Astrophysical S-factor of the radiative proton capture on 14C at low energies

2014/02/21 by S. B. Dubovichenko, N. Burtebaev, A. V. Dzhazairov-Kakhramanov +1 · 2 citations
Physics and Astronomy · #nucl-th

paper · pdf · doi:10.1142/s0217732314501259

published as Mod. Phys. Lett. A, Vol. 29, No. 24 (2014) 1450125 · 10 fig., 1 tab., 64 ref., 16p

arxiv created 2014/02/21 · arxiv updated 2014/07/30

Abstract

The phase shift analysis for position location of the 2S1/2 resonance at 1,5 MeV was carried out on the basis of the known experimental measurements. Also, the possibility to describe the available experimental data on the astrophysical S-factor for the proton capture reaction on 14C to the ground state of 15N at astrophysical energies was considered in the frame of modified potential cluster model.

Cited by

• Study of the neutron and proton capture reactions 10,11b(n, g), 11b(p, g), 14c(p, g), and 15n(p, g) at thermal and astrophysical energies
• Phase Shift Analysis of the p14C Scattering at the Energy of the 2S1/2 Resonance

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• Astrophysical S-factor of 14N(p,g)15O
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