Search results for "Horizon"

showing 10 items of 600 documents

Quantum gravity effects near the null black hole singularity

1998

The structure of the Cauchy Horizon singularity of a black hole formed in a generic collapse is studied by means of a renormalization group equation for quantum gravity. It is shown that during the early evolution of the Cauchy Horizon the increase of the mass function is damped when quantum fluctuations of the metric are taken into account.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsEvent horizonCauchy horizonFOS: Physical sciencesNaked singularityGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Gravitational singularityBlack hole thermodynamicsRing singularityBlack hole complementarityPhysical Review D
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Non-extremal black holes of N = 2, d = 4 supergravity

2011

We propose a generic recipe for deforming extremal black holes into non-extremal black holes and we use it to find and study the non-extremal black-hole solutions of several N=2,d=4 supergravity models (SL(2,R)/U(1), CPn and STU with four charges). In all the cases considered, the non-extremal family of solutions smoothly interpolates between all the different extremal limits, supersymmetric and not supersymmetric. This fact can be used to find explicitly extremal non-supersymmetric solutions in the cases in which the attractor mechanism does not completely fix the values of the scalars on the event horizon and they still depend on the boundary conditions at spatial infinity. We compare (su…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsEvent horizonSupergravitySuperpotentialFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyModuli spaceBlack holeCombinatoricsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)AttractorCentral chargeSymplectic geometryJournal of High Energy Physics
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Horizon geometry, duality and fixed scalars in six dimensions

1998

We consider the problem of extremizing the tension for BPS strings in D=6 supergravities with different number of supersymmetries. General formulae for fixed scalars and a discussion of degenerate directions is given. Quantized moduli, according to recent analysis, are supposed to be related to conformal field theories which are the boundary of three dimensional anti-de Sitter space time.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsHorizonSpace timeDegenerate energy levelsFOS: Physical sciencesBoundary (topology)Duality (optimization)FísicaField (mathematics)Conformal mapModuliGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Particle Physics - TheoryMathematical physics
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Late-time correlations in semiclassical particle-black hole scattering

2002

We analyse the quantum corrected geometry and radiation in the scattering of extremal black holes by low-energy neutral matter. We point out the fact that the correlators of local observables inside the horizon are the same as those of the vacuum. Outside the horizon the correlators at late times are much bigger than those of the (thermal) case obtained neglecting the backreaction. This suggests that the corrected Hawking radiation could be compatible with unitarity.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuantum field theory in curved spacetimeUnitarityGeneral relativityEvent horizonScatteringFOS: Physical sciencesSemiclassical physicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyPartícules (Física nuclear)Black holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsQuantum mechanicsHawking radiation
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Constraining inverse-curvature gravity with supernovae

2005

We show that the current accelerated expansion of the Universe can be explained without resorting to dark energy. Models of generalized modified gravity, with inverse powers of the curvature can have late time accelerating attractors without conflicting with solar system experiments. We have solved the Friedman equations for the full dynamical range of the evolution of the Universe. This allows us to perform a detailed analysis of Supernovae data in the context of such models that results in an excellent fit. Hence, inverse curvature gravity models represent an example of phenomenologically viable models in which the current acceleration of the Universe is driven by curvature instead of dar…

High Energy Physics - TheoryPhysicsPhantom energyAstrophysics (astro-ph)FOS: Physical sciencesGeneral Physics and AstronomyBig RipGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGeneral Relativity and Quantum CosmologyParticle horizonMetric expansion of spaceTheoretical physicsHigh Energy Physics - Theory (hep-th)De Sitter universeZero-energy universeFlatness problemScale factor (cosmology)
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Geodesically complete BTZ-type solutions of $2+1$ Born-Infeld gravity

2016

We study Born-Infeld gravity coupled to a static, nonrotating electric field in $2+1$ dimensions and find exact analytical solutions. Two families of such solutions represent geodesically complete, and hence nonsingular, spacetimes. Another family represents a point-like charge with a singularity at the center. Despite the absence of rotation, these solutions resemble the charged, rotating BTZ solution of General Relativity but with a richer structure in terms of horizons. The nonsingular character of the first two families turn out to be attached to the emergence of a wormhole structure on their innermost region. This seems to be a generic prediction of extensions of General Relativity for…

High Energy Physics - TheoryPhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsGeneral relativityDegrees of freedom (physics and chemistry)FOS: Physical sciencesCharge (physics)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyConnection (mathematics)General Relativity and Quantum CosmologySingularityHigh Energy Physics - Theory (hep-th)Born–Infeld model0103 physical sciencesHorizon (general relativity)Wormhole010306 general physicsMathematical physics
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Acoustic white holes in flowing atomic Bose-Einstein condensates

