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Decay Properties of 253, 255Rf Using the Relativistic Mean-Field Framework within the Preformed Cluster-Decay Model 在预制簇衰变模型中利用相对论均场框架研究 253、255Rf 的衰变特性
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060249
J. T. Majekodunmi, N. Jain, K. Anwar, N. Abdullah, R. Kumar, M. Bhuyan

Most neutron-deficient α emitters are known to be of great relevance to the astrophysical rapid neutron capture process in superheavy nuclei. Therefore, in the present work, the decay properties of newly observed superheavy nuclei with Z = 102, i.e., (^{{249}})No isotope from the α-decay of (^{{253}})Rf is theoretically investigated using the relativistic mean field (RMF) framework and the NL3* parameter set within the preformed cluster-decay model (PCM). The α-decay chain of (^{{255}})Rf is also considered. The RMF densities are folded with the R3Y nucleon-nucleon (NN) potential to deduce the nuclear interaction potential between the decaying fragments. A complete understanding of the penetration of an α-particle across the nuclear Coulomb barrier gives outstanding credence to the assumptions of quantum mechanics. The presence of shell/sub-shell closure is indicated by the formation of peaks along the decay chain and was found to alter the conventional scaling factor observed earlier in the results of the PCM. The calculated half-lives are in close agreement with recent experimental measurements.

众所周知,大多数中子缺陷α发射体与超重原子核的天体物理快速中子俘获过程密切相关。因此,在本研究中,使用相对论平均场(RMF)框架和预制簇衰变模型(PCM)中的NL3*参数集,对新观测到的Z=102的超重核,即来自(^{{249}})Rf的α衰变的(^{253}})No同位素的衰变特性进行了理论研究。同时还考虑了 α-decay chain of (^{{255}})Rf。用 R3Y 核子-核子(NN)势折叠 RMF 密度,从而推导出衰变碎片之间的核相互作用势。对 α 粒子穿过核库仑势垒的完整理解,使量子力学的假设得到了充分的证实。沿衰变链形成的峰值表明存在壳/亚壳闭合,并发现它改变了先前在 PCM 结果中观察到的传统缩放因子。计算得出的半衰期与最近的实验测量结果非常吻合。
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引用次数: 0
Monitoring and Control System for the SRC Experiment at BM@N 用于 BM@N 的 SRC 实验的监测和控制系统
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060365
T. Smolyanin, D. S. Egorov, R. V. Nagdasev, V. B. Shutov

The SRC (Short Range Correlation) [1] experiment searches for short-period two-nucleon correlations using the detector subsystems of the BM@N (Baryonic Matter at Nuclotron) facility. Р•xperiments of this kind require an easy-to-operate, reliable system for controlling and monitoring the slowly changing parameters of the experimental hardware. These parameters are high and low supply voltages, environmental parameters, data from gas subsystems, etc. The equipment very often comes from a large number of hardware manufacturers. The Slow Control System provides solutions to the following tasks: control and monitoring parameters of detectors and other subsystems. During the operation of the experimental facility, timely detection of failures in operation and alarming of emergencies, monitoring of environmental parameters are vitally important. Archiving of facility parameters in the database for further use in the analysis of experimental data is also provided.

SRC(短程相关)[1] 实验利用 BM@N(核光子重子物质)设施的探测器子系统搜索短周期双核相关性。这类 Р 实验需要一个易于操作的可靠系统来控制和监测实验硬件的缓慢变化参数。这些参数包括高低电源电压、环境参数、气体子系统数据等。这些设备通常来自众多硬件制造商。慢速控制系统为以下任务提供解决方案:控制和监测探测器及其他子系统的参数。在实验设施的运行过程中,及时发现运行中的故障并发出紧急警报、监测环境参数都是至关重要的。此外,还可将设施参数存入数据库,以便在分析实验数据时进一步使用。
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引用次数: 0
An Isomonodromic Approach to Scalar Fields on Sasaki–Einstein Spaces Yp, q 笹木-爱因斯坦空间 Yp, q 上标量场的等单旋转方法
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060043
V. Avramov, R. Rashkov, T. Vetsov

In this study, we investigate the Schrödinger equation equation for scalar particles on the Yp, q. An equation of general Heun type is obtained for one of the coordinates and its associated Painlevé VI equation is derived. Consequently, we take some particular limits of the Yp,q geometry, which result in a coalescence of singularities of the equation of motion. Finally, the associated isomondromic flows are examined.

