教师主页移动版

更新日期：2019年5月9日 姓 名 文德华 性 别 男 出生年月 1972年5月 籍贯 四川仪陇县 民 族 汉族 政治面貌 中国共产党党员 最后学历 博士研究生 最后学位 理学博士 技术职称 教授 导师类别 博、硕导 行政职务 系主任 Email wendehua@scut.edu.cn 工作单位 物理学院 邮政编码 510640 通讯地址 广州市天河区华南理工大学18号楼 单位电话 02087113934 个人简介 文德华（Wen Dehua）：汉族，四川南充人。1995年毕业于四川师范大学物理系，获物理专业学士学位；1998年毕业于重庆大学物理系，获理论物理专业硕士学位；2004年毕业于中山大学物理系，获理论物理博士学位。2005年至2006年在中山大学数学系做博士后研究；2008年7月-2009年8月、2011年7-8月，2018年7月-10月先后三次在美国Texas A&M University-Commerce做访问学者；2010年在意大利的国际理论物理研究中心（ICTP）访问学习。1998年至今在华南理工大学物理系工作，2005年晋升为副教授，2011年晋升为教授，2012年被批准为博士生导师。至今指导硕士研究生11人，指导博士研究生4名。     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。同时还结合地面重离子碰撞试验对致密物质物态的约束研究了中子星振动模式的稳定性及其引力辐射。创造性地在中子星中引入了非牛顿引力机制，解决了软物态方程无法支撑大质量中子星的观测疑难，该工作得到了国际同行的高度关注和认可。在Phys. Rev. Lett.等期刊上发表SCI论文60篇。主持研究国家自然科学基金三项；主持华南理工大学中央高校基本科研业务费资助项目三项（包括面上、重点及滚动项目各一项），主持教育部留学回国科研启动基金一项；主持中国博士后科学基金一项。在《物理评论快报》（Physical Review Letters）上发表的科研论文《Supersoft Symmetry Energy Encountering Non-Newtonian Gravity in Neutron Stars》[[Phys. Rev.Lett., 103, 211102(2009)]是华南理工大学首次以第一作者、第一署名单位发表在该国际物理顶级刊物上的论文。该论文获得了广东省第二届南粤科技创新优秀学术论文二等奖。     长期担任《大学物理》课程，也承担了相关的教学研究课题，参与编写了由邓文基教授主编、高等教育出版社出版社出版的教材《大学物理》。指导多名学生参加SRP研究项目，其中一名学生发表了SCI论文，也因此获得了2011年度学生科技创新优秀指导教师一等奖。坚持每年指导本科生的毕业设计（论文），获得了华南理工大学本科毕业设计（论文）优秀指导教师奖。另外还多次获得华南理工大学教学优秀奖和教学成果奖。还开设了全校通识课《天体与宇宙》，新生研讨课《宇宙的演化》，研究生课程《天体物理导论》等课程。 社会、学会及学术兼职 广东省物理学会监事。 发表论文 1. 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)   2. H. Y. Chen, D. H. Wen* and N. Zhang，Suitable resolution of EOS tables for neutron star investigations, Chin. Phys. C 43, 054108(2019) 3. 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) 4. 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) 5. S. J. Cheng, G. C. Yong, and D. H. Wen， Effects of the symmetry energy in the 132Sn+124Sn reaction at 300 MeV/nucleon，Phys. Rev. C 94, 064621 (2016) 6. Z. Z. Jing and D. H. Wen, A New Solution in Understanding Massive White Dwarfs，CHIN. PHYS. LETT. 33, (2016) 050401 7. 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(2015)109501 8. H. L. Liu, G.C. Yong, and Wen D. H., Decomposition of the sensitivity of the symmetry energy observables，Phys. Rev. C 91, 044609 (2015) 9. H. L. Liu, G.C. Yong, and Wen D. H., Probing the momentum dependence of the symmetry potential by the free n/ p ratio of pre-equilibrium emission, Phys. Rev. C 91, 024604 (2015) 10. Wen D. H., H. L. Liu, X. D. Zhang, The mass limit of white dwarfs with strong magnetic fields in general relativity, Chin. Phys. B Vol. 23, No. 8 (2014) 089501 11. H. L. Liu, X. D. Zhang, and Wen D. H., One possible solution of peculiar type Ia supernovae explosions caused by a charged white dwarf，Phys. Rev.  