文德华 - 华南理工大学 - 物理与光电学院

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-2009年在美国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；2011年再次在美国Texas A&M University-Commerce做访问学者。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。

研究领域

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

近期论文

查看导师最新文章（温馨提示：请注意重名现象，建议点开原文通过作者单位确认）

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