Author

Han, Ming-Zhe

INSPIRE profile1800688 ORCID0000-0001-9034-0866

4 papers·331 citations in this corpus

	Paper	Category
Apr 14, 2025#62504.08514	Dependence of postmerger properties on the thermal heating efficiency in neutron star mergers Ming-Zhe Han🇩🇪 · Yong Gao🇩🇪 · Kenta Kiuchi🇩🇪 · Masaru Shibata🇩🇪	↳ astro-ph.HE	PRD	6
Nov 27, 2023#122311.13805	Mass and radius of the most massive neutron star: The probe of the equation of state and perturbative QCD Shao-Peng Tang🇨🇳 · Ming-Zhe Han🇨🇳 · Yong-Jia Huang🇨🇳 · Yi-Zhong Fan🇨🇳 · Da-Ming Wei🇨🇳	↳ astro-ph.HE	PRD	8
Sep 25, 2023#82309.12644	Maximum gravitational mass $M_{TOV} = 2.2 5_{- 0.07}^{+ 0.08} M_{⊙}$ inferred at about $3%$ precision with multimessenger data of neutron stars Yi-Zhong Fan🇨🇳 · Ming-Zhe Han🇨🇳 · Jin-Liang Jiang🇩🇪 · Dong-Sheng Shao🇨🇳 · Shao-Peng Tang🇨🇳	↳ astro-ph.HE	PRD	101
Jun 9, 2021#32106.04204	Constraints on the phase transition and nuclear symmetry parameters from PSR $J 0740 + 6620$ and multimessenger data of other neutron stars Shao-Peng Tang🇨🇳 · Jin-Liang Jiang🇨🇳 · Ming-Zhe Han🇨🇳 · Yi-Zhong Fan🇨🇳 · Da-Ming Wei🇨🇳	nucl-th	PRD	41

Dependence of postmerger properties on the thermal heating efficiency in neutron star mergers
Ming-Zhe Han🇩🇪 · Yong Gao🇩🇪 · Kenta Kiuchi🇩🇪 · Masaru Shibata🇩🇪
Apr 14, 2025#6↳ astro-ph.HEPRD6 citations
Mass and radius of the most massive neutron star: The probe of the equation of state and perturbative QCD
Shao-Peng Tang🇨🇳 · Ming-Zhe Han🇨🇳 · Yong-Jia Huang🇨🇳 · Yi-Zhong Fan🇨🇳 · Da-Ming Wei🇨🇳
Nov 27, 2023#12↳ astro-ph.HEPRD8 citations
Maximum gravitational mass $M_{TOV} = 2.2 5_{- 0.07}^{+ 0.08} M_{⊙}$ inferred at about $3%$ precision with multimessenger data of neutron stars
Yi-Zhong Fan🇨🇳 · Ming-Zhe Han🇨🇳 · Jin-Liang Jiang🇩🇪 · Dong-Sheng Shao🇨🇳 · Shao-Peng Tang🇨🇳
Sep 25, 2023#8↳ astro-ph.HEPRD101 citations
Constraints on the phase transition and nuclear symmetry parameters from PSR $J 0740 + 6620$ and multimessenger data of other neutron stars
Shao-Peng Tang🇨🇳 · Jin-Liang Jiang🇨🇳 · Ming-Zhe Han🇨🇳 · Yi-Zhong Fan🇨🇳 · Da-Ming Wei🇨🇳
Jun 9, 2021#3nucl-thPRD41 citations

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Han, Ming-Zhe

Dependence of postmerger properties on the thermal heating efficiency in neutron star mergers

Mass and radius of the most massive neutron star: The probe of the equation of state and perturbative QCD

Maximum gravitational mass MTOV​=2.25−0.07+0.08​M⊙​ inferred at about 3% precision with multimessenger data of neutron stars

Constraints on the phase transition and nuclear symmetry parameters from PSR J0740+6620 and multimessenger data of other neutron stars

Maximum gravitational mass $M_{TOV} = 2.2 5_{- 0.07}^{+ 0.08} M_{⊙}$ inferred at about $3%$ precision with multimessenger data of neutron stars

Constraints on the phase transition and nuclear symmetry parameters from PSR $J 0740 + 6620$ and multimessenger data of other neutron stars