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| Neutron star and quark star: What is the matter state at exceedingly high density |
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Seminar Title |
Neutron star and quark star: What is the matter state at exceedingly high density |
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| Speaker: |
Dr.LI Ang |
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Affiliation: |
(XMU) |
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| When |
Thursday morning, Oct. 24, 10:00 a.m. |
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Where: |
Room 212, Astronomy Building |
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Welcome to Attend |
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( PMO Academic Committee & Academic Circulating committee) |
| | Abstract: A long-standing, open problem in astrophysics, nuclear physics and particle physics is the equation of state (EOS) of dense matter. It is an exciting scientific issue in the physics of compact stars and in the observations at NICER, eXTP, HIAF, etc. Formerly the understanding of this issue relies on electromagnetic observations and heavy-ion experiments, multimessenger observations of neutron star mergers help advance this field of research. Constraints on EOS mainly come from theoretical many-body calculations, laboratory measurements of nuclear properties & reactions and observations in astronomy. I will give a short introduction on the calculations of EOS as well as present constraints. |
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Copyright？ Purple Mountain Observatory, CAS, No.10 Yuanhua Road, Qixia District, Nanjing 210023, China
Phone: 0086 25 8333 2000 Fax: 8333 2091 http://english.pmo.cas.cn |
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