Shear-free dust solution in general covariant Hořava-Lifshitz gravity
DOI10.1007/s10714-015-2013-2zbMath1334.83027arXiv1509.02685OpenAlexW2144920789MaRDI QIDQ265754
F. Blanchet-Sadri, M. Dambrine
Publication date: 12 April 2016
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1509.02685
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Cites Work
- Pathological behaviour of the scalar graviton in Hořava-Lifshitz gravity
- Hořava-Lifshitz cosmology
- Models of non-relativistic quantum gravity: the good, the bad and the healthy
- Lessons from the decoupling limit of Hořava gravity
- Vaidya solutions in general covariant Hořava–Lifshitz gravity without projectability: Infrared limit
- Hořava–Lifshitz cosmology: a review
- Note on trapped surfaces in the Vaidya solution
- Perturbative instabilities in Hořava gravity
- STABILITY OF THE DE SITTER SPACETIME IN HORAVA–LIFSHITZ THEORY
- Vaidya solution in general covariant Hořava–Lifshitz gravity with the minimum coupling and without projectability: Infrared limit
- An alternative approach for general covariant Hořava–Lifshitz gravity and matter coupling
This page was built for publication: Shear-free dust solution in general covariant Hořava-Lifshitz gravity
