Study of the 3H(1H, γ)4He Reaction in the Energy Range 12-34 keV; Journal of Experimental and Theoretical Physics; Vol. 135, iss. 3

Study of the 3H(1H, γ)4He Reaction in the Energy Range 12-34 keV; Journal of Experimental and Theoretical Physics; Vol. 135, iss. 3

Bibliografske podrobnosti
Parent link:	Journal of Experimental and Theoretical Physics Vol. 135, iss. 3.— 2022.— [P. 291-303]
Corporate Authors:	Национальный исследовательский Томский политехнический университет Физико-технический институт Лаборатория № 33 ядерного реактора, Национальный исследовательский Томский политехнический университет Инженерная школа новых производственных технологий Научно-производственная лаборатория "Импульсно-пучковых, электроразрядных и плазменных технологий"
Drugi avtorji:	Varlachev V. A. Valery Aleksandrovich, Dudkin G. N. Gennadiy Nikolaevich, Nechaev B. A. Boris Aleksandrovich, Penkov F. M. Fedor Mikhaylovich, Filippov A. V. Aleksandr Viktorovich
Izvleček:	Title screen The study of the 3H(1H, ?)4He reaction is of relevance for both nuclear physics and nuclear astrophysics. In nuclear astrophysics, more accurate data should be obtained on the rate of primordial nucleosynthesis reactions that lead to the production of 4He. In nuclear physics, there are theoretical models in which the behavior of the cross section and the S-factor of this reaction in the energy range of the order of tens of keV are in poor agreement with experiment. Thereby, more accurate experimental study of S-factor behavior should be performed in the astrophysical energy range. The experimentally obtained values of the yields for various energies of 1H+ ions were used to describe the behavior of the 3H(1H, ?)4He reaction S-factor depending on the energy. As a result, the accuracy of determination of the S-factor of the 3H(1H, ?)4He reaction has been improved several times. Режим доступа: по договору с организацией-держателем ресурса
Jezik:	angleščina
Izdano:	2022
Serija:	Nuclei, particles, fields, gravitation, and astrophysics
Teme:	электронный ресурс труды учёных ТПУ ядерная физика нуклеосинтез энергия астрофизика
Online dostop:	https://doi.org/10.1134/S1063776122080143
Format:	Elektronski Book Chapter
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=668505

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