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arXiv · 1308.1272

AD 775 Pulse of Cosmogenic Radionuclides Production as Imprint of a Galactic Gamma-Ray Burst

A. K. Pavlov·A. V. Blinov·A. N. Konstantinov·V. M. Ostryakov·G. I. Vasilyev·M. A. Vdovina·P. A. Volkov
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Abstract

We suggest an explanation of a sharp increase in the abundance of cosmogenic radiocarbon found in tree rings dated AD 775. The increase could originate from high-energy irradiation of the atmosphere by a galactic gamma-ray burst. We argue that, unlike a cosmic ray event, a gamma-ray burst does not necessarily result in a substantial increase in long-lived 10Be atmospheric production. At the same time, the 36Cl nuclide would be generated in the amounts detectable in the corresponding ice core samples from Greenland and Antarctica. These peculiar features allow experimental discrimination of nuclide effects caused by gamma-ray bursts and by powerful proton events.

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A. K. Pavlov, A. V. Blinov, A. N. Konstantinov, V. M. Ostryakov, G. I. Vasilyev, M. A. Vdovina, P. A. Volkov. 2013-08-06. AD 775 Pulse of Cosmogenic Radionuclides Production as Imprint of a Galactic Gamma-Ray Burst. https://doi.org/10.1093/mnras%2Fstt1468

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