Search results for "vit.C"

showing 10 items of 297 documents

Can conformal Transformations change the fate of 2D black holes?

1998

By using a classical Liouville-type model of two dimensional dilaton gravity we show that the one-loop theory implies that the fate of a black hole depends on the conformal frame. There is one frame for which the evaporation process never stops and another one leading to a complete disappearance of the black hole. This can be seen as a consequence of the fact that thermodynamic variables are not conformally invariant. In the second case the evaporation always produces the same static and regular end-point geometry, irrespective of the initial state.

PhysicsAstrofísicaHigh Energy Physics - TheoryNuclear and High Energy PhysicsGravitacióFOS: Physical sciencesConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Dilaton
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Free fields via canonical transformations of matter-coupled two-dimensional dilaton gravity models

1998

It is shown that the 1+1-dimensional matter-coupled Jackiw-Teitelboim model and the model with an exponential potential can be converted by means of appropriate canonical transformations into a bosonic string theory propagating on a flat target space with an indefinite signature. This makes it possible to consistently quantize these models in the functional Schroedinger representation thus generalizing recent results on CGHS theory.

PhysicsAstrofísicaNuclear and High Energy PhysicsGravity (chemistry)GravitacióCanonical quantizationBosonic string theorySpace (mathematics)symbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheorysymbolsDilatonSignature (topology)Representation (mathematics)Schrödinger's catMathematical physics
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Constraints on black-hole charges with the 2017 EHT observations of M87*

2021

Full list of authors: Kocherlakota, Prashant; Rezzolla, Luciano; Falcke, Heino; Fromm, Christian M.; Kramer, Michael; Mizuno, Yosuke; Nathanail, Antonios; Olivares, Héctor; Younsi, Ziri; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Algaba, Juan Carlos; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; …

PhysicsGravitació010308 nuclear & particles physicsAstronomyKinoAstrophysics::High Energy Astrophysical Phenomenagr-qcChatterjeeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Creative commons01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciencesAstronomiaFish <Actinopterygii>010306 general physicsGeneral relativity and quantum cosmologyHumanitiesPhysical Review D. Particles and Fields
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Cosmic censorship conjecture in some matching spherical collapsing metrics

2017

A physically plausible Lema{\^{\i}}tre-Tolman-Bondi collapse in the marginally bound case is considered. By "physically plausible" we mean that the corresponding metric is ${\cal C}^1$ matched at the collapsing star surface and further that its {\em intrinsic} energy is, as due, stationary and finite. It is proved for this Lema{\^{\i}}tre-Tolman-Bondi collapse, for some parameter values, that its intrinsic central singularity is globally naked, thus violating the cosmic censorship conjecture with, for each direction, one photon, or perhaps a pencil of photons, leaving the singularity and reaching the null infinity. Our result is discussed in relation to some other cases in the current liter…

PhysicsGravitacióConjecture010308 nuclear & particles physicsStar (game theory)media_common.quotation_subjectCosmic censorship hypothesisNull (mathematics)Collapse (topology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsInfinity01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologySingularityRelativitat general (Física)0103 physical sciencesGravitational singularity010306 general physicsMathematical physicsmedia_common
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Method to obtain shear-free two-fluid solutions of Einstein's equations.

1989

We use the Einstein equations, stated as an initial-value problem (3+1 formalism), to present a method for obtaining a class of solutions which may be interpreted as the gravitational field produced by a mixture of two perfect fluids. The four-velocity of one of the components is assumed to be a shear-free, irrotational, and geodesic vector field. The solutions are given up to a set of a hyperbolic quasilinear system.

PhysicsGravitacióGeodesicPerfect fluidConservative vector fieldRelativitat (Física)symbols.namesakeGravitational fieldEinstein field equationssymbolsVector fieldEinsteinRicci curvatureMathematical physicsPhysical review. D, Particles and fields
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Stability of the intrinsic energy vanishing in the Schwarzschild metric under a slow rotation

2014

The linearized Kerr metric is considered and put in some Gauss coordinates which are further {\em intrinsic} ones. The linear and angular 4-momenta of this metric are calculated in these coordinates and the resulting value is just zero. Thus, the global vanishing previously found for the Schwarzschild metric remains linearly stable under slow rotational perturbations of this metric.

