1(2420)$. A proposed mechanism for production of this state is suggested, and tests are suggested.
hep-ph
a resonancelike structure in the pipm psi2s mass spectrum arising in b to k pipm psi2s has recently been reported it is noted that the mass of this structure 4433 pm 4 pm 1 mev is not far from the threshold for production of d bard_12420 a proposed mechanism for production of this state is suggested and tests are suggested
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708.3497
A Mechanism for Kaluza-Klein Number Violation in UED and Implications for LHC
If the Higgs does not propagate into an otherwise universal extra dimension, then tree-level Kaluza-Klein number is not conserved in the Yukawa interactions. This leads to mixing between zero-mode fermions and their associated Kaluza-Klein excitations. The effect can be quite large for the top quark, since its mass (171.4 plus or minus 2.1 GeV) is approximately one-half the current Tevatron mass bound (about 350-400 GeV) for Kaluza-Klein excitations of quarks with one universal extra dimension. In contrast to the SM, the bi-unitary transformation that diagonalizes the mass matrix does not diagonalize the effective 4D Yukawa coupling matrix because of the presence of the 5D kinetic terms. This leads to violation of tree-level Kaluza-Klein number conservation in the gauge sector due to a unique feature of the 5D theory. This allows Kaluza-Klein excitations of the fermions to be produced singly, and opens up new decay channels in the gauge sector. We compute the cross section for the production of the lowest-lying Kaluza-Klein excitations of the top and bottom quarks in the non-universal Higgs model at the Large Hadron Collider, and consider their subsequent decays. The effect is quite large: For example, pair production of Kaluza-Klein excitations of the bottom quark will lead to a pair of top quarks plus a pair of charged weak gauge bosons. Since the production is via the strong interaction, such final states stand out well against the Standard Model background, and are observable at the LHC for a wide range of compactification scales. Finally, we discuss the effects that such a model has on the T- parameter, and propose a model with maximal mixing where the compactification scale may be as large as a universal extra dimension.
hep-ph
if the higgs does not propagate into an otherwise universal extra dimension then treelevel kaluzaklein number is not conserved in the yukawa interactions this leads to mixing between zeromode fermions and their associated kaluzaklein excitations the effect can be quite large for the top quark since its mass 1714 plus or minus 21 gev is approximately onehalf the current tevatron mass bound about 350400 gev for kaluzaklein excitations of quarks with one universal extra dimension in contrast to the sm the biunitary transformation that diagonalizes the mass matrix does not diagonalize the effective 4d yukawa coupling matrix because of the presence of the 5d kinetic terms this leads to violation of treelevel kaluzaklein number conservation in the gauge sector due to a unique feature of the 5d theory this allows kaluzaklein excitations of the fermions to be produced singly and opens up new decay channels in the gauge sector we compute the cross section for the production of the lowestlying kaluzaklein excitations of the top and bottom quarks in the nonuniversal higgs model at the large hadron collider and consider their subsequent decays the effect is quite large for example pair production of kaluzaklein excitations of the bottom quark will lead to a pair of top quarks plus a pair of charged weak gauge bosons since the production is via the strong interaction such final states stand out well against the standard model background and are observable at the lhc for a wide range of compactification scales finally we discuss the effects that such a model has on the t parameter and propose a model with maximal mixing where the compactification scale may be as large as a universal extra dimension
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708.3498
Voltage Controlled Resistance
The paper discusses an application of the field effected transistor (FET) as a voltage controlled resistance which can be done in under-graduate labs either as a routine experiment or as a project.
physics.ed-ph
the paper discusses an application of the field effected transistor fet as a voltage controlled resistance which can be done in undergraduate labs either as a routine experiment or as a project
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708.3499
Comparison of Tree-Child Phylogenetic Networks
Phylogenetic networks are a generalization of phylogenetic trees that allow for the representation of non-treelike evolutionary events, like recombination, hybridization, or lateral gene transfer. In this paper, we present and study a new class of phylogenetic networks, called tree-child phylogenetic networks, where every non-extant species has some descendant through mutation. We provide an injective representation of these networks as multisets of vectors of natural numbers, their path multiplicity vectors, and we use this representation to define a distance on this class and to give an alignment method for pairs of these networks. To the best of our knowledge, they are respectively the first true distance and the first alignment method defined on a meaningful class of phylogenetic networks strictly extending the class of phylogenetic trees. Simple, polynomial algorithms for reconstructing a tree-child phylogenetic network from its path multiplicity vectors, for computing the distance between two tree-child phylogenetic networks, and for aligning a pair of tree-child phylogenetic networks, are provided, and they have been implemented as a Perl package and a Java applet, and they are available at http://bioinfo.uib.es/~recerca/phylonetworks/mudistance
q-bio.PE cs.CE cs.DM
phylogenetic networks are a generalization of phylogenetic trees that allow for the representation of nontreelike evolutionary events like recombination hybridization or lateral gene transfer in this paper we present and study a new class of phylogenetic networks called treechild phylogenetic networks where every nonextant species has some descendant through mutation we provide an injective representation of these networks as multisets of vectors of natural numbers their path multiplicity vectors and we use this representation to define a distance on this class and to give an alignment method for pairs of these networks to the best of our knowledge they are respectively the first true distance and the first alignment method defined on a meaningful class of phylogenetic networks strictly extending the class of phylogenetic trees simple polynomial algorithms for reconstructing a treechild phylogenetic network from its path multiplicity vectors for computing the distance between two treechild phylogenetic networks and for aligning a pair of treechild phylogenetic networks are provided and they have been implemented as a perl package and a java applet and they are available at httpbioinfouibesrecercaphylonetworksmudistance
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708.35
Monte Carlo simulation of the nuclear medium: Fermi gases, nuclei and the role of Pauli potentials
The role of Pauli potentials in the semiclassical simulation of Fermi gases at low temperatures is investigated. An alternative Pauli potential to the usual bivariate Gaussian form by Dorso et al. is proposed. This new Pauli potential allows for a simultaneous good reproduction of not only the kinetic energy per particle but also the momentum distribution and the two-body correlation function. The reproduction of the binding energies in finite nuclei in the low and medium mass range is also analyzed. What is found is that given a reasonable short-range atractive nuclear interaction one can include correlation effects in a suitable chosen density dependent Pauli potential.
nucl-th
the role of pauli potentials in the semiclassical simulation of fermi gases at low temperatures is investigated an alternative pauli potential to the usual bivariate gaussian form by dorso et al is proposed this new pauli potential allows for a simultaneous good reproduction of not only the kinetic energy per particle but also the momentum distribution and the twobody correlation function the reproduction of the binding energies in finite nuclei in the low and medium mass range is also analyzed what is found is that given a reasonable shortrange atractive nuclear interaction one can include correlation effects in a suitable chosen density dependent pauli potential
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708.3501
The Meaning Of The Fine Structure Constant
A possible explanation is offered for the longstanding mystery surrounding the meaning of the fine structure constant. The reasoning is based on a discrete self-similar cosmological paradigm that has shown promise in explaining the general scaling properties of nature's global hierarchy. The discrete scale invariance of the paradigm implies that "strong gravity" governs gravitational interactions within atomic scale systems. Given the revised gravitational coupling constant and Planck mass, one can demonstrate that the fine structure constant is the ratio of the strengths of the unit electromagnetic interaction and the unit gravitational interaction within atomic scale systems. [Abridged]
physics.gen-ph
a possible explanation is offered for the longstanding mystery surrounding the meaning of the fine structure constant the reasoning is based on a discrete selfsimilar cosmological paradigm that has shown promise in explaining the general scaling properties of natures global hierarchy the discrete scale invariance of the paradigm implies that strong gravity governs gravitational interactions within atomic scale systems given the revised gravitational coupling constant and planck mass one can demonstrate that the fine structure constant is the ratio of the strengths of the unit electromagnetic interaction and the unit gravitational interaction within atomic scale systems abridged
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708.3502
Child mortality in Penna ageing model
Assuming the deleterious mutations in the Penna ageing model to affect mainly the young ages, we get an enhanced mortality at very young age, followed by a minimum of the mortality, and then the usual exponential increase of mortality with age.
