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035 _a(RuTPU)RU\TPU\network\15027
035 _aRU\TPU\network\14343
090 _a649857
100 _a20160829a2016 k y0engy50 ba
101 0 _aeng
135 _adrcn ---uucaa
181 0 _ai
182 0 _ab
200 1 _aA method for investigation of the D(4He, γ)6Li reaction in the Ultralow energy region under a high background
_fV. M. Bystritsky [et al.]
203 _aText
_celectronic
300 _aTitle screen
320 _a[References: p. 30 (30 tit.)]
330 _aThe cosmological lithium problem, that is, a noticeable discrepancy between the predicted and observed abundances of lithium, is in conflict with the Standard Big Bang Nucleosynthesis model. For example, the abundance of 7Li is 2-4 times smaller than predicted by the Standard Big Bang Nucleosynthesis. As to the abundance of 6Li, recent more accurate optical investigations have yielded only the upper limit on the 6Li/7Li ratio, which makes the problem of 6Li abundance and accordingly of disagreement with the Standard Big Bang Nucleosynthesis predictions less acute. However, experimental study of the D(4He, γ)6Li reaction cross section is still of current importance because there is a theoretical approach predicting its anomalously large value in the region of energies below the Standard Big Bang Nucleosynthesis energy. The work is dedicated to the measurement of the cross section for the D(4He, γ)6Li reaction proceeding in zirconium deuteride at the incident 4He+ion energy of 36 keV. The experiment is performed at a pulsed Hall plasma accelerator with an energy spread of 20% FWHM. A method for direct measurement of the background from the reaction chain D(4He,4He)D→D(D, n)3He→(n, γ) and/or (n, n′γ) ending with activation of the surrounding material by neutrons is proposed and implemented in the work. An upper limit on the D(4He, γ)6Li reaction cross section σ≤7·10−36 cm2 at the 90% confidence level is obtained.
333 _aРежим доступа: по договору с организацией-держателем ресурса
461 _tNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
_d1984-
463 _tVol. 825
_v[P. 24-30]
_d2016
610 1 _aэлектронный ресурс
610 1 _aтруды учёных ТПУ
701 1 _aBystritsky
_bV. M.
_gVyacheslav Mikhaylovich
701 1 _aDudkin
_bG. N.
_cspecialist in the field of nuclear physics
_cSenior researcher of Tomsk Polytechnic University, Candidate of physical and mathematical sciences
_f1944-
_gGennadiy Nikolaevich
_2stltpush
_3(RuTPU)RU\TPU\pers\34190
701 1 _aKrylov
_bA. R.
_gAleksandr Romanovich
701 1 _aGazi
_bS.
_gStefan
701 1 _aGuran
_bYe.
_gYezhek
701 1 _aNechaev
_bB. A.
_cphysicist
_cleading engineer of Tomsk Polytechnic University
_f1945-
_gBoris Aleksandrovich
_2stltpush
_3(RuTPU)RU\TPU\pers\34601
701 1 _aPadalko
_bV. N.
_cphysicist
_cLeading engineer of Tomsk Polytechnic University
_f1949-
_gVladimir Nikolaevich
_2stltpush
_3(RuTPU)RU\TPU\pers\32978
701 1 _aSadovsky
_bA. B.
_gAndrey Borisovich
701 1 _aTuleushev
_bYu. Zh.
_gYury Zhianshakhovich
701 1 _aFilipovich
_bM.
_gMarius
701 1 _aFilippov
_bA. V.
_gAleksandr Viktorovich
712 0 2 _aНациональный исследовательский Томский политехнический университет (ТПУ)
_bФизико-технический институт (ФТИ)
_bЛаборатория № 33 ядерного реактора
_h6474
_2stltpush
_3(RuTPU)RU\TPU\col\19896
801 2 _aRU
_b63413507
_c20161031
_gRCR
856 4 _uhttp://dx.doi.org/10.1016/j.nima.2016.04.034
942 _cCF