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王善钦
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广西南宁市大学东路100号物理科学与工程技术学院A803
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硕士研究生导师
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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
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国家自然科学基金评审专家库成员
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《大学物理》I《恒星与星系物理导论》《吸积与喷流》《物理学史与科学精神》
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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，光学暂现源的尘埃辐射
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主持一项国家自然科学基金：超亮超新星能源研究（**），2020年01月至2023年12月
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已发表/被接受出版的论文（29篇,23篇研究论文+6篇综述论文）研究论文[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] Wang, S. Q*., Li, L. Exploring the Energy Sources Powering the Light Curve of the Type Ibn Supernova PS15dpn and the Mass-Loss History of the SN Progenitor, The Astrophysical Journal, 900, 83, pp. 1-13, (2020)[7] 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, 891, 98, pp. 1-8, (2020) [8] Gan, W. P., Wang, S. Q*., Liang E. W*. The Study of Dust Formation of Four Type Ibn Supernovae, The Astrophysical Journal, Accepted (2021)[9] Li, L., Dai, Z. G.*, Wang, S. Q*., Zhong, S. Q., On the Energy Sources of the Most Luminous Supernova ASASSN-15lh, The Astrophysical Journal, 900, 121, pp. 1-13, (2020)[10] 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)[11] 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)[12] 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)[13] 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)[14] 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)[15] 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)[16] 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)[17] 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)[18] 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)[19] 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)[20] 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[21] Xie,Wen-Jin, Zou, Le, Liu, Hong-Bang, Wang, Shan-Qin, Liang, En-Wei, Magnetar as Central Engine of Gamma-Ray Bursts: Quasi-Universal Jet, Event Rate and X-ray Luminosity Function of Dipole Radiation, The Astrophysical Journal, 894, 52, pp. 1-10, 2020 [22] Gangopadhyay, A., Misra K., Hiramatsu, D., Wang, S. Q., Hosseinzadeh, G. et al. Optical studies of two stripped envelope supernovae SN 2015ap (Type Ib) and SN 2016P (Type Ic), Monthly Notices of the Royal Astronomical Society, in press [23] Li L., Wang, X. G., Zheng, W. K., et al. [including Shanqin Wang] GRB 140423A: A Case of Stellar Wind to Interstellar Medium Transition in the Afterglow, The Astrophysical Journal, in press, 2020综述论文（6 篇）[24] 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 [25] 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[26] 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)[27] 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)[28] 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)[29] 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
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