Can an evolving Universe host a static event horizon?
arXiv:1210.0753 · doi:10.1103/PhysRevD.86.104061
Abstract
We prove the existence of general relativistic perfect fluid black hole solutions, and demonstrate the phenomenon for the class of equations of state. While admitting a local time-like Killing vector on the event horizon itself, the various black hole configurations are necessarily time dependent (thereby avoiding a well known no-go theorem) away from the horizon. Consistently, Hawking's imaginary time periodicity is globally manifest on the entire spacetime manifold.
10 PRD pages, no figures; v.2: few typos corrected
References in corpus (15)
- General Laws of Black-Hole Dynamics
- Inhomogeneous cosmological models: exact solutions and their applications
- Influence of global cosmological expansion on local dynamics and kinematics
- McVittie's Legacy: Black Holes in an Expanding Universe
- A point mass in an isotropic universe. Existence, uniqueness and basic properties
- Does the mass of a black hole decrease due to the accretion of phantom energy
- More on McVittie's Legacy: A Schwarzschild - de Sitter black and white hole embedded in an asymptotically CDM cosmology
- The effect of a massive object on an expanding universe
- A point mass in an isotropic universe: III. The region
- The effect of an expanding universe on massive objects
- What is the fate of a black hole embedded in an expanding universe?
- Black Holes in the Universe: Generalized Lemaitre-Tolman-Bondi Solutions
- Black Hole in the Expanding Universe from Intersecting Branes
- The spacetime in the neighborhood of a general isolated black hole
- Black Hole in the Expanding Universe with Arbitrary Power-Law Expansion
Cited by in corpus (5)
- Searching for dynamical black holes in various theories of gravity
- Black hole event horizons are cosmologically coupled
- D-bound and Bekenstein bound for McVittie solution surrounded by dark energy cosmological fields
- Black Hole solutions in a cosmological spacetime background
- The Atmosphere of a Black Hole