Antide Sittertype 2+1 spacetime of a charged rotating mass
Abstract
The exact charged rotating solution of 2+1 EinsteinMaxwell equations with $\Lambda$ term is obtained and its properties outlined. It generalizes the CataldoCruzdel CampoGarc{\'ı}a relativistic charged massive black hole on the 2+1 antide Sitter cosmological background. We show that rotating solutions correspond to inhomogeneous field equations, thus presence of sources in 2+1 Maxwell's equations cannot be identified with existence of a charge distribution. Instead, these sources are related to the 2+1 Machian 2form field, and the overall Lagrangian structure of the rotating system is reconstructed.
 Publication:

arXiv eprints
 Pub Date:
 January 2001
 arXiv:
 arXiv:grqc/0101029
 Bibcode:
 2001gr.qc.....1029M
 Keywords:

 General Relativity and Quantum Cosmology
 EPrint:
 9 pages, LaTeX file using amssym.def