在这项研究中,我们研究了 Yp, q 上标量粒子的薛定谔方程。我们得到了其中一个坐标的一般 Heun 型方程,并推导出与之相关的 Painlevé VI 方程。因此,我们对 Yp,q 几何图形进行了一些特殊的限制,这导致了运动方程奇点的凝聚。最后,我们对相关的等容流动进行了研究。
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引用次数: 0
Schwinger–Dyson Equation for Quarks in a QCD Inspired Model QCD 启发模型中的夸克施文格-戴森方程
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060341
V. I. Shilin, V. N. Pervushin

We discuss formulation of QCD in Minkowski–spacetime and effect of an operator product expansion by means of normal ordering of fields in the QCD Lagrangian. The formulation of QCD in the Minkowski–spacetime allows us to solve a constraint equation and decompose the gauge field propagator in the sum of an instantaneous part, which forms a bound state, and a retarded part, which contains the relativistic corrections. In Quantum Field Theory, for a Lagrangian with unordered operator fields, one can make normal ordering by means of the operator product expansion, then the gluon condensate appear. This gives us a natural way of obtaining a dimensional parameter in QCD, which is missing in the QCD Lagrangian. We derive a Schwinger–Dyson equation for a quark, which is studied both numerically and analytically. The critical value of the strong coupling constant ({{alpha }_{s}} = {4 mathord{left/ {vphantom {4 pi }} right. kern-0em} pi }), above which a nontrivial solution appears and a spontaneous chiral symmetry breaking occurs, is found. For the sake of simplicity, the considered model describes only one flavor massless quark, but the methods can be used in more general case. The Fourier-sine transform of a function with log-power asymptotic was performed.

我们讨论了闵科夫斯基时空中的 QCD 形式,以及通过对 QCD 拉格朗日中的场进行正常排序来实现算子乘积展开的效果。在闵科夫斯基时空中的 QCD 表述允许我们求解约束方程,并将规量场传播子分解为瞬时部分(形成束缚态)和迟滞部分(包含相对论修正)之和。在量子场论中,对于无序算子场的拉格朗日,我们可以通过算子乘积展开进行正常排序,然后出现胶子凝聚态。这为我们提供了一种自然的方法来获得 QCD 拉格朗日中缺少的维度参数。我们推导了夸克的施文格-戴森方程,并对其进行了数值和分析研究。强耦合常数的临界值({{alpha }_{s}} = {4 mathord{left/ {vphantom {4 pi }}.right.kern-0em}),在此之上会出现一个非微观解,并发生自发的手性对称破缺。为了简单起见,所考虑的模型只描述了一种味道的无质量夸克,但这些方法可以用于更一般的情况。对具有对数幂渐近的函数进行了傅里叶正弦变换。
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引用次数: 0
A Remark on the q-Hypergeometric Integral Bailey Pair and the Solution to the Star-Triangle Equation 关于 q-超几何积分贝利对和星三角方程解法的备注
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060080
E. Catak

We rewrite the recently constructed q-hypergeometric integral Bailey pair in a general form. Then with the help of the Bailey pair and (q)-beta hypergeometric sum-integral, we construct the star-triangle relation.

我们以一般形式重写了最近构建的 q- 超几何积分贝利对。然后,借助贝利对和(q)-beta 超几何和积分,我们构建了星三角关系。
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引用次数: 2
Anisotropy of Prompt Fission Neutron Spectra of 239Pu(n, F) and 235U(n, F) 239Pu(n, F) 和 235U(n, F) 裂变中子谱图的各向异性
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060262
V. M. Maslov

Angular anisotropy of secondary neutrons is evidenced in neutron emission spectra (NES) and prompt fission neutron spectra (PFNS). In case of NES that is due to angular dependence of elastic scattering, direct excitations of discrete collective levels and pre-equilibrium/direct emission of (n, nX)1 neutrons, while in case of PFNS it is because of these neutrons are evidenced in exclusive pre-fission neutrons in (nxnf)1. In 239Pu(n, xnf)1,...x and 235U(n, xnf)1,...x PFNS demonstrate different responses to forward and backward (n, xnf)1 neutrons emission with respect to the incident neutron momentum. Average energy of (n, nf)1 neutrons depends on the emission angle θ, i.e., fission cross section, prompt neutron number and total kinetic energy depend on θ as well. Exclusive neutron spectra (n, xnf)1,...x at θ ~ 90° are consistent with 235U(nF)(235U(n, xn)) and 239Pu(n, F)(239Pu(n, xn)) reaction cross sections within En ~ 0.01–20 MeV energy range. Exclusive neutron spectra of (n, xnf)1,..x, (n, nγ) and (n, xn)1,...x are calculated within Hauser–Feshbach formalism alongside with (n, F) and (n, хn) reaction cross sections, angular dependence of first neutron (nnX)1 emission (omega (theta )) being included. Approximation obtained for (omega (theta )) fits the measured NES at 14 MeV. The correlation of angular dependence of (n, xnf)1 neutron emission with emissive fission (n, xnf) contribution to the observed fission cross section and angular anisotropy of NES. The ratios of mean PFNS energies (leftlangle E rightrangle ) for forward and backward emission of 235U(n, xnf) and 239Pu(n, xnf) pre-fission neutrons are consistent with measured data.

