黑洞X射线谱的相对论计算
Black hole X-ray spectra: notes on the relativistic calculations
摘要：
这是计算黑洞周围几何薄和光学厚的吸积盘的电磁谱的笔记集。演示文稿是故意教学和大多数计算报告一步一步。在盘-日冕模型中，源的光谱有三个分量：来自盘的热分量、来自日冕的康普顿化分量和来自盘的反射分量。这些注释只回顾相对论计算。这里给出的公式适用于静止、轴对称、渐近平坦、圆形时空，因此它们可以潜在地用于一大类黑洞解。
英文摘要：
This is a collection of notes to calculate electromagnetic spectra of geometrically thin and optically thick accretion disks around black holes. The presentation is intentionally pedagogical and most calculations are reported step by step. In the disk-corona model, the spectrum of a source has three components: a thermal component from the disk, a Comptonized component from the corona, and a reflection component from the disk. These notes review only the relativistic calculations. The formulas presented here are valid for stationary, axisymmetric, asymptotically-flat, circular spacetimes, so they can be potentially used for a large class of black hole solutions.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
