Search results for "High Energy Physics - Theory"

showing 10 items of 775 documents

Evaporation of Near-Extremal Reissner-Nordström Black Holes

2000

The formation of near-extremal Reissner-Nordstrom black holes in the S-wave approximation can be described, near the event horizon, by an effective solvable model. The corresponding one-loop quantum theory remains solvable and allows to follow analytically the evaporation process which is shown to require an infinite amount of time.

AstrofísicaHigh Energy Physics - TheoryPhysicsEvent horizonMembrane paradigmAstronomyAstronomical PhenomenaEvaporationFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Models TheoreticalFuzzballGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Theory (hep-th)Nonsingular black hole modelsAstronomiaCamps Teoria quàntica deBlack hole thermodynamicsMathematical physicsPhysical Review Letters
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Critical energy flux and mass in solvable theories of 2D dilaton gravity

1998

In this paper we address the issue of determining the semiclassical threshold for black hole formation in the context of a one-parameter family of theories which continuously interpolates between the RST and BPP models. We find that the results depend significantly on the initial static configuration of the spacetime geometry before the influx of matter is turned on. In some cases there is a critical energy density, given by the Hawking rate of evaporation, as well as a critical mass $m_{cr}$ (eventually vanishing). In others there is neither $m_{cr}$ nor a critical flux.

AstrofísicaHigh Energy Physics - TheoryPhysicsGravitacióNuclear and High Energy PhysicsGravity (chemistry)EvaporationFOS: Physical sciencesFluxSemiclassical physicsContext (language use)General Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsCritical massCritical energyDilatonMathematical physicsPhysical Review D
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Integrable models and degenerate horizons in two-dimensional gravity

1999

We analyse an integrable model of two-dimensional gravity which can be reduced to a pair of Liouville fields in conformal gauge. Its general solution represents a pair of ``mirror'' black holes with the same temperature. The ground state is a degenerate constant dilaton configuration similar to the Nariai solution of the Schwarzschild-de Sitter case. The existence of $\phi=const.$ solutions and their relation with the solution given by the 2D Birkhoff's theorem is then investigated in a more general context. We also point out some interesting features of the semiclassical theory of our model and the similarity with the behaviour of AdS$_2$ black holes.

AstrofísicaHigh Energy Physics - TheoryPhysicsGravitacióNuclear and High Energy PhysicsIntegrable systemCanonical quantizationDegenerate energy levelsFOS: Physical sciencesSemiclassical physicsConformal mapContext (language use)General Relativity and Quantum CosmologyClassical mechanicsde Sitter–Schwarzschild metricHigh Energy Physics - Theory (hep-th)DilatonMathematical physicsPhysical Review D
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Revising the observable consequences of slow-roll inflation

2009

We study the generation of primordial perturbations in a (single-field) slow-roll inflationary Universe. In momentum space, these (Gaussian) perturbations are characterized by a zero mean and a nonzero variance Delta(2) (k, t). However, in position space the variance diverges in the ultraviolet. The requirement of a finite variance in position space forces one to regularize Delta(2) (k, t). This can (and should) be achieved by proper renormalization in an expanding Universe in a unique way. This affects the predicted scalar and tensorial power spectra (evaluated when the modes acquire classical properties) for wavelengths that today are at observable scales. As a consequence, the imprint of…

AstrofísicaPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Slow roll010308 nuclear & particles physicsFOS: Physical sciencesUnivers inflacionariPrivate communicationGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyManagementHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanics0103 physical sciences010306 general physicsUltraviolet radiationAstrophysics - Cosmology and Nongalactic Astrophysics
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The Cauchy problem in hybrid metric-Palatini f(X)-gravity

2013

The well-formulation and the well-posedness of the Cauchy problem is discussed for {\it hybrid metric-Palatini gravity}, a recently proposed modified gravitational theory consisting of adding to the Einstein-Hilbert Lagrangian an $f(R)$ term constructed {\it \`{a} la} Palatini. The theory can be recast as a scalar-tensor one predicting the existence of a light long-range scalar field that evades the local Solar System tests and is able to modify galactic and cosmological dynamics, leading to the late-time cosmic acceleration. In this work, adopting generalized harmonic coordinates, we show that the initial value problem can always be {\it well-formulated} and, furthermore, can be {\it well-…

Cauchy problemHarmonic coordinatesPhysicsHigh Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsFOS: Physical sciencesAcceleration (differential geometry)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesMetric (mathematics)Initial value problemBoundary value problem010303 astronomy & astrophysicsScalar fieldMathematical physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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MultivariateApart: Generalized partial fractions

2021

We present a package to perform partial fraction decompositions of multivariate rational functions. The algorithm allows to systematically avoid spurious denominator factors and is capable of producing unique results also when being applied to terms of a sum separately. The package is designed to work in Mathematica, but also provides interfaces to the Form and Singular computer algebra systems.

