First Constraints on Nuclear Coupling of Axionlike Particles from the Binary Neutron Star Gravitational Wave Event GW170817
Light axion fields, if they exist, can be sourced by neutron stars due to their coupling to nuclear matter, and play a role in binary neutron star mergers. We report on a search for such axions by analysing the gravitational waves from the binary neutron star inspiral GW170817. We find no evidence o...
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creator | Zhang, Jun Lyu, Zhenwei Huang, Junwu Johnson, Matthew C Sagunski, Laura Sakellariadou, Mairi Yang, Huan |
description | Light axion fields, if they exist, can be sourced by neutron stars due to their coupling to nuclear matter, and play a role in binary neutron star mergers. We report on a search for such axions by analysing the gravitational waves from the binary neutron star inspiral GW170817. We find no evidence of axions in the sampled parameter space. The null result allows us to impose constraints on axions with masses below \(10^{-11} {\rm eV}\) by excluding the ones with decay constants ranging from \(1.6\times10^{16} {\rm GeV}\) to \(10^{18} {\rm GeV}\) at \(3\sigma\) confidence level. Our analysis provides the first constraints on axions from neutron star inspirals, and rules out a large region in parameter space that has not been probed by the existing experiments. |
doi_str_mv | 10.48550/arxiv.2105.13963 |
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We report on a search for such axions by analysing the gravitational waves from the binary neutron star inspiral GW170817. We find no evidence of axions in the sampled parameter space. The null result allows us to impose constraints on axions with masses below \(10^{-11} {\rm eV}\) by excluding the ones with decay constants ranging from \(1.6\times10^{16} {\rm GeV}\) to \(10^{18} {\rm GeV}\) at \(3\sigma\) confidence level. 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subjects | Binary stars Confidence intervals Decay rate Gravitational waves Neutron stars Neutrons Nuclear matter Parameters Physics - General Relativity and Quantum Cosmology Physics - High Energy Astrophysical Phenomena Physics - High Energy Physics - Phenomenology Physics - High Energy Physics - Theory |
title | First Constraints on Nuclear Coupling of Axionlike Particles from the Binary Neutron Star Gravitational Wave Event GW170817 |
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