A Charged Kerr Metric Solution in New General Relativity

Details A Charged Kerr Metric Solution in New General Relativity A Charged Kerr Metric Solution in New General Relativity

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pthph..87..583k&link_type=abstract

Progress of Theoretical Physics, Vol. 87, No. 3, pp. 583-598

Physics

24

Scientific paper

We give an exact solution of the gravitational and electromagnetic field equations with a charged rotating source in new general relativity. The solution has three parameters Q, h and a, and it gives a charged Kerr metric space-time. The parallel vector fields and the electromagnetic vector potential are axially symmetric. In this space-time, we cannot discriminate new general relativity from general relativity, so far as scalar, the Dirac and the Yang-Mills fields and macroscopic bodies are used as probes. The space-time does not have singularities at all, although it has an ``effective singularity''. Two kinds of Reissner-Nordström metric solutions, one is our solution with h = 0 and the other is a solution given by Hayashi and Shirafuji, are physically equivalent with each other. Nevertheless, these are markedly different from each other with regard to the asymptotic behavior of the torsion tensor for r -> infty and the space-time singularities.

Affiliated with

Also associated with

No associations

Rating

A Charged Kerr Metric Solution in New General Relativity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A Charged Kerr Metric Solution in New General Relativity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Charged Kerr Metric Solution in New General Relativity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1491209