Mean-field description of heavy-ion scattering at low energies and fusion

The nuclear mean-field potential built up during the 12 C + 12 C and 16 O + 16 O collisions at low energies relevant for the carbon- and oxygen-burning processes is constructed within the double-folding model (DFM) using the realistic ground-state densities of 12 C and 16 O, and CDM3Yn density-depen...

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Published inNuclear science and techniques Vol. 29; no. 12; pp. 102 - 111
Main Authors Khoa, Dao T., Chien, Le Hoang, Cuong, Do Cong, Phuc, Nguyen Hoang
Format Journal Article
LanguageEnglish
Published Singapore Springer Singapore 01.12.2018
Department of Nuclear Physics and Nuclear Engineering, Faculty of Physics and Engineering Physics, University of Science, VNU-HCM, 227 Nguyen Van Cu Street, District 5, Ho Chi Minh City, Vietnam
Institute for Nuclear Science and Technology, VINATOM, 179 Hoang Quoc Viet, Hanoi, Vietnam%Institute for Nuclear Science and Technology, VINATOM, 179 Hoang Quoc Viet, Hanoi, Vietnam
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Summary:The nuclear mean-field potential built up during the 12 C + 12 C and 16 O + 16 O collisions at low energies relevant for the carbon- and oxygen-burning processes is constructed within the double-folding model (DFM) using the realistic ground-state densities of 12 C and 16 O, and CDM3Yn density-dependent nucleon–nucleon (NN) interaction. The rearrangement term, indicated by the Hugenholtz–van Hove theorem for the single-particle energy in nuclear matter, is properly considered in the DFM calculation. To validate the use of the density-dependent NN interaction at low energies, an adiabatic approximation was suggested for the dinuclear overlap density. The reliability of the nucleus–nucleus potential predicted through this low-energy version of the DFM was tested in the optical model (OM) analysis of the elastic 12 C + 12 C and 16 O + 16 O scattering data at energies below 10 MeV/nucleon. These OM results provide a consistently good description of the elastic angular distributions and 90 ∘ excitation function. The dinuclear mean-field potential predicted by the DFM is further used to determine the astrophysical S factor of the 12 C + 12 C and 16 O + 16 O fusions in the barrier penetration model. Without any adjustment of the potential strength, our results reproduce the non-resonant behavior of the S factor of the 12 C + 12 C and 16 O + 16 O fusions very well over a wide range of energies.
ISSN:1001-8042
2210-3147
DOI:10.1007/s41365-018-0517-7