Angular Momentum Loss and Gravitational wave amplitudes for X-ray Binaries with a Neutron Star Component

2016/03/12 by T. İçli, İçli, T., K. Yakut +1
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Pulsars and Gravitational Waves Research #Solar and Stellar Astrophysics (astro-ph.SR) #astro-ph.HE #astro-ph.SR

paper · pdf · doi:10.48550/arxiv.1603.03905

4 pages, 3 figures. Proceedings 28th Texas Symposium on Relativistic Astrophysics, Geneva (Switzerland), 13-18 December 2015

arxiv created 2016/03/12 · openalex publication_date 2016/03/12 · arxiv updated 2016/03/15 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Binary systems with neutron stars and double degenerate systems are crucial objects to test current stellar evolution models and Einstein's general relativity. In this study, we present angular momentum loss mechanism via gravitational radiation and magnetized stellar winds for some selected systems with a neutron star. We calculated and plotted their time scales for angular momentum loss. Gravitational wave amplitudes of binary systems with a neutron star components are also estimated and their detectability with a gravitational wave detector (LISA) has been plotted.

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