D 89, 104043 (2014) 12. Zhou Y. and Wen D. H., Constraints on Non-Radial Oscillation Modes by Symmetry Energy Slope, Commun. Theor. Phys. 61 (2014) 469–474 13. Wen D. H. and zhou Y., Gravitational waves from the axial oscillation of neutron star considering non-Newtonian gravity, Nuclear Science and Techniques, 24 (2013) 040302 14. Wen D. H. and zhou Y., Effects of the symmetry energy slope on the axial oscillations of neutron stars, Chin. Phys. B, 22 (2013) 080401 15. Yan J. and Wen D. H.，R-mode Instability of Neutron Star with Non-Newtonian Gravity, Commun. Theor. Phys. 59 (2013) 47–52 16. Fu H.Y.,Wen D. H., Yan J., Properties of rapid rotating hybrid stars with non-Newtonian gravity, Acta Phys. Sin. 61 (2012) 209701 17. Wen D. H., Yan J. and Liu X.M., One possible mechanism for massive neutron star supported by soft EOS, International Journal of Modern Physics D, 21 (2012) 1250036 18. Wen D. H., Yan J. and Liu X.M., Gravitational waves from the axial perturbations of hyperon star, Chin. Phys. B, 21 (2012) 060402 19. Wen D. H., W. G. Newton and Li B. A., Sensitivity of the neutron star r-mode instability window to the density dependence of nuclear symmetry energy, Phys. Rev. C 85(2012)025801(1-7) 20. Wen D. H. Fu H. Y. and Chen W., Impact of neutron star crust on gravitational waves from the axial w-modes, Chin. Phys. B Vol. 20, No. 6 (2011) 060402 21. Huang Q.Z. and Wen D. H.，Impact of Crust Matter on Properties of Neutron Star with Supersoft Symmetry Energy，Commun. Theor. Phys. 55 (2011) 729–732 22. Wen D. H. and Chen W., Properties of hyperon stars rotating at Keplerian frequency, Chin. Phys. B, 20 (2011) 029701 23. Wen D. H., Equation of State in the σ-ω-ρ Model Supported by the Observational Data of 4U 1608-52 Neutron Star; Chin. Phys. Lett., 27 (2010) 010401(1-3)   24. Wen D. H., Li B.A. and Krastev P.G., Effects of the nuclear symmetry energy on gravitational waves from the axial w-modes of isolated neutron stars, Int. J. Mod. Phys. E, 19 (2010) 1712~1719 (International Journal of Modern Physics E) 25. Wen D. H., Li B.A. and Chen L. W., Supersoft Symmetry Energy Encountering Non-Newtonian Gravity in Neutron Stars, Phys. Rev. Lett 103, 211102 (2009) 26. Wen D. H., Li B.A. and Krastev P.G., Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron stars, Phys. Rev. C 80, 025801 (2009) 27. Wen D. H., Chen W.， Lu Y. G. and Liu L. G., Frame Dragging Effect on Moment of inertia and Radius of Gyration of Neutron Star, Mod. Phys. Lett. A, 2007(22), 631-636   28. Wen D. H., Chen W.，Lu Y. G. and Liu L. G., Properties of Neutron Stars Rotating at Kepler Frequency with Uniform Strong Magnetic Field, Chin. Phys. Lett. 2007(24), 628~631   29. Wen D. H., Chen W. and Liu L. G., Structure of Rotating Neutron Stars in Uniform Strong Magnetic Field, Commun. Theor. Phys. 2007(47), 653–657 30. Wen D. H., Hu J.X. and Liu L. G., Structural and Special Characters of Neutron Star in Relativistic   Model, Commun. Theor. Phys. 2006(45), 853~857 31. Wen D. H., Hu J.X., Chen W. and Liu L. G., Numerical Solution for the Energy Density of a Static Spherically Symmetric Gravitational Field, Chin. J. Phys. 2006(44), 263~273 32. Wen D. H., Chen W. and Liu L. G., Rotational Deformation of Neutron Star, Chin. Phys. Lett., 2005 (22), 1604~1607 33. Wen D. H., Chen W., Wang X.J., Ai B.Q., Liu G.T.