动力学能动量守恒推导时的一个问题
在余辉动力学的推导中，才用动量守恒时是考虑辐射光子的极束效应，认为光子全部是辐射（E_g）向前的，然后对应的动量是E_g/c。这是不对的。（见小问题集2006.11.24）
伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章，另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.
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- Thoene2006 谱分析GRB030329的ISM
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- Ji2006 简单的流体力学扰动不能转移吸积盘的角动量 3
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- Thompson2006 原始磁星作为伽玛暴的中心引擎
- 再测试一次用writely写blogger。
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- Re: 测试
- Campana2006 GRB050904周围丰金属分子云
- Lazzati2006 伽玛暴前身星和暴周环境
- Grupe2006 GRB060729的超长X射线余辉观测 3
- Ghisellini2006 Blazar和伽玛暴
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- Nuza2006 长暴宿主星系在等级理论中的模拟
- Berger2006 几个高红移短暴的观测
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- Su2006 伽玛暴与其他方法共同限制宇宙学参数
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