2010

International audience; We study acoustic white holes in a steadily flowing atomic Bose-Einstein condensate. A white hole configuration is obtained when the flow velocity goes from a super-sonic value in the upstream region to a sub-sonic one in the downstream region. The scattering of phonon wavepackets on a white hole horizon is numerically studied in terms of the Gross-Pitaevskii equation of mean-field theory: dynamical stability of the acoustic white hole is found, as well as a signature of a nonlinear back-action of the incident phonon wavepacket onto the horizon. The correlation pattern of density fluctuations is numerically studied by means of the truncated-Wigner method which includ…

High Energy Physics - Theory[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]PhononWhite holeGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology010305 fluids & plasmaslaw.inventionGeneral Relativity and Quantum CosmologyCorrelation functionlaw0103 physical sciences010306 general physicsSUPERFLOWBLACK-HOLESQuantum fluctuationPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]HorizonMean field theoryHigh Energy Physics - Theory (hep-th)Quantum Gases (cond-mat.quant-gas)Quantum electrodynamics[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Condensed Matter - Quantum GasesBose–Einstein condensateHawking radiation
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Quantum Backreaction on Three-Dimensional Black Holes and Naked Singularities

2016

We analytically investigate backreaction by a quantum scalar field on two rotating Ba\~nados-Teitelboim-Zanelli (BTZ) geometries: that of a black hole and that of a naked singularity. In the former case, we explore the quantum effects on various regions of relevance for a rotating black hole space-time. We find that the quantum effects lead to a growth of both the event horizon and the radius of the ergosphere, and to a reduction of the angular velocity, compared to the unperturbed values. Furthermore, they give rise to the formation of a curvature singularity at the Cauchy horizon and show no evidence of the appearance of a superradiant instability. In the case of a naked singularity, we f…

High Energy Physics - Theoryblack hole: rotationeffect: quantumvelocitysemiclassicalEvent horizonperturbationspace-time: black holeGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)angular momentum01 natural sciencesErgospherePenrose processGeneral Relativity and Quantum Cosmologyhorizon[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]black hole: BTZGeneral Relativity and Quantum CosmologyQuantum mechanics0103 physical sciencescurvature: singularity010306 general physicsRing singularityPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationNaked singularitycoupling: conformalstabilityfield theory: scalarBlack holeClassical mechanicsHigh Energy Physics - Theory (hep-th)Apparent horizonback reaction: quantum[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]massGravitational singularitysuperradianceblack hole: geometry
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(208)po populated through EC/beta(+) decay

2020

The structure of 208Po resulting from the EC/β + decay of 208At was studied at CERN’s ISOLDE Decay Station (IDS). The high statistics afforded by the high yield of 208At and the high efficiency HPGe clusters at the IDS allowed for greater insight into lower intensity transitions and thus significant expansion of the 208Po level scheme. Furthermore, investigation into the isomeric state yielded a new half life 377(9) ns in addition to uncovering new transitions populating the state.

HistoryHorizon (archaeology)010308 nuclear & particles physicsIndustrial strategy01 natural scienceslanguage.human_language3100Computer Science ApplicationsEducationGermanPolitical science0103 physical scienceslanguageEconomic historymedia_common.cataloged_instanceFísica nuclearNuclear Physics - ExperimentEuropean union010306 general physicsydinfysiikkapoloniummedia_common
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On the thermal instability in a horizontal rectangular porous channel heated from below by a constant flux

2014

Published version of an article in the journal: Journal of Physics: Conference Series. Also available from the publisher at: http://dx.doi.org/10.1088/1742-6596/501/1/012003 Open Access The onset of thermoconvective instability in a rectangular horizontal channel filled with a fluid-saturated porous medium is studied. The channel is heated from below with a constant flux. The top wall is maintained at a uniform constant temperature, while the lateral boundaries are permeable and perfectly conducting. The stability of the basic motionless state is analysed with respect to small-amplitude disturbances. The eigenvalue problem for the neutral stability condition is solved analytically for the n…

HistorySeries (mathematics)Chemistryhorizontal channelFluxMechanicsthermoconvective instabilityVDP::Mathematics and natural science: 400::Physics: 430Computer Science ApplicationsEducationPorous channelRAYLEIGH–BÉNARD PROBLEMPhysics::Fluid DynamicsRECTANGULAR DUCTClassical mechanicsPOROUS MEDIUMEIGENVALUESThermal instabilityLINEAR STABILITY ANALYSISConstant (mathematics)pos medium
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