Search results for "Map"

showing 10 items of 3484 documents

Finite temperature phase diagrams of gauge theories

2012

We discuss finite temperature phase diagrams of SU(N) gauge theory with massless fermions as a function of the number of fermion flavors. Inside the conformal window we find a phase boundary separating two different conformal phases. Below the conformal window we find different phase structures depending on if the beta function of the theory has a first or higher order zero at the lower boundary of the conformal window. We also outline how the associated behaviors will help in distinguishing different types of theories using lattice simulations.

PhysicsNuclear and High Energy PhysicsThermal quantum field theoryta114Conformal field theoryConformal anomalyHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)Boundary conformal field theoryFOS: Physical sciencesConformal mapFermionTheoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)Conformal symmetryQuantum electrodynamicsGauge theoryPhysical Review D
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Brownian dynamics simulations with hard-body interactions: Spherical particles

2012

A novel approach to account for hard-body interactions in (overdamped) Brownian dynamics simulations is proposed for systems with non-vanishing force fields. The scheme exploits the analytically known transition probability for a Brownian particle on a one-dimensional half-line. The motion of a Brownian particle is decomposed into a component that is affected by hard-body interactions and into components that are unaffected. The hard-body interactions are incorporated by replacing the affected component of motion by the evolution on a half-line. It is discussed under which circumstances this approach is justified. In particular, the algorithm is developed and formulated for systems with spa…

PhysicsNumerical analysisFOS: Physical sciencesGeneral Physics and AstronomyProteinsComputational Physics (physics.comp-ph)Condensed Matter - Soft Condensed MatterModels BiologicalDiffusionMotionProbability theoryModels ChemicalProtein Interaction MappingBrownian dynamicsSoft Condensed Matter (cond-mat.soft)Computer SimulationStatistical physicsColloidsPhysical and Theoretical ChemistryPhysics - Computational PhysicsBrownian motionAlgorithms
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Null conformal Killing-Yano tensors and Birkhoff theorem

2015

We study the space-times admitting a null conformal Killing-Yano tensor whose divergence defines a Killing vector. We analyze the similitudes and differences with the recently studied non null case (Gen. Relativ. Grav. (2015) {\bf 47} 1911). The results by Barnes concerning the Birkhoff theorem for the case of null orbits are analyzed and generalized.

PhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsNull (mathematics)FOS: Physical sciencesConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyDivergenceKilling vector field0103 physical sciencesTensor010306 general physicsMathematical physics
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A Rainich-like approach to the Killing-Yano tensors

2002

The Rainich problem for the Killing-Yano tensors posed by Collinson \cite{col} is solved. In intermediate steps, we first obtain the necessary and sufficient conditions for a 2+2 almost-product structure to determine the principal 2--planes of a skew-symmetric Killing-Yano tensor and then we give the additional conditions on a symmetric Killing tensor for it to be the square of a Killing-Yano tensor.We also analyze a similar problem for the conformal Killing-Yano and the conformal Killing tensors. Our results show that, in both cases, the principal 2--planes define a maxwellian structure. The associated Maxwell fields are obtained and we outline how this approach is of interest in studying …

PhysicsPhysics and Astronomy (miscellaneous)GeodesicFirst integralsStructure (category theory)FOS: Physical sciencesConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)Square (algebra)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyKilling tensorTensorMathematics::Differential GeometryMathematical physics
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τ hadronic spectral function moments in a nonpower QCD perturbation theory

2016

Abstract The moments of the hadronic spectral functions are of interest for the extraction of the strong coupling and other QCD parameters from the hadronic decays of the τ lepton. We consider the perturbative behavior of these moments in the framework of a QCD nonpower perturbation theory, defined by the technique of series acceleration by conformal mappings, which simultaneously implements renormalization-group summation and has a tame large-order behavior. Two recently proposed models of the Adler function are employed to generate the higher order coefficients of the perturbation series and to predict the exact values of the moments, required for testing the properties of the perturbativ…

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHadronPerturbation (astronomy)Conformal map01 natural sciencesSeries accelerationstrong coupling0103 physical sciencesCentre for High Energy PhysicsPerturbation theory (quantum mechanics)010306 general physicsReference modeltau decaysLeptonNuclear and Particle Physics Proceedings
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On Chiral Quantum Superspaces

2011

We give a quantum deformation of the chiral Minkowski superspace in 4 dimensions embedded as the big cell into the chiral conformal superspace. Both deformations are realized as quantum homogeneous superspaces: we deform the ring of regular functions together with a coaction of the corresponding quantum supergroup.

