Gamma rays from black holes

作者: G. H. DAHLBACKA , G. F. CHAPLINE , T. A. WEAVER

DOI: 10.1038/250036A0

关键词:

摘要: As a result of electron ion decoupling, the compression interstellar matter falling on to an isolated black hole results in temperatures greater than 100 MeV as approaches Schwarzschild radius. Here, experimental pion production cross sections are used calculate rate γ rays from this hot gas. A characteristic γ-ray spectrum is produced, which peaks at 18 regardless mass or density.

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