GRB 240715A: Revealing a Novel Intrinsic Mechanism by Different Individual Pulses

作者：Wen-Jun Tan, Chen-Wei Wang, S. L. Xiong, S. J. Zheng, Jiang He, Xiao-Yun Zhao, Y. Huang, Shu-Xu Yi, Bing Li, He Gao, Bobing Wu, Bing Zhang, F. Daigne, M. G. Bernardini, Bin‐Bin Zhang, S. Basa, Bertrand Cordier, Jinsong Deng, Yongwei Dong, Damien Dornic, O. Godet, X. H. Han, Maohai Huang, C. Lachaud, Hua-Li Li, P. Maggi, F. Piron, Yulei Qiu, Stéphane Schanne, L. M. Song, D. Turpin, S. D. Vergani, Jing Wang, Ping Wang, Jian‐Yan Wei, Chao Wu, L. P. Xin, Yang Xu, Li Zhang, Shuang‐Nan Zhang · 发表于：The Astrophysical Journal Letters · 年份：2025 · DOI：10.3847/2041-8213/ae2020 · 被引用次数：2 · 研究领域：Gamma-ray bursts and supernovae、Astrophysics and Cosmic Phenomena、CCD and CMOS Imaging Sensors

Abstract The Space-based multiband astronomical Variable Objects Monitor (SVOM) detected its first short gamma-ray burst (GRB), GRB 240715A, in flight, which was jointly observed by Fermi. Based on observational data of SVOM/GRM and Fermi/GBM, we perform a comprehensive temporal and spectral analysis of individual pulses in the prompt emission of this burst, and novel characteristics are revealed. First, opposite evolutions of spectral lag are found in the first and third pulse of this burst. Second, the large negative lag of the first pulse is an outlier in the short GRB sample, especially when the pulse duration is considered. Spectral analysis shows that the negative lag of the first pulse is caused by the evolution of the spectrum index and is irrelevant to E peak , which is inconsistent with the previous study. The intrinsic mechanism is probably attributed to electron cooling in the decaying magnetic field, which leads to the continuous hardening of the spectrum index and results in negative lag. Furthermore, spectral analysis also shows that the third pulse is more likely to be described by a quasi-thermal spectrum, indicating the existence of photospheric emission. It is difficult to explain how the synchrotron radiation appears before photospheric emission in a single GRB, and some assumptions are discussed.