Positive Temperature Effect of Cosmic Rays

スポンサーリンク

概要

• 論文の詳細を見る

• The temperature effect for the intensity of μ-mesons at sea-level is investigated by taking π-μ decays into account. The positive temperature coefficient is calculated by paying special attention to the difference in the attenuation mean free path of the N-component and the absorption mean free path of π-mesons and to the atmospheric depth which gives main contributions to the coefficient. The magnitude of the coefficient is obtained as 0.05% / °C and the depth of main contributions is found to be 200 mb. Influence of heavy mesons is qualitatively discussed

• 理論物理学刊行会の論文

著者

• Hayakawa Satio

  Research Institute For Fundamental Physics Kyoto University

• Terashima Yoshinosuke

  Yoshida College Kyoto University

• Terashima Yoshinosuke

  Department Of Nuclear Science Kyoto University

• Ito Kensai

  Faculty Of Science Kyoto University

• Ito Kensai

  Department Of Physics Rikkyo University

• Hayakawa Satio

  Research Information Center Institute Of Plasma Physics Nagoya University

• ITO Kensai

  Department of Physics, Kyoto University

関連論文

• Inelastic Scattering of Neutrons by Rotational Excitation
• Observations of Ultraheavy Cosmic Ray Particles with Z>45 at 10 GV Geomagnetic Cutoff Rigidity
• Oxygen Transport and Line Emissions in a Tokamak Plasma
• Nuclear Reactions at Moderate Energies and Fermi Gas Model
• Isotopic Abundance of Carbon in Primary Cosmic Rays
• Energy Loss of a Charged Particle Traversing Superconductors
• Energy Loss of a Charged Particle Traversing Ionized Gas and Injection Energies of Cosmic Rays
• Helium Capturing Reactions in Stars
• On the Plural-Multiple Model of High Energy Meson Showers
• Origin of Cosmic Rays
• Positive Temperature Effect of Cosmic Rays
• Interpretation of the Optical Model in Nuclear Reactions
• Electromagnetic Radiation from Electron Plasma
• Very High Energy Nuclear Reactions and Alpha-Particle Model
• Part III Composition of Primary Cosmic Rays
• Measurement of the Excitation Function of N^+_2 First Negative Bands by Electron Impact
• Neutrino and Gravity
• Origin of Cosmic Rays Revealed in the Rigidity Spectrum of Primary Particles
• Relation between the Nuclear Collective Model and the Individual Particle Model with Configurational Mixing
• On Fissionability of Heavy Nuclei
• A Possible Effect of Cosmic Rays on Celestial Chemical Composition
• Supernova Origin of Cosmic Rays
• Stellar Synthesis of the Proton-Rich Heavy Elements
• A Possible Effect of Cosmic Rays on Celestial Chemical Composition

もっと見る 閉じる

スポンサーリンク