Exact Schwarzschild-de Sitter black holes in a family of massive gravity models

2011/03/29 by Theo M. Nieuwenhuizen, Th. M. Nieuwenhuizen · 9 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Pulsars and Gravitational Waves Research #astro-ph.CO #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.84.024038

published as Phys.Rev.D84:024038,2011 · 4 pages

arxiv created 2011/03/29 · openalex publication_date 2011/07/20 · arxiv updated 2011/08/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30

Abstract

The Schwarzschild--de Sitter and Reissner-Nordstr"om--de Sitter black hole metrics appear as exact solutions in the recently formulated massive gravity of de Rham, Gabadadze and Tolley, where the mass term sets the curvature scale. They occur within a two-parameter family of de Rham, Gabadadze and Tolley mass terms. They show no trace of a cloud of scalar graviton modes, and in the limit of vanishing graviton mass they go smoothly to the Schwarzschild and Reissner-Nordstr"om metrics.

Citations

• On relativistic wave equations for particles of arbitrary spin in an electromagnetic field
• Resummation of Massive Gravity
• Generalization of the Fierz-Pauli Action
• Massive and mass-less Yang-Mills and gravitational fields

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