THE REACTION 8Li(n,γ)9Li AT ASTROPHYSICAL ENERGIES AND ITS ROLE IN PRIMORDIAL NUCLEOSYNTHESIS

Sergey Borisovich Dubovichenko, A. V. Dzhazairov-Kakhramanov

2016

Closed access Metadata (CSL-JSON)
DOI 10.3847/0004-637x/819/1/78
Data confidence 70 medium
How this score is calculated

It is built from checkable properties of the record itself: whether the article has a DOI, how many independent sources confirmed its data, whether the required fields are filled in, and how recent the latest confirmation is. Disagreement between sources and a missing identifier lower it. A value of 80 or above means the record was published without further checking; 60 to 79 means it is published at reduced confidence, with a manual check advisable. A record verified by an editor by hand is never pushed below 90 by a recalculation. This scores our data about the article, not the article itself.

Abstract

ABSTRACT The possibility of describing available experimental data for the total cross sections of neutron radiative capture on 8Li at thermal and astrophysical energies was considered within the framework of the modified potential cluster model with the state classification of nuclear particles according to the Young tableaux. Our approach allows one to transmit available data in the energy range 0.1–1.0 MeV quite well, and predicts the behavior of the total cross sections at super-low energies, down to 25.3 × 10−9 MeV.