Charged perfect fluids in the presence of a cosmological constant
arXiv:1010.1367 · doi:10.1007/s10714-011-1223-5
Abstract
We consider the static and spherically symmetric field equations of general relativity for charged perfect fluid spheres in the presence of a cosmological constant. Following work by Florides (1983) we find new exact solutions of the field equations, and discuss their mass radius ratios. These solutions, for instance, require the charged Nariai metric to be the vacuum part of the spacetime. We also find charged generalizations of the Einstein static universe and speculate that the smallness problem of the cosmological constant might become less problematic if charge is taken into account.
14 pages, 2 figures; revised version, one subsection removed, minor changes throughout the text
References in corpus (3)
Cited by in corpus (4)
- Bounds on M/R for Charged Objects with positive Cosmological constant
- An exact static two-mass solution using Nariai spacetime
- The Tolman VII Space-time in the Presence of a Charge and a Cosmological Constant
- Static Charged Polytropic Spheres with a Cosmological Constant: Physical Acceptability and Trapped Orbits