个人简介
姓名：王德华
职称/职务：副教授/理论物理方向硕士生导师
【乐动官方】（中国）集团有限公司/部门：物理与电子科学【乐动官方】（中国）集团有限公司/天文系
学习经历
博士：2009-2014，北京师范大学，天体物理专业
本科：2005-2009，中国地质大学（北京）
工作经历
2014年至今，贵州师范大学，物理与电子科学【乐动官方】（中国）集团有限公司
研究方向
1、低质量X射线双星准周期震荡
2、吸积中子星周期-磁场演化
3、毫秒脉冲星形成与演化
教学成果
主教课程：电磁场与电磁波、射电天文学
指导学生情况：目前已带过两届硕士研究生
科研成果
1、学术论文
[1] Wang De-Hua, Zhang Cheng-Min, Wang Shuang-Qiang, Investigation of
the Millisecond Pulsar Origins by their Spin Periods at the Wavebands of Radio, X-Ray, and γ-Ray, Publications of the Astronomical Society of the Pacific, 2019.2, 131(996): 024201
[2] Wang De-Hua, Zhang Cheng-Min, Qu Jin-Lu, The kHz QPOs as a probe
of the X-ray color-color diagram and accretion-disk structure for the atoll source 4U 1728-34, Astronomy & Astrophysics, 2018.11, 618: A181
[3] Wang De-Hua, Zhang Cheng-Min, Qu Jin-Lu, Yang Yi-Yan, Correlation
s between the frequencies of twin kHz QPOs and spins of neutron stars in LMXBs, Monthly Notices of the Royal Astronomical Society, 2018.2, 473(4):
4862~4867
[4] Wang D. H., Zhang C. M., Lei Y. J., Chen L., Qu J. L., Zhi Q. J., Probing the accretion disc structure by the twin kHz QPOs and spins of neutron stars in LMXBs, Monthly Notices of the Royal Astronomical Society, 2017.4, 466(1): 1111~1117
[5] Wang D. H., Chen L., Zhang C. M., Lei Y. J., Qu J. L., Song L. M., Investigation of the emission radii of kHz QPOs for the accreting millisecond X-Ray pulsars, Atoll and Z sources, Monthly Notices of the Royal Astronomical Society, 2015.12, 454(2): 1231~1237
[6] Wang D.H., Chen L., Zhang C.M., Lei Y.J., Qu J.L., Statistical
properties of twin kilohertz quasi-periodic oscillations in neutron star
low-mass X-ray binaries, Astronomische Nachrichten, 2014.02, 335(2): 168~177
[7] Wang D. H., Chen L., Zhang C. M., Lei Y. J., Qu J. L., Constraints
on kilohertz quasi-periodic oscillation models and stellar equations of state from SAX J1808.4–3658, Cyg X-2 and 4U 1820–30, Monthly Notices of the Royal Astronomical Society, 2013.11, 435(4): 3494~3499
[8] Ye, Chang-Qing, Wang, De-Hua, et al., Evolution implications of neutron starmagnetic fields: inferred from pulsars and cyclotron lines of HMXBs, 2019, Astrophysics and Space Science, 364, 198
[9] Wang, Shuang-Qiang, ..., Wang, D. H., et al., Interpretation of no radio pulsar inside supernova 1987A: The high plasma cut-off frequency by the remnant media, 2019, New Astronomy, 69, 43
[10] Wang, Shuang-Qiang, ..., Wang, D. H., et al., An Explanation for the Undetection of Radio Pulsar in Supernova 1987A, 2017, Chinese Physics Letters , 34, 129702
[11] Shang Lun-Hua, ..., Wang De-Hua, et al., State Switching of the X-Ray/Radio Transitional Millisecond Pulsar , Astrophysical Journal, 2017.11, 849(2): 87
[12] Shang Lun-Hua, ..., Wang De-Hua, et al., Investigating the multifrequency pulse profiles of PSRs B0329+54 and B1642-03 in an inverse Compton scattering model , Monthly Notices of the Royal Astronomical Society, 2017.7, 468(4): 4389~4398
[13] Yang Yi-Yan, ..., Wang De-Hua, et al., Similarity of PSR J1906+0746 TO PSR J0737–3039: A Candidate of a New Double Pulsar System?, The strophysical Journal, 2017.2, 835(2): 185
[14] Lei Ya-Juan, ..., Wang De-Hua, et al., Evolution of the Cross-correlation and Time Lag of 4U 1735-44 along the Branches, The Astronomical Journal, 2013.9, 146(3): 60
[15] Li Zhao-sheng, ..., Wang De-hua, The cross spectral time lag evolution along branches in XTE J1701-462, The Astrophysical Journal, 2013.4, 767(2): 167
[16]) Wang J., ..., Wang D.H., et al., Morphological analysis on the coherence of kHz QPOs, Astrophysics and Space Science, 2012.12, 342(2): 357~364
[17] Li Zhaosheng, ..., Wang Dehua, Spectral Lags Obtained by CCF of Smoothed Light Curves, Publications of the Astronomical Society of the Pacific,2012.4, 124(914): 297~303
[18] Wang J., ..., Wang D.H., et al., Statistical analysis for the Q-factor of twin kHz QPOs, Astronomische Nachrichten, 2012.4,333(3): 274~279
[19] 叶长青, 王德华, 等, X射线双星回旋吸收线研究进展, 2019, 天文学进展,37(2)
[20] 吴庆东, 王德华, 等, 低能损率射电脉冲星辐射研究, 2019, 天文学报, 60(2)
[21] 王双强, …, 王德华, 等, 特殊类型脉冲星的研究进展, 2018, 天文学进展, 36(1)
[22] 刘鹏, …, 王德华, 等, 中子星质量分布与诞生方式的研究, 2018, 天文学报, 59(3)
[23] 付妍妍, …, 王德华, 中子星吸积加速与引力辐射影响, 2015, 天文学报, 56(3)
[24] 张月竹, …, 王德华, 脉冲星减速研究与电磁和引力波辐射, 2015, 天文学报, 56(3)
[25] 程争, …, 王德华，等, 中子星质量分布的统计研究, 2013, 天文学报, 54(6)
[26] 卜庆翠, …, 王德华, 伽玛暴数据处理中的贝叶斯方法, 2013, 天文学进展, 31(3)
[27] 李兆升, …, 王德华, 伽玛射线暴的光度-光变复杂度关系, 2011, 天文学进展, 29(2)
2、教材、专著
[1] 张承民，潘元月，王德华，杨佚沿，中子星与脉冲星天体物理，科学出版社，2019，197千字，ISBN：9787030492821
科研项目
[1] 低质量X射线双星千赫兹准周期震荡研究，国家自然科学基金，11703003，主持
[2] 低质量X射线双星辐射性质及演化研究，贵州省科学技术基金，黔科合基础[2020]1Y016，主持
[3] 吸积中子星atoll/Z源演化研究，贵州省联合基金，黔科合LH字[2016]7226号，主持
[4] 中子星千赫兹准周期震荡研究，贵州省科学技术基金，黔科合J字[2015]2113号，主持
[5] 基于FAST飘移扫描巡天的脉冲星统计观测和理论研究，国家自然科学基金，U1731238，参与
[6] 天体中R过程重元素合成机制网络计算研究，国家自然科学基金，11565010，参与
