GRB 170714A: A good sample for investigating screen of magnetic field?

IF 1.6 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Shuang Du, Shujin Hou
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引用次数: 0

Abstract

X-ray afterglow of the gamma-ray burst (GRB), GRB 170714A, may exhibit an intriguing characteristic: It comprises two plateaus, each followed by a precipitous decay segment. We posit that this unusual feature can be rationalized within the framework of GRB magnetar scenario. Specifically, initial break in the X-ray afterglow is attributed to the decay of magnetic field of the central magnetar, whereas the subsequent break corresponds to the collapse of this magnetar. We argue that the decay of magnetar’s magnetic field is caused by the fall-back accretion. Given this current understanding, we deduce that rare hypercritical fall-back accretion is layered, with density profile of the fallback matter along the radial direction being notably discontinuous. Our work potentially shows the prospect of employing GRBs as a tool to investigate intricacies of highly uncertain fall-back accretion processes.

GRB 170714A:是研究磁场屏的好样品吗?
伽马射线暴(GRB)的x射线余辉,GRB 170714A,可能表现出一个有趣的特征:它包括两个高原,每个高原后面都有一个陡峭的衰减段。我们假设这种不寻常的特征可以在GRB磁星情景的框架内合理化。具体来说,x射线余辉的初始破裂归因于中央磁星磁场的衰减,而随后的破裂则对应于该磁星的坍缩。我们认为磁星磁场的衰减是由回退吸积引起的。根据目前的理解,我们推断,罕见的超临界退积是分层的,退积物质沿径向的密度分布明显不连续。我们的工作潜在地显示了利用grb作为研究高度不确定的回退吸积过程复杂性的工具的前景。
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来源期刊
Journal of Astrophysics and Astronomy
Journal of Astrophysics and Astronomy 地学天文-天文与天体物理
CiteScore
1.80
自引率
9.10%
发文量
84
审稿时长
>12 weeks
期刊介绍: The journal publishes original research papers on all aspects of astrophysics and astronomy, including instrumentation, laboratory astrophysics, and cosmology. Critical reviews of topical fields are also published. Articles submitted as letters will be considered.
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