0000000001136224

AUTHOR

Eugeny Babichev

0000-0003-4932-587x

showing 2 related works from this author

Instability of black holes in massive gravity

2013

We show that linear perturbations around the simplest black hole solution of massive bi-gravity theories, the bi-Schwarzschild solution, exhibit an unstable mode featuring the Gregory-Laflamme instability of higher dimensional black strings. The result is obtained for the massive gravity theory which is free from the Boulware-Deser ghost, as well as for its extension with two dynamical metrics. These results may indicate that static black holes in massive gravity do not exist. For the graviton mass of the order of the Hubble scale, however, the instability timescale is of order of the Hubble time.

High Energy Physics - TheoryPhysics and Astronomy (miscellaneous)Field (physics)Scale (ratio)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFieldGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesInstabilityGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum Cosmology0103 physical sciencesBlack stringStrings010306 general physicsPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]GravitonP-BranesBlack holeMassive gravityHigh Energy Physics - Theory (hep-th)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
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Stability analysis of black holes in massive gravity: a unified treatment

2014

We consider the analytic solutions of massive (bi)gravity which can be written in a simple form using advanced Eddington-Finkelstein coordinates. We analyse the stability of these solutions against radial perturbations. First we recover the previously obtained result on the instability of the bidiagonal bi-Schwarzschild solutions. In the non-bidiagonal case (which contains, in particular, the Schwarzschild solution with Minkowski fiducial metric) we show that generically there are physical spherically symmetric perturbations, but no unstable modes.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Kerr metricFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesInstabilityGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesMinkowski spaceSchwarzschild metric010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Massive gravityClassical mechanicsHigh Energy Physics - Theory (hep-th)Reissner–Nordström metric[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Deriving the Schwarzschild solution[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]
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