Question

陈伟的成果简介

Answer 1

　　现已发表论文30余篇，其中30篇被SCI收录。　　代表论文：　　发表的论文：
[1] 陈伟，梅仲豪，刘良钢，核物质物态方程的研究，高能物理与核物理，23(1999)681。(SCI)
[2] W. Chen, L.G. Liu, the Thermal Properties of D-Resonance Nuclear matter, IL NUOVO CIMENTO, 112A(1999)1509。(SCI)
[3] W Chen, B.Q. Ai, X.P. Zheng, L.G. Liu, the Influence of the Renormalization Condition to the Equation of State of Nuclear Matter, Commun. Thero. Phys. 36(2)(2001)。(SCI)
[4] 陈伟，艾保全，郑小平，刘良钢，s介子的自相互作用对核物质物态方程的影响，高能物理与核物理，25(2000)23。 (SCI)
[5] W Chen, L.G. Liu, the Tachyon pole in the Relativistic s-w Model, Commun. Thero. Phys. 36(1)(2001)。(SCI)
[6] W. Chen, Q.G. Li, L.G. Liu, the Properties of Pure Neutron Star, Commun. Thero. Phys. 36(2001)。(SCI)
[7] W. Chen, D. H Wen, L. G. Liu, Softness of nuclear matter and the production of Strange particles in neutron stars, Chin. Phy. Lett. 20(3)(2003) 436-439 。(SCI)
[8] W. Chen, D. H. Wen, G. T. Liu, X. J. Wang, and L. G. Liu, Thermal Dynamics Behavior of Protoneutron Star Matter, Commun. Theor. Phys. 39(3)(2003)317-322。(SCI)
[9] W. Chen, D. H. Wen, and L.G. Liu, The Properties of Neutron Star in Its Evolution, IL NUOVO CIMENTO, 118B(1)(2003)71-77。(SCI)
[10] 陈伟，文德华，刘良钢，Study of the Gravitational Energy in Neutron Stars，中山大学学报(自然科学版) 42(3)(2003)16-18。
[11] W. Chen, D.Q. Dong, D. H. Wen, G. T. Liu, and L. G. Liu,，Equation of State of Nuclear Matter in Chiral $\sigma$-$\omega$ Model，Commun. Theor. Phys.，41(2004)925-928。(SCI)
[12] 陈伟，刘良钢，均匀强磁场中中子星物质的物态方程，高能物理与核物理，29(2005)17-20.(SCI)
[13] 陈伟，董东桥，文德华，刘良钢，手征模型研究的进展，中山大学学报，43(3)(2004)25-27。
[14] L.G. Liu, X.Q. Luo, Q.F. Zhou, W. Chen, M. Nakano, N , N, Excitation for Pion Propagator in Nuclear Matter, Phys. Rev. C56(1997)800。(SCI)
[15] L.G. Liu, X.Q. Luo, W. Chen, A New Regularization method in 3-Diemnsional Momentum Space, Nuovo Cimento, 110A(1998)1。(SCI)
[16] L.G. Liu, W. Chen，Study of the Binding Energy of Relativistic Nuclear Matter in Relativistic s - w －p Model, Comm. Theor. Phys.，29(1998)81。(SCI)
[17] L.G. Liu, W. Chen，Z.H. Mei, Nakano M.，The binding energy of nuclear matter with pionic degree of freedom, Nuovo Cimento，111A(1998)1。(SCI)
[18] L.G. Liu, W. Chen, X.Q. Luo, M. Nakano，Antiparticle Excitation Effect in the Relativistic Spin-Isospin-Dependent Response Function of Nucleus, Comm. Theor. Phys., 34(2000)101。(SCI)
[19] L.G. Liu, W. Chen, B.Q. Ai, X.P. Zheng, M. Nakano, Relativistic Spin-Isospin Dependent Response Function of Nucleus, Chin. Phys. Lett.,17(2000)652。(SCI)
[20] 文德华，陈伟，王先菊，艾保全，刘国涛，刘良钢，静态球对称星体结构方程的不同推导与比较，中山大学学报 42（2）(2003)15-17。
[21] D.H. Wen, W. Chen, X.J. Wang, B.Q. Ai, G.T. Liu, L.G. Liu, Energy of Gravitational Field of Static Spherically Symmetric Neutron Stars, Commun. Theor. Phys., 40(5) (2003)637-640。(SCI)
[22] B.Q. Ai, X.J. Wang, G. T. Liu, D.H. Wen, W. Chen and L.G. Liu, Efficiency optimization in a correlation ratchet with asymmetric unbiased fluctuations, Phys. Rev. E. 68(6) (2003)061105。(SCI)
[23] B.Q. Ai, W. Chen, X.J. Wang, G.T. Liu, D.H. Wen , L.G. Liu, Noise in Genotype Selection Model, Commun. Theor. Phys. 39 (2003) 765-768。(SCI)
[24] B.Q. Ai, W. Chen, X.J. Wang, G.T. Liu, D.H. Wen, H.Z. Xie and L.G. Liu, Noise in an Insect Outbreak Model, Chin. J. Phys. 40 (4)(2003) 422-429。(SCI)
[25] 文德华，陈伟，李绍新，郑华，对大学物理教材立体化建设的几点认识，大学物理物理教育专刊 27（2003）78。
[26] D.H. Wen, W. Chen, X.J. Wang, B.Q. Ai, G.T. Liu, D.Q. Dong, L.G. Liu, Structures of rotating traditional neutron stars and hyperon stars in the relativistic sigma-omega model, Eurp. Phys. J. A 21(2)(2004)349-354。(SCI)
[27] B.Q.Ai, X.J. Wang, G.T. Liu, D.H. Wen, W. Chen and L.G. Liu, Current Reversals in a inhomogeneous system with asymmetric unbiased fluctuations, Eur. Phys. J. B37(4)(2004)523-526。(SCI)
[28] D.H. Wen, W. Chen, X.J. Wang, B.Q. Ai, G.T. Liu, L.G. Liu, Properties of Rotating Neutron Stars in the Relativistic Model, Commun. Theor. Phys.,41(1)(2004)51-54。(SCI)
[29] D.H. Wen, W. Chen, X.J. Wang, B.Q. Ai, G.T. Liu, D.Q. Dong, L.G. Liu, Energy of Gravitational Field of the Slowly Rotating Neutron Stars, Chin. J. Phys. 41(6)(2003)595-600。(SCI)
[30] D.Q. Dong, W. Chen, D. H. Wen, L. G. Liu, and M. Nakano，Dispersion relation of s meson and pion at finite nuclear density in chiral s model, Commun. Theor. Phys. 41(5)(2004)741-745。(SCI)
[31] 董东桥，陈伟，文德华，刘良钢，手征s模型中s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, 27（10）(2003)892-896。(SCI)
[32] 陈伟，文德华，刘良钢，a Study of the Tachyon Pole in the Chiral s-w model, Chin. J. Phys., 43(2)(2005).(SCI)
[33] D.H. Wen, W. Chen, X.J. Wang, B.Q. Ai, G.T. Liu, D.Q. Dong, L.G. Liu, Structures of rotating traditional neutron stars and hyperon stars in the relativistic sigma-omega model, Eurp. Phys. J. A 21(2)(2004)349-354。(SCI)
[34] D.H. Wen, W. Chen, L.G. Liu, Rotational Deformation of Neutron Stars, Chin. Phys. Lett. 22(7)(2005)1604-1607。(SCI)
[35] D.H. Wen, W. Chen, L.G. Liu, Comparation of Two Methods for Calculating Properties of Rotating Neutron Stars, 原子核物理评论，22(1)(2005)23-26。