Time-Dependent Analysis of the Coulomb Breakup Determination of the Astrophysical S Factor
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概要
- 論文の詳細を見る
The time-dependent mesh method is applied to the Coulomb breakup of a projectile into two charged fragments. The projectile is described in the potential model and its center of mass follows a classical trajectory. The astrophysical S factor extracted from this Coulomb breakup calculation is compared with the exact S factor derived under the same model assumptions. A study of the ^17F + ^208Pb ⟶ ^16O + p + ^208Pb breakup provides domains of validity of the extracted S factor for the ^16O(p,γ)^17F radiative capture reaction to the ^17F ground state.
- 理論物理学刊行会の論文
- 2002-12-26
著者
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Baye D
Physique Nucleaire Theorique Et Physique Mathematique Uriiversite Libre De Bruxelles
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Baye D.
Physique Nucleaire Theorique Et Physique Mathematique
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Baye D.
Physique Nucleaire Theorique Et Physique Mathematique C. P. 229 Universite Libre De Bruxelles
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MELEZHIK V.S.
Physique Nucleaire Theorique et Physique Mathematique, Uriiversite Libre de Bruxelles
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Melezhik V.s.
Physique Nucleaire Theorique Et Physique Mathematique Uriiversite Libre De Bruxelles:joint Institute
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Melezhik V.
Physique Nucleaire Theorique Et Physique Mathematique C. P. 229 Universite Libre De Bruxelles
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MELEZHIK V.S.
Physique Nucleaire Theorique et Physique Mathematique, Uriiversite Libre de Bruxelles:Joint Institute for Nuclear Research, Dubna
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