Search results for "Kretschmann scalar"

showing 2 items of 2 documents

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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Palatini $f(R)$ Black Holes in Nonlinear Electrodynamics

2011

The electrically charged Born-Infeld black holes in the Palatini formalism for $f(R)$ theories are analyzed. Specifically we study those supported by a theory $f(R)=R\pm R^2/R_P$, where $R_P$ is Planck's curvature. These black holes only differ from their General Relativity counterparts very close to the center, but may give rise to different geometrical structures in terms of inner horizons. The nature and strength of the central singularities are also significantly affected. In particular, for the model $f(R)=R - R^2/R_P$ the singularity is shifted to a finite radius, $r_+$, and the Kretschmann scalar diverges only as $1/(r-r_+)^{2}$.

PhysicsNuclear and High Energy PhysicsGeneral relativityKretschmann scalarFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)CurvatureGeneral Relativity and Quantum CosmologyNonlinear systemFormalism (philosophy of mathematics)General Relativity and Quantum CosmologySingularityQuantum mechanicsGravitational singularity
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