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2020

Neutron star tidal deformability and equation of state constraints

Chatziioannou, Katerina

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Despite their long history and astrophysical importance, some of the key properties of neutron stars are still uncertain.

The extreme conditions encountered in their interiors, involving matter of uncertain composition at extreme density and isospin asymmetry, uniquely determine the stars' macroscopic properties within General Relativity.
Astrophysical constraints on those macroscopic properties, such as neutron star masses and radii, have long been used to understand the microscopic properties of the matter that forms them.
In this article we discuss another astrophysically observable macroscopic property of neutron stars that can be used to study their interiors: their tidal deformation.

Neutron star tidal deformability and equation of state constraints · Around

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