PLANE SYMMETRIC SOLUTIONS IN HOŘAVA–LIFSHITZ THEORY
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Publication:3070385
DOI10.1142/S0218271810018232zbMath1205.83059arXiv0911.1877OpenAlexW2124964349MaRDI QIDQ3070385
Davood Momeni, Mohammad R. Setare
Publication date: 3 February 2011
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0911.1877
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 (9)
Horava-Lifshitz cosmology and quark-hadron phase transition ⋮ Killing and Noether symmetries of plane symmetric spacetime ⋮ A slowly rotating black hole in Horava-Lifshitz gravity and a 3+1 dimensional topological black hole: motion of particles and BSW mechanism ⋮ Caustic singularity in Hořava-Lifshitz gravity ⋮ Cosmic strings in a model of non-relativistic gravity ⋮ Global dynamics of the Hořava-Lifshitz cosmological system ⋮ SPACING OF THE ENTROPY SPECTRUM FOR KS BLACK HOLE IN HOŘAVA–LIFSHITZ GRAVITY ⋮ Singularities of the Casimir energy for quantum field theories with Lifshitz dimensions ⋮ PLANAR SYMMETRY IN f(T) GRAVITY
Cites Work
- Hořava-Lifshitz cosmology
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- Non-static non-conformally flat fluid plates of embedding class one
- Plane symmetric self-gravitating fluids with pressure equal to energy density
- Isentropic Hydrodynamics in Plane Symmetric Space-Times
- The renormalizability of Hořava–Lifshitz-type gravities
- Hořava–Lifshitz holography
- Perturbative instabilities in Hořava gravity
- TIMELIKE GEODESIC MOTION IN HORAVA–LIFSHITZ SPACE–TIME
- A note on plane-symmetric static perfect-fluid spacetimes
- A static cylindrically symmetric solution for perfect fluid in general relativity
- Homothetic perfect fluid spacetimes
- Conformal symmetry inheritance with cosmological constant
- The kinematical role of automorphisms in the orthonormal frame approach to Bianchi cosmology
- A class of self-similar perfect-fluid spacetimes, and a generalisation
- Empty space-times admitting a three parameter group of motions
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