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https://doi.org/10.3938/NPSM.70.97
Gravitational Waves and Measurability of Neutron Star Tidal Deformability
New Phys.: Sae Mulli 2020; 70: 97~102
Published online January 31, 2020;  https://doi.org/10.3938/NPSM.70.97
© 2020 New Physics: Sae Mulli.

Yong-Beom CHOI, Hee-Suk CHO1, Chang-Hwan LEE1*, Young-Min KIM2

1Department of Physics, Pusan National University, Busan 46241, Korea
2Department of Physics, Ulsan National Institute of Science and Technologh (UNIST), Ulsan 44919, Korea
Correspondence to: clee@pusan.ac.kr
Received October 5, 2019; Revised November 29, 2018; Accepted December 2, 2019.
cc This is an open-access article distributed under the terms of the Creative Commons Attribution Non-Commercial License (http://creativecommons.org/licenses/by-nc/3.0/) which permits unrestricted non-commercial use, distribution, and reproduction in any medium, provided the original work is properly cited.
Abstract
Gravitational waves from the binary black hole merger GW150914 were detected in 2015. In addition, gravitational waves from the binary neutron star merger GW170817 were detected in 2017, followed by electromagnetic observations at various wavelengths from gamma-ray to radio wavelengths. These observations opened a new era of multi-messenger astronomy and astrophysics. Due to the short distance to the source, the tidal deformability of neutron stars, which contains information on their inner structure, has been estimated for GW170817. In this work, we discuss the possibilities of using gravitational waves to measure the tidal deformability of neutron stars.
PACS numbers: 04.25.Nx, 04.30.Tv, 26.60.Kp
Keywords: Gravitational waves, Neutron stars, Tidal deformabilit


January 2020, 70 (1)
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