According to general relativity, a binary consisting of spinning bodies will precess due to spin-orbit and spin-spin coupling. The corresponding modulation of its gravitational waves might be a serious problem for detecting such waves with simple post-Newtonian templates. A new family of templates that takes into account the complications arising from the orbital precession is proposed and its application and performance are discussed.
@article{bwmeta1.element.bwnjournal-article-bcpv41z2p19bwm, author = {Apostolatos, Theocharis}, title = {Gravitational waveforms from spinning objects}, journal = {Banach Center Publications}, volume = {38}, year = {1997}, pages = {19-22}, zbl = {0900.83007}, language = {en}, url = {http://dml.mathdoc.fr/item/bwmeta1.element.bwnjournal-article-bcpv41z2p19bwm} }
Apostolatos, Theocharis. Gravitational waveforms from spinning objects. Banach Center Publications, Tome 38 (1997) pp. 19-22. http://gdmltest.u-ga.fr/item/bwmeta1.element.bwnjournal-article-bcpv41z2p19bwm/
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