TL;DR
This paper reviews how nuclear theory, especially effective Chiral models, helps understand the dense matter in neutron stars and links nuclear properties to star characteristics.
Contribution
It provides a comprehensive review connecting nuclear matter models with neutron star properties using effective Chiral theories.
Findings
Correlates nuclear saturation properties with neutron star characteristics
Highlights the role of vacuum properties in dense matter modeling
Discusses the equation of state derived from effective Chiral models
Abstract
Neutron stars are the most dense objects in the observable Universe and conventionally one uses nuclear theory to obtain the equation of state (EOS) of dense hadronic matter and the global properties of these stars. In this work, we review various aspects of nuclear matter within an effective Chiral model and interlink fundamental quantities both from nuclear saturation as well as vacuum properties and correlate it with the star properties.
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Taxonomy
TopicsAtomic and Subatomic Physics Research · Pulsars and Gravitational Waves Research · Astro and Planetary Science