Problems in the General Theory of Relativity and Theory of Group Representations 1979
DOI: 10.1007/978-1-4684-0676-4_4
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The Newman-Penrose Method in the Theory of General Relativity

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Cited by 20 publications
(35 citation statements)
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“…x is a function of time x ≡ x(t), are denoted as Multiple time derivative from function F (t, x) is denoted by 21) so that its action on the time integrals eliminates integration in the sense that 22) and…”
Section: Notations and Conventionsmentioning
confidence: 99%
See 1 more Smart Citation
“…x is a function of time x ≡ x(t), are denoted as Multiple time derivative from function F (t, x) is denoted by 21) so that its action on the time integrals eliminates integration in the sense that 22) and…”
Section: Notations and Conventionsmentioning
confidence: 99%
“…At each point of space-time we introduce a complex null tetrad (l α , n α , m α , m α ) associated with a congruence of light rays [20,21]. It is obvious that such field of complex null tetrads is not uniquely determined by the congruence of null rays and the normalization conditions.…”
Section: Equations For Propagation Of Polarization Propertiesmentioning
confidence: 99%
“…The eikonal Eq. (3.8) is a direct consequence of Maxwell's equations [3,26,31] and its solution describes a wave front of an electromagnetic wave propagating in curved space-time defined by the metric tensor in Eqs. (2.1), (2.5).…”
Section: The Speed Of Gravity and The Newtonian Limitmentioning
confidence: 99%
“…(3.8) is not related to the specific properties of the electromagnetic field, but is completely determined by the structure of space-time, or, more accurately, its geometry defined by Eqs. (2.1), (2.5) [26].…”
Section: The Speed Of Gravity and The Newtonian Limitmentioning
confidence: 99%
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