旋转黑洞周围的二温度吸积流与源Kerr参数的确定
高能天体物理现象
2016-11-15 v1 广义相对论与量子宇宙学
摘要
我们自洽地模拟了旋转黑洞周围亚开普勒、光学薄区域中的二温度黏性吸积流，并包含了重要的辐射效应。该模型成功解释了从超亮到欠亮源的观测光度，并预测了黑洞的自旋参数。
引用
@article{arxiv.1101.4626,
title = {Two temperature accretion flows around rotating black holes and determining the kerr parameter of sources},
author = {Banibrata Mukhopadhyay},
journal= {arXiv preprint arXiv:1101.4626},
year = {2016}
}
备注
4 pages including a figure; to appear in the proceedings of MG12, Marcel Grossman Meeting, Paris, France, 12-18 July 2009