0000000000735440

AUTHOR

Helios Sanchis-alepuz

showing 5 related works from this author

Static quantum corrections to the Schwarzschild spacetime

2005

We study static quantum corrections of the Schwarzschild metric in the Boulware vacuum state. Due to the absence of a complete analytic expression for the full semiclassical Einstein equations we approach the problem by considering the s-wave approximation and solve numerically the associated backreaction equations. The solution, including quantum effects due to pure vacuum polarization, is similar to the classical Schwarzschild solution up to the vicinity of the classical horizon. However, the radial function has a minimum at a time-like surface close to the location of the classical event horizon. There the g_{00} component of the metric reaches a very small but non-zero value. The analys…

PhysicsHigh Energy Physics - TheoryHistorySpacetimeEvent horizonVacuum stateSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyComputer Science ApplicationsEducationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Horizon (general relativity)Schwarzschild metricVacuum polarizationSchwarzschild radiusMathematical physics
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Semiclassical zero-temperature corrections to Schwarzschild spacetime and holography

2005

Motivated by the quest for black holes in AdS braneworlds, and in particular by the holographic conjecture relating 5D classical bulk solutions with 4D quantum corrected ones, we numerically solve the semiclassical Einstein equations (backreaction equations) with matter fields in the (zero temperature) Boulware vacuum state. In the absence of an exact analytical expression for in four dimensions we work within the s-wave approximation. Our results show that the quantum corrected solution is very similar to Schwarzschild till very close to the horizon, but then a bouncing surface for the radial function appears which prevents the formation of an event horizon. We also analyze the behavior of…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsCosmologiaQuantum field theory in curved spacetimeEvent horizonWhite holeKerr metricFOS: Physical sciencesNaked singularityGeneral Relativity and Quantum Cosmology (gr-qc)Partícules (Física nuclear)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsDeriving the Schwarzschild solutionSchwarzschild radiusPhysical Review D
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Geonic black holes and remnants in Eddington-inspired Born–Infeld gravity

2014

We show that electrically charged solutions within the Eddington-inspired Born–Infeld theory of gravity replace the central singularity by a wormhole supported by the electric field. As a result, the total energy associated with the electric field is finite and similar to that found in the Born–Infeld electromagnetic theory. When a certain charge-to-mass ratio is satisfied, in the lowest part of the mass and charge spectrum the event horizon disappears, yielding stable remnants. We argue that quantum effects in the matter sector can lower the mass of these remnants from the Planck scale down to the TeV scale.

PhysicsHigh Energy Physics - TheoryGravity (chemistry)Scale (ratio)Physics and Astronomy (miscellaneous)Event horizonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCharge (physics)General Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyGravitationSingularityHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsElectric fieldWormholeRegular Article - Theoretical PhysicsEngineering (miscellaneous)The European Physical Journal C
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Dynamical Aspects of Generalized Palatini Theories of Gravity

2009

We study the field equations of modified theories of gravity in which the Lagrangian is a general function of the Ricci scalar and Ricci-squared terms in Palatini formalism. We show that the independent connection can be expressed as the Levi-Civitagrave connection of an auxiliary metric which, in particular cases of interest, is related with the physical metric by means of a disformal transformation. This relation between physical and auxiliary metric boils down to a conformal transformation in the case of f(R) theories. We also show with explicit models that the inclusion of Ricci-squared terms in the action can impose upper bounds on the accessible values of pressure and density, which m…

PhysicsNuclear and High Energy PhysicsBlack hole formationFOS: Physical sciencesConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)CosmologyGeneral Relativity and Quantum CosmologyGravitationsymbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicssymbolsf(R) gravityPhenomenology (particle physics)LagrangianMathematical physicsScalar curvature
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Bouncing Cosmologies in Palatini $f(R)$ Gravity

2009

7 pages, 4 figures.-- PACS nrs.: 04.50.Kd; 98.80.-k; 98.80.Qc.-- ArXiv pre-print available at: http://arxiv.org/abs/0907.0318

PhysicsNuclear and High Energy Physicsmedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)UniverseCosmologyGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsQuantum cosmologyGravitational collapsef(R) gravityGravitational singularityBig Bouncemedia_commonLoop quantum cosmology
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