Measurement of the astrophysical S factor for dd interaction at ultralow deuteron-collision energies using the inverse Z pinch; Physics of Atomic Nuclei; Vol. 66, iss. 9

Dettagli Bibliografici
Parent link:Physics of Atomic Nuclei: Scientific Journal.— , 2000-
Vol. 66, iss. 9.— 2003.— [P. 1683-1690]
Altri autori: Bystritsky V. M., Gerasimov V. V., Krylov A. R., Parzhitski S. S., Pen'kov F. M., Shvyryaev O. M., Stolupin V. A,., Dudkin G. N. Nikolay Aleksandrovich, Nechaev B. A. Boris Aleksandrovich, Padalko V. N. Vladimir Nikolaevich, Wozniak J., Mesyats G. A. Gennady Andreyevich, Bystritskii V. M., Makhrin V. I., Ratakhin N. A. Nikolay Aleksandrovich
Riassunto:Title screen
This paper is devoted to measurement of the astrophysical S factor and cross sections of the d + d → 3He + n reaction at ultralow deuteron-collision energies. Formation of the flow of the accelerated deuterons incident on the CD2 solid-state target was made within the scheme of the inverse Z pinch. The liner in the initial state was a hollow supersonic deuterium jet of radius of 15 mm and length of 20 mm. The experiment was carried out at the pulsed high-current accelerator (I=950 kA, τ=80 ns) of the Institute of High-Current Electronics (Tomsk, Russia). Measurement of the deuteron energy distribution was performed through an analysis of the time distributions of the intensity of the liner radiation (Hα and Hβ lines) generated during the liner radial movement from the axis. Recording of this radiation was carried out by optical detectors placed along the direction of the liner moving from its axis.
Режим доступа: по договору с организацией-держателем ресурса
Lingua:inglese
Pubblicazione: 2003
Soggetti:
Accesso online:http://dx.doi.org/10.1134/1.1611583
Natura: Elettronico Capitolo di libro
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=653321