Saravani, M. (2013). Dynamical Emergence of Universal Horizons during the formation of Black Holes . Perimeter Institute for Theoretical Physics. https://pirsa.org/13110087
MLA
Saravani, Mehdi. Dynamical Emergence of Universal Horizons during the formation of Black Holes . Perimeter Institute for Theoretical Physics, Nov. 07, 2013, https://pirsa.org/13110087
BibTex
@misc{ scivideos_PIRSA:13110087,
doi = {10.48660/13110087},
url = {https://pirsa.org/13110087},
author = {Saravani, Mehdi},
keywords = {Strong Gravity},
language = {en},
title = {Dynamical Emergence of Universal Horizons during the formation of Black Holes },
publisher = {Perimeter Institute for Theoretical Physics},
year = {2013},
month = {nov},
note = {PIRSA:13110087 see, \url{https://scivideos.org/index.php/pirsa/13110087}}
}
In many theories with fundamental preferred frame, such as Einstein-Aether or Gravitational Aether theories, K-essence, Cuscuton theory, Shape Dynamics, or (non-projectable) Horava-Lifshitz gravity, the low energy theory contains a fluid with superluminal or incompressible excitations. In this talk, I study the formation of black holes in the presence of such a fluid. In particular, I focus on the incompressible limit of the fluid (or Constant Mean Curvature foliation) in the space-time of a spherically collapsing shell within an asymptotically cosmological space-time. In this case, I show that an observer inside 3/4 of the Schwarzschild radius cannot send a signal outside, after a stage in collapse, even using signals that propagate infinitely fast in the preferred frame. This confirms the dynamical emergence of universal horizons that have been previously found in static solutions [arXiv:1110.2195, arXiv:1104.2889, arXiv:1212.1334].
