Search results for "HAWKING"

showing 9 items of 49 documents

Accretion-driven gravitational radiation from nonrotating compact objects. Infalling quadrupolar shells

2004

This paper reports results from numerical simulations of the gravitational radiation emitted from non--rotating compact objects(both neutron stars and Schwarzschild black holes) as a result of the accretion of matter. A hybrid procedure is adopted: we evolve, in axisymmetry, the linearized equations describing metric and fluid perturbations, coupled with a nonlinear hydrodynamics code that calculates the motion of the accreting matter. The initial matter distribution is shaped in the form of extended quadrupolar shells of dust or perfect fluid. Self--gravity and radiation reaction effects of the accreting fluid are neglected. This idealized setup is used to understand the qualitative featur…

PhysicsNuclear and High Energy PhysicsWhite holeAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsCompact starGeneral Relativity and Quantum CosmologyBlack holeNumerical relativityGeneral Relativity and Quantum CosmologyGravitational collapseStellar black holeSpaghettificationAstrophysics::Galaxy AstrophysicsHawking radiation
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Quantum-mechanical model of the Kerr-Newman black hole

2000

We consider a Hamiltonian quantum theory of stationary spacetimes containing a Kerr-Newman black hole. The physical phase space of such spacetimes is just six-dimensional, and it is spanned by the mass $M$, the electric charge $Q$ and angular momentum $J$ of the hole, together with the corresponding canonical momenta. In this six-dimensional phase space we perform a canonical transformation such that the resulting configuration variables describe the dynamical properties of Kerr-Newman black holes in a natural manner. The classical Hamiltonian written in terms of these variables and their conjugate momenta is replaced by the corresponding self-adjoint Hamiltonian operator and an eigenvalue …

PhysicsNuclear and High Energy PhysicsWhite holeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)FuzzballGeneral Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyRotating black holeNonsingular black hole modelsQuantum mechanicsExtremal black holeBlack hole thermodynamicsHawking radiation
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Signatures of primordial black hole dark matter at DUNE and THEIA

2021

Primordial black holes (PBHs) are a potential dark matter candidate whose masses can span over many orders of magnitude. If they have masses in the $10^{15}-10^{17}$ g range, they can emit sizeable fluxes of MeV neutrinos through evaporation via Hawking radiation. We explore the possibility of detecting light (non-)rotating PBHs with future neutrino experiments. We focus on two next generation facilities: the Deep Underground Neutrino Experiment (DUNE) and THEIA. We simulate the expected event spectra at both experiments assuming different PBH mass distributions and spins, and we extract the expected 95% C.L. sensitivities to these scenarios. Our analysis shows that future neutrino experime…

PhysicsPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesAstronomy and AstrophysicsPrimordial black holeAstrophysicsParameter spaceHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Orders of magnitude (time)Deep Underground Neutrino ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsHawking radiation
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The role of the Planck scale in black hole radiance

2008

Lorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially requires an integration in arbitrarily small distances or, equivalently, in unbounded energies. New physics at the Planck scale could, therefore, potentially modify the emission spectrum. We argue, however, that the kinematic invariance can be deformed in such a way that the thermal spectrum remains insensitive to trans-Planckian physics.

PhysicsPlanck energyPlanck particlePlanck massAstronomy and Astrophysicssymbols.namesakeMicro black holePlanck forceSpace and Planetary ScienceQuantum mechanicssymbolsVirtual black holeMathematical PhysicsHawking radiationPlanck length
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General Solution for Self-Gravitating Spherical Null Dust

1997

We find the general solution of equations of motion for self-gravitating spherical null dust as a perturbative series in powers of the outgoing matter energy-momentum tensor, with the lowest order term being the Vaidya solution for the ingoing matter. This is done by representing the null-dust model as a 2d dilaton gravity theory, and by using a symmetry of a pure 2d dilaton gravity to fix the gauge. Quantization of this solution would provide an effective metric which includes the back-reaction for a more realistic black hole evaporation model than the evaporation models studied previously.

