Astrophysical Radiative Neutron Capture on 10B Taking into Account Resonance at 475 keV - Open Access Library Journal

OALibJ > Vol.2 No.1, January 2015

Astrophysical Radiative Neutron Capture on ¹⁰B Taking into Account Resonance at 475 keV ()

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DOI: 10.4236/oalib.1101263 619 Downloads 1,158 Views

Author(s)

S. B. Dubovichenko^1,2*, A. V. Dzhazairov-Kakhramanov^1,2

Affiliation(s)

¹V. G. Fessenkov Astrophysical Institute “NCSRT” NSA, Almaty, Kazakhstan.
²Institute of Nuclear Physics CAE MINT RK, Almaty, Kazakhstan.

ABSTRACT

The possibility of the description of the available experimental data for cross sections of the neutron capture reaction on ¹⁰B at thermal and astrophysical energies, taking into account the resonance at 475 keV, was considered within the framework of the modified potential cluster model with forbidden states and accounting for the resonance behavior of the scattering phase shifts.

KEYWORDS

Nuclear Astrophysics, Primordial Nucleosynthesis, Light Atomic Nuclei, Low and Astrophysical Energies, Radiative Capture, Thermonuclear Processes

Share and Cite:

Dubovichenko, S. and Dzhazairov-Kakhramanov, A. (2015) Astrophysical Radiative Neutron Capture on ¹⁰B Taking into Account Resonance at 475 keV. Open Access Library Journal, 2, 1-13. doi: 10.4236/oalib.1101263.

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