测量超新星残余的宇宙射线加速效率
E A Helder1, J Vink, C G Bassa
1Astronomical Institute Utrecht, Utrecht University, Post Office Box 80000, NL-3508 TA Utrecht, Netherlands. e.a.helder@uu.nl
概括
宇宙射线是宇宙中最有能量的粒子,主要是由超新星遗留物加速的. 这项研究揭示了宇宙射线占超新星残骸RCW 86中后冲击压力的50%以上,影响了冲击加热机制.
科学领域:
- 天体物理学 天体物理学
- 高能粒子物理学 高能粒子物理学
背景情况:
- 超新星残骸是加速宇宙射线的主要候选者.
- 精确的加速机制和效率仍然不太清楚.
研究的目的:
- 为了研究宇宙射线对超新星残余冲击背后压力的贡献.
- 为了确定超新星残骸RCW 86.6中的宇宙射线含量.
主要方法:
- 光学光谱测量热多普勒扩大.
- 进行X射线观测,分析同步子辐射和自身运动.
- 冲击后质子温度与冲击速度的比较.
主要成果:
- 宇宙射线压力超过RCW 86东北冲击背后的热压.
- 超相对论电子主导着X射线同步子发射.
- 宇宙射线占震后压力的50%以上.
结论:
- 标准冲击加热模型不足以解释RCW 86.中的观察结果.
- 超新星残留物可以显著加速粒子到宇宙射线能量.
- 这为超新星残骸中的宇宙射线加速提供了直接证据.
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