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 analyzing 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  eV by excluding the ones with decay constants ranging from 1.6×1016 to 1018  GeV at a 3⁢𝜎 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.

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Metadaten
Author:Jun ZhangORCiD, Zhenwei LyuORCiD, Junwu HuangORCiD, Matthew C. Johnson, Laura SagunskiORCiDGND, Mairi SakellariadouORCiD, Huan YangORCiD
URN:urn:nbn:de:hebis:30:3-868615
DOI:https://doi.org/10.1103/PhysRevLett.127.161101
ISSN:1079-7114
ISSN:0031-9007
ArXiv Id:http://arxiv.org/abs/2105.13963
Parent Title (English):Physical review letters
Publisher:American Physical Society
Place of publication:College Park, Md.
Document Type:Article
Language:English
Date of Publication (online):2021/10/11
Date of first Publication:2021/10/11
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2024/09/02
Volume:127
Issue:16, 161101
Article Number:161101
Page Number:6
Institutes:Physik / Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - CC BY - Namensnennung 4.0 International