Properties of nuclear pastas
Jorge A. Lopez, Claudio O. Dorso, Guillermo A. Frank
TL;DR
This review explores the formation and properties of nuclear pasta phases in neutron star cores, analyzing their structure in nuclear matter, the influence of electron gas, and their behavior in neutron star environments.
Contribution
It provides a comprehensive overview of nuclear pasta properties, including the effects of electron gas and the conditions in neutron star matter, which advances understanding of dense matter phases.
Findings
Nuclear pasta phases are influenced by the presence of an electron gas.
Different pasta structures form under varying neutron star conditions.
The study highlights the importance of nuclear interactions in pasta formation.
Abstract
In this Review we study the nuclear pastas as they are expected to be formed in neutron star cores. We start with a study of the pastas formed in nuclear matter (composed of protons and neutrons), we follow with the role of the electron gas on the formation of pastas, and we then investigate the pastas in neutron star matter (nuclear matter embedded in an electron gas).
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