Onthe Analysis of the Slow Particles Emitted from Cosmic-Ray Stars (II)

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概要

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• Observations have been made on the heavy fragments from stars produced by cosmic-rays and 6.2BeV protons from the Bevatrons. The charges of the heavy fragments were determined by measuring the width of tracks. The charge distribution of the heavy fragments emitted from silver or bromine nuclei seems approximately to decrease exponentially. The energy distributions of lithium and beryllium nearly agreed with the curves deduced from the evaporation model, assuming the appropriate nuclear temperatures and Coulomb barrier heights. The angular distributions of them were nearly isotropic. According to these results, the process of slow fragment emission seems to be interpreted as that of evaporation.

• 社団法人日本物理学会の論文
• 1957-07-05

著者

• Okudaira Kiyoaki

  Department of Physics, Rikkyo University

• TAMAI Eiji

  Department of Microbiology, Faculty of Pharmaceutical Sciences Okayama University

• Tamai Eiji

  Department Of Physics Rikkyo (st. Paul's) University

• Tamai Eiji

  Department Of Infectious Diseases School Of Pharmacy Matsuyama University

• Okudaira Kiyoaki

  Department Of Physics Rikkyo (st. Paul's) University

• Okudaira Kiyoaki

  Department Of Physics Faculty Of Science Rikkyo University

• NAKAGAWA Shigeo

  Department of Physics, Rikkyo (St. Paul's) University

• HUZITA Humiaki

  Department of Physics, Rikkyo (St. Paul's) University

• Huzita Humiaki

  Department Of Physics Rikkyo (st. Paul's) University

• Nakagawa Shigeo

  Department Of Physics Rikkyo (st. Paul's) University

• Nakagawa Shigeo

  Department Of Biology Faculty Of Science Osaka University:(present)sanki Engineering Limited

• OKUDAIRA Kiyoaki

  Department of Physics, Rikkyo (St. Paul's) University

• TAMAI Eiji

  Department of Physics, Rikkyo (St. Paul's) University

• HUZITA Humiaki

  Department of Physics, Rikkyo (St. Paul's) University

• NAKAGAWA Shigeo

  Department of Physics, Rikkyo (St. Paul's) University

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