Ridges in rotating neutron-star properties due to first order phase transitions

DOI10.1016/J.AOP.2023.169487arXiv2307.15366MaRDI QIDQ6188442

Pablo Navarro Moreno, Felipe J. Llanes-Estrada, Eva Lope-Oter

Publication date: 7 February 2024

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2307.15366

zbMATH Keywords

phase transitioncompact starHartle-Thorne metriclight ringrotating neutron star

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Cites Work

• Keplerian frequency of uniformly rotating neutron stars and strange stars

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