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33744712162
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note
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Notation: ";" denotes covariant derivative in curved spacetime, "," derivative in flat spacetime, Greek indices go from 0 to 3, and Latin indices, from 1 to 3.
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26
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0042408414
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A.M. Volkov, A.A. Izmest'ev, and G.V. Skrotskii, Zh. Eksp. Teor. Fiz. 59, 1254 (1970) [Sov. Phys. JETP 32, 686 (1971)].
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0001471901
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A.M. Volkov, A.A. Izmest'ev, and G.V. Skrotskii, Zh. Eksp. Teor. Fiz. 59, 1254 (1970) [Sov. Phys. JETP 32, 686 (1971)].
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28
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33744701232
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note
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In the more general case of stationary spacetimes, G + (Combining right arrow above sign)≠0, and the constituitive relations will be more complicated.
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31
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This is not true in cases in which the source of the gravitational field is a rotating body. See B. Mashhoon, Phys. Rev. D 11, 2679 (1975).
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33744687994
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B. Mashhoon [29]
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B. Mashhoon [29].
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