Angular momentum transfer to a star by gravitational waves

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dc.creatorKhosroshahi, H. G.
dc.creatorSobouti, Y.
dc.date1998-06-07
dc.date.accessioned2026-07-07T02:27:08Z
dc.date.available2026-07-07T02:27:08Z
dc.descriptionInteraction of a stochastic background of gravitational radiation with celestial systems changes their dynamical elements in a random manner and give rise to secular changes in time. In this spirit we study the angular momentum transfer from a random background of radiation either to a rotating star or to an oscillating one. The angular momentum transferred to such objects by a continuous plane wave is proportional to time, $t$, and by an stochastic background is proportional to $t^{1/2}$.
dc.description5 Pages, Presented in GR15
dc.identifierhttps://arxiv.org/abs/astro-ph/9806102
dc.identifierhttp://arxiv.org/abs/astro-ph/9806102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12562
dc.subjectAstrophysics
dc.titleAngular momentum transfer to a star by gravitational waves
dc.typetext

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