，Dong D.Q. and Liu L.G., Structures of Rotating Traditional Neutron Stars and Hyperon Stars in the Relativistic sigma-omega Model，Eur. Phys. J. A., 2004(21), 349~354   34. Wen D. H., Chen W., Wang X.J., Ai B.Q., Liu G.T. and Liu L.G., Properties of Rotating Neutron Stars in the Relativistic sigma-omega Model, Commun. Theor. Phys., 2004(41), 51~54   35. Wen D. H., Chen W., Wang X.J., Ai B.Q., Liu G.T. and Liu L.G., Energy of Gravitational Field of Static Spherically Symmetric Neutron Stars, Commun. Theor. Phys., 2003 (40), 637~640   36. Wen D. H., Chen W., Wang X.J., Ai B.Q., Liu G.T. and Liu L.G., Energy of Gravitational Field of the Slowly Rotating Neutron Stars, Chin. J. Phys. 2003(41),595~600   37. Wen D. H., Li F. Y. and Liu L.G., energy-momentum psendo-tensor of cylindrical gravitational waves of both polarized states, Chin. Phys. Lett., 2002(19), 626~627   38. Guo Y.Y. Wen D. H., and Hu J.X., Frame Dragging Effect on Properties of Rotating Neutron Stars with Strong Magnetic Field, Commun. Theor. Phys. 50 (2008) 1469~1472 39. Chen W., B. J. Li, Wen D. H. and Liu L.G., 3P2 superfluidity in neutron star matter, PHYSICAL REVIEW C 77, 065804(1-6) (2008)   40. Chen W. Lam Y.Y., Wen D. H. and Liu L.G., Chin. Phys. Lett., 2006 (23), 271~274 41. Chen W, Wen DH, Liu LG, A study of the tachyon pole in the chiral sigma-omega model, Chin. J. Phys. 2005(43), 445-456 42. Chen W. Wen D. H. and Liu L.G., The softness of Nuclear Matter and the Production of Strange Particles in Neutron Stars, Chin. Phys. Lett., 2003 (20), 436~439   43. Chen W., Wen D. H.， Liu G.T., Wang X.J. and Liu L.G., Thermal dynamics of proton neutron star matter, Commun. Theor. Phys., 2003 (39), 317~322   44. Chen W., Wen D. H. and Liu L.G., The properties of neutron star in its evolution, Nuovo Cimento, 2003 (11),71~77   45. Chen W., Dong D. Q., Wen D. H., Liu G. T., Liu L. G., Equation of state of nuclear matter in chiral sigma-omega model, Commun. Theor. Phys., 2004,(41), 925~928 46. 董东桥，陈伟，文德华，刘良钢，手征模型中介子的质量与核物质结合能曲线关系的研究，高能物理与核物理，2003(27), 982~896   47. Dong D.Q., Chen W., Wen D. H., Liu L.G. and M. Nakano, Dispersion Relation of Sigma Meson and Pion at Finite Nuclear Density in Chiral Sigma Model, Commun. Theor. Phys., 2004 (41), 741-745 48. Li S. X., Hua B., Han G.Z. and Wen D.H., Mechanism and Estimation of Negative Entropy Flow in Terrestrial System, Prog. in Natural Sci., 2004(15), 185-188 49. Li Fang-yu, Tang Meng-xi and Wen De-hua, Coherent Resonance of a strong