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Searching for events in Chinese ancient records to explain the increase in ^(14)C from AD 774–775 and AD 993–994

Searching for events in Chinese ancient records to explain the increase in ^(14)C from AD 774–775 and AD 993–994
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摘要 According to analysis of the ^14C content in two Japanese trees, that grew over a period of approximately 3000 years, with high time resolution, Miyake et al. found a rapid increase at AD 774-775 and another one at AD 993-994. These increases correspond to high-energy events that happened within those years and radi- ated "),-ray energy of about 7x 1034 erg toward the Earth. The origin of these events is a mystery. Such strong events should have an unusual optical counterpart, and have been recorded in historical literatures. We searched Chinese historical materi- als around AD 744-775 and AD 993-994, but no remarkable event was found except for a violent thunderstorm in AD 775. However, the possibility of a thunderstorm containing so much energy is unlikely. We conclude that the events, which caused the 14C increase, are still unclear. These events most probably had no optical counterpart, and a short gamma-ray burst, giant flare of a soft gamma-ray repeater or a terrestrial γ-ray flash could all be candidates. According to analysis of the ^14C content in two Japanese trees, that grew over a period of approximately 3000 years, with high time resolution, Miyake et al. found a rapid increase at AD 774-775 and another one at AD 993-994. These increases correspond to high-energy events that happened within those years and radi- ated "),-ray energy of about 7x 1034 erg toward the Earth. The origin of these events is a mystery. Such strong events should have an unusual optical counterpart, and have been recorded in historical literatures. We searched Chinese historical materi- als around AD 744-775 and AD 993-994, but no remarkable event was found except for a violent thunderstorm in AD 775. However, the possibility of a thunderstorm containing so much energy is unlikely. We conclude that the events, which caused the 14C increase, are still unclear. These events most probably had no optical counterpart, and a short gamma-ray burst, giant flare of a soft gamma-ray repeater or a terrestrial γ-ray flash could all be candidates.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2015年第9期1504-1512,共9页 天文和天体物理学研究(英文版)
基金 supported by the National Natural Science Foundation of China (Grant No. U1231101) the National Basic Research Program of China (973 Program, Grant No. 2014CB845800)
关键词 astroparticle -- ^14C -- gamma rays: general -- astronomical history --astrobiology astroparticle -- ^14C -- gamma rays: general -- astronomical history --astrobiology
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