Astrophysical S-factor of the radiative proton capture on 14C at low energies-Reference-Cited by-同舟云学术

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

Published:2014-08-07 Issue:24 Volume:29 Page:1450125
ISSN:0217-7323
Container-title:Modern Physics Letters A
language:en
Short-container-title:Mod. Phys. Lett. A

Author:

Dubovichenko Sergey¹²,Burtebaev Nasurlla²,Dzhazairov-Kakhramanov Albert¹²,Alimov Dilshod²

Affiliation:

1. V. G. Fessenkov Astrophysical Institute "NCSRT" NSA RK, 050020, Observatory 23, Kamenskoe Plato, Almaty, Kazakhstan

2. Institute of Nuclear Physics CAE MINT RK, 050032, Str. Ibragimova 1, Almaty, Kazakhstan

Abstract

The phase shift analysis for position location of the [Formula: see text] resonance at 1.5 MeV was carried out on the basis of the known experimental measurements of the excitation functions of the p14 C elastic scattering at four angles from 90° to 165° and more than 100 energy values in the range from 600–800 keV to 2200–2400 keV. Also, the possibility to describe the available experimental data on the astrophysical S-factor for the proton capture reaction on 14 C to the ground state (GS) of 15 N at astrophysical energies was considered in the frame of modified potential cluster model (MPCM).

Publisher

World Scientific Pub Co Pte Lt

Subject

General Physics and Astronomy,Astronomy and Astrophysics,Nuclear and High Energy Physics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0217732314501259

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