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Cryogenic Liquid Jets for High Repetition Rate Discovery Science
Published on: May 9, 2020
来自黑洞系统的相对论喷射的能量学的一个通用缩放
R S Nemmen1, M Georganopoulos, S Guiriec
1NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. rodrigo.nemmen@nasa.gov
概括
黑洞在马射线爆发 (GRB) 和活跃星系核 (AGN) 中产生相对论喷射. 两者都表现出类似的能量-功率相关性,这表明在不同的黑洞尺度上存在普遍的喷气物理.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- 黑洞物理学 黑洞物理学
背景情况:
- 黑洞,包括马射线爆发 (GRB) 中的恒星质量黑洞和活跃银河系核 (AGN) 中的超大质量黑洞,产生协同相对论喷射.
- 喷气物理从恒星到超大质量黑洞的扩展仍然不太了解.
研究的目的:
- 研究来自GRB和AGN的相对论喷射中的动力功率和发光度之间的关系.
- 为了确定黑洞喷射物理学是否存在一个普遍的缩放定律.
主要方法:
- 对马射线爆发 (GRB) 和活跃星系核 (AGN) 的观测数据的分析.
- 对于两种类型的源,加速粒子携带的喷气动力和马射线发光度之间的相关性进行比较.
主要成果:
- 在AGN和GRB产生的喷射中,在动力功率和马射线发光度之间发现了一致的相关性.
- 活跃的星系核 (AGN) 和马射线爆发 (GRBs) 分别代表了这种统一相关的低亮度和高亮度末端.
结论:
- 这些发现暗示,黑洞喷射中的能量消耗效率在广泛的喷射功率 (大小10级) 中非常相似.
- 这就建立了活跃银河系核和马射线爆发产生的喷气之间的基本物理类比.
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