人物經歷
1995年畢業於
四川師範大學物理系,獲物理
專業學士學位;1998年畢業於重慶大學物理系,獲理論物理專業碩士學位;2004年畢業於中山大學物理系,獲理論物理博士學位。2005年至2006年在中山大學數學系做博士後研究;2008年-2009年在美國Texas A&M University-Commerce做訪問學者;2010年在義大利的國際理論物理研究中心(ICTP)訪問學習;2011年再次在美國Texas A&M University-Commerce做訪問學者。1998年至今在
華南理工大學物理系工作,2005年晉升為副教授,2011年晉升為教授,2012年被批准為博士生導師。
研究方向
主要從事核天體物理及緻密物質物態的研究,特別是對中子星等
緻密天體的性質和結構有較深入的研究。
教育教學
主講《大學物理》課程,指導多名學生參加SRP研究項目,還曾擔任過《技術物理》的主講,並編寫了相應的講義,開設全校通識課《天體與宇宙》。
科研項目
主持研究
國家自然科學基金三項;主持華南理工大學中央高校基本科研業務費資助項目三項(包括面上、重點及滾動項目各一項),主持教育部留學回國科研啟動基金一項;主持
中國博士後科學基金一項。
論著
參與編寫了由鄧文基教授主編、華南理工大學出版社出版的教材《大學物理》。
論文
在Phys. Rev. Lett.等期刊上發表SCI論文50餘篇。
1.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
2.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,PHYSICAL REVIEW D 89, 104043 (2014)
3.Zhou Y. and Wen D. H., Constraints on Non-Radial Oscillation Modes by Symmetry Energy Slope, Commun. Theor. Phys. 61 (2014) 469–474
4.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
5.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
6.Yan J. and Wen D. H.,R-mode Instability of Neutron Star with Non-Newtonian Gravity, Commun. Theor. Phys. 59 (2013) 47–52
7.Fu H.Y.,Wen D. H., Yan J., Properties of rapid rotating hybrid stars with non-Newtonian gravity, Acta Phys. Sin. 61 (2012) 209701
8.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
9.Wen D. H., Yan J. and Liu X.M., Gravitational waves from the axial perturbations of hyperon star, Chin. Phys. B, 21 (2012) 060402
10.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)
11.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
12.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
13.Wen D. H. and Chen W., Properties of hyperon stars rotating at Keplerian frequency, Chin. Phys. B, 20 (2011) 029701
14.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)
15.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)
16.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)
17.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)
18.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
19.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
20.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
21.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
22.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
23.Wen D. H., Chen W. and Liu L. G., Rotational Deformation of Neutron Star, Chin. Phys. Lett., 2005 (22), 1604~1607
24.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
25.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
26.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
27.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
28.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
29. 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
30.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)
31.Chen W. Lam Y.Y., Wen D. H. and Liu L.G., Chin. Phys. Lett., 2006 (23), 271~274
32. 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
33.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
34.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
35.Chen W., Wen D. H. and Liu L.G., The properties of neutron star in its evolution, Nuovo Cimento, 2003 (11),71~77
36.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
37.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
38.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
39.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
40.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
41.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
42.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
43.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)
44.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
45.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
46.William G. Newton1,a, 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
47.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
獲獎記錄
2011年度學生科技創新優秀指導教師一等獎。
華南理工大學本科畢業設計(論文)優秀指導教師獎。
多次獲得華南理工大學教學優秀獎和教學成果獎。