q-bio.PE
assuming the deleterious mutations in the penna ageing model to affect mainly the young ages we get an enhanced mortality at very young age followed by a minimum of the mortality and then the usual exponential increase of mortality with age
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708.3503
On the theorem of M.Golomb
Let $X_{1},...,X_{n}$ be compact spaces and $X=X_{1}\times ... \times X_{n}.$ Consider the approximation of a function $f\in C(X)$ by sums $g_{1}(x_{1})+... g_{n}(x_{n}),$ where $g_{i}\in C(X_{i}),$ $i=1,...,n.$ In [8], M.Golomb obtained a formula for the error of this approximation in terms of measures constructed on special points of $X$, called "projection cycles". However, his proof had a gap, which was pointed out by Marshall and O'Farrell [15]. But the question if the formula was correct, remained open. The purpose of the paper is to prove that Golomb's formula holds in a stronger form.
math.FA
let x_1x_n be compact spaces and xx_1times times x_n consider the approximation of a function fin cx by sums g_1x_1 g_nx_n where g_iin cx_i i1n in 8 mgolomb obtained a formula for the error of this approximation in terms of measures constructed on special points of x called projection cycles however his proof had a gap which was pointed out by marshall and ofarrell 15 but the question if the formula was correct remained open the purpose of the paper is to prove that golombs formula holds in a stronger form
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708.3504
Anisotropic conductivity of disordered 2DEGs due to spin-orbit interactions
We show that the conductivity tensor of a disordered two-dimensional electron gas becomes anisotropic in the presence of both Rashba and Dresselhaus spin-orbit interactions (SOI). This anisotropy is a mesoscopic effect and vanishes with vanishing charge dephasing time. Using a diagrammatic approach including zero, one, and two-loop diagrams, we show that a consistent calculation needs to go beyond a Boltzmann equation approach. In the absence of charge dephasing and for zero frequency, a finite anisotropy \sigma_{xy} e^2/lhpf arises even for infinitesimal SOI.
cond-mat.mes-hall
we show that the conductivity tensor of a disordered twodimensional electron gas becomes anisotropic in the presence of both rashba and dresselhaus spinorbit interactions soi this anisotropy is a mesoscopic effect and vanishes with vanishing charge dephasing time using a diagrammatic approach including zero one and twoloop diagrams we show that a consistent calculation needs to go beyond a boltzmann equation approach in the absence of charge dephasing and for zero frequency a finite anisotropy sigma_xy e2lhpf arises even for infinitesimal soi
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708.3505
Gaze as a Supplementary Modality for Interacting with Ambient Intelligence Environments
We present our current research on the implementation of gaze as an efficient and usable pointing modality supplementary to speech, for interacting with augmented objects in our daily environment or large displays, especially immersive virtual reality environments, such as reality centres and caves. We are also addressing issues relating to the use of gaze as the main interaction input modality. We have designed and developed two operational user interfaces: one for providing motor-disabled users with easy gaze-based access to map applications and graphical software; the other for iteratively testing and improving the usability of gaze-contingent displays.
cs.HC
we present our current research on the implementation of gaze as an efficient and usable pointing modality supplementary to speech for interacting with augmented objects in our daily environment or large displays especially immersive virtual reality environments such as reality centres and caves we are also addressing issues relating to the use of gaze as the main interaction input modality we have designed and developed two operational user interfaces one for providing motordisabled users with easy gazebased access to map applications and graphical software the other for iteratively testing and improving the usability of gazecontingent displays
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708.3506
Stability Analysis of Continuous Waves in Nonlocal Random Nonlinear Media
On the basis of the competing cubic-quintic nonlinearity model, stability (instability) of continuous waves in nonlocal random non-Kerr nonlinear media is studied analytically and numerically. Fluctuating media parameters are modeled by the Gaussian white noise. It is shown that for different response functions of a medium nonlocality suppresses, as a rule, both the growth rate peak and bandwidth of instability caused by random parameters. At the same time, for a special form of the response functions there can be an ''anomalous'' subjection of nonlocality to the instability development which leads to further increase of the growth rate. Along with the second-order moments of the modulational amplitude, higher-order moments are taken into account.
nlin.PS nlin.CD
on the basis of the competing cubicquintic nonlinearity model stability instability of continuous waves in nonlocal random nonkerr nonlinear media is studied analytically and numerically fluctuating media parameters are modeled by the gaussian white noise it is shown that for different response functions of a medium nonlocality suppresses as a rule both the growth rate peak and bandwidth of instability caused by random parameters at the same time for a special form of the response functions there can be an anomalous subjection of nonlocality to the instability development which leads to further increase of the growth rate along with the secondorder moments of the modulational amplitude higherorder moments are taken into account
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708.3507
Relativistic Tunneling Through Two Successive Barriers
We study the relativistic quantum mechanical problem of a Dirac particle tunneling through two successive electrostatic barriers. Our aim is to study the emergence of the so-called \emph{Generalized Hartman Effect}, an effect observed in the context of nonrelativistic tunneling as well as in its electromagnetic counterparts, and which is often associated with the possibility of superluminal velocities in the tunneling process. We discuss the behavior of both the phase (or group) tunneling time and the dwell time, and show that in the limit of opaque barriers the relativistic theory also allows the emergence of the Generalized Hartman Effect. We compare our results with the nonrelativistic ones and discuss their interpretation.
quant-ph
we study the relativistic quantum mechanical problem of a dirac particle tunneling through two successive electrostatic barriers our aim is to study the emergence of the socalled emphgeneralized hartman effect an effect observed in the context of nonrelativistic tunneling as well as in its electromagnetic counterparts and which is often associated with the possibility of superluminal velocities in the tunneling process we discuss the behavior of both the phase or group tunneling time and the dwell time and show that in the limit of opaque barriers the relativistic theory also allows the emergence of the generalized hartman effect we compare our results with the nonrelativistic ones and discuss their interpretation
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708.3508
The young stellar population of NGC 4214 as observed with HST. I. Data and methods
We present the data and methods that we have used to perform a detailed UV-optical study of the nearby dwarf starburst galaxy NGC 4214 using multifilter HST/WFPC2+STIS photometry. We explain the process followed to obtain high-quality photometry and astrometry of the stellar and cluster populations of this galaxy. We describe the procedure used to transform magnitudes and colors into physical parameters using spectral energy distributions. The data show the existence of both young and old stellar populations that can be resolved at the distance of NGC 4214 (2.94 Mpc) and we perform a general description of those populations.
astro-ph
we present the data and methods that we have used to perform a detailed uvoptical study of the nearby dwarf starburst galaxy ngc 4214 using multifilter hstwfpc2stis photometry we explain the process followed to obtain highquality photometry and astrometry of the stellar and cluster populations of this galaxy we describe the procedure used to transform magnitudes and colors into physical parameters using spectral energy distributions the data show the existence of both young and old stellar populations that can be resolved at the distance of ngc 4214 294 mpc and we perform a general description of those populations
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708.3509
Modeling polymerization of microtubules: a quantum mechanical approach
In this paper a quantum mechanical description of the assembly/disassembly process for microtubules is proposed. We introduce creation and annihilation operators that raise or lower the microtubule length by a tubulin layer. Following that, the Hamiltonian and corresponding equations of motion for the quantum fields are derived that describe the dynamics of microtubules. These Heisenberg-type equations are then transformed to semi-classical equations using the method of coherent structures. We find that the dynamics of a microtubule can be mathematically expressed via a cubic-quintic nonlinear Schr\"{o}dinger (NLS) equation. We show that a vortex filament, a generic solution of the NLS equation, exhibits linear growth/shrinkage in time as well as temporal fluctuations about some mean value which is qualitatively similar to the dynamic instability of microtubules.
