Conversion of gravitational waves into electromagnetic waves in a Bianchi type I universe with a uniform magnetic field — Cosmological implications

1988 ◽  
Vol 64 (4) ◽  
pp. 327-338
Author(s):  
D. Boccaletti ◽  
W. Agostini
1981 ◽  
Vol 24 (2) ◽  
pp. 305-319 ◽  
Author(s):  
Augusto Sagnotti ◽  
Barton Zwiebach

2019 ◽  
Vol 34 (03n04) ◽  
pp. 1950011 ◽  
Author(s):  
C. Aktaş

In this study, we obtain Einstein, Bergmann–Thomson (BT), Landau–Lifshitz (LL), Møller, Papapetrou (PP) and Tolman energy–momentum (EM) distributions for Ruban universe model in general relativity (GR) and teleparallel gravity (TG). We obtain same results for Einstein, Bergmann–Thomson and Landau–Lifshitz energy–momentum distributions in GR and TG. Also, we get same results for Einstein and Tolman energy–momentum distributions in GR. The Møller energy–momentum results are different in GR and TG. Also, using Ruban universe model, we obtain LRS Bianchi type I solutions and we get zero energy–momentum results for this universe model in GR and TG. These results of LRS Bianchi type I universe model agree with Aygün et al., Taşer et al., Doğru et al., Banerjee–Sen, Tryon and Xulu in different gravitation theories.


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