Equations of State for Dense Matter and Astrophysical Constraints
Rafael B\'an Jacobsen, Ver\^onica Dexheimer, Ricardo Luciano Sonego, Farias
TL;DR
This paper reviews modern methods for modeling dense baryonic matter, emphasizing online repositories and astrophysical constraints to improve understanding of neutron star properties.
Contribution
It introduces the use of online repositories like CompOSE and MUSES for calculating neutron star properties and discusses relevant astrophysical constraints.
Findings
Use of online repositories enhances EOS calculations.
Astrophysical constraints inform dense matter models.
Improved understanding of neutron star mass-radius relations.
Abstract
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.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Astro and Planetary Science