Einstein--Proca model: spherically symmetric solutions
arXiv:gr-qc/0004081 · doi:10.1002/(SICI)1521-3889(199909)8:6<497::AID-ANDP497>3.0.CO;2-5
Abstract
The Proca wave equation describes a classical massive spin 1 particle. We analyze the gravitational interaction of this vector field. In particular, the spherically symmetric solutions of the Einstein-Proca coupled system are obtained numerically. Although at infinity the metric field approaches the usual Schwarzschild (Reissner-Nordström) limit, we demonstrate the absence of black hole type configurations.
20 p., Revtex, 3 Postscript figures
Cited by in corpus (9)
- Proca Stars: gravitating Bose-Einstein condensates of massive spin 1 particles
- Bopp-Podolsky black holes and the no-hair theorem
- Geometric Proca with Matter in Metric-Palatini Gravity
- The Maxwell-Chern-Simons gravity and its cosmological implications
- A numeric solution for metric-affine gravity and Einstein's gravitational theory with Proca matter
- On the static solutions in gravity with massive scalar field in three dimensions
- Yukawa Black Holes from Interacting Vacuum
- Second order formalism in Poincare gauge theory
- On dynamic aspects of the Proca field screening by a black hole