q-bio.BM cond-mat.stat-mech q-bio.QM
in this paper a quantum mechanical description of the assemblydisassembly process for microtubules is proposed we introduce creation and annihilation operators that raise or lower the microtubule length by a tubulin layer following that the hamiltonian and corresponding equations of motion for the quantum fields are derived that describe the dynamics of microtubules these heisenbergtype equations are then transformed to semiclassical equations using the method of coherent structures we find that the dynamics of a microtubule can be mathematically expressed via a cubicquintic nonlinear schrodinger nls equation we show that a vortex filament a generic solution of the nls equation exhibits linear growthshrinkage in time as well as temporal fluctuations about some mean value which is qualitatively similar to the dynamic instability of microtubules
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708.351
The young stellar population of NGC 4214 as observed with HST. II. Results
We present the results of a detailed UV-optical study of the nearby dwarf starburst galaxy NGC 4214 using multifilter HST/WFPC2+STIS photometry. The stellar extinction is found to be quite patchy, with some areas having values of E(4405-5495)< 0.1 mag and others, associated with star forming regions, much more heavily obscured, a result which is consistent with previous studies of the nebular extinction. We determined the ratio of blue-to-red supergiants and found it to be consistent with theoretical models for the metallicity of the SMC. The stellar IMF of the field in the range 20-100 solar masses is found to be steeper than Salpeter. A number of massive clusters and associations with ages between a few and 200 million years are detected and their properties are discussed.
astro-ph
we present the results of a detailed uvoptical study of the nearby dwarf starburst galaxy ngc 4214 using multifilter hstwfpc2stis photometry the stellar extinction is found to be quite patchy with some areas having values of e44055495 01 mag and others associated with star forming regions much more heavily obscured a result which is consistent with previous studies of the nebular extinction we determined the ratio of bluetored supergiants and found it to be consistent with theoretical models for the metallicity of the smc the stellar imf of the field in the range 20100 solar masses is found to be steeper than salpeter a number of massive clusters and associations with ages between a few and 200 million years are detected and their properties are discussed
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708.3511
Formulation of a constrained system in terms of extended Lagrangian and its local symmetries
It is shown that an arbitrary singular Lagrangian theory (with first and second class constraints up to $N$-th stage in the Hamiltonian formulation) can be reformulated as a theory with at most third-stage constraints. The corresponding Lagrangian $\tilde L$ can be obtained by pure algebraic methods, its manifest form in terms of quantities of the initial formulation is found. Local symmetries of $\tilde L$ are obtained in closed form. All the first class constraints of the initial Lagrangian turn out to be gauge symmetry generators for $\tilde L$.
hep-th math-ph math.MP
it is shown that an arbitrary singular lagrangian theory with first and second class constraints up to nth stage in the hamiltonian formulation can be reformulated as a theory with at most thirdstage constraints the corresponding lagrangian tilde l can be obtained by pure algebraic methods its manifest form in terms of quantities of the initial formulation is found local symmetries of tilde l are obtained in closed form all the first class constraints of the initial lagrangian turn out to be gauge symmetry generators for tilde l
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708.3512
An estimate for the location of QCD critical end point
It is proposed that a study of the ratio of shear viscosity to entropy density $\frac{\eta}{s}$ as a function of the baryon chemical potential $\mu_B$, and temperature T, provides a dynamic probe for the critical end point (CEP) in hot and dense QCD matter. An initial estimate from an elliptic flow excitation function gives $\mu^{\text{cep}}_B \sim 150-180$ MeV and $T_{\text{cep}} \sim 165 - 170$ MeV for the location of the the CEP. These values place the CEP in the range for "immediate" validation at RHIC.
nucl-ex
it is proposed that a study of the ratio of shear viscosity to entropy density fracetas as a function of the baryon chemical potential mu_b and temperature t provides a dynamic probe for the critical end point cep in hot and dense qcd matter an initial estimate from an elliptic flow excitation function gives mutextcep_b sim 150180 mev and t_textcep sim 165 170 mev for the location of the the cep these values place the cep in the range for immediate validation at rhic
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708.3513
Computational complexity of quantum optimal control landscapes
We study the Hamiltonian-independent contribution to the complexity of quantum optimal control problems. The optimization of controls that steer quantum systems to desired objectives can itself be considered a classical dynamical system that executes an analog computation. The system-independent component of the equations of motion of this dynamical system can be integrated analytically for various classes of discrete quantum control problems. For the maximization of observable expectation values from an initial pure state and the maximization of the fidelity of quantum gates, the time complexity of the corresponding computation belongs to the class continuous log (CLOG), the lowest analog complexity class, equivalent to the discrete complexity class NC. The simple scaling of the Hamiltonian-independent contribution to these problems with quantum system dimension indicates that with appropriately designed search algorithms, quantum optimal control can be rendered efficient even for large systems.
quant-ph
we study the hamiltonianindependent contribution to the complexity of quantum optimal control problems the optimization of controls that steer quantum systems to desired objectives can itself be considered a classical dynamical system that executes an analog computation the systemindependent component of the equations of motion of this dynamical system can be integrated analytically for various classes of discrete quantum control problems for the maximization of observable expectation values from an initial pure state and the maximization of the fidelity of quantum gates the time complexity of the corresponding computation belongs to the class continuous log clog the lowest analog complexity class equivalent to the discrete complexity class nc the simple scaling of the hamiltonianindependent contribution to these problems with quantum system dimension indicates that with appropriately designed search algorithms quantum optimal control can be rendered efficient even for large systems
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708.3514
Characteristic 2 approach to bivariate interpolation problems
We investigate bivariate interpolation problems in characteristic 2. Given a nonnegative integer $t$, we describe all the sub-linear systems generated by monomials, in which there is no curve passing through a general point with multiplicity at least $2^t$. As an application, we show that a certain linear system of plane curves with 10 base points is non-special.
math.AG math.NA
we investigate bivariate interpolation problems in characteristic 2 given a nonnegative integer t we describe all the sublinear systems generated by monomials in which there is no curve passing through a general point with multiplicity at least 2t as an application we show that a certain linear system of plane curves with 10 base points is nonspecial
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708.3515
Intransitive geometries and fused amalgams
We study geometries that arise from the natural $G_2(K)$ action on the geometry of one-dimensional subspaces, of nonsingular two-dimensional subspaces, and of nonsingular three-dimensional subspaces of the building geometry of type $C_3(K)$ where $K$ is a perfect field of characteristic 2. One of these geometries is intransitive in such a way that the non-standard geometric covering theory by the first and the last author is not applicable. In this paper we introduce the concept of fused amalgams in order to extend the geometric covering theory so that it applies to that geometry. This yields an interesting new amalgamation result for the group $G_2(K)$.
math.GR math.CO
we study geometries that arise from the natural g_2k action on the geometry of onedimensional subspaces of nonsingular twodimensional subspaces and of nonsingular threedimensional subspaces of the building geometry of type c_3k where k is a perfect field of characteristic 2 one of these geometries is intransitive in such a way that the nonstandard geometric covering theory by the first and the last author is not applicable in this paper we introduce the concept of fused amalgams in order to extend the geometric covering theory so that it applies to that geometry this yields an interesting new amalgamation result for the group g_2k
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708.3516
Annihilation Rate of Heavy 0^{++} P-wave Quarkonium in Relativistic Salpeter Method
Two-photon and two-gluon annihilation rates of P-wave scalar charmonium and bottomonium up to third radial excited states are estimated in the relativistic Salpeter method. We solved the full Salpeter equation with a well defined relativistic wave function and calculated the transition amplitude using the Mandelstam formalism. Our model dependent estimates for the decay widths: $\Gamma(\chi_{c0} \to 2\gamma)=3.78$ keV, $\Gamma(\chi'_{c0} \to 2\gamma)=3.51$ keV, $\Gamma(\chi_{b0} \to 2\gamma)=48.8$ eV and $\Gamma(\chi'_{b0} \to 2\gamma)=50.3$ eV. We also give estimates of total widths by the two-gluon decay rates: $\Gamma_{tot}(\chi_{c0})=10.3$ MeV, $\Gamma_{tot}(\chi'_{c0})=9.61$ MeV, $\Gamma_{tot}(\chi_{b0})=0.887$ MeV and $\Gamma_{tot}(\chi'_{b0})=0.914$ MeV.
