课题基金 / 基金详情

"Study on the Origin of High Energy Cosmic Ray Nuclei by Analyzing the Data from Antarctic Long Duration Balloon Experiments"

"Study on the Origin of High Energy Cosmic Ray Nuclei by Analyzing the Data from Antarctic Long Duration Balloon Experiments"
《通过分析南极长时气球实验数据研究高能宇宙线核的起源》
批准号:
10640273
负责人:
TOMINAGA Takahiro
金额:
$2.18万
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
1998
资助国家:
日本
项目状态:
已结题
起止时间:
1998 至 1999

项目摘要

项目成果

相关文献

中文摘要
翻译
本研究的目的是研制一套核乳胶板自动扫描系统,研究100 TeV/粒子能区宇宙线核的成分。在第一年,我们开发了一个分析系统,借助显微镜和PC机上的CCD摄像机和AD单元,对照相乳胶板中带电粒子径迹的显微照片进行分析。并将其应用于入射核电荷测定的标定中,计算乳胶层径迹吸收的光量。在第二年,已经开始使用我们的新系统分析南极长期气球暴露的数据。分析集中在高能量事件,以避免由于高背景粒子噪声的缺陷。到目前为止,已经完成了大约60个最高能量事件的初级粒子识别。分析工作尚未完成,但我们的第一个目标,即建立一个乳液实验室,用于分析长期实验的数据,已经至少实现。通过对前期观测数据的整理和重新分析,我们公布了宇宙线质子和氦能谱,包括首次南极气球实验的初步观测数据。作为对宇宙线相互作用(包括反常的电子对)的重新研究结果,报道了新中性玻色子衰变假说的可行性。
英文摘要
The objective of this research is to develop an auto-scanning system of nuclear emulsion plates, and to study on the composition of cosmic ray nuclei in the energy region of 100 TeV/particle. In the first year, we developed an analysis system to digitize a photomicrograph of the charged particle tracks in photographic emulsion plates with the aid of CCD camera and AD unit on a microscope and PC. And it has been applied to the calibration for charge determinations of incident nuclei to calculate the amount of light to be absorbed by the track in the emulsion layer. In the second year, the analysis of the data from Antarctic Long Duration Balloon Exposure has been started using our new system. The analysis has been concentrated on only high-energy events to avoid the defect due to high-back-ground particle noise. So far the primary particle identification of about 60 highest energy events has been done. The analysis is not completed yet, but our first objective to built an emulsion laboratory for analyzing the data from Long-Duration-Balloon-Experiments has been at leased achieved. Regarding with compilation and re-analysis of our previous data, cosmic-ray proton and helium energy spectra including the preliminary data from first Antarctic Balloon Experiment has been published. And as results of re-examination on the cosmic ray interactions, which include anomalous number of electron pairs, the feasibility of a hypothesis of a decay of new neutral boson has reported.
期刊论文(13)
专著(0)
科研奖励(0)
会议论文
Y.Takahashi(for the JACEE Collaboratios): "Elemental Abundance of High Energy Cosmic Rays"Nuclear Physics. 60B. 83-92 (1998)
Y.Takahashi(JACEE Collaboratios):“高能宇宙射线的元素丰度”核物理。
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通讯作者:
H.Wilczynski, et al.: "Interpreting anomalous electron pairs as new particle decays"Journal of Physics G Nuclear and Particle Physics. 25. L133-L137 (1999)
H.Wilczynski 等人:“将异常电子对解释为新粒子衰变”《物理 G 核与粒子物理学杂志》。
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M.L.Cherry(for the JACEE Collaboration): "Where Is the Bend in the Cosmic Ray Proton Spectrum?"Proceeding of 26^<th> International Cosmic Ray Conference. 3. 187-190 (1999)
M.L.Cherry(JACEE 协作):“宇宙射线质子光谱的弯曲在哪里?”第 26 届国际宇宙射线会议论文集。
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H.Wilczynski, et al.: "Interpreting anomalous electron pairs as new particle decays"Proceeding of 26^<th> International Cosmic Ray Conference. 2. 352-355 (1999)
H.Wilczynski 等人:“将异常电子对解释为新粒子衰变”第 26 届国际宇宙射线会议论文集。
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