Computer Science - Symbolic ComputationHigh Energy Physics - TheoryFOS: Computer and information sciencesPolynomialComputer scienceFOS: Physical sciencesGeneral Physics and AstronomyRational functionSymbolic Computation (cs.SC)Partial fraction decomposition01 natural sciencesGröbner basisHigh Energy Physics - Phenomenology (hep-ph)ComputingMethodologies_SYMBOLICANDALGEBRAICMANIPULATION0103 physical sciences010306 general physicsSpurious relationshipcomputer.programming_language010308 nuclear & particles physicsFunction (mathematics)Symbolic computationAlgebraHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Hardware and ArchitectureComputer Science::Mathematical SoftwareWolfram LanguagecomputerComputer Physics Communications
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Path integral quantization for massive vector bosons

2010

A parity-conserving and Lorentz-invariant effective field theory of self-interacting massive vector fields is considered. For the interaction terms with dimensionless coupling constants the canonical quantization is performed. It is shown that the self-consistency condition of this system with the second-class constraints in combination with the perturbative renormalizability leads to an SU(2) Yang-Mills theory with an additional mass term.

Coupling constantPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsCanonical quantizationFOS: Physical sciencesAstronomy and AstrophysicsYang–Mills existence and mass gapAtomic and Molecular Physics and OpticsRenormalizationQuantization (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Path integral formulationEffective field theoryVector fieldMathematical physics
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Towards a kinetic theory for fermions with quantum coherence

2008

A new density matrix and corresponding quantum kinetic equations are introduced for fermions undergoing coherent evolution either in time (coherent particle production) or in space (quantum reflection). A central element in our derivation is finding new spectral solutions for the 2-point Green's functions written in the Wigner representation, that are carrying the information of the quantum coherence. Physically observable density matrix is then defined from the bare singular 2-point function by convoluting it with the extrenous information about the state of the system. The formalism is shown to reproduce familiar results from the Dirac equation approach, like Klein problem and nonlocal re…

Density matrixPhysicsHigh Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsAstrophysics (astro-ph)FOS: Physical sciencesObservableFermionAstrophysics01 natural sciencessymbols.namesakeOpen quantum systemHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Classical mechanicsHigh Energy Physics - Theory (hep-th)Dirac equationQuantum processQuantum mechanics0103 physical sciencessymbolsQuantum operation010306 general physicsCoherence (physics)
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Quantum kinetic theory for fermions in temporally varying backrounds

2008

We derive quantum kinetic equations for fermions in a homogeneous time-dependent background in presence of decohering collisions, by use of the Schwinger-Keldysh CTP-formalism. The quantum coherence (between particles and antiparticles) is found to arise from new spectral solutions for the dynamical 2-point correlation function in the mean field limit. The physical density matrix $\rho$ and its dynamics is shown to be necessarily dependent on the extrenous information on the system, and expressions that relate $\rho$ to fundamental coherence functions and fermionic particle and antiparticle numbers are derived. For an interacting system we demonstrate how smooth decoherence effects are indu…

Density matrixPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsQuantum decoherenceThermal quantum field theoryAstrophysics (astro-ph)FOS: Physical sciencesFermionAstrophysicsHigh Energy Physics - PhenomenologyThermalisationHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanicsQuasiparticleQuantumCoherence (physics)
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A new formulation of the loop-tree duality at higher loops

2019

We present a new formulation of the loop-tree duality theorem for higher loop diagrams valid both for massless and massive cases. $l$-loop integrals are expressed as weighted sum of trees obtained from cutting $l$ internal propagators of the loop graph. In addition, the uncut propagators gain a modified $i \delta$-prescription, named dual-propagators. In this new framework one can go beyond graphs and calculate the integrand of loop amplitudes as a weighted sum of tree graphs, which form a tree-like object. These objects can be computed efficiently via recurrence relations.

Discrete mathematicsHigh Energy Physics - TheoryLoop (graph theory)Recurrence relationDuality (mathematics)PropagatorFOS: Physical sciencesObject (computer science)Tree (graph theory)Massless particleHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Mathematics
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