English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We examine the effects of spin-orbit and spin-spin coupling on the inspiralof a coalescing binary system of spinning compact objects and on thegravitational radiation emitted therefrom. Using a formalism developed byBlanchet, Damour, and Iyer, we calculate the contributions due to the spins ofthe bodies to the symmetric trace-free radiative multipole moments which areused to calculate the waveform, energy loss, and angular momentum loss from theinspiralling binary. Using equations of motion which include terms due tospin-orbit and spin-spin coupling, we evolve the orbit of a coalescing binaryand use the orbit to calculate the emitted gravitational waveform. We find thespins of the bodies affect the waveform in several ways: 1) The spin termscontribute to the orbital decay of the binary, and thus to the accumulatedphase of the gravitational waveform. 2) The spins cause the orbital plane toprecess, which changes the orientation of the orbital plane with respect to anobserver, thus causing the shape of the waveform to be modulated. 3) The spinscontribute directly to the amplitude of the waveform. We discuss the size andimportance of spin effects for the case of two coalescing neutron stars, andfor the case of a neutron star orbiting a rapidly rotating $10M_\odot$ blackhole.Comment: 60 pages, revtex 3.0, 16 figures available upon request, to appear in  Physical Review

physical review. d. particles, fields, gravitation, and cosmology/physical review. d. particles and fields

Coalescing binary systems of compact objects to (post<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn>5</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>-Newtonian order. V. Spin effects

Coalescing binary systems of compact objects to (post)5/2-Newtonian order. V. Spin effects