hep-ph
twophoton and twogluon annihilation rates of pwave scalar charmonium and bottomonium up to third radial excited states are estimated in the relativistic salpeter method we solved the full salpeter equation with a well defined relativistic wave function and calculated the transition amplitude using the mandelstam formalism our model dependent estimates for the decay widths gammachi_c0 to 2gamma378 kev gammachi_c0 to 2gamma351 kev gammachi_b0 to 2gamma488 ev and gammachi_b0 to 2gamma503 ev we also give estimates of total widths by the twogluon decay rates gamma_totchi_c0103 mev gamma_totchi_c0961 mev gamma_totchi_b00887 mev and gamma_totchi_b00914 mev
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708.3517
Sparse inverse covariance estimation with the lasso
We consider the problem of estimating sparse graphs by a lasso penalty applied to the inverse covariance matrix. Using a coordinate descent procedure for the lasso, we develop a simple algorithm that is remarkably fast: in the worst cases, it solves a 1000 node problem (~500,000 parameters) in about a minute, and is 50 to 2000 times faster than competing methods. It also provides a conceptual link between the exact problem and the approximation suggested by Meinhausen and Buhlmann (2006). We illustrate the method on some cell-signaling data from proteomics.
stat.ME
we consider the problem of estimating sparse graphs by a lasso penalty applied to the inverse covariance matrix using a coordinate descent procedure for the lasso we develop a simple algorithm that is remarkably fast in the worst cases it solves a 1000 node problem 500000 parameters in about a minute and is 50 to 2000 times faster than competing methods it also provides a conceptual link between the exact problem and the approximation suggested by meinhausen and buhlmann 2006 we illustrate the method on some cellsignaling data from proteomics
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708.3518
A Look at the Abandoned Contributions to Cosmology of Dirac, Sciama and Dicke
The separate contributions to cosmology of the above researchers are revisited and a cosmology encompassing their basic ideas is proposed. We study Dirac's article on the large number hypothesis (1938), Sciama's proposal of realizing Mach's principle (1953), and Dicke's considerations (1957) on a flat-space representation of general relativity with a variable speed of light (VSL). Dicke's tentative theory can be formulated in a way which is compatible with Sciama's hypothesis on the gravitational constant G. Additionally, such a cosmological model is shown to satisfy Dirac's second `large number' hypothesis on the total number of particles in the universe being proportional to the square of the epoch. In the same context, Dirac's first hypothesis on an epoch-dependent G-contrary to his prediction- does not necessarily produce a visible time dependence of G. While Dicke's proposalreproduces the classical tests of GR in first approximation, the cosmological redshift is described by a shortening of measuring rods rather than an expansion of space. Since the temporal evolution of the horizon R is governed by \dot R(t) =c(t), the flatness and horizon problems do not arise in the common form.
physics.gen-ph gr-qc
the separate contributions to cosmology of the above researchers are revisited and a cosmology encompassing their basic ideas is proposed we study diracs article on the large number hypothesis 1938 sciamas proposal of realizing machs principle 1953 and dickes considerations 1957 on a flatspace representation of general relativity with a variable speed of light vsl dickes tentative theory can be formulated in a way which is compatible with sciamas hypothesis on the gravitational constant g additionally such a cosmological model is shown to satisfy diracs second large number hypothesis on the total number of particles in the universe being proportional to the square of the epoch in the same context diracs first hypothesis on an epochdependent gcontrary to his prediction does not necessarily produce a visible time dependence of g while dickes proposalreproduces the classical tests of gr in first approximation the cosmological redshift is described by a shortening of measuring rods rather than an expansion of space since the temporal evolution of the horizon r is governed by dot rt ct the flatness and horizon problems do not arise in the common form
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708.3519
Photons inside a waveguide as massive particles
In the paper, we show that there exists a close analogy between the behavior of de Broglie matter waves and that of electromagnetic waves inside a hollow waveguide, such that the guided photons can be treated as free massive particles subject to a relativistic quantum-mechanical equation. Inspired by the effective rest mass of guided photons and the zitterbewegung phenomenon of the Dirac electron, at variance with the well-known Higgs mechanism we present some different heuristic ideas on the origin of mass.
quant-ph
in the paper we show that there exists a close analogy between the behavior of de broglie matter waves and that of electromagnetic waves inside a hollow waveguide such that the guided photons can be treated as free massive particles subject to a relativistic quantummechanical equation inspired by the effective rest mass of guided photons and the zitterbewegung phenomenon of the dirac electron at variance with the wellknown higgs mechanism we present some different heuristic ideas on the origin of mass
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708.352
Prisoner's Dilemma in One-Dimensional Cellular Automata: Visualization of Evolutionary Patterns
The spatial Prisoner's Dilemma is a prototype model to show the emergence of cooperation in very competitive environments. It considers players, at site of lattices, that can either cooperate or defect when playing the Prisoner's Dilemma with other z players. This model presents a rich phase diagram. Here we consider players in cells of one-dimensional cellular automata. Each player interacts with other z players. This geometry allows us to vary, in a simple manner, the number of neighbors ranging from one up to the lattice size, including self-interaction. This approach has multiple advantages. It is simple to implement numerically and we are able to retrieve all the previous results found in the previously considered lattices, with a faster convergence to stationary values. More remarkable, it permits us to keep track of the spatio-temporal evolution of each player of the automaton. Giving rise to interesting patterns. These patterns allow the interpretation of cooperation/defection clusters as particles, which can be absorbed and collided among themselves. The presented approach represents a new paradigm to study the emergence and maintenance of cooperation in the spatial Prisoner's Dilemma.
physics.comp-ph physics.soc-ph
the spatial prisoners dilemma is a prototype model to show the emergence of cooperation in very competitive environments it considers players at site of lattices that can either cooperate or defect when playing the prisoners dilemma with other z players this model presents a rich phase diagram here we consider players in cells of onedimensional cellular automata each player interacts with other z players this geometry allows us to vary in a simple manner the number of neighbors ranging from one up to the lattice size including selfinteraction this approach has multiple advantages it is simple to implement numerically and we are able to retrieve all the previous results found in the previously considered lattices with a faster convergence to stationary values more remarkable it permits us to keep track of the spatiotemporal evolution of each player of the automaton giving rise to interesting patterns these patterns allow the interpretation of cooperationdefection clusters as particles which can be absorbed and collided among themselves the presented approach represents a new paradigm to study the emergence and maintenance of cooperation in the spatial prisoners dilemma
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708.3521
A novel operation associated with Gauss' arithmetic-geometric means
The arithmetic mean is the mean for addition and the geometric mean is that for multiplication. Then what kind of binary operation is associated with the arithmetic-geometric mean (AGM) due to C. F. Gauss? If it is possible to construct an arithmetic operation such that AGM is the mean for this operation, it can be regarded as an intermediate operation between addition and multiplication in view of the meaning of AGM. In this paper such an operation is introduced and several of its algebraic properties are proved.
math.NT math.GM
the arithmetic mean is the mean for addition and the geometric mean is that for multiplication then what kind of binary operation is associated with the arithmeticgeometric mean agm due to c f gauss if it is possible to construct an arithmetic operation such that agm is the mean for this operation it can be regarded as an intermediate operation between addition and multiplication in view of the meaning of agm in this paper such an operation is introduced and several of its algebraic properties are proved
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708.3522
Bounding the Betti numbers and computing the Euler-Poincar\'e characteristic of semi-algebraic sets defined by partly quadratic systems of polynomials
Let $\R$ be a real closed field, $ {\mathcal Q} \subset \R[Y_1,...,Y_\ell,X_1,...,X_k], $ with $ \deg_{Y}(Q) \leq 2, \deg_{X}(Q) \leq d, Q \in {\mathcal Q}, #({\mathcal Q})=m,$ and $ {\mathcal P} \subset \R[X_1,...,X_k] $ with $\deg_{X}(P) \leq d, P \in {\mathcal P}, #({\mathcal P})=s$, and $S \subset \R^{\ell+k}$ a semi-algebraic set defined by a Boolean formula without negations, with atoms $P=0, P \geq 0, P \leq 0, P \in {\mathcal P} \cup {\mathcal Q}$. We prove that the sum of the Betti numbers of $S$ is bounded by \[ \ell^2 (O(s+\ell+m)\ell d)^{k+2m}. \] This is a common generalization of previous results on bounding the Betti numbers of closed semi-algebraic sets defined by polynomials of degree $d$ and 2, respectively. We also describe an algorithm for computing the Euler-Poincar\'e characteristic of such sets, generalizing similar algorithms known before. The complexity of the algorithm is bounded by $(\ell s m d)^{O(m(m+k))}$.
