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 in | Nuclear science and techniques Vol. 29; no. 12; pp. 102 - 111 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
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. |
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ISSN: | 1001-8042 2210-3147 |
DOI: | 10.1007/s41365-018-0517-7 |