PhysicsRing (mathematics)High Energy Physics::LatticeConformal mapSupersymmetryQUANTUM GROUPSSuperspaceGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryTheoretical physicsNonlinear Sciences::Exactly Solvable and Integrable SystemsMathematics::Quantum AlgebraQuantum mechanicsMinkowski spaceAffine varietySUPERSYMMETRYSupergroupQuantum
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Hyperboloidal slicing approach to quasinormal mode expansions: The Reissner-Nordström case

2018

We study quasi-normal modes of black holes, with a focus on resonant (or quasi-normal mode) expansions, in a geometric frame based on the use of conformal compactifications together with hyperboloidal foliations of spacetime. Specifically, this work extends the previous study of Schwarzschild in this geometric approach to spherically symmetric asymptotically flat black hole spacetimes, in particular Reissner-Nordstr\"om. The discussion involves, first, the non-trivial technical developments needed to address the choice of appropriate hyperboloidal slices in the extended setting as well as the generalization of the algorithm determining the coefficients in the expansion of the solution in te…

PhysicsSpacetime010308 nuclear & particles physicsGeneral relativitynumbers: 0425dgCauchy distributionalternative theories of gravityConformal map04.30.-w16. Peace & justice01 natural sciencesSlicingGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum Cosmology02.30.MvGeneral relativityRegularization (physics)0103 physical sciencesQuasinormal mode[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010306 general physicsSchwarzschild radiusPhysical Review D
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Towards asteroseismology of core-collapse supernovae with gravitational wave observations – II. Inclusion of space–time perturbations

2018

Improvements in ground-based, advanced gravitational wave (GW) detectors may allow in the near future to observe the GW signal of a nearby core-collapse supernova. For the most common type of progenitors, likely with slowly rotating cores, the dominant GW emission mechanisms are the post-bounce oscillations of the proto-neutron star (PNS) before the explosion. We present a new procedure to compute the eigenmodes of the system formed by the PNS and the stalled accretion shock in general relativity including spacetime perturbations. The new method improves on previous results by accounting for perturbations of both the lapse function and the conformal factor. We apply our analysis to two nume…

PhysicsSpacetime010308 nuclear & particles physicsGravitational waveGeneral relativitySpace timeAstronomy and AstrophysicsConformal mapAstrophysics01 natural sciencesAsteroseismologyInstabilitySupernovaSpace and Planetary Science0103 physical sciences010303 astronomy & astrophysicsMonthly Notices of the Royal Astronomical Society
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Scaling laws in the distribution of galaxies

2004

Research done during the previous century established our Standard Cosmological Model. There are many details still to be filled in, but few would seriously doubt the basic premise. Past surveys have revealed that the large-scale distribution of galaxies in the Universe is far from random: it is highly structured over a vast range of scales. To describe cosmic structures, we need to build mathematically quantifiable descriptions of structure. Identifying where scaling laws apply and the nature of those scaling laws is an important part of understanding which physical mechanisms have been responsible for the organization of clusters, superclusters of galaxies and the voids between them. Find…

PhysicsStructure (mathematical logic)EXTRA-GALACTIC NEBULAEMICROWAVE BACKGROUND-RADIATIONCOSMIC cancer databaseCold dark matterAstrophysics (astro-ph)Cosmic microwave backgroundCAMPANAS REDSHIFT SURVEY2-POINT CORRELATION-FUNCTIONFOS: Physical sciencesGeneral Physics and AstronomyAstrophysicsN-BODY SIMULATIONSAstrophysicsPOINT CORRELATION-FUNCTIONSGalaxyCOLD DARK-MATTERFractalPROBE WMAP OBSERVATIONSDIGITAL SKY SURVEYPEAK-PATCH PICTUREStatistical physicsScalingGalaxy clusterReviews of Modern Physics
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QPOs expected in rotating accretion flows around a supermassive black hole

2006

AbstractIt is well known that rotating inviscid accretion flows with adequate injection parameters around black holes could form shock waves close to the black holes, after the flow passes through the outer sonic point and can be virtually stopped by the centrifugal force. We numerically examine such shock waves in 2D accretion flows with 10−5 to 106 Eddington critical accretion rates around a supermassive black hole with 106M⊙. As the results, the luminosities show QPO phenomena with modulations of a factor 2–3 and with quasi-periods of a few to several hours.

PhysicsSupermassive black holeActive galactic nucleusBinary black holeRotating black holeSpace and Planetary ScienceIntermediate-mass black holeAstronomyReverberation mappingAstronomy and AstrophysicsStellar black holeSpin-flipAstrophysicsProceedings of the International Astronomical Union
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