math.AG cs.SC math.AT math.GT
let r be a real closed field mathcal q subset ry_1y_ellx_1x_k with deg_yq leq 2 deg_xq leq d q in mathcal q mathcal qm and mathcal p subset rx_1x_k with deg_xp leq d p in mathcal p mathcal ps and s subset rellk a semialgebraic set defined by a boolean formula without negations with atoms p0 p geq 0 p leq 0 p in mathcal p cup mathcal q we prove that the sum of the betti numbers of s is bounded by ell2 osellmell dk2m this is a common generalization of previous results on bounding the betti numbers of closed semialgebraic sets defined by polynomials of degree d and 2 respectively we also describe an algorithm for computing the eulerpoincare characteristic of such sets generalizing similar algorithms known before the complexity of the algorithm is bounded by ell s m dommk
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708.3523
Polarized neutron scattering study on antiferromagnetic states in CeRh0.6Co0.4In5
Polarized neutron scattering experiments were performed on mixed compound CeRh0.6Co0.4In5 to clarify the nature of the low-temperature ordered states. Three nonequivalent Bragg peaks, characterized by the wave vectors of q_h ~ (1/2,1/2,0.3), q_1 ~ (1/2,1/2,0.4) and q_c=(1/2,1/2,1/2), were observed at 1.4 K. These Bragg peaks are found to occur entirely in spin-flip channel. This indicates that these Bragg peaks originate from the magnetic scattering, i.e., the antiferromagnetic orders with three different modulations appear in this compound.
cond-mat.str-el
polarized neutron scattering experiments were performed on mixed compound cerh06co04in5 to clarify the nature of the lowtemperature ordered states three nonequivalent bragg peaks characterized by the wave vectors of q_h 121203 q_1 121204 and q_c121212 were observed at 14 k these bragg peaks are found to occur entirely in spinflip channel this indicates that these bragg peaks originate from the magnetic scattering ie the antiferromagnetic orders with three different modulations appear in this compound
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708.3524
The nanoscale phase separation in hole-doped manganites
A macroscopic phase separation, in which ferromagnetic clusters are observed in an insulating matrix, is sometimes observed, and believed to be essential to the colossal magnetoresistive (CMR) properties of manganese oxides. The application of a magnetic field may indeed trigger large magnetoresistance effects due to the percolation between clusters allowing the movement of the charge carriers. However, this macroscopic phase separation is mainly related to extrinsic defects or impurities, which hinder the long-ranged charge-orbital order of the system. We show in the present article that rather than the macroscopic phase separation, an homogeneous short-ranged charge-orbital order accompanied by a spin glass state occurs, as an intrinsic result of the uniformity of the random potential perturbation induced by the solid solution of the cations on the $A$-sites of the structure of these materials. Hence the phase separation does occur, but in a more subtle and interesting nanoscopic form, here referred as ``homogeneous''. Remarkably, this ``nanoscale phase separation'' alone is able to bring forth the colossal magnetoresistance in the perovskite manganites, and is potentially relevant to a wide variety of other magnetic and/or electrical properties of manganites, as well as many other transition metal oxides, in bulk or thin film form as we exemplify throughout the article.
cond-mat.mtrl-sci cond-mat.str-el
a macroscopic phase separation in which ferromagnetic clusters are observed in an insulating matrix is sometimes observed and believed to be essential to the colossal magnetoresistive cmr properties of manganese oxides the application of a magnetic field may indeed trigger large magnetoresistance effects due to the percolation between clusters allowing the movement of the charge carriers however this macroscopic phase separation is mainly related to extrinsic defects or impurities which hinder the longranged chargeorbital order of the system we show in the present article that rather than the macroscopic phase separation an homogeneous shortranged chargeorbital order accompanied by a spin glass state occurs as an intrinsic result of the uniformity of the random potential perturbation induced by the solid solution of the cations on the asites of the structure of these materials hence the phase separation does occur but in a more subtle and interesting nanoscopic form here referred as homogeneous remarkably this nanoscale phase separation alone is able to bring forth the colossal magnetoresistance in the perovskite manganites and is potentially relevant to a wide variety of other magnetic andor electrical properties of manganites as well as many other transition metal oxides in bulk or thin film form as we exemplify throughout the article
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708.3525
Gauge invariance and time symmetry breaking
Employing an arbitrary velocity gauge transformation this contribution argues that the breaking of time symmetry is a natural consequence of irreversibility.
physics.gen-ph
employing an arbitrary velocity gauge transformation this contribution argues that the breaking of time symmetry is a natural consequence of irreversibility
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708.3526
1/N_c corrections to the magnetic susceptibility of the QCD vacuum
We investigate the magnetic susceptibility of the QCD vacuum with the $1/N_c$ corrections taken into account, based on the instanton vacuum. Starting from the instanton liquid model we derive the gauged light-quark partition function in the presence of the current quark mass as well as of external Abelian vector and tensor fields. We consider the $1/N_c$ meson-loop corrections which are shown to contribute to the magnetic susceptibility by around 15% for the up (and down) quarks. We also take into account the tensor terms of the quark-quark interaction from the instanton vacuum as well as the finite-width effects, both of which are of order $\mathcal{O}(1/N_c)$. The effects of the tensor terms and finite width turn out to be negligibly small. The final results for the up-quarks are given as: $\chi< i\psi^\dagger \psi>_0 \simeq 35-40 \mathrm{MeV}$ with the quark condensate $<i\psi^\dagger \psi>_0$. We also discuss the pion mass dependence of the magnetic susceptibility in order to give a qualitative guideline for the chiral extrapolation of lattice data.
hep-ph
we investigate the magnetic susceptibility of the qcd vacuum with the 1n_c corrections taken into account based on the instanton vacuum starting from the instanton liquid model we derive the gauged lightquark partition function in the presence of the current quark mass as well as of external abelian vector and tensor fields we consider the 1n_c mesonloop corrections which are shown to contribute to the magnetic susceptibility by around 15 for the up and down quarks we also take into account the tensor terms of the quarkquark interaction from the instanton vacuum as well as the finitewidth effects both of which are of order mathcalo1n_c the effects of the tensor terms and finite width turn out to be negligibly small the final results for the upquarks are given as chi ipsidagger psi_0 simeq 3540 mathrmmev with the quark condensate ipsidagger psi_0 we also discuss the pion mass dependence of the magnetic susceptibility in order to give a qualitative guideline for the chiral extrapolation of lattice data
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708.3527
Science-Based Comparative Culture: A New Theme of Experiment for Freshmen in Tohoku University
In 2004, Tohoku University created a new introductory science experimental course for freshmen. The course is a compulsory subject for students in all natural science fields. The course is not designed for a professional education, but as a liberal education, in which students are trained to become familiar with nature and to discover natural laws for themselves. We present here one of 12 themes - "science and culture: vibration of string instrument and music", in which we expect students to study two aspects: 1) the universality of natural laws and 2) the variety of value judgments from the evidence.
physics.ed-ph physics.pop-ph physics.soc-ph
in 2004 tohoku university created a new introductory science experimental course for freshmen the course is a compulsory subject for students in all natural science fields the course is not designed for a professional education but as a liberal education in which students are trained to become familiar with nature and to discover natural laws for themselves we present here one of 12 themes science and culture vibration of string instrument and music in which we expect students to study two aspects 1 the universality of natural laws and 2 the variety of value judgments from the evidence
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708.3528
Determination of Penetration Depth of Transverse Spin Current in Ferromagnetic Metals by Spin Pumping
Spin pumping in nonmagnetic/ferromagnetic metal multilayers is studied both theoretically and experimentally. We show that the line widths of the ferromagnetic resonance (FMR) spectrum depend on the thickness of the ferromagnetic metal layers, which must not be in resonance with the oscillating magnetic field. We also show that the penetration depths of the transverse spin current in ferromagnetic metals can be determined by analyzing the line widths of their FMR spectra. The obtained penetration depths in NiFe, CoFe and CoFeB were 3.7 [nm], 2.5 [nm] and 12.0 [nm], respectively.
