Prog. Theor. Phys. Vol. 66 No. 4 (1981) pp. 1500-1503

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Letters

Axially Symmetric and Stationary Solution of New General Relativity

Department of Applied Mathematics, Faculty of Engineering Science, Osaka University, Toyonaka, Osaka 560
^*Institute of Physics, University of Tokyo, Komaba, Tokyo 153

(Received May 1, 1981)

Abstract:

In New General Relativity and axially symmetric and stationary gravitational field equation agrees with that of General Relativity with ω replaced by ω=(1+x/ λ)^1/2ω, provided the integrated orbital angular momentum L and the integrated spin angular momentum S are connected by L=(λ/x -1)S at spatial infinity. Here λ is a new parameter, which might agree with the Einstein constant x.

URL : http://ptp.ipap.jp/link?PTP/66/1500/
DOI : 10.1143/PTP.66.1500

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Citing Article(s) :

Progress of Theoretical Physics Vol. 71 No. 6 (1984) pp. 1213-1220 :
The Kasner Type Universe in New General Relativity

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Progress of Theoretical Physics Vol. 76 No. 4 (1986) pp. 938-944 :
Bianchi Type-I Universe in New General Relativity

Masayasu Fukui, Junnichi Masukawa and Shinsuke Ogino
Progress of Theoretical Physics Vol. 86 No. 3 (1991) pp. 659-670 :
A Kerr Metric Solution in New General Relativity

Naoki Toma
Progress of Theoretical Physics Vol. 87 No. 3 (1992) pp. 583-598 :
A Charged Kerr Metric Solution in New General Relativity

Toshiharu Kawai and Naoki Toma
Progress of Theoretical Physics Vol. 96 No. 2 (1996) pp. 347-375 :
A New Gravitational Energy-Momentum Pseudotensor in Tetrad Form

Hideharu Hirashima