Efficiency of Neutrino Annihilation around Spinning Black Holes

I. Zalamea, A. Beloborodov
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引用次数: 3

Abstract

A fraction of neutrino emission from GRB accretion disks annihilates above the disk, creating e± plasma that can drive GRB explosions. We calculate the efficiency of this annihilation using the recent detailed model of hyper‐accretion disks around Kerr black holes. Our calculation is fully relativistic and based on a geodesic‐tracing method. We find that the efficiency is a well‐defined function of (1) accretion rate and (2) spin of the black hole. It is practically independent of the details of neutrino transport in the opaque zone of the disk. The results help identify the accretion disks whose neutrino emission can power GRBs.
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旋转黑洞周围中微子湮灭的效率
来自GRB吸积盘的中微子发射的一小部分在盘上湮灭,产生可以驱动GRB爆炸的e±等离子体。我们利用克尔黑洞周围超吸积盘的最新详细模型计算了这种湮灭的效率。我们的计算是完全相对论性的,并基于测地线追踪方法。我们发现效率是(1)吸积速率和(2)黑洞自旋的一个定义良好的函数。它实际上与圆盘不透明区域的中微子输运细节无关。这些结果有助于识别那些中微子发射可以为grb提供动力的吸积盘。
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