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Oliveira, C. G.; Marcio do Amaral, C.

Spinor formalism in gravitation. (English) Zbl 0152.46003

Nuovo Cimento, X. Ser. A 47, 9-18 (1967).
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Cited in 2 Documents

Keywords:

classical field theory, relativity theory
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References:

[1] H. Weyl:Zeits. Phys.,56, 330 (1929). · doi:10.1007/BF01339504
[2] L. Infeld andB. L. van der Waerden:Sitzber. preuss. Akad. Wiss. Physik.-math. Kl.,9, 380 (1933).
[3] W. L. Bade andH. Jehle:Rev. Mod. Phys.,25, 714 (1953). · Zbl 0051.20705 · doi:10.1103/RevModPhys.25.714
[4] P. G. Bergmann:Phys. Rev.,107, 624 (1957). · Zbl 0078.19101 · doi:10.1103/PhysRev.107.624
[5] L. Witten: Phys. Rev.,113, 357 (1959). · Zbl 0083.42701 · doi:10.1103/PhysRev.113.357
[6] R. Penrose:Ann. of Phys.,10, 171 (1960). · Zbl 0091.21404 · doi:10.1016/0003-4916(60)90021-X
[7] C. G. Oliveira:Suppl. Nuovo Cimento,3, 192 (1965).
[8] R. Penrose: ARL 63-56, Technical Report, March 1963.
[9] We are defining the Ricci tensor byR {\(\beta\)}{\(\mu\)}=g {\(\alpha\)}{\(\lambda\)} R {\(\alpha\)}{\(\beta\)}{\(\lambda\)}{\(\mu\)}, which differs of the definition of ref. (4) by a sign.
[10] A. Komar andP. G. Bergmann:Phys. Rev. Lett.,4, 432 (1960). · doi:10.1103/PhysRevLett.4.432
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