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Constraining the p-Mode-g-Mode Tidal Instability with GW170817

Citation

Abbott, BP and Abbott, R and Siellez, K and Zweizig, J, LIGO Scientific Collaboration and Virgo Collaboration, Constraining the p-Mode-g-Mode Tidal Instability with GW170817, Physical Review Letters, 122, (6) Article 061104. ISSN 0031-9007 (2019) [Refereed Article]


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Copyright Statement

© 2019 American Physical Society. This is an open-access article distributed under the terms of the Creative Commons Attribution 4.0 International (CC BY 4.0) License (https://creativecommons.org/licenses/by/4.0/). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. Must link to published article.

DOI: doi:10.1103/PhysRevLett.122.061104

Abstract

We analyze the impact of a proposed tidal instability coupling p modes and g modes within neutron stars on GW170817. This nonresonant instability transfers energy from the orbit of the binary to internal modes of the stars, accelerating the gravitational-wave driven inspiral.

Item Details

Item Type:Refereed Article
Keywords:p-mode, g-mode, tidal instability, neutron stars, gravitational waves
Research Division:Physical Sciences
Research Group:Astronomical sciences
Research Field:General relativity and gravitational waves
Objective Division:Expanding Knowledge
Objective Group:Expanding knowledge
Objective Field:Expanding knowledge in the physical sciences
UTAS Author:Siellez, K (Dr Karelle Siellez)
ID Code:151945
Year Published:2019
Web of Science® Times Cited:28
Deposited By:Physics
Deposited On:2022-08-09
Last Modified:2022-09-27
Downloads:0

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