Electromagnetic Wave Beam to a Standing Gravitational Wave, Chin. Phys. Lett., 1999(16), 12~14   50. Ai B.Q., Chen W., Wang X.J., Liu G.T., Wen D. H. and Liu L.G., Noise in Genotype Selection Model, Commun. Theor. Phys. 2003(39), 765~768   51. Ai B.Q., Chen W., Wan X.J., Liu G.T., Wen D. H. and Liu L.G., Noise in Insect Outbreak Model, Chin. J. Phys. 2003(41), 422~429   52. Ai B.Q., Chen W., Liu G.T., Xie H. Zh. , Wen D. H. and Liu L.G., Current reversals in an inhomogeneous system with asymmetric unbiased fluctuations, Eur.Phys.J.B 2004 (37), 523 ~526   53. Ai B.Q., Wan X.J., Liu G.T., Wen D. H., Chen W. and Liu L.G., Efficiency optimization in a correlation ratchet with asymmetric unbiased fluctuations,  Phys. Rev. E. 2003(68), 061105-1~5   54. Ai B.Q., Liu G.T., Xie H.Z., Wen D. H., Wang X.J., Chen W., Liu L.G., Efficiency and current in a correlated ratchet, CHAOS, 2004 (14), 957~962 55. Ai B.Q., Xie H.Z., Wen D. H., Liu X. M. and Liu L.G., Heat flow and efficiency in a microscopic engine, Eur.Phys.J.B, 2005 (48), 101 –106 56. Ai B.Q., Xie H.Z., Wen D. H., Liu X. M. and Liu L.G., Bistable kinetic model driven by an inhomogeneous noise, Mod. Phys. Lett. B, 2006(27)1749-1753 57. Li B. A., Chen L. W., Ko C. M., Krastev P. G., Wen D. H., Worley A., Xiao Z. G., Xu J., Yong G. C., and Zhang M., Constraining the EOS of Neutron-Rich Nuclear Matter and Properties of Neutron Stars with Heavy-Ion Reactions， (AIP Conf. Proc. ) AIP Conference Proceedings , 1128 (2009)131-143 58. Li B. A., Chen L. W., Wen D. H., Xiao Z. G., Xu C., Yong G. C., and Zhang M., Recent Progress in Constraining the Equation of State of Dense Neutron-Rich Nuclear Matter with Heavy-Ion Reactions, Nuclear Physics A 834 (2010) 509c–514c 59. Lin W. K., Li B. A., Xu J., Ko C. M. and Wen D. H., Energy release from hadron-quark phase transition in neutron stars and the axial w mode of gravitational waves, PHYSICAL REVIEW C 83, 045802 (2011) 60. Bao-An Li , Lie-Wen Chen , Michael Gearheart , Joshua Hooker , Che Ming Ko, Plamen G. Krastev1, Wei-Kang Lin, William G. Newton1, De-Hua Wen, Chang Xu and Jun Xu ，Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars，Journal of Physics: Conference Series 312 (2011) 042006 61. Newton, W. G.; Gearheart, M.; Wen, De-Hua; Li, Bao-An，Constraints on the symmetry energy from neutron star observations， J. Phys.: Conf. Ser. 420 （2013）012145 62. William G. Newton, Joshua Hooker, Michael Gearheart, Kyleah Murphy, De-HuaWen, Farrukh J. Fattoyev,and Bao-An Li, Constraints on the symmetry energy from observational probes of the neutron star crust, Eur. Phys. J. A (2014) 50: 41 63. Weikang Lin, Bao-An Li, Lie-Wen Chen, De-Hua Wen and Jun Xu, Breaking the EOS-gravity degeneracy with masses and pulsating frequencies of neutron stars, J. Phys. G: Nucl. Part. Phys. 41 (2014) 075203