cond-mat.mes-hall cond-mat.other
spin pumping in nonmagneticferromagnetic metal multilayers is studied both theoretically and experimentally we show that the line widths of the ferromagnetic resonance fmr spectrum depend on the thickness of the ferromagnetic metal layers which must not be in resonance with the oscillating magnetic field we also show that the penetration depths of the transverse spin current in ferromagnetic metals can be determined by analyzing the line widths of their fmr spectra the obtained penetration depths in nife cofe and cofeb were 37 nm 25 nm and 120 nm respectively
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708.3529
Tuning Co valence state in cobalt oxyhydrate superconductor by post reduction
We report a successful tuning of Co valence state in cobalt oxyhydrate superconductor via a facile post reduction using NaOH as reducing agent. The change in Co valence was precisely determined by measuring the volume of the released oxygen. The possible hydronium-incorporation was greatly suppressed in concentrated NaOH solution, making the absolute Co valence determinable. As a result, an updated superconducting phase diagram was obtained, which shows that the superconducting transition temperature increases monotonically with increasing Co valence in a narrow range from +3.58 to +3.65.
cond-mat.supr-con cond-mat.str-el
we report a successful tuning of co valence state in cobalt oxyhydrate superconductor via a facile post reduction using naoh as reducing agent the change in co valence was precisely determined by measuring the volume of the released oxygen the possible hydroniumincorporation was greatly suppressed in concentrated naoh solution making the absolute co valence determinable as a result an updated superconducting phase diagram was obtained which shows that the superconducting transition temperature increases monotonically with increasing co valence in a narrow range from 358 to 365
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708.353
Gravity localization on thick branes: a numerical approach
We introduce a numerical procedure to investigate the spectrum of massive modes and its contribution for gravity localization on thick branes. After considering a model with an analytically known Schroedinger potential, we present the method and discuss its applicability. With this procedure we can study several models even when the Schroedinger potential is not known analytically. We discuss both the occurrence of localization of gravity and the correction to the Newtonian potential given by the massive modes.
hep-th
we introduce a numerical procedure to investigate the spectrum of massive modes and its contribution for gravity localization on thick branes after considering a model with an analytically known schroedinger potential we present the method and discuss its applicability with this procedure we can study several models even when the schroedinger potential is not known analytically we discuss both the occurrence of localization of gravity and the correction to the newtonian potential given by the massive modes
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708.3531
Networked Multiple Description Estimation and Compression with Resource Scalability
We present a joint source-channel multiple description (JSC-MD) framework for resource-constrained network communications (e.g., sensor networks), in which one or many deprived encoders communicate a Markov source against bit errors and erasure errors to many heterogeneous decoders, some powerful and some deprived. To keep the encoder complexity at minimum, the source is coded into K descriptions by a simple multiple description quantizer (MDQ) with neither entropy nor channel coding. The code diversity of MDQ and the path diversity of the network are exploited by decoders to correct transmission errors and improve coding efficiency. A key design objective is resource scalability: powerful nodes in the network can perform JSC-MD distributed estimation/decoding under the criteria of maximum a posteriori probability (MAP) or minimum mean-square error (MMSE), while primitive nodes resort to simpler MD decoding, all working with the same MDQ code. The application of JSC-MD to distributed estimation of hidden Markov models in a sensor network is demonstrated. The proposed JSC-MD MAP estimator is an algorithm of the longest path in a weighted directed acyclic graph, while the JSC-MD MMSE decoder is an extension of the well-known forward-backward algorithm to multiple descriptions. Both algorithms simultaneously exploit the source memory, the redundancy of the fixed-rate MDQ, and the inter-description correlations. They outperform the existing hard-decision MDQ decoders by large margins (up to 8dB). For Gaussian Markov sources, the complexity of JSC-MD distributed MAP sequence estimation can be made as low as that of typical single description Viterbi-type algorithms.
cs.IT math.IT
we present a joint sourcechannel multiple description jscmd framework for resourceconstrained network communications eg sensor networks in which one or many deprived encoders communicate a markov source against bit errors and erasure errors to many heterogeneous decoders some powerful and some deprived to keep the encoder complexity at minimum the source is coded into k descriptions by a simple multiple description quantizer mdq with neither entropy nor channel coding the code diversity of mdq and the path diversity of the network are exploited by decoders to correct transmission errors and improve coding efficiency a key design objective is resource scalability powerful nodes in the network can perform jscmd distributed estimationdecoding under the criteria of maximum a posteriori probability map or minimum meansquare error mmse while primitive nodes resort to simpler md decoding all working with the same mdq code the application of jscmd to distributed estimation of hidden markov models in a sensor network is demonstrated the proposed jscmd map estimator is an algorithm of the longest path in a weighted directed acyclic graph while the jscmd mmse decoder is an extension of the wellknown forwardbackward algorithm to multiple descriptions both algorithms simultaneously exploit the source memory the redundancy of the fixedrate mdq and the interdescription correlations they outperform the existing harddecision mdq decoders by large margins up to 8db for gaussian markov sources the complexity of jscmd distributed map sequence estimation can be made as low as that of typical single description viterbitype algorithms
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708.3532
Three-dimensional multi-mesh material point method for solving collision problems
Contact algorithm between different bodies plays an important role in solving collision problems. Usually it is not easy to be treated very well. Several ones for material point method were proposed by Bardenhangen, Brackbill, and Sulsky\cite{Bardenhagen2000,Bardenhagen2001}, Hu and Chen\cite{Hu_Chen2003}. An improved one for three-dimensional material point method is presented in this paper. The improved algorithm emphasizes the energy conservation of the system and faithfully recovers opposite acting forces between contacting bodies. Contrasted to the one by Bardenhagen, both the normal and tangential contacting forces are more appropriately applied to the contacting bodies via the contacting nodes of the background mesh; Contrasted to the one by Hu and Chen, not only the tangential velocities but also the normal ones are handled separately in respective individual mesh. This treatment ensures not only the contact/sliding/separation procedure but also the friction between contacting bodies are recovered. The presented contact algorithm is validated via numerical experiments including rolling simulation, impact of elastic spheres, impact of a Taylor bar and impact of plastic spheres. The numerical results show that the multi-mesh material point method with the improved contact algorithm is more suitable for solving collision problems.
physics.comp-ph cond-mat.mtrl-sci physics.class-ph
contact algorithm between different bodies plays an important role in solving collision problems usually it is not easy to be treated very well several ones for material point method were proposed by bardenhangen brackbill and sulskycitebardenhagen2000bardenhagen2001 hu and chencitehu_chen2003 an improved one for threedimensional material point method is presented in this paper the improved algorithm emphasizes the energy conservation of the system and faithfully recovers opposite acting forces between contacting bodies contrasted to the one by bardenhagen both the normal and tangential contacting forces are more appropriately applied to the contacting bodies via the contacting nodes of the background mesh contrasted to the one by hu and chen not only the tangential velocities but also the normal ones are handled separately in respective individual mesh this treatment ensures not only the contactslidingseparation procedure but also the friction between contacting bodies are recovered the presented contact algorithm is validated via numerical experiments including rolling simulation impact of elastic spheres impact of a taylor bar and impact of plastic spheres the numerical results show that the multimesh material point method with the improved contact algorithm is more suitable for solving collision problems
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708.3533
Stability and convergence of the Method of Fundamental Solutions for Helmholtz problems on analytic domains
The Method of Fundamental Solutions (MFS) is a popular tool to solve Laplace and Helmholtz boundary value problems. Its main drawback is that it often leads to ill-conditioned systems of equations. In this paper we investigate for the interior Helmholtz problem on analytic domains how the singularities (charge points) of the MFS basis functions have to be chosen such that approximate solutions can be represented by the MFS basis in a numerically stable way. For Helmholtz problems on the unit disc we give a full analysis which includes the high frequency (short wavelength) limit. For more difficult and nonconvex domains such as crescents we demonstrate how the right choice of charge points is connected to how far into the complex plane the solution of the boundary value problem can be analytically continued, which in turn depends on both domain shape and boundary data. Using this we develop a recipe for locating charge points which allows us to reach error norms of typically 10^{-11} on a wide variety of analytic domains. At high frequencies of order only 3 points per wavelength are needed, which compares very favorably to boundary integral methods.
