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Hybrid Neutron Stars Based on a Modified PNJL Model

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Publication:3083715
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DOI10.1143/PTPS.186.81zbMath1213.85022arXiv1009.1181OpenAlexW3124251549MaRDI QIDQ3083715

Jens Berdermann, David B. Blaschke, Rafał Łastowiecki

Publication date: 23 March 2011

Published in: Progress of Theoretical Physics Supplement (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1009.1181



Mathematics Subject Classification ID

Strong interaction, including quantum chromodynamics (81V05) Magnetohydrodynamics and electrohydrodynamics (76W05) 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)


Related Items (1)

Relativistic neutron stars: rheological type extensions of the equations of state







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