0000000000042562

AUTHOR

Cecilia Bejarano

showing 2 related works from this author

Geometric inequivalence of metric and Palatini formulations of General Relativity

2020

Projective invariance is a symmetry of the Palatini version of General Relativity which is not present in the metric formulation. The fact that the Riemann tensor changes nontrivially under projective transformations implies that, unlike in the usual metric approach, in the Palatini formulation this tensor is subject to a gauge freedom, which allows some ambiguities even in its scalar contractions. In this sense, we show that for the Schwarzschild solution there exists a projective gauge in which the (affine) Kretschmann scalar, K≡R R , can be set to vanish everywhere. This puts forward that the divergence of curvature scalars may, in some cases, be avoided by a gauge transformation of the …

General RelativityNuclear and High Energy PhysicsRiemann curvature tensorFísica-Modelos matemáticosGeneral relativityScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology//purl.org/becyt/ford/1 [https]symbols.namesakeGeneral Relativity and Quantum Cosmology0103 physical sciencesSchwarzschild metricFísica matemáticaGauge theoryTensorGeometric inequivalence010306 general physicsMathematical PhysicsMathematical physicsPhysics010308 nuclear & particles physicsKretschmann scalar//purl.org/becyt/ford/1.3 [https]Mathematical Physics (math-ph)lcsh:QC1-999Symmetry (physics)symbolslcsh:PhysicsPhysics Letters
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What is a singular black hole beyond general relativity?

2017

Exploring the characterization of singular black hole spacetimes, we study the relation between energy density, curvature invariants, and geodesic completeness using a quadratic $f(R)$ gravity theory coupled to an anisotropic fluid. Working in a metric-affine approach, our models and solutions represent minimal extensions of General Relativity (GR) in the sense that they rapidly recover the usual Reissner-Nordstr\"{o}m solution from near the inner horizon outwards. The anisotropic fluid helps modify only the innermost geometry. Depending on the values and signs of two parameters on the gravitational and matter sectors, a breakdown of the correlations between the finiteness/divergence of the…

High Energy Physics - TheoryPhysicsMODIFIED THEORIES OF GRAVITY010308 nuclear & particles physicsGeneral relativityCiencias FísicasFOS: Physical sciences//purl.org/becyt/ford/1.3 [https]General Relativity and Quantum Cosmology (gr-qc)COSMIC CENSORSHIPOtras Ciencias Físicas01 natural sciencesCLASSICAL BLACK HOLESGeneral Relativity and Quantum Cosmology//purl.org/becyt/ford/1 [https]General Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)EINSTEIN-MAXWELL SPACETIMEQuantum mechanics0103 physical sciences010306 general physicsHumanitiesCIENCIAS NATURALES Y EXACTASPhysical Review D
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