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Angular Momentum Loss by Gravitational Radiation
Phys. Rev. D 2, 2123 – Published 15 November, 1970
DOI: https://doi.org/10.1103/PhysRevD.2.2123
Abstract
The angular momentum flux from a confined gravitational radiator is calculated in the linear approximation using the Landau-Lifshitz energy-momentum pseudotensor. This flux can be written in a simple form involving a total angular momentum operator, in complete analogy with the electromagnetic result. A multipole expansion is used which allows the flux to be expressed for the first time to all multipole orders.
References (13)
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Omitted endnote
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Omitted endnote
Omitted endnote
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Omitted endnote
- Cooperstock and Booth ([3])