平流层x射线乳化室法数据再处理结果的10-500 TeV能量范围内星系粒子谱

IF 0.7 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY
I. S. Zayarnaya
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引用次数: 0

摘要

我们给出了能量为10 TeV <; E0 <; 500 TeV的初级星系粒子的光谱,这是在俄罗斯-日本RUNJOB气球实验中,在平流层以~ 10 g/cm2的速度暴露在4个x射线乳剂室(RECs)中测量的核-核相互作用相关事件的再处理数据中获得的。该光谱在统计误差范围内与RUNJOB实验最终处理结果上公布的质子光谱一致。本文给出的星系粒子光谱包括在核-核相互作用中发现和丢失单电荷初级粒子的事件,并与仅由探测到初级质子的事件和RUNJOB实验中宇宙射线质子组分的最终光谱构建的光谱进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Spectrum of Galactic Particles in the 10‒500 TeV Energy Range from the Results of Reprocessing of the Data Obtained by the Stratospheric X-ray Emulsion Chamber Method

Spectrum of Galactic Particles in the 10‒500 TeV Energy Range from the Results of Reprocessing of the Data Obtained by the Stratospheric X-ray Emulsion Chamber Method

We present a spectrum of primary galactic particles with energies of 10 TeV < E0 < 500 TeV, obtained from the data of reprocessing of events related to nucleon‒nucleus interactions measured in four X-ray emulsion chambers (RECs) exposed in the stratosphere at ∼10 g/cm2 for 6‒7 days in the Russian‒Japanese RUNJOB balloon experiment. The spectrum agrees within statistical errors with the proton spectrum published on the results of the final processing of the RUNJOB experiment [1]. The presented spectrum of galactic particles includes events with found and missing single-charged primary particles in nucleon‒nucleus interactions, and is compared with the spectrum constructed only from events with detected primary protons and the final spectrum of the cosmic ray proton component of the RUNJOB experiment.

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来源期刊
Bulletin of the Lebedev Physics Institute
Bulletin of the Lebedev Physics Institute PHYSICS, MULTIDISCIPLINARY-
CiteScore
0.70
自引率
25.00%
发文量
41
审稿时长
6-12 weeks
期刊介绍: Bulletin of the Lebedev Physics Institute is an international peer reviewed journal that publishes results of new original experimental and theoretical studies on all topics of physics: theoretical physics; atomic and molecular physics; nuclear physics; optics; lasers; condensed matter; physics of solids; biophysics, and others.
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