Fitting the Crab Supernova with a Gamma-Ray Burst

IF 2.5 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Universe Pub Date : 2024-06-25 DOI:10.3390/universe10070275
Remo Ruffini, Costantino Sigismondi
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引用次数: 0

Abstract

Here, we reconsider the historical data, assuming a gamma-ray burst (GRB) as its source. A Supernova correlated with the GRB explains well the fading time observed by the ancient Chinese astronomers in the daytime and the nighttime, while the GRB power law explains the present X-rays and GeV emission of the Crab. On the grounds of a recent understanding of the first episode of binary-driven hypernova GRB (BDHN GRB) in terms of the collapse of a ten solar masses core, we propose the possible identification of the real Supernova event at an earlier time than Chinese chronicles. This work allows a new understanding of the significance of historical astronomical observations, including a fireball due to gamma-ray air shower observation and a plague of acute radiation syndrome, documented with several thousands of victims in the Eurasian area (Egypt, Iraq, and Syria).
用伽马射线暴拟合蟹状超新星
在这里,我们假定伽马射线暴(GRB)是其来源,重新考虑了历史数据。与伽玛射线暴相关的超新星可以很好地解释中国古代天文学家在白天和夜晚观测到的衰减时间,而伽玛射线暴的幂律则可以解释蟹号现在的X射线和GeV辐射。根据最近对双星驱动超新星GRB(BDHN GRB)第一次事件的理解,即10个太阳质量内核的坍缩,我们提出可能在比中国编年史更早的时间发现了真正的超新星事件。这项工作让我们对历史天文观测的意义有了新的认识,包括伽马射线气雨观测引起的火球和急性辐射综合症瘟疫,在欧亚地区(埃及、伊拉克和叙利亚)有数千名受害者的记录。
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来源期刊
Universe
Universe Physics and Astronomy-General Physics and Astronomy
CiteScore
4.30
自引率
17.20%
发文量
562
审稿时长
24.38 days
期刊介绍: Universe (ISSN 2218-1997) is an international peer-reviewed open access journal focused on fundamental principles in physics. It publishes reviews, research papers, communications, conference reports and short notes. Our aim is to encourage scientists to publish their research results in as much detail as possible. There is no restriction on the length of the papers.
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