On the Anisotropic Interior Solutions in Hořava Gravity and Einstein-æther Theory
arXiv:1706.06608 · doi:10.1209/0295-5075/121/30002
Abstract
We find a reconstruction algorithm able to generate all the static spherically symmetric interior solutions in the framework of Hořava gravity and Einstein-æther theory in presence of anisotropic fluids. We focus for simplicity on the case of a static æther finding a large class of possible viable interior star solutions which present a very rich phenomenology. We study one illustrative example in more detail.
v1: 5 pages, 1 figure; v2: 6 pages, 1 figure. Matches published version in EPL
References in corpus (8)
- Quantum Gravity at a Lifshitz Point
- Masses, Radii, and Equation of State of Neutron Stars
- Models of non-relativistic quantum gravity: the good, the bad and the healthy
- Black holes in Einstein-aether and Horava-Lifshitz gravity
- Slowly rotating black holes in Horava-Lifshitz gravity
- Cosmological constraints on deviations from Lorentz invariance in gravity and dark matter
- Quantization of the Horava theory at the kinetic-conformal point
- New Asymptotically Lifshitz Black Holes in Horava gravity
Cited by in corpus (8)
- Einstein-Klein-Gordon by gravitational decoupling
- A simple method to generate exact physically acceptable anisotropic solutions in general relativity
- Extended phase-space analysis of the Horava-Lifshitz cosmology
- Asymptotically flat vacuum solution in modified theory of Einstein's gravity
- Quark stars with isotropic matter in Hořava gravity and Einstein-æther theory
- Anisotropic fluid spheres in Hořava gravity and Einstein-æther theory with a non-static æther
- Relativistic polytropic equations of state in Hořava gravity and Einstein-æther theory
- Black hole solutions with a linear equation of state in Hořava gravity and Einstein--æther theory