​李增花
发布时间:2015-05-04   浏览次数:

姓名:李增花

职称:教授

联系电话:021-55664700

电子邮件:zhli09@fudan.edu.cn

工作经历

2005年毕业于中国科学院近代物理研究所粒子物理与原子核物理专业,获博士学位;2005年至2006年上海交通大学物理系博士后;2006年至2008年意大利INFN国家实验室Fellowship2009至今复旦大学现代物理研究所任教,历经讲师,副教授教授;硕士、博士生导师。

教学工作

本科生专业课:《核物理》;《理论物理()

研究领域

核物质状态方程与核天体物理,近年来代表性论文:

[1]J.Zhang,H.M.Liu,Z.H.Li,G.F.Burgio, H.-J.Schulze, Nuclear liquid-gas phase transition within a Brueckner-Hartree-Fock approach, Chin. Phys. C Vol.46, No. 11 (2022) 114105

[2]H.M.Liu, J.Zhang, Z.H.Li, J.B.Wei, G.F.Burgio, H.-J. Schulze, Microscopic nuclear equation of state at finite temperature and stellar stability, Phys. Rev. C106(2022)025801  

[3] F.Li, J.J.Lu, Z.H.Li, and C.Y. Chen, G.F.Burgio and H.-J.Schulze, Accurate nuclear symmetry energy at finite temperature within a Brueckner-Hartree-Fock approach, Phys. Rev. C103, 024307 (2021)

[4] A. Figura, Fan Li, J.J.Lu, G. F. Burgio, Z.H. Li, and H.-J.Schulze, Binary neutron star merger simulations with hot microscopic equations of state, Phys. Rev. D103,083012 (2021)

[5] A. Figura, J.J.Lu, G.F.Burgio, Z.H.Li, and H.J.Schulze, Hybrid equation of state approach in binary neutron-star merger simulations, Phys. Rev. D102 (2020) 043006

[6]J.B.Wei, J.J.Lu, G.F.Burgio, Z.H.Li, and H.J.Schulze, Are nuclear matter properties correlated to neutron star observables? (Topical Issue on "First joint gravitational wave and electromagnetic observations: Implications for nuclear and particle physics")Eur. Phys. J. A56(2020)63

[7]J.J.Lu, Z.H.Li, G.F.Burgio, A.Figura and H.J.Schulze, Hot neutron stars with microscopic equations of state, Phys. Rev. C100 (2019) 054335

[8]J.J.Lu, Z.H.Li, C.Y.Chen, M.Baldo and H.J.Schulze, Neutron matter in the hole-line expansion, Phys. Rev. C98 (2018) 064322

[9]J.J.Lu, Z.H.Li, C.Y.Chen, M.Baldo and H.J.Schulze, Convergence of the hole-line expansion with modern nucleon-nucleon potentials, Phys. Rev. C96 (2017) 044309Editors’ Suggestion

[10]Z.H.Li, H.J.Schulze, Correlation strength with modern nucleon-nucleon potentials in the Brueckner-Hartree-Fock approach. Phys .Rev. C94 (2016) 024322