Constraints on the appearance of a maximum in astrophysical S-factor

Bibliographic Details
Parent link:	Physics Letters B Vol. 824.— 2022.— [136792, 5 p.]
Corporate Author:	Национальный исследовательский Томский политехнический университет Школа базовой инженерной подготовки Отделение математики и информатики
Other Authors:	Sargsyan V. V. Vazgen Valerikovich, Adamyan G. G. Gurgen Grigorjevich, Antonenko N. V. Nikolay Viktorovich, Lenske H. Horst
Summary:	Title screen For fusion reactions of astrophysical interest, the existence of a maximum of S-factor is revealed within the extended quantum diffusion approach. The available experimental data are well described. The reason and consequences of the existence of the S-factor maximum are explained. An universal formula for the position of the maximum is proposed.
Published:	2022
Subjects:	электронный ресурс труды учёных ТПУ astrophysical S-factor deep sub-barrier fusion (capture) dissipative dynamics астрофизический S-фактор диссипативная динамика
Online Access:	https://doi.org/10.1016/j.physletb.2021.136792
Format:	Electronic Book Chapter
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=669489

Description
Summary:	Title screen For fusion reactions of astrophysical interest, the existence of a maximum of S-factor is revealed within the extended quantum diffusion approach. The available experimental data are well described. The reason and consequences of the existence of the S-factor maximum are explained. An universal formula for the position of the maximum is proposed.
DOI:	10.1016/j.physletb.2021.136792

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