math.NA
the method of fundamental solutions mfs is a popular tool to solve laplace and helmholtz boundary value problems its main drawback is that it often leads to illconditioned systems of equations in this paper we investigate for the interior helmholtz problem on analytic domains how the singularities charge points of the mfs basis functions have to be chosen such that approximate solutions can be represented by the mfs basis in a numerically stable way for helmholtz problems on the unit disc we give a full analysis which includes the high frequency short wavelength limit for more difficult and nonconvex domains such as crescents we demonstrate how the right choice of charge points is connected to how far into the complex plane the solution of the boundary value problem can be analytically continued which in turn depends on both domain shape and boundary data using this we develop a recipe for locating charge points which allows us to reach error norms of typically 1011 on a wide variety of analytic domains at high frequencies of order only 3 points per wavelength are needed which compares very favorably to boundary integral methods
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708.3534
Momentum-resolved charge excitations in high-Tc cuprates studied by resonant inelastic x-ray scattering
We report a Cu K-edge resonant inelastic x-ray scattering (RIXS) study of high-Tc cuprates. Momentum-resolved charge excitations in the CuO2 plane are examined from parent Mott insulators to carrier-doped superconductors. The Mott gap excitation in undoped insulators is found to commonly show a larger dispersion along the [pi,pi] direction than the [pi,0] direction. On the other hand, the resonance condition displays material dependence. Upon hole doping, the dispersion of the Mott gap excitation becomes weaker and an intraband excitation appears as a continuum intensity below the gap at the same time. In the case of electron doping, the Mott gap excitation is prominent at the zone center and a dispersive intraband excitation is observed at finite momentum transfer.
cond-mat.str-el cond-mat.supr-con
we report a cu kedge resonant inelastic xray scattering rixs study of hightc cuprates momentumresolved charge excitations in the cuo2 plane are examined from parent mott insulators to carrierdoped superconductors the mott gap excitation in undoped insulators is found to commonly show a larger dispersion along the pipi direction than the pi0 direction on the other hand the resonance condition displays material dependence upon hole doping the dispersion of the mott gap excitation becomes weaker and an intraband excitation appears as a continuum intensity below the gap at the same time in the case of electron doping the mott gap excitation is prominent at the zone center and a dispersive intraband excitation is observed at finite momentum transfer
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708.3535
Probability, unitarity, and realism in generally covariant quantum information
The formalism of covariant quantum theory, introduced by Reisenberger and Rovelli, casts the description of quantum states and evolution into a framework compatable with the principles of general relativity. The leap to this covariant formalism, however, outstripped the standard interpretation used to connect quantum theory to experimental predictions, leaving the predictions of the RR theory ambiguous. Here we discuss in detail some implications of our recently proposed description of covariant quantum information (CQI), which addresses these problems. We show explicit agreement with standard quantum mechanics in the appropriate limit. In addition to compatability with general covariance, we show that our framework has other attractive and satisfying features -- it is fully unitary, realist, and self-contained. The full unitarity of the formalism in the presence of measurements allows us to invoke time-reversal symmetry to obtain new predictions closely related to the quantum Zeno effect.
quant-ph gr-qc
the formalism of covariant quantum theory introduced by reisenberger and rovelli casts the description of quantum states and evolution into a framework compatable with the principles of general relativity the leap to this covariant formalism however outstripped the standard interpretation used to connect quantum theory to experimental predictions leaving the predictions of the rr theory ambiguous here we discuss in detail some implications of our recently proposed description of covariant quantum information cqi which addresses these problems we show explicit agreement with standard quantum mechanics in the appropriate limit in addition to compatability with general covariance we show that our framework has other attractive and satisfying features it is fully unitary realist and selfcontained the full unitarity of the formalism in the presence of measurements allows us to invoke timereversal symmetry to obtain new predictions closely related to the quantum zeno effect
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708.3536
Suzaku Observations of Hercules X-1 : Measurements of the Two Cyclotron Harmonics
The accretion-powered pulsar Her X-1 was observed with Suzaku twice in its main-on state, on 2005 October 5-6 and 2006 March 29-30, for a net exposure of 30.5 ks and 34.4 ks, respectively. In the 2005 and 2006 observations, the source was detected at an average 10-30 keV intensity of 290 mCrab and 230 mCrab, respectively. The intrinsic pulse period was measured on both occasions at 1.23776 s by HXD-PIN, after barycentric and binary corrections. The pulse phase-averaged spectra in the energy range above 10 keV are well fitted by ``Negative and Positive power-law times EXponential (NPEX)'' model, multiplied by a fundamental cyclotron resonance scattering feature at ~36 keV which appears very significantly in the HXD-PIN data. The resonance profiles were reproduced successfully by the Lorentzian type scattering cross section, rather than by a Gaussian type alternative. The pulse phase-averaged HXD-GSO data, covering 50-120 keV, are featureless. However, in a differential spectrum between the pulse-decay phase and off-pulse phase, the second harmonic cyclotron resonance was detected in the GSO data at ~73 keV, with a depth of 1.6_-0.7^+0.9. This makes Her X-1 a 6th pulsar with established second harmonic resonance. Implications of these results are briefly discussed.
astro-ph
the accretionpowered pulsar her x1 was observed with suzaku twice in its mainon state on 2005 october 56 and 2006 march 2930 for a net exposure of 305 ks and 344 ks respectively in the 2005 and 2006 observations the source was detected at an average 1030 kev intensity of 290 mcrab and 230 mcrab respectively the intrinsic pulse period was measured on both occasions at 123776 s by hxdpin after barycentric and binary corrections the pulse phaseaveraged spectra in the energy range above 10 kev are well fitted by negative and positive powerlaw times exponential npex model multiplied by a fundamental cyclotron resonance scattering feature at 36 kev which appears very significantly in the hxdpin data the resonance profiles were reproduced successfully by the lorentzian type scattering cross section rather than by a gaussian type alternative the pulse phaseaveraged hxdgso data covering 50120 kev are featureless however in a differential spectrum between the pulsedecay phase and offpulse phase the second harmonic cyclotron resonance was detected in the gso data at 73 kev with a depth of 16_0709 this makes her x1 a 6th pulsar with established second harmonic resonance implications of these results are briefly discussed
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708.3537
Studies on the Chazy equations
In this paper, we study the Chazy III,IX and X equations. For the Chazy III equation, by making the birational transformations the Chazy III equation is transformed into a third-order ordinary differential equation of rational type. For this equation, we find its meromorphic solutions, whose free parameters are essentially two. We also show that the system associated with this equation admits new special solutions solved by $tanh(t)$. For the Chazy IX equation, we transform the Chazy IX equation to a system of the first-order ordinary differential equations by birational transformations. For this system, we give two new birational B{\"a}cklund transformations. We also give the holomorphy condition of this system. Thanks to this holomorphy condition, we obtain a new partial differential system in two variables involving the Chazy IX equation, This system satisfies the compatibility condition, and admits a travelling wave solution. For the Chazy X equation, we transform the Chazy X equation to a system of the first-order ordinary differential equations by birational transformations. For this system, we give two birational B{\"a}cklund transformations. One of them is new. We also give the holomorphy condition of this system. Thanks to this holomorphy condition, we can recover this system.
math.AG math.CA math.DS
in this paper we study the chazy iiiix and x equations for the chazy iii equation by making the birational transformations the chazy iii equation is transformed into a thirdorder ordinary differential equation of rational type for this equation we find its meromorphic solutions whose free parameters are essentially two we also show that the system associated with this equation admits new special solutions solved by tanht for the chazy ix equation we transform the chazy ix equation to a system of the firstorder ordinary differential equations by birational transformations for this system we give two new birational backlund transformations we also give the holomorphy condition of this system thanks to this holomorphy condition we obtain a new partial differential system in two variables involving the chazy ix equation this system satisfies the compatibility condition and admits a travelling wave solution for the chazy x equation we transform the chazy x equation to a system of the firstorder ordinary differential equations by birational transformations for this system we give two birational backlund transformations one of them is new we also give the holomorphy condition of this system thanks to this holomorphy condition we can recover this system
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708.3538
Quark Confinement and the Fractional Quantum Hall Effect
Working in the physics of Wilson factor and Aharonov-Bohm effect, we find in the fluxtube-quark system the topology of a baryon consisting three heavy flavor quarks resembles that of the fractional quantum Hall effect (FQHE) in condensed matter. This similarity yields the result that the constituent quarks of baryon have the "filling factor" 1/3, thus the previous conjecture that quark confinement is a correlation effect was confirmed. Moreover, by deriving a Hamiltonian of the system analogous to that of FQHE, we predict an energy gap for the ground state of a heavy three-quark system.
