Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/123630
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Type: Journal article
Title: Roles of crust and core in the tidal deformability of neutron stars
Author: Kalaitzis, A.M.
Motta, T.F.
Thomas, A.W.
Citation: International Journal of Modern Physics E: nuclear physics, 2019; 28(9):1950081-1-1950081-8
Publisher: World Scientific Publising Co.
Issue Date: 2019
ISSN: 0218-3013
1793-6608
Statement of
Responsibility: 
A.M. Kalaitzis, T.F. Motta and A.W. Thomas
Abstract: With the recent measurement of GW170817 providing constraints on the tidal deformability (TD) of a neutron star, it is very important to understand what features of the equation of state (EoS) have the biggest effect on it. We therefore study the contribution of the crust to the TD and the moment of inertia (MoI) of a neutron star for a variety of well-known EoS. It is found that the contributions to these quantities from the low-density crust are typically quite small and as a result the determination of the TD provides an important constraint on the EoS of dense matter.
Keywords: Neutron stars; gravitational waves; equation of state
Rights: © The Author(s). This is an Open Access article published by World Scientific Publishing Company. It is distributed under the terms of the Creative Commons Attribution 4.0 (CC BY) License which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
DOI: 10.1142/S0218301319500812
Grant ID: http://purl.org/au-research/grants/arc/DP150103101
http://purl.org/au-research/grants/arc/DP180100497
Published version: http://dx.doi.org/10.1142/S0218301319500812
Appears in Collections:Aurora harvest 4
Physics publications

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