个人简介
文德华，教授，博士生导师，广东省物理学会监事、广东省本科高校物理学类专业教学指导委员会副主任委员、教育部大学物理教指委中南地区工作委员副秘书长。主要从事核天体物理及致密物质物态的研究，特别是对中子星等致密天体的性质和结构有较深入的研究。在Phys. Rev. Lett.、Phys. Rev. C、 Phys. Rev. D等期刊上发表SCI论文70余篇。先后主持四项国家自然科学基金；两项广东省自然科学基金；一项教育部留学回国科研启动基金； 一项中国博士后科学基金；三项中央基本科研业务费资助项目。
已培养毕业10余名硕士、博士研究生。其中三位同学获得国家奖学金；一位同学获得威尼斯wnsr9778优秀博士论文奖励。
主讲公共基础课《大学物理》、全校通识课《天体与宇宙》、以及新生研讨课《宇宙的演化》。参与编写由邓文基教授等主编、中国高等教育出版社出版的教材《大学物理》。指导多名本科学生参加学生研究项目并发表SCI科研论文。多次获得威尼斯wnsr9778教学优秀奖和教学成果奖。主持多项教学研究项目，包括省级质量工程项目。
教育与工作经历
1995-1998 重庆大学，理论物理，硕士
2001-2004 中山大学，理论物理，博士
2005-2006 中山大学，博士后
2008-2009，2011及2018 美国德州农工大学(Commerce分校)，访问学者
代表性成果
1. S. Yang, D. H. Wen∗, Systematic correlation analysis between the nuclear matter parameters and neutron star properties within relativistic mean-field theory，Phys. Rev. D 107, 063009 (2023)
2. J. Wang, S. Yang, D. H. Wen*, Constraining properties of massive neutron star through R-mode, Eur. Phys. J. A, 58, 132 (2022)
3. S. Yang, D. H. Wen∗, J. Wang and J. Zhang, Exploring the universal relations with the correlation analysis of neutron star properties, Phys. Rev. D 105, 063023 (2022)
4. Y. X. Li, J. Wang, Z. H. Wu and D. H. Wen*, Inferring the gravitational binding energy and moment of inertia of PSR J0030 + 0451 and PSR J0740 + 6620 from new universal relations, Class. Quantum Grav. 39, 035014 (2022)
5.Y. X. Li, H. Y. Chen, D. H. Wen* and J. Zhang, Constraining the nuclear symmetry energy and properties of the neutron star from GW170817 by Bayesian analysis, Eur. Phys. J. A 57，31(2021)
6.W. J. Sun, D. H. Wen* and J. Wang, New quasi-universal relations for static and rapid rotating neutron stars, Phys. Rev. D 102, 023039 (2020)
7.R. R. Jiang, D. H. Wen* and H. Y. Chen, Universal behavior of compact star based upon gravitational binding energy, Phys. Rev. D 100, 123010 (2019).
8.B. A. Li, P. G. Krastev, D. H. Wen and N. B. Zhang, Towards understanding astrophysical effects of nuclear symmetry energy, Eur. Phys. J. A 55, 117 (2019)
9.D. H. Wen, B. A. Li, * H. Y. Chen and N. B. Zhang, GW170817 implications on the frequency and damping time of f -mode oscillations of neutron stars, Phys. Rev. C 99, 045806 (2019)
10.H. Y. Chen, D. H. Wen* and N. Zhang, Suitable resolution of EOS tables for neutron star investigations, Chin. Phys. C 43, 054108(2019)
11.N. Zhang, D. H. Wen* and H. Y. Chen，Imprint of the speed of sound in nuclear matter on global properties of neutron stars，Phys. Rev. C 99, 035803 (2019)
12.Y. M. Wen and D. H. Wen*, Theoretical constraints on the properties of low-mass neutron stars from the equation of state of nuclear matter in the inner crust, Phys. Rev. C 95, 065804 (2017)
13.Z. Z. Jing, D. H. Wen* and X. D. Zhang, Electrically charged: An effective mechanism for soft EOS supporting massive neutron star. Sci China-Phys Mech Astron, 58, 109501(2015)
14.D. H. Wen, W. G. Newton and B. A. Li *, Sensitivity of the neutron star r-mode instability window to the density dependence of nuclear symmetry energy, Phys. Rev. C 85, 025801(1-7) (2012)
15.D. H. Wen, B.A. Li and L. W. Chen, Supersoft Symmetry Energy Encountering Non-Newtonian Gravity in Neutron Stars, Phys. Rev. Lett 103, 211102 (2009)
16. D. H. Wen, B.A. Li and P.G. Krastev, Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron stars, Phys. Rev. C 80, 025801 (2009)
联系方式
电子邮箱：wendehua@scut.edu.cn