在中子发射光谱(NES)和瞬裂变中子谱(PFNS)中可以看到二次中子的角度各向异性。在 NES 中,这是由于弹性散射的角度依赖性、离散集合级的直接激发以及 (n,nX)1 中子的预平衡/直接发射造成的;而在 PFNS 中,则是由于这些中子在 (n,xnf)1 中表现为排他性的预裂变中子。在 239Pu(n,xnf)1,...x 和 235U(n,xnf)1,...x 中,PFNS 对正向和反向(n, xnf)1 中子发射的反应与入射中子动量不同。(n,nf)1 中子的平均能量取决于发射角 θ,即裂变截面、迅速中子数和总动能也取决于 θ。θ~90°时的专属中子谱(n,xnf)1,...x 与 En ~ 0.01-20 MeV 能量范围内的 235U(n, F)(235U(n, xn)) 和 239Pu(n, F)(239Pu(n, xn)) 反应截面一致。在 Hauser-Feshbach 公式中计算了(n, xnf)1,...x, (n, nγ) 和 (n, xn)1,...x 的专属中子谱,同时还计算了(n, F)和(n, хn)反应截面,包括第一中子(n, nX)1 发射的角度依赖性(omega (theta ) )。所得到的(omega (theta ))近似值与14 MeV时测得的NES相吻合。n,xnf)1 中子发射的角度依赖性与发射裂变(n,xnf)对观测到的裂变截面和 NES 的角度各向异性的贡献的相关性。235U(n, xnf)和239Pu(n, xnf)前裂变中子向前和向后发射的平均PFNS能量之比(左角和右角)与测量数据一致。
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引用次数: 0
Study of the Medical Isotope 177Lu Production in Photonuclear Reactions on 178Hf-Enriched Targets 在富集 178Hf 靶件的光核反应中生产医用同位素 177Lu 的研究
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060420
M. V. Zheltonozhskaya, P. D. Remizov, A. P. Chernyaev, V. N. Yatsenko, S. L. Burtsev

This paper presents the results of studying the yield averaged over the bremsstrahlung flux of the promising medical radioisotope 177Lu in the (γ, p) reaction from hafnium targets enriched in 178Hf (92%) after irradiation with electron bremsstrahlung at a cutoff energy of 55 MeV. An assessment is made of the conditions under which the 177Lu can be produced in quantities necessary for nuclear medicine. The amount of 177mLu and other accompanying isotopes of lutetium that form simultaneously with 177Lu in the proposed production method is estimated.

本文介绍了对富含 178Hf (92%)的铪靶经过截止能量为 55 MeV 的电子轫致辐射辐照后,在(γ,p)反应中产生的有前途的医用放射性同位素 177Lu 的轫致辐射通量平均值的研究结果。对在何种条件下可以生产出核医学所需的 177Lu 数量进行了评估。估算了在拟议生产方法中与 177Lu 同时形成的 177mLu 和其他伴随镥同位素的数量。
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引用次数: 0
Research and Development of the Polarized Deuteron Source for the Electrostatic Accelerator 静电加速器极化氘核源的研究与开发
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060146
I. V. Gapienko, D. V. Belov, A. N. Fedorov, G. M. Gurevich, Yu. A. Plis, Yu. A. Usov

The prototype of polarized deuteron source was made for the Van de Graaff accelerator of the Czech Technical University in Prague with aim to create full scale setup for producing polarized neutron beam for experiments on measurement (Delta {{sigma }_{{text{L}}}}) and (Delta {{sigma }_{{text{T}}}}), longitudinal and transversal spin asymmetries in transmission polarized neutron beam through frozen polarized deuteron target. It is based on Kaminsky’s experiment on channeling deuterons through a magnetized Ni single crystal foil of 1–2 μm. It is proposed to use the reaction T({{(d,n)}^{4}})He with polarized deuterons of an energy 150–200 keV. For a nonchanneled beam (the goniometer in a random position), the tensor polarization measurements were carried out with a TiT target. Our result is ({{P}_{{zz}}} = - 0.10 pm 0.02). This result indicates that deuterium atoms that have passed outside the channels also become polarized due to the capture of polarized electrons from the nickel crystal.

偏振氘核源的原型是为布拉格捷克技术大学的范德格拉夫加速器制造的,目的是为产生偏振中子束制造全尺寸装置,用于测量通过冷冻偏振氘核靶的透射偏振中子束中的(△{{sigma }_{text{L}}}})和(△{{sigma }_{{text{T}}}})、纵向和横向自旋不对称。它是基于卡明斯基关于引导氘核通过 1-2 μm 的磁化镍单晶箔的实验。建议使用能量为 150-200 keV 的极化氘核与 T({{(d,n)}^{4}})He 反应。对于非通道光束(测角器处于随机位置),张量极化测量是用一个 TiT 靶进行的。我们的结果是({{P}_{zz}}} = - 0.10 pm 0.02)。这一结果表明,由于俘获了镍晶体中的极化电子,通过通道外的氘原子也会发生极化。
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引用次数: 0
Parton Distribution Function of Positron in Electron in QED QED 中电子中正电子的粒子分布函数
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S1547477123060407
U. E. Voznaya, A. B. Arbuzov

Iterative solution of the evolution equation of parton distribution functions in QED is discussed. The results for the functions of positron-in-electron type are given in the next-to-leading logarithmic approximation.

讨论了 QED 中粒