Hostname: page-component-77c89778f8-vpsfw Total loading time: 0 Render date: 2024-07-19T07:16:49.454Z Has data issue: false hasContentIssue false

A Class of Solutions of Einstein-Maxwell Equations with the Cosmological Constant

Published online by Cambridge University Press:  07 February 2017

J. F. Plebański*
Affiliation:
The Institute of Theoretical Physics of the University of Warsaw, Hozdot;a 69, Warsaw, Poland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Working in the signature (+ + + -) and units such that G = 1 = c, it was found a solution of Einstein-Maxwell equations with λ (without current and pseudo-current). In real coordinates xμ=(p, σ, q, τ) the solutions is: (1)(2) where (3) is pure imaginary; in (1) ‘d’ denotes the external differential]. Not all constants m0, n0, e0, g0, b, ∊, λ are physically significant: by re-scaling coordinates ∊ can be made equal to +1,0, or −1. The solution is of the type D: the double Debever-Penrose vectors (4) have the common complex expansion Z = (q + ip)-1. Among C(a)'s only C(3) given by: (5) is in general ≠0. The invariants of the electromagnetic field are: (6)

Type
Part III: Accretion of Matter and X-Ray Sources
Copyright
Copyright © Reidel 1974