Rafael Bán Jacobsen, Verônica Dexheimer, Ricardo Luciano Sonego Farias
Published 2023-01-30Version 1
This conference proceeding presents an overview of the modern approaches in the study of baryonic matter at high densities, focusing on the use of online repositories such as CompOSE and MUSES for the calculation of neutron star properties. In this context, relevant astrophysical constraints for the equations of state (mass-radius relation, speed of sound, tidal deformability) are discussed.
Comments: 4 pages. 4 figures. Conference proceeding of the "International Workshop on Astronomy and Relativistic Astrophysics - IWARA 2022"
Role of the crust on the tidal deformability of a neutron star within a unified treatment of dense matter
Significance of lower energy density region of neutron star and universalities among neutron star properties
Tidal Deformability as a Probe of Dark Matter in Neutron Stars
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