PhysicsGravitacióPhysics and Astronomy (miscellaneous)GaussKerr metricZero (complex analysis)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Stability (probability)General Relativity and Quantum CosmologySlow rotationRelativitat general (Física)Metric (mathematics)Schwarzschild metricEnergy (signal processing)Mathematical physicsGeneral Relativity and Gravitation
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On the uniqueness of the space-time energy in General Relativity. The illuminating case of the Schwarzschild metric

2013

The case of asymptotic Minkowskian space-times is considered. A special class of asymptotic rectilinear coordinates at the spatial infinity, related to a specific system of free falling observers, is chosen. This choice is applied in particular to the Schwarzschild metric, obtaining a vanishing energy for this space-time. This result is compared with the result of some known theorems on the uniqueness of the energy of any asymptotic Minkowskian space, showing that there is no contradiction between both results, the differences becoming from the use of coordinates with different operational meanings. The suitability of Gauss coordinates when defining an {\em intrinsic} energy is considered a…

PhysicsGravitacióPhysics and Astronomy (miscellaneous)General relativitySpace timemedia_common.quotation_subjectGaussFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)InfinitySpace (mathematics)General Relativity and Quantum CosmologyRelativitat general (Física)Schwarzschild metricUniquenessEnergy (signal processing)media_commonMathematical physics
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Holography, degenerate horizons and entropy

1999

We show that a realization of the correspondence AdS_2/CFT_1 for near extremal Reissner-Nordstrom black holes in arbitrary dimensional Einstein-Maxwell gravity exactly reproduces, via Cardy's formula, the deviation of the Bekenstein-Hawking entropy from extremality. We also show that this mechanism is valid for Schwarzschild-de Sitter black holes around the degenerate solution dS_2xS^n. These results reinforce the idea that the Bekenstein-Hawking entropy can be derived from symmetry principles.

PhysicsHigh Energy Physics - TheoryAstrofísicaNuclear and High Energy PhysicsGravitacióCosmologiaDegenerate energy levelsHolographyFOS: Physical scienceslaw.inventionHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)lawEntropy (arrow of time)Mathematical physics
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Solvable Models for radiating Black Holes and Area-preserving Diffeomorphisms

1995

Solvable theories of 2D dilaton gravity can be obtained from a Liouville theory by suitable field redefinitions. In this paper we propose a new framework to generate 2D dilaton gravity models which can also be exactly solved in the semiclassical approximation. Our approach is based on the recently introduced scheme to quantize massless scalar fields coupled to 2D gravity maintaining invariance under area-preserving diffeomorphisms and Weyl transformations. Starting from the CGHS model with the new effective action we reestablish the full diffeomorphism invariance by means of an adequate family of field redefinitions. The original theory is therefore mapped into a large family of solvable mo…

PhysicsHigh Energy Physics - TheoryAstrofísicaNuclear and High Energy PhysicsGravitacióField (physics)CGHS modelScalar (physics)Semiclassical physicsFOS: Physical sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)symbolsDilatonDiffeomorphismEinsteinEffective actionMathematical physics
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Backlund transformations in 2-D dilaton gravity

1998

We give a B\"acklund transformation connecting a generic 2D dilaton gravity theory to a generally covariant free field theory. This transformation provides an explicit canonical transformation relating both theories.

PhysicsHigh Energy Physics - TheoryAstrofísicaNuclear and High Energy PhysicsGravity (chemistry)GravitacióGeneral Physics and AstronomyAstronomy and AstrophysicsCanonical transformationFree fieldGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyTransformation (function)Covariant transformationDilatonMathematical physics
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