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|Title:||Roles of crust and core in the tidal deformability of neutron stars|
|Citation:||International Journal of Modern Physics E, 2019; 28(9):1950081-1-1950081-8|
|Publisher:||World Scientific Publising Co.|
|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.|
|Appears in Collections:||Physics publications|
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