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Study of 19F Levels with Ex = 6.7 - 7.7 MeV by the 15N+α Scattering Experiment
The intense γ -rays from classical novae are emitted due to the β -decay of 18 F which is produced by the Hot-CNO cycle. The reaction rate of 18 F( p , α ) 15 O affects the prediction of the abundance of 18 F. The main contribution to this reaction rate is from the resonances in 19 Ne near and above...
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Published in: | Journal of the Korean Physical Society 2018, 73(3), , pp.265-270 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | The intense
γ
-rays from classical novae are emitted due to the
β
-decay of
18
F which is produced by the Hot-CNO cycle. The reaction rate of
18
F(
p
,
α
)
15
O affects the prediction of the abundance of
18
F. The main contribution to this reaction rate is from the resonances in
19
Ne near and above the proton threshold. Hence, many experiments and theoretical works have been performed on the low-lying
18
F+
p
resonances. One of the methods for investigating
19
Ne parameters is studying the mirror nucleus
19
F. α elastic scattering experiment was performed with a 7 MeV/u
15
N beam for investigating the resonance parameters in
19
F using the thick target method in inverse kinematics at the radioactive beam facility CRIB of the Center for Nuclear Study, the University of Tokyo. The excitation function of
19
F was obtained for the excitation energy
E
x
= 6.7 - 7.7 MeV, and the parameters of the resonance states in
19
F were determined using an R-matrix analysis. |
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ISSN: | 0374-4884 1976-8524 |
DOI: | 10.3938/jkps.73.265 |