Published January 9, 2006 | Version v1
Journal article

Description of the 17F(p, γ)18Ne radiative capture reaction in the continuum shell model

  • 1. Grand Accelerateur National d'Ions Lourds (GANIL), CEA/DSM-CNRS/IN2P3, BP 55027, F-14076 Caen Cedex 05 (France)
  • 2. Institute of Nuclear Physics, Radzikowskiego 152, PL-31342 Krakow (Poland)

Description

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, γ)18Ne. The dominant contribution to the cross-section at very low-energies is due to M1 transitions Jiπ=2+->Jfπ=21+ whose magnitude is controlled by a weakly bound 22+ state at the excitation energy Ex=3.62MeV

Additional details

Identifiers

DOI
10.1016/j.nuclphysa.2005.10.002;
arXiv
arXiv:nucl-th/0509026v1;
PII
S0375-9474(05)01158-9;

Publishing Information

Journal Title
Nuclear Physics. A
Journal Volume
764
Journal Page Range
p. 528-550
ISSN
0375-9474
CODEN
NUPABL

Optional Information

Copyright
Copyright (c) 2005 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.