教师个人信息表
姓名 王善钦 性别
本人照片
出生年月   政治面貌 群众
籍贯 福建霞浦 职称 助理教授
学历 博士研究生 学位 博士
联系电话 邮政编码
Email shanqinwang@gxu.edu.cn
QQ 微信
通讯地址 广西南宁市西乡塘区大学东路100号物理科学与工程技术学院A811
所在学院 物理科学与工程技术学院 导师类型 校内导师
导师类别 硕士研究生导师
指导学科一
门类:理学 一级学科:天文学 二级学科:天体物理
指导学科二
学习和工作经历 2011.09-2018.06 南京大学天文与空间科学学院
2016.11-2018.05 加州大学伯克利分校(University of California, Berkeley)天文系
学术兼职 国家自然科学基金评审专家
主讲课程 《大学物理》I
《吸积与喷流》
主要研究方向 超亮超新星,伽玛射线暴成协的超新星,普通Ibc型与II型超新星,伴随引力波的光学暂现源(千新星)、潮汐瓦解事件
主持(或参与)的主要科研项目 主持一项国家自然科学基金:
超亮超新星能源研究(11963001),2020年01月至2023年12月
取得的主要成果 已发表的研究论文(17 篇)
[1] Wang, S. Q., Wang, L. J., Dai, Z. G., & Wu, X. F., Superluminous Supernovae Powered by Magnetars: Late-time Light Curves and Hard Emission Leakage, The Astrophysical Journal, 799, 107: 1-8 (2015)
[2] Wang, S. Q., Wang, L. J., Dai, Z. G., & Wu, X. F., A Unified Energy-reservoir Model Containing Contributions from 56Ni and Neutron Stars and Its Implication for Luminous Type Ic Supernovae, The Astrophysical Journal, 807, 147: 1-10 (2015)
[3] Wang, S. Q., Liu, L. D., Dai, Z. G., Wang, L. J., & Wu, X. F., A Triple-energy-source Model for Superluminous Supernova iPTF13ehe, The Astrophysical Journal, 828, 87: 1-5 (2016)
[4] Wang, S. Q., Cano, Z., Wang, L. J., et al., Modeling The Most Luminous Supernova Associated with a Gamma-Ray Burst, SN 2011kl, The Astrophysical Journal, 850, 148: 1-9 (2017)
[5] Wang, S. Q., Cano, Z., Li, L., et al., Modeling the Light Curves of the Luminous Type Ic Supernova 2007D, The Astrophysical Journal, 877, 20: 1-7 (2019)
[6] Li, L., Wang, S. Q*., Liu, L. D., Wang X.G., Liang E.W., Dai, Z.G. The Energy Sources of Double-peaked superluminous supernova PS1-12cil and luminous supernova SN 2012aa, The Astrophysical Journal, in press (2020)
[7] Wang, L. J, Wang, S. Q., Dai, Z. G., Xu D., Han, Y. H., Wu, X. F., & Wei, J. Y., Optical Transients Powered by Magnetars: Dynamics, Light Curves, and Transition to the Nebular Phase, The Astrophysical Journal, 821, 22: 1-10 (2016)
[8] Dai, Z. G., Wang, S. Q., Wang, J. S., Wang, L. J., & Yu, Y. W., The Most Luminous Supernova ASASSN-15lh: Signature of a Newborn Rapidly Rotating Strange Quark Star, The Astrophysical Journal, 817, 132: 1-6 (2016)
[9] Liu, L. D., Wang, S. Q., Wang, L. J., Dai, Z. G., Yu, H., & Peng, Z. K., A Monte Carlo Approach to Magnetar-powered Transients. I. Hydrogen-deficient Superluminous Supernovae, The Astrophysical Journal, 842, 26 : 1-11 (2017)
[10] Peng, Z. K., Wang, S. Q., Liu, L. D., Dai, Z. G., Yu, H. Constraining the Environmental Properties of FRB 131104 Using the Unified Dynamical Afterglow Model, The Astrophysical Journal, 861, 147: 1-9 (2018)
[11] Wang, L. J., Cano, Z., Wang, S. Q., Zheng, W., et al. A Monte Carlo Approach to Magnetar-powered Transients: II. Broad-lined Type Ic Supernovae Not Associated with GRBs, The Astrophysical Journal, 851, 54: 1-16 (2017)
[12] Wang, L. J., Wang, X. F., Wang, S. Q., Dai, Z. G., Liu, L. D., Song, L. M., Rui, L. M., Cano, Z., & Li, B., A fallback accretion model for the unusual type II-P supernova iPTF14hls, The Astrophysical Journal, The Astrophysical Journal, 865, 95:1-8 (2018)
[13] Liu, L. D., Wang, L. J., Wang, S. Q., & Dai, Z. G., A Multiple Ejecta-circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc, The Astrophysical Journal, 856, 59: 1-8 (2018)
[14] Wang, L. J., Han, Y. H., Xu, D., Wang, S. Q., Dai, Z. G., Wu, X. F., & Wei, J. Y., Solving the 56Ni Puzzle of the Magnetar-powered Broad-lined Type Ic Supernovae, The Astrophysical Journal, 831, 41: 1-7 (2016)
[15] Wang, L. J., Yu, H., Liu, L. D., Wang, S. Q., Han, Y. H., Xu, D., Dai, Z. G, Qiu, Y. L., & Wei, J. Y., Evidence for Magnetar Formation in broad-lined Type Ic Supernovae 1998bw and 2002ap, The Astrophysical Journal, 837, 128: 1-7 (2017)
[16] Wang, L. J., Wang, X. F., Cano,Z., Wang, S. Q., Liu, L. D., Dai, Z. G., et al. Broad-lined Type Ic Supernova iPTF16asu: A Challenge to All Existing Models, Monthly Notices of the Royal Astronomical Society, 489, 110 (2019)
[17] Gangopadhyay, A., Misra K., Hiramatsu, D., Wang, S. Q., Hosseinzadeh, G. et al. Flash ionization signatures in the type Ibn supernova SN 2019uo, The Astrophysical Journal, 889, 170, pp. 1-14, 2020


已发表的综述论文(6 篇)
[18] Wang, S. Q., Dai, Z. G., & Wu, X. F. Research Developments in Li-Paczyński Novae(kilonovae) (I): Theoretical Aspect, ChAA, 40, 2: 141-175, 2016
[19] Wang, S. Q., Dai, Z. G., & Wu, X. F. Research Developments in Li-Paczyński Novae (kilonovae) (II): Observational Aspect, ChAA, 40, 4: 439-473, 2016
[20] Wang, S. Q., Wang, L. J., & Dai, Z. G., The Energy Sources of Superluminous Supernovae, Invited Review accepted for publication in Research in Astronomy and Astrophysics, 19, 63: 1-20 (2019)
[21] Cano, Z., Wang, S. Q., Dai, Z. G., & Wu, X. F. The Observer's Guide to the Gamma-Ray Burst Supernova Connection, AdAst, 2017, E5: 1-42 (2017)
[22] 王善钦,戴子高,吴雪峰.《GRB 130427A/SN 2013cq与伽玛射线暴-超新星成协》,《天文学进展》, 32, 481 (2014)
[23] 耿金军,肖笛,王善钦,戴子高,《引力波的电磁对应体》,《中国科学》, 48(7), 079802, 2018
数据更新日期 2020-02-17 填报责任人 王善钦
本信息由教师个人提供,文责自负!