hep-ph
working in the physics of wilson factor and aharonovbohm effect we find in the fluxtubequark system the topology of a baryon consisting three heavy flavor quarks resembles that of the fractional quantum hall effect fqhe in condensed matter this similarity yields the result that the constituent quarks of baryon have the filling factor 13 thus the previous conjecture that quark confinement is a correlation effect was confirmed moreover by deriving a hamiltonian of the system analogous to that of fqhe we predict an energy gap for the ground state of a heavy threequark system
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708.3539
An EL-labeling of the subgroup lattice
In a 2001 paper, Shareshian conjectured that the subgroup lattice of a finite, solvable group has an EL-labeling. We construct such a labeling, and verify that our labeling has the expected properties.
math.CO math.GR
in a 2001 paper shareshian conjectured that the subgroup lattice of a finite solvable group has an ellabeling we construct such a labeling and verify that our labeling has the expected properties
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708.354
On the endomorphism algebra of modular Gelfand-Graev representations
We study the endomorphism algebras of a modular Gelfand-Graev representation of a finite reductive group by investigating modular properties of homomorphisms constructed by Curtis and Curtis-Shoji.
math.RT
we study the endomorphism algebras of a modular gelfandgraev representation of a finite reductive group by investigating modular properties of homomorphisms constructed by curtis and curtisshoji
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708.3541
Degenerations of quadratic differentials on CP1
We describe the connected components of the complement of a natural "diagonal" of real codimension 1 in a stratum of quadratic differentials on CP1. We establish a natural bijection between the set of these connected components and the set of generic configurations that appear on such "flat spheres". We also prove that the stratum has only one topological end. Finally, we elaborate a necessary toolkit destined to evaluation of the Siegel-Veech constants.
math.GT
we describe the connected components of the complement of a natural diagonal of real codimension 1 in a stratum of quadratic differentials on cp1 we establish a natural bijection between the set of these connected components and the set of generic configurations that appear on such flat spheres we also prove that the stratum has only one topological end finally we elaborate a necessary toolkit destined to evaluation of the siegelveech constants
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708.3542
Congestion, equilibrium and learning: The minority game
The minority game is a simple congestion game in which the players' main goal is to choose among two options the one that is adopted by the smallest number of players. We characterize the set of Nash equilibria and the limiting behavior of several well-known learning processes in the minority game with an arbitrary odd number of players. Interestingly, different learning processes provide considerably different predictions.
physics.soc-ph
the minority game is a simple congestion game in which the players main goal is to choose among two options the one that is adopted by the smallest number of players we characterize the set of nash equilibria and the limiting behavior of several wellknown learning processes in the minority game with an arbitrary odd number of players interestingly different learning processes provide considerably different predictions
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708.3543
Space-time orientations and Maxwell's equations
An analysis of the concept of orientation used in electrodynamics is presented. At least two different versions are encountered in the literature. Both are clearly identified and comparisons are made.
math-ph math.DG math.MP
an analysis of the concept of orientation used in electrodynamics is presented at least two different versions are encountered in the literature both are clearly identified and comparisons are made
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708.3544
A crystal theoretic method for finding rigged configurations from paths
The Kerov--Kirillov--Reshetikhin (KKR) bijection gives one to one correspondences between the set of highest paths and the set of rigged configurations. In this paper, we give a crystal theoretic reformulation of the KKR map from the paths to rigged configurations, using the combinatorial R and energy functions. This formalism provides tool for analysis of the periodic box-ball systems.
math.QA math-ph math.MP
the kerovkirillovreshetikhin kkr bijection gives one to one correspondences between the set of highest paths and the set of rigged configurations in this paper we give a crystal theoretic reformulation of the kkr map from the paths to rigged configurations using the combinatorial r and energy functions this formalism provides tool for analysis of the periodic boxball systems
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708.3545
Applied statistics: A review
The main phases of applied statistical work are discussed in general terms. The account starts with the clarification of objectives and proceeds through study design, measurement and analysis to interpretation. An attempt is made to extract some general notions.
stat.AP
the main phases of applied statistical work are discussed in general terms the account starts with the clarification of objectives and proceeds through study design measurement and analysis to interpretation an attempt is made to extract some general notions
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708.3546
Field Experimental "Star Type" Metropolitan Quantum Key Distribution Network
Quantum key distribution (QKD) network has recently attracted growing attentions. Due to the special characteristics of quantum information, to build a full-connectivity QKD network without trusted relays is a stimulating challenge. In this letter, we report on the first realization of QKD network without trusted relays which covers metropolis in the commercial backbone optical fiber networks. The star topology four-user QKD network automatically addresses the quantum signal with a quantum router (QR) and every user in the network can receive and distribute quantum keys to any others simultaneously. The longest and the shortest length of fibers between two geographically separated nodes are 42.6km and 32km respectively, and the maximum average quantum bit error rate (QBER) is below 8%. This result opens a new possibility for the use of QKD into existing network.
quant-ph
quantum key distribution qkd network has recently attracted growing attentions due to the special characteristics of quantum information to build a fullconnectivity qkd network without trusted relays is a stimulating challenge in this letter we report on the first realization of qkd network without trusted relays which covers metropolis in the commercial backbone optical fiber networks the star topology fouruser qkd network automatically addresses the quantum signal with a quantum router qr and every user in the network can receive and distribute quantum keys to any others simultaneously the longest and the shortest length of fibers between two geographically separated nodes are 426km and 32km respectively and the maximum average quantum bit error rate qber is below 8 this result opens a new possibility for the use of qkd into existing network
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708.3547
New Probable Dwarf Galaxies in Northern Groups of the Local Supercluster
We have searched for nearby dwarf galaxies in 27 northern groups with characteristic distances 8-15 Mpc based on the Second Palomar Sky Survey prints. In a total area of about 2000 square degrees, we have found 90 low-surface-brightness objects, more than 60% of which are absent from known catalogs and lists. We have classified most of these objects (~80%) as irregular dwarf systems. The first 21-cm line observations of the new objects with the 100-m Effelsberg radio telescope showed that the typical linear diameters (1-2 kpc), internal motions (30 km/s), and hydrogen masses (~2*10^7M_sun) galaxies correspond to those expected for the dwarf population of nearby groups.
astro-ph
we have searched for nearby dwarf galaxies in 27 northern groups with characteristic distances 815 mpc based on the second palomar sky survey prints in a total area of about 2000 square degrees we have found 90 lowsurfacebrightness objects more than 60 of which are absent from known catalogs and lists we have classified most of these objects 80 as irregular dwarf systems the first 21cm line observations of the new objects with the 100m effelsberg radio telescope showed that the typical linear diameters 12 kpc internal motions 30 kms and hydrogen masses 2107m_sun galaxies correspond to those expected for the dwarf population of nearby groups
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708.3548
One-dimensional fermionic gases with attractive p-wave interaction in a hard-wall trap
We investigate the ground state of the one-dimensional fermionic system enclosed in a hard-wall trap with attractive contact p-wave interactions. Based on the Bethe ansatz method, the explicit wave function is derived by numerically solving the Bethe ansatz equations for the full physical regimes ($-\infty \leq c_F\leq 0$). With the exact wave function some quantities which are important in many-body physics are obtained, including the one-body density matrix and the momentum distribution of the ground state for finite system. It is shown that the shell structure of the density profiles disappears with the increase of the interaction and in the fermionic Tonks-Girardeau (FTG) limit the density distribution shows the same behavior as that of an ideal Bose gas. However the one-body density matrix and the momentum distribution exhibit completely different structures compared with their bosonic counterparts.
cond-mat.other cond-mat.str-el
we investigate the ground state of the onedimensional fermionic system enclosed in a hardwall trap with attractive contact pwave interactions based on the bethe ansatz method the explicit wave function is derived by numerically solving the bethe ansatz equations for the full physical regimes infty leq c_fleq 0 with the exact wave function some quantities which are important in manybody physics are obtained including the onebody density matrix and the momentum distribution of the ground state for finite system it is shown that the shell structure of the density profiles disappears with the increase of the interaction and in the fermionic tonksgirardeau ftg limit the density distribution shows the same behavior as that of an ideal bose gas however the onebody density matrix and the momentum distribution exhibit completely different structures compared with their bosonic counterparts
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