Searching for Tetraneutron in Bismuth Nucleus Photodisintegration Reaction

IF 0.5 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY Journal of Contemporary Physics (Armenian Academy of Sciences) Pub Date : 2023-06-18 DOI:10.1134/S1068337223010127
T. V. Kotanjyan, A. Y. Aleksanyan, A. O. Kechechyan, S. M. Amirkhanyan, H. R. Gulkanyan, V. S. Pogosov, L. A. Poghosyan
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引用次数: 1

Abstract

At the linear electron accelerator AANL (YerPhI), at mean electron energies Êе = 28 and 30 MeV (with a Gaussian width σе ≈ 0.7 MeV), an attempt is undertaken to search for near-threshold production of the four-neutron system in the reaction 209Bi(γ,4n)205Bi (with the threshold energy \(E_{\gamma }^{{{\text{th}}}}\) = 29.5 MeV) induced by bremsstrahlung photons. The induced activity method was applied in the experiment. The gamma-spectroscopic measurements were carried out in the underground low background laboratory of the AANL. Owing to low-background conditions in the laboratory, one achieves, at Êе = 30 MeV, reliable identification of 205Bi radionuclide and the first determination of the near-threshold cross sections of this rare process, namely, the weighted by the spectrum of bremsstrahlung photons cross-section σw = (4.42 ± 0.48) × 10–4 mb and the averaged over the spectrum of bremsstrahlung photons cross-section \(\left\langle \sigma \right\rangle \) = (1.95 ± 0.22) mb. No 205Bi production was observed at Êе = 28 MeV. Low-background conditions allow one also to identify the rare decays of the 208Bi nucleus produced in the reaction 209Bi(γ, n)208Bi, and measure its weighted and averaged cross sections at Êе = 28 and 30 MeV: σw = (19.6 ± 3.5) and (16.4 ± 2.2) mb and \(\left\langle \sigma \right\rangle \) = (139 ± 25) and (142 ± 19) mb, respectively. From the data at Êе= 28 MeV, an upper limit of the yield of a hypothetical four-neutron bound state (tetraneutron) production reaction relative to the yield of the reaction 209Bi(γ, n)208Bi is estimated to be 10–5. The obtained experimental data are compared with predictions of the TALYS1.9 and FLUKA models. It is shown that the measured at Êе = 30 MeV cross-section of the reaction 209Bi(γ,4n)205Bi strongly overestimates (by more than one order of magnitude) the theoretical value. This disagreement can be caused by the fact that the models do not foresee the production of correlated neutron clusters, in particular, the four-neutron resonance state with 2.4 MeV excitation energy observed recently in the reaction 1H(8He, 1H + 4He)4n. The near-threshold production of the four-neutron system, observed in the present work, can, probably, serve as an indirect indication of its resonance nature.

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寻找铋核光分解反应中的四中子
在线性电子加速器AANL (YerPhI)上,在平均电子能Êе = 28和30 MeV(高斯宽度σ δ≈0.7 MeV)下,尝试寻找由轫致辐射光子诱导的209Bi(γ,4n)205Bi反应(阈值能量\(E_{\gamma }^{{{\text{th}}}}\) = 29.5 MeV)中四中子体系的近阈值产生。实验采用诱导活性法。伽玛光谱测量是在AANL地下低背景实验室进行的。在实验室低背景条件下,在Êе = 30 MeV下,实现了205Bi放射性核素的可靠鉴定,并首次测定了这一罕见过程的近阈值截面,即轫致辐射光子截面谱加权σw =(4.42±0.48)× 10 - 4mb和轫致辐射光子截面谱平均值\(\left\langle \sigma \right\rangle \) =(1.95±0.22)mb。在Êе = 28 MeV下,未观察到205Bi的产生。在低背景条件下,还可以识别209Bi(γ, n)208Bi反应中产生的罕见的208Bi核衰变,并测量其在Êе = 28和30 MeV时的加权和平均截面:σw =(19.6±3.5)和(16.4±2.2)mb, \(\left\langle \sigma \right\rangle \) =(139±25)和(142±19)mb。根据Êе= 28 MeV的数据,相对于反应209Bi(γ, n)208Bi的产率,假设的四中子束缚态(四中子)产生反应的产率上限估计为10-5。得到的实验数据与TALYS1.9和FLUKA模型的预测结果进行了比较。结果表明,在Êе = 30 MeV处测量到的209Bi(γ,4n)205Bi反应截面大大高估了理论值(超过一个数量级)。这种分歧可能是由于模型没有预见到相关中子团的产生,特别是最近在1H(8He, 1H + 4He)4n反应中观测到的激发能为2.4 MeV的四中子共振态。在本工作中观察到的四中子系统的近阈值产生,可能作为其共振性质的间接指示。
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来源期刊
CiteScore
1.00
自引率
66.70%
发文量
43
审稿时长
6-12 weeks
期刊介绍: Journal of Contemporary Physics (Armenian Academy of Sciences) is a journal that covers all fields of modern physics. It publishes significant contributions in such areas of theoretical and applied science as interaction of elementary particles at superhigh energies, elementary particle physics, charged particle interactions with matter, physics of semiconductors and semiconductor devices, physics of condensed matter, radiophysics and radioelectronics, optics and quantum electronics, quantum size effects, nanophysics, sensorics, and superconductivity.
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