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Astrophysics > High Energy Astrophysical Phenomena

arXiv:1009.4648 (astro-ph)
[Submitted on 23 Sep 2010 (v1) , last revised 25 Sep 2010 (this version, v2)]

Title: What do we know about gamma-ray bursts?

Title: 我们对伽马射线暴了解多少?

Authors:Ehud Nakar
Abstract: Decades of improving data and extensive theoretical research have led to a popular model of gamma-ray bursts. According to this model, a catastrophic event in a stellar system results in the formation of a compact central engine, which releases a fraction of a solar rest-mass energy within seconds in the form of ultra-relativistic jets. Dissipation of the jets energy leads first to prompt gamma-ray emission and later to a long lasting afterglow. Here I summarize the introduction that I gave to the debate "where do we stand?" in the conference "The Shocking Universe" held in Venice. This is a very brief summary of my view of the facts that we are (almost) certain about, models that are popular but may need rethinking, and main open questions.
Abstract: 几十年来数据的改进和广泛理论研究导致了伽马射线暴的一个流行模型。 根据这个模型,恒星系统中的灾难性事件会导致一个致密的核心引擎形成,在几秒钟内以超相对论喷流的形式释放出一部分太阳静止质量能量。 喷流能量的耗散首先导致瞬时伽马射线辐射,随后产生持续时间较长的余辉。 在这里,我总结了我在“我们目前处于什么位置?”辩论中所做的介绍,该辩论是在威尼斯举行的“令人震惊的宇宙”会议上进行的。 这是我对我认为我们几乎可以确定的事实、流行的但可能需要重新考虑的模型以及主要开放问题的简要总结。
Comments: proceedings of the The Shocking Universe meeting, Venice, September 2009
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE)
Cite as: arXiv:1009.4648 [astro-ph.HE]
  (or arXiv:1009.4648v2 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.1009.4648
arXiv-issued DOI via DataCite

Submission history

From: Ehud Nakar [view email]
[v1] Thu, 23 Sep 2010 15:54:29 UTC (10 KB)
[v2] Sat, 25 Sep 2010 03:46:11 UTC (10 KB)
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