Self-accelerating cosmologies and hairy black holes in ghost-free bigravity and massive gravity
From MaRDI portal
Publication:2861838
DOI10.1088/0264-9381/30/18/184009zbMath1277.83122arXiv1304.0238OpenAlexW3100812664MaRDI QIDQ2861838
Publication date: 11 November 2013
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1304.0238
Relativistic cosmology (83F05) Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (20)
Charged black hole solutions in Gauss-Bonnet-massive gravity ⋮ Einstein-Born-Infeld-massive gravity: AdS-black hole solutions and their thermodynamical properties ⋮ Combining cosmological and local bounds on bimetric theory ⋮ Constraints on bimetric gravity from Big Bang nucleosynthesis ⋮ Topological charged black holes in massive gravity's rainbow and their thermodynamical analysis through various approaches ⋮ Thermodynamics of black string from Rényi entropy in de Rham–Gabadadze–Tolley massive gravity theory ⋮ Quasi normal modes and P-V criticallity for scalar perturbations in a class of dRGT massive gravity around black holes ⋮ Thermodynamical structure of AdS black holes in massive gravity with stringy gauge-gravity corrections ⋮ Non-singular black holes in massive gravity: time-dependent solutions ⋮ Greybody factors of black holes in dRGT massive gravity coupled with nonlinear electrodynamics ⋮ Cosmological perturbation and matter power spectrum in bimetric massive gravity ⋮ No hair theorem in quasi-dilaton massive gravity ⋮ De Sitter vacua in ghost-free massive gravity theory ⋮ Strong lensing constraints on bimetric massive gravity ⋮ Stable FLRW solutions in generalized massive gravity ⋮ Massive spin-2 field in arbitrary spacetimes—the detailed derivation ⋮ A general theory of linear cosmological perturbations: bimetric theories ⋮ Massive gravity ⋮ Constraints on bimetric gravity. Part I. Analytical constraints ⋮ Constraints on bimetric gravity. Part II. Observational constraints
This page was built for publication: Self-accelerating cosmologies and hairy black holes in ghost-free bigravity and massive gravity