BOAT GRB 221009A:以波因廷通量为主的窄喷流,周围是以物质为主的结构喷流翼

IF 10.2 4区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Journal of High Energy Astrophysics Pub Date : 2024-01-04 DOI:10.1016/j.jheap.2024.01.002
Bing Zhang , Xiang-Yu Wang , Jian-He Zheng
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引用次数: 0

摘要

我们认为,对史上最亮(BOAT)GRB 221009A 的宽波段观测揭示了一种物理图景,其中包括两个喷流成分:一个是以波因廷流为主的窄的(0.6 度半开角)铅笔束喷流,另一个是以物质为主的具有角度结构的更宽的喷流。我们讨论了支持这种情况的各种观测证据。为了解决这个问题,我们建立了一个结构射流分析模型,用于分析减速阶段以物质为主的结构射流翼的正向和反向冲击发射。我们讨论了这种双分量喷流配置对这一特定爆发以及一般的全球记录暴的物理影响。我们认为,在一个准普遍结构喷流情景中,一些明亮的X射线耀斑可能是类似的窄喷流,其视角略微超出窄喷流锥,而且窄喷流可能存在于更多的未被探测到的GRB中。
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The BOAT GRB 221009A: A Poynting-flux-dominated narrow jet surrounded by a matter-dominated structured jet wing

We argue that the broad-band observations of the brightest-of-all-time (BOAT) GRB 221009A reveal a physical picture involving two jet components: a narrow (∼0.6 degree half opening angle) pencil-beam jet that has a Poynting-flux-dominated jet composition, and a broader matter-dominated jet with an angular structure. We discuss various observational evidence that supports such a picture. To treat the problem, we develop an analytical structured jet model for both forward and reverse shock emission from the matter dominated structured jet wing during the deceleration phase. We discuss the physical implications of such a two-component jet configuration for this particular burst and for GRBs in general. We argue that in a quasi-universal structured jet scenario, some bright X-ray flares could be similar narrow jets viewed slightly outside the narrow jet cone and that narrow jets may exist in many more GRBs without being detected.

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来源期刊
Journal of High Energy Astrophysics
Journal of High Energy Astrophysics Earth and Planetary Sciences-Space and Planetary Science
CiteScore
9.70
自引率
5.30%
发文量
38
审稿时长
65 days
期刊介绍: The journal welcomes manuscripts on theoretical models, simulations, and observations of highly energetic astrophysical objects both in our Galaxy and beyond. Among those, black holes at all scales, neutron stars, pulsars and their nebula, binaries, novae and supernovae, their remnants, active galaxies, and clusters are just a few examples. The journal will consider research across the whole electromagnetic spectrum, as well as research using various messengers, such as gravitational waves or neutrinos. Effects of high-energy phenomena on cosmology and star-formation, results from dedicated surveys expanding the knowledge of extreme environments, and astrophysical implications of dark matter are also welcomed topics.
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