dorsal/arxiv
View SchemaDescription of the 17F(p,gamma)18Ne radiative capture reaction in the continuum shell model
| Authors | R. Chatterjee, J. Okolowicz, M. Ploszajczak |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0509026 |
| URL | https://arxiv.org/abs/nucl-th/0509026 |
| DOI | 10.1016/j.nuclphysa.2005.10.002 |
| Journal | Nucl.Phys. A764 (2006) 528-550 |
Abstract
The shell model embedded in the continuum is applied to calculate the astrophysical S-factor and the reaction rate for the radiative proton capture reaction 17F(p,gamma)18Ne. The dominant contribution to the cross-section at very low energies is due to M1 transitions J_i^pi = 2^+ --> J_f^pi = 2_1^+ whose magnitude is controlled by a weakly bound 2_2^+ state at the excitation energy E_x = 3.62 MeV.
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"abstract": "The shell model embedded in the continuum is applied to calculate the\nastrophysical S-factor and the reaction rate for the radiative proton capture\nreaction 17F(p,gamma)18Ne. The dominant contribution to the cross-section at\nvery low energies is due to M1 transitions J_i^pi = 2^+ --\u003e J_f^pi = 2_1^+\nwhose magnitude is controlled by a weakly bound 2_2^+ state at the excitation\nenergy E_x = 3.62 MeV.",
"arxiv_id": "nucl-th/0509026",
"authors": [
"R. Chatterjee",
"J. Okolowicz",
"M. Ploszajczak"
],
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"nucl-th",
"astro-ph",
"nucl-ex"
],
"doi": "10.1016/j.nuclphysa.2005.10.002",
"journal_ref": "Nucl.Phys. A764 (2006) 528-550",
"title": "Description of the 17F(p,gamma)18Ne radiative capture reaction in the continuum shell model",
"url": "https://arxiv.org/abs/nucl-th/0509026"
},
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