Study of astrophysical S-factor, S (E) and thermonuclear fusion reaction rate, TNFRR for some α-trapped interactions

Diverse types of reactions among nuclei occurring at the interior of stars which are at the accreting stage are tremendously affected by plasma environment of high density. Nuclear fusions at very low energy end (~ keV), much below the mutual Coulomb potential barrier, play a pivotal role in the Big...

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Bibliographic Details
Main Authors: Mohammad N., Mondal S.H., Islam Rabiul, Khan Abdul
Format: Article
Language:English
Published: EDP Sciences 2025-01-01
Series:EPJ Web of Conferences
Subjects:
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2025/10/epjconf_iemphys2025_01010.pdf
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