Evaluation of Effective Astrophysical S Factor for Non-Resonant Reactions
スポンサーリンク
概要
- 論文の詳細を見る
- 2002-12-26
著者
-
UEDA Manabu
Institute of Physics, University of Tsukuba
-
Ueda Manabu
Institute Of Physics University Of Tsukuba
-
SARGEANT A.
Nuclear Theory and Elementary Particle Phenomenology Group, Instituto de Fisica, Universidade de Sao
-
PATO M.
Nuclear Theory and Elementary Particle Phenomenology Group, Instituto de Fisica, Universidade de Sao
-
HUSSEIN M.
Nuclear Theory and Elementary Particle Phenomenology Group, Instituto de Fisica, Universidade de Sao
-
Pato M.
Nuclear Theory And Elementary Particle Phenomenology Group Instituto De Fisica Universidade De Sao P
-
Sargeant A.
Nuclear Theory And Elementary Particle Phenomenology Group Instituto De Fisica Universidade De Sao P
-
Hussein M.
Nuclear Theory And Elementary Particle Phenomenology Group Instituto De Fisica Universidade De Sao P
関連論文
- Fusion Reaction of Halo Nuclei : Proton Halo versus Neutron Halo
- Absorbing Boundary Condition Approach for Breakup Reactions of Halo Nuclei
- Evaluation of Effective Astrophysical S Factor for Non-Resonant Reactions
- Energy Averages over Regular and Chaotic States in the Decay Out of Superdeformed Bands
- Evaluation of Effective Astrophysical S Factor for Non-Resonant Reactions
- Attenuation of the Intensities within a Superdeformed Band (原子核の量子トンネル崩壊現象)
- Forward Nuclear Glory Scattering of a Halo Nucleus