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Effects of symmetry energy on the radius and tidal deformability of neutron stars in the relativistic mean-field model

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Publication:5156520
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DOI10.1093/ptep/ptaa016zbMath1477.85005arXiv2002.00562OpenAlexW3017320950MaRDI QIDQ5156520

Hong Shen, Shishao Bao, Ying Zhang, K. Sumiyoshi, Ken'Ichiro Nakazato, Jinniu Hu

Publication date: 18 October 2021

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

Full work available at URL: https://arxiv.org/abs/2002.00562


Mathematics Subject Classification ID

Nuclear physics (81V35) Gravitational energy and conservation laws; groups of motions (83C40) Galactic and stellar structure (85A15) Gravitational waves (83C35)


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Non-radial oscillation modes in hybrid stars: consequences of a mixed phase, Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter



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