Hybrid stars with sequential phase transitions: the emergence of the g2 mode

DOI10.1088/1475-7516/2021/02/009zbMath1484.85025arXiv2009.03769OpenAlexW3083990801MaRDI QIDQ5027424

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Publication date: 4 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2009.03769

zbMATH Keywords

neutron starsgravitational waves/theory

Mathematics Subject Classification ID

Nuclear physics (81V35) Strong interaction, including quantum chromodynamics (81V05) Phase transitions (general) in equilibrium statistical mechanics (82B26) Galactic and stellar structure (85A15) Gravitational waves (83C35)

Related Items (1)

Non-radial oscillation modes in hybrid stars: consequences of a mixed phase

Cites Work

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• Two lectures on color superconductivity
• Discriminating hadronic and quark stars through gravitational waves of fluid pulsation modes
• Relativistic stellar pulsations in the Cowling approximation
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• On Massive Neutron Cores
• Theory of Superconductivity
• Quasi-normal modes of stars and black holes

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