华南理工大学理学院(物理)导师介绍:文德华
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姓名:文德华 性别:男 职称:教授 学院:理学院(物理) 研究方向:核天体物理 导师简
共发表被SCI收录的论文四十余篇,其中第一作者论文二十余篇,下面是近年发表的部分第一作者论文:
1.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)
2.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)
3.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)
4.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
5.Wen D. H., Yan J. and Liu X.M., Gravitational waves from the axial perturbations of hyperon star, Chin. Phys. B Vol. 21, No. 6 (2012) 060402
6.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
7.Wen D. H. and Chen W., Properties of hyperon stars rotating at Keplerian frequency, Chin. Phys. B, 20 (2011) 029701
8.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)
9.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
10. 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
11.Wen D. H., Chen W. and Liu L. G., Rotational Deformation of Neutron Star, Chin. Phys. Lett., 2005 (22), 1604~1607
12.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
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