PhysicsShock waveHigh Energy Physics - TheoryNuclear and High Energy PhysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyQuantization (physics)High Energy Physics::TheoryGeneral Relativity and Quantum CosmologyClassical mechanicsSolution of equationsHigh Energy Physics - Theory (hep-th)DilatonHawking radiationGauge fixing
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The runaway instability of thick discs around black holes. II. Non constant angular momentum discs

2003

We present results from a comprehensive number of relativistic, time-dependent, axisymmetric simulations of the runaway instability of non-constant angular momentum thick discs around black holes. This second paper extends earlier results where only constant angular momentum discs were considered. All relevant aspects of the theory of stationary thick discs around rotating black holes, necessary to build the initial state in our simulations, are presented in great detail. The angular momentum of the discs is assumed to increase outwards with the radial distance according to a power law. The main simplifying assumptions of our approach are not to include magnetic fields and self-gravity in t…

PhysicsWhite holeAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyRotating black holeBinary black holeSpace and Planetary ScienceExtremal black holeStellar black holeAstrophysics::Earth and Planetary AstrophysicsSchwarzschild radiusHawking radiation
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Generalized Virasoro anomaly and stress tensor for dilaton coupled theories

2003

We derive the anomalous transformation law of the quantum stress tensor for a 2D massless scalar field coupled to an external dilaton. This provides a generalization of the Virasoro anomaly which turns out to be consistent with the trace anomaly. We apply it together with the equivalence principle to compute the expectation values of the covariant quantum stress tensor on a curved background. Finally we briefly illustrate how to evaluate vacuum polarization and Hawking radiation effects from these results.

Tensor contractionPhysicsAstrofísicaHigh Energy Physics - TheoryNuclear and High Energy PhysicsCauchy stress tensorDilaton coupled theoriesHawking radiationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Stress tensorDilatonCovariant transformationVacuum polarizationVacuum polarizationAnomaly (physics)Tensor densityScalar fieldVirasoro and trace anomaliesMathematical physics
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Scattering of Co-Current Surface Waves on an Analogue Black Hole

2018

We report on what is to our knowledge the first scattering experiment of surface waves on an accelerating transcritical flow, which in the analogue gravity context is described by an effective spacetime with a black-hole horizon. This spacetime has been probed by an incident co-current wave, which partially scatters into an outgoing countercurrent wave on each side of the horizon. The measured scattering amplitudes are compatible with the predictions of the hydrodynamical theory, where the kinematical description in terms of the effective metric is exact.

surface: deformationGeneral Physics and AstronomyFOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)black hole: horizonGravitation and Astrophysics01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical scienceswave: scatteringsurfaceeffect: Hawkingcorrelation function010306 general physicsPhysicsSpacetimeScatteringHorizonFluid Dynamics (physics.flu-dyn)Physics - Fluid Dynamics[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Scattering amplitudeBlack holeFlow (mathematics)space-timeSurface waveQuantum electrodynamics[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
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Remembering an Era: Roger Penrose’s Paper on “Gravitational Collapse: The Role of General Relativity”

2018

Back in the 1960s, Einstein’s theory of general relativity re-emerged as a field of important research activity. Much of the impetus behind this resurgence came from powerful new mathematical ideas that Roger Penrose and Stephen Hawking applied to prove general singularity theorems for global space-time structures. Their results stirred the imaginations of astrophysicists and gave relativistic cosmology an entirely new research agenda. A decade later, black holes and the big hang model were on the tongues of nearly everyone who followed recent trends in science. As popular expositions dealing with quasars, pulsars, and the geometry of black holes began to appear in magazines and textbooks, …

symbols.namesakeImportant researchHawkingGeneral relativityPhilosophyGravitational collapsesymbolsEinsteinCosmologyClassics
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