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Testing general relativity using gravitational waves from binary neutron stars: Effect of spins

2013/05/13 by M. Agathos, Michalis Agathos, Walter Del Pozzo +13
Computer Science · Earth and Planetary Sciences · Physics and Astronomy · #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Geophysics and Gravity Measurements #Pulsars and Gravitational Waves Research #Seismology and Earthquake Studies #gr-qc

paper · pdf · doi:10.48550/arxiv.1305.2963

3 pages, 1 figure, submitted to Proceedings of the 13th Marcel Grossmann Meeting (MG13), Stockholm, Sweden, 1-7 July 2012

openalex publication_date 2013/05/13 · arxiv created 2013/08/05 · arxiv updated 2013/08/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We present a Bayesian data analysis pipeline for testing GR using gravitational wave signals from coalescing compact binaries, and in particular binary neutron stars. In this study, we investigate its performance when sources with spins are taken into account.

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