Search results for "Wormholes"

showing 6 items of 6 documents

Semiclassical geons as solitonic black hole remnants

2013

We find that the end state of black hole evaporation could be represented by non-singular and without event horizon stable solitonic remnants with masses of the order the Planck scale and up to similar to 16 units of charge. Though these objects are locally indistinguishable from spherically symmetric, massive electric (or magnetic) charges, they turn out to be sourceless geons containing a wormhole generated by the electromagnetic field. Our results are obtained by interpreting semiclassical corrections to Einstein's theory in the first-order (Palatini) formalism, which yields second-order equations and avoids the instabilities of the usual (metric) formulation of quadratic gravity. We als…

Electromagnetic fieldHigh Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)Event horizonDark matterSemiclassical physicsFOS: Physical sciencesPrimordial black holeGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum Cosmology0103 physical sciencesWormhole010306 general physicsmodified gravityMathematical physicsPhysics010308 nuclear & particles physicsprimordial black holesAstronomy and Astrophysicsquantum field theory on curved spaceBlack holeHigh Energy Physics - Theory (hep-th)WormholesAstrophysics - Cosmology and Nongalactic Astrophysics
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Semiclassical geons at particle accelerators

2014

We point out that in certain four-dimensional extensions of general relativity constructed within the Palatini formalism stable self-gravitating objects with a discrete mass and charge spectrum may exist. The incorporation of nonlinearities in the electromagnetic field may effectively reduce their mass spectrum by many orders of magnitude. As a consequence, these objects could be within (or near) the reach of current particle accelerators. We provide an exactly solvable model to support this idea.

High Energy Physics - TheoryElectromagnetic fieldPhysicsGeneral relativityquantum black holesFOS: Physical sciencesSemiclassical physicsAstronomy and AstrophysicsParticle acceleratorGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmologylaw.inventionHigh Energy Physics - PhenomenologyFormalism (philosophy of mathematics)Theoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)lawMass spectrumWormholeWormholesGeon (physics)modified gravityJournal of Cosmology and Astroparticle Physics
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New scalar compact objects in Ricci-based gravity theories

2019

Taking advantage of a previously developed method, which allows to map solutions of General Relativity into a broad family of theories of gravity based on the Ricci tensor (Ricci-based gravities), we find new exact analytical scalar field solutions by mapping the free-field static, spherically symmetric solution of General Relativity (GR) into quadratic $f(R)$ gravity and the Eddington-inspired Born-Infeld gravity. The obtained solutions have some distinctive feature below the would-be Schwarzschild radius of a configuration with the same mass, though in this case no horizon is present. The compact objects found include wormholes, compact balls, shells of energy with no interior, and a new …

High Energy Physics - TheoryModified gravityFísica-Modelos matemáticosGeneral relativityGravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesFísica matemáticaWormhole010306 general physicsRicci curvaturePhysics010308 nuclear & particles physicsScalar (physics)Astronomy and AstrophysicsGR black holesBlack holeHigh Energy Physics - Theory (hep-th)Horizon (general relativity)WormholesScalar fieldSchwarzschild radius
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Dynamical generation of wormholes with charged fluids in quadratic Palatini gravity

2014

The dynamical generation of wormholes within an extension of General Relativity (GR) containing (Planck's scale-suppressed) Ricci-squared terms is considered. The theory is formulated assuming the metric and connection to be independent (Palatini formalism) and is probed using a charged null fluid as a matter source. This has the following effect: starting from Minkowski space, when the flux is active the metric becomes a charged Vaidya-type one, and once the flux is switched off the metric settles down into a static configuration such that far from the Planck scale the geometry is virtually indistinguishable from that of the standard Reissner-Nordstr\"om solution of GR. However, the innerm…

High Energy Physics - TheoryNuclear and High Energy PhysicsGeneral relativityPhysical constantDynamical generation of wormholesFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvature01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationTheoretical physicsGeneral Relativity and Quantum CosmologySingularityFísica Aplicada0103 physical sciencesMinkowski spaceWormhole010306 general physicsQuantumPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsHigh Energy Physics - Theory (hep-th)Astrophysics - High Energy Astrophysical PhenomenaQuadratic Palatini gravityCharged fluids
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Nonsingular Black Holes in $f(R)$ Theories

2015

We study the structure of a family of static, spherically symmetric space-times generated by an anisotropic fluid and governed by a particular type of $f(R)$ theory. We find that for a range of parameters with physical interest, such solutions represent black holes with the central singularity replaced by a finite size wormhole. We show that time-like geodesics and null geodesics with nonzero angular momentum never reach the wormhole throat due to an infinite potential barrier. For null radial geodesics, it takes an infinite affine time to reach the wormhole. This means that the resulting space-time is geodesically complete and, therefore, nonsingular despite the generic existence of curvat…

PhysicsHigh Energy Physics - TheoryAngular momentumGeodesicNull (mathematics)General Physics and AstronomyFOS: Physical sciencesnonsingular black holesGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)CurvaturewormholesGeneral Relativity and Quantum Cosmologylaw.inventionGeneral Relativity and Quantum CosmologySingularityInvertible matrixHigh Energy Physics - Theory (hep-th)lawWormholemodified gravityMathematical physics
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Rotating black holes in Eddington-inspired Born-Infeld gravity: an exact solution

2020

We find an exact, rotating charged black hole solution within Eddington-inspired Born-Infeld gravity. To this end we employ a recently developed correspondence or {\it mapping} between modified gravity models built as scalars out of contractions of the metric with the Ricci tensor, and formulated in metric-affine spaces (Ricci-Based Gravity theories) and General Relativity. This way, starting from the Kerr-Newman solution, we show that this mapping bring us the axisymmetric solutions of Eddington-inspired Born-Infeld gravity coupled to a certain model of non-linear electrodynamics. We discuss the most relevant physical features of the solutions obtained this way, both in the spherically sym…

PhysicsHigh Energy Physics - TheoryGravity (chemistry)Modified gravityFísica-Modelos matemáticos010308 nuclear & particles physicsGeneral relativityRotational symmetryFOS: Physical sciencesAstronomy and AstrophysicsGR black holesGeneral Relativity and Quantum Cosmology (gr-qc)Charged black hole01 natural sciencesGravitational-wave astronomyGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyExact solutions in general relativityHigh Energy Physics - Theory (hep-th)0103 physical sciencesMetric (mathematics)Física matemáticaWormholesRicci curvature
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