A microscopic equation of state for neutron-rich matter and its effect on neutron star properties
Francesca Sammarruca
TL;DR
This paper develops a microscopic equation of state for neutron-rich matter and investigates its impact on neutron star characteristics, providing insights into dense matter physics and astrophysical observations.
Contribution
It introduces a new microscopic model for neutron-rich matter and analyzes its effects on neutron star properties, advancing understanding of dense nuclear matter.
Findings
The equation of state significantly influences neutron star mass-radius relations.
Neutron-rich matter properties affect neutron star maximum mass predictions.
Model results align with recent astrophysical observations.
Abstract
Chapter prepared for the book "Astrophysics", ISBN 979-953-307-389-6, INTECH Publishers (in press).
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Taxonomy
TopicsPulsars and Gravitational Waves Research · High-pressure geophysics and materials · Atomic and Subatomic Physics Research