Measurement of fusion cross sections for 14N + 14N and 12C + 16O at low energles☆
References (41)
- et al.
Nucl. Phys.
(1971) - et al.
Nucl. Phys.
(1974) - et al.
Nucl. Phys.
(1976) - et al.
Nucl. Phys.
(1969) - et al.
Nucl. Phys.
(1976) - et al.
Nucl. Instr.
(1975) - et al.
Nucl. Instr.
(1975) - et al.
Nucl. Phys.
(1973) - et al.
Nucl. Phys.
(1976) - et al.
Nucl. Phys.
(1969)
Nucl. Phys.
Phys. Rev.
Astrophys. J. Supp.
Principles of stellar evolution and nucleosynthesis
Europhysics Study conf. on intermediate processes in nuclear reactions
Springer Verlag Lecture Notes in Physics
Phys. Rev.
Phys. Rev.
Phys. Rev.
Phys. Rev.
Cited by (42)
Systematic study of fusion barriers with energy dependent barrier radius
2023, Atomic Data and Nuclear Data TablesMeasurement of the cross-section of <sup>14</sup>N(<sup>16</sup>O,α) <sup>26</sup>Al with AMS
2005, Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and AtomsCitation Excerpt :The results of the 14N(16O,α)26Al cross section together with relevant parameters, the effective energies of 16O, the 26Al/27Al ration, the weight of 27Al carrier, the dose of 16O beam and the thickness of TiN targets are summarized in Table 1. In Switkowskip’s work [4] the γ-ray (417 keV) photopeak area were corrected for summing and branching effects [7] and converted to cross-sections for the production of specific evaporation residues (26Al), and these cross-sections were given in Fig. 6 of [4]. For the evaporation residues of 26Al, not all the populating levels will transition to the ground level (5+) which have the half-life of 7.4 × 105 yr, there are many levels will transition to the metastable state 0+, the metastable state will decay to 26Mg.
Heavy ion reactions below the Coulomb barrier
1994, Nuclear Physics, Section AThe competition between p<sup>2</sup>n, dn AND t emission in heavy-ion induced nuclear reactions
1990, Nuclear Physics, Section ASubbarrier fusion of atomic nuclei
1985, Physics Reports
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Supported in part by the National Science Foundation [PHY76-02724].
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Present address: School of Physics, University of Melbourne, Parkville, 3052m Australia.
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Operated by Union Carbide Corp. for the Energy Research and Development Administration.
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Present address: Physics Divisionm Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830, USA.
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Present address: Franklin and Marshall College, Lancaster, Pa. 17604, USA.