14N fusion with 13C and 16O at sub-barrier energies☆
References (15)
- et al.
Nucl. Phys.
(1976)et al.Nucl. Phys.
(1976) - et al.
Phys. Rev. Lett.
(1976) - et al.
Nucl. Data Tables
(1970) - et al.
Phys. Rev. Lett.
(1976) - et al.
Nucl. Phys.
(1976) - et al.
Cited by (40)
Systematic study of fusion barriers with energy dependent barrier radius
2023, Atomic Data and Nuclear Data TablesAMS measurement of <sup>26</sup>Al cross section for the reaction <sup>14</sup>N(<sup>16</sup>O,α)<sup>26</sup>Al<sup>g</sup>
2007, Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and AtomsCitation Excerpt :In order to estimate the contribution of this reaction in the galaxy, its excitation function is needed. There is so far only one work to measure the total fusion cross section of the 16O + 14N by determining prompt γ-rays emitted in the reaction with a thick quartz disk as an oxygen-containing target [4]. Some interesting pieces of work have been carried out to measure cross sections with AMS technique for its high sensitivity for long-lived nuclides measurement e.g. [5,6].
Measurement 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 :There is one opinion that the reaction of 14N(16O,α)26Al may be one of the sources of the 1.809 MeV γ-rays in the interstellar medium during the supernova explosion, such as SNIa[3]. The cross-sections of this reaction have been measured by determining prompt γ-ray emitted in the reaction using a thick quartz disk as an oxygen-containing target [4]. In present work, the cross-sections of these reactions were measured in the sub-barrier energy region using AMS.
The extended optical model with dispersion relation for the fusion of light heavy-ion systems
1994, Nuclear Physics, Section AHeavy ion reactions below the Coulomb barrier
1994, Nuclear Physics, Section A
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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 3052, Australia.
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Operated by Union Carbide Corp. for the Energy Research and Development Administration.
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Present address: Franklin and Marshall College, Lancaster, Pennsylvania 17604,USA.