Using a hall accelerator to investigate d(d, n)3He and d(p, γ)3He reactions in the astrophysical energy region

Bibliographic Details
Parent link:	Bulletin of the Russian Academy of Sciences: Physics: Scientific Journal Vol. 74, iss. 4.— 2010.— [P. 531-534]
Other Authors:	Bystritsky V. M., Gerasimov V. V., Krylov A. R., Parzhitskii S. S., Il’guzin D. A., Anan’in P. S., Dudkin G. N. Gennadiy Nikolaevich, Kaminsky V. L. Valery Ludvigovich, Nechaev B. A. Boris Aleksandrovich, Padalko V. N. Vladimir Nikolaevich, Petrov A. V., Mesyats G. A. Gennady Andreyevich, Filipowicz M., Wozniak J., Bystritskii Vit. M.
Summary:	Title screen We present new results on astrophysical S-factors and cross sections for reactions dd → 3He + n(2.5MeV) and pd → 3He + γ (5.5MeV) in ultra-low energy ranges 2.3-6.2 keV and 8.3-10.1 keV, respectively. Experiments were performed with proton and neutron beams produced by a pulsed Hall accelerator (Nuclear Physics Institute, Tomsk) and deuterated polyethylene (CD2) and frozen heavy water (D2O) targets. Within measurement errors, our results are consistent with the literature's experimental results on pd and dd reactions for the given energy ranges, where D2O or gaseous deuterium targets were used. Режим доступа: по договору с организацией-держателем ресурса
Published:	2010
Subjects:	электронный ресурс труды учёных ТПУ
Online Access:	http://dx.doi.org/10.3103/S1062873810040234
Format:	Electronic Book Chapter
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=641596

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