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首页> 外文期刊>Bulletin of the Russian Academy of Sciences. Physics >Searching for High Energy Cosmic-Ray Protons Using a New Way of Finding and Tracking Particles in Stratospheric X-Ray Emulsion Chambers (According to Data from the Russian-Japanese RUNJOB Experiment)
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Searching for High Energy Cosmic-Ray Protons Using a New Way of Finding and Tracking Particles in Stratospheric X-Ray Emulsion Chambers (According to Data from the Russian-Japanese RUNJOB Experiment)

机译:使用在平流层X射线乳液室中的发现和跟踪粒子的新方法来寻找高能量宇宙射线质子(根据来自俄语 - 日本跑步实验的数据)

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摘要

An continuing search for primary particles is performed using a new means of finding and tracking particles in nuclear emulsions. Particle interactions registered in stratospheric X-ray emulsion chambers (XECs) are attributed to nucleon-nuclei interactions recorded in the Russian-Japanese RUNJOB experiment. According to the data from processing the interactions between galactic particles and matter in XECs RUNJOB-3B, 6A, and RUNJOB-11A, 11B with energy thresholds ΣE_γ ≥ 3 and ΣE_γ ≥ 5 TeV, respectively, around 50% of all proton tracks went unidentified, which coincides with the initial results from the RUNJOB experiment.
机译:使用一种新的方法来寻找和跟踪核乳胶中的粒子,对初级粒子进行了持续的搜索。平流层X射线乳胶室(XEC)中记录的粒子相互作用归因于俄罗斯-日本RUNJOB实验中记录的核子-核相互作用。根据XECs RUNJOB-3B、6A和RUNJOB-11A、11B中处理星系粒子与物质相互作用的数据,能量阈值为∑E_uγ≥ 3和∑E_uγ≥ 分别为5 TeV,大约50%的质子轨道未被识别,这与RUNJOB实验的初步结果一致。

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