Search results for "black holes [stars]"

showing 3 items of 3 documents

Three Duality Symmetries between Photons and Cosmic String Loops, and Macro and Micro Black Holes

2015

We present a review of two thermal duality symmetries between two different kinds of systems: photons and cosmic string loops, and macro black holes and micro black holes, respectively. It also follows a third joint duality symmetry amongst them through thermal equilibrium and stability between macro black holes and photon gas, and micro black holes and string loop gas, respectively. The possible cosmological consequences of these symmetries are discussed.

Particle physicsPhysics and Astronomy (miscellaneous)General MathematicsAstrophysics::High Energy Astrophysical PhenomenaDuality (optimization)cosmic string loopDuality symmetryString (physics)black holes thermodynamicsMicro black holeGeneral Relativity and Quantum Cosmologyblack holes thermodynamicComputer Science (miscellaneous)photonsSettore MAT/07 - Fisica MatematicaBlack hole thermodynamicsduality symmetryPhysicsPhotonslcsh:MathematicsphotonPhoton gasCosmic string loopslcsh:QA1-939Black holeCosmic stringChemistry (miscellaneous)photons; cosmic string loops; black holes thermodynamics; duality symmetryBlack holes thermodynamicscosmic string loopsHawking radiation
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Dynamical formation of a hairy black hole in a cavity from the decay of unstable solitons

2016

Recent numerical relativity simulations within the Einstein--Maxwell--(charged-)Klein-Gordon (EMcKG) system have shown that the non-linear evolution of a superradiantly unstable Reissner-Nordstr\"om black hole (BH) enclosed in a cavity, leads to the formation of a BH with scalar hair. Perturbative evidence for the stability of such hairy BHs has been independently established, confirming they are the true endpoints of the superradiant instability. The same EMcKG system admits also charged scalar soliton-type solutions, which can be either stable or unstable. Using numerical relativity techniques, we provide evidence that the time evolution of some of these $\textit{unstable}$ solitons leads…

PhysicsRadiation or classical fieldsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsScalar (mathematics)Time evolutionFOS: Physical sciencesSuperradianceGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesInstabilityEinstein–Maxwell spacetimesGeneral Relativity and Quantum CosmologyBlack holeNumerical relativityGeneral Relativity and Quantum CosmologyNumerical studies of black holes and black-hole binaries0103 physical sciencesSpacetimes with fluidsSoliton010306 general physicsRelativity and gravitationClassical black holesBosonMathematical physics
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A duality-invariant Einstein-Planck relation and its consequences on micro-black holes.

2013

We discuss the consequences of a duality-invariant Einstein–Planck (DIEP) relation on the equation of state of micro black holes. The results are analogous to those obtained from the "world-crystal" model, but with some significative differences, as for instance a limiting vanishing value for temperature for very small black holes. The model leads to a total evaporation of micro black holes but with the final stage being very slow.

Physicsduality symmetryBlack holes thermodynamicAstrophysics::High Energy Astrophysical PhenomenaEinstein–Planck relationFOS: Physical sciencesAstronomy and AstrophysicsLimitingGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)General Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsMicro black holeGeneral Relativity and Quantum CosmologySpace and Planetary SciencesymbolsEinsteinPlanckSettore MAT/07 - Fisica MatematicaMathematical PhysicsWorld crystal
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