Propagation of the Cosmic Radiation through Interstellar Space

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概要

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• Various theories on the origin of the cosmic radiation are critically surveyed. Expected phenomena resulting from the galactic origin theory in which charged cosmic rays are trapped by the glactic magnetic field are discussed with special regard to the secondaries due to the collisions with interstellar hydrogen. Electrons through the decay process π→μ→e are then expected to amount 3〜9% of the total intensity, depending upon the magnetic field strength in our galaxy. An alternative hypothesis that the cosmic radiation propagates in a straight way is also examined. It is proposed that this may be tested by observing primary photons, resulting from the decay process π^○→2_γ, which could be several percent of the total radiation at low latitudes.

• 理論物理学刊行会の論文

著者

• Kobayashi Shinsaku

  Department Of Physics Faculty Of Science Kyoto University

• Kobayashi Shinsaku

  Department Of Physics Osaka University

• HAYAKAWA Saito

  Department of Physics, Osaka City Univervsity

• Hayakawa Saito

  Department Of Physics Osaka City Univervsity

• KOBAYASHI Shinsaku

  Department of Physics, Osaka University

関連論文

• Deuteron Break-Up Reaction on ^4He
• Two-Step Process in the ^C (d,p)^C Reaction
• Polarization in the Elastic Scattering of Protons from ^C at Energies around 4.81 MeV Resonance
• Propagation of the Cosmic Radiation through Interstellar Space

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