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Автор Rafael A. Porto
Автор Andreas Ross
Автор Ira Z. Rothstein
Дата выпуска 2011-03-01
dc.description Using effective field theory techniques we calculate the source multipole moments needed to obtain the spin contributions to the power radiated in gravitational waves from inspiralling compact binaries to third Post-Newtonian order (3PN). The multipoles depend linearly and quadratically on the spins and include both spin(1)spin(2) and spin(1)spin(1) components. The results in this paper provide the last missing ingredient required to determine the phase evolution to 3PN including all spin effects which we will report in a separate paper.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order
Тип paper
DOI 10.1088/1475-7516/2011/03/009
Electronic ISSN 1475-7516
Журнал Journal of Cosmology and Astroparticle Physics
Том 2011
Первая страница 9
Последняя страница 009
Выпуск 03

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