Abstract
Imaging Atmospheric Cherenkov Telescopes have revealed more than 100 TeV sources along the galactic plane, around 45% of them remain unidentified. However, radio observations revealed that dense molecular clumps are associated with 67% of 18 unidentified TeV sources. In this paper, we propose that an electron–positron magnetospheric accelerator emits detectable TeV gamma-rays when a rapidly rotating black hole enters a gaseous cloud. Since the general-relativistic effect plays an essential role in this magnetospheric lepton accelerator scenario, the emissions take place in the direct vicinity of the event horizon, resulting in a point-like gamma-ray image. We demonstrate that their gamma-ray spectra have two peaks around 0.1 GeV and 0.1 TeV and that the accelerators become most luminous when the mass accretion rate becomes about 0.01% of the Eddington accretion rate. We compare the results with alternative scenarios such as the cosmic-ray hadron scenario, which predicts an extended morphology of the gamma-ray image with a single power-law photon spectrum from GeV to 100 TeV.
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Notes
TeV Catalog (http://www.tevcat.uchicado.edu).
LAT Performance (https://www.slac.stanford.edu/exp/glast/groups/canda/lat_Performance.htm).
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Hirotani, K., Pu, HY. & Matsushita, S. Lightning black holes as unidentified TeV sources. J Astrophys Astron 39, 50 (2018). https://doi.org/10.1007/s12036-018-9545-2
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DOI: https://doi.org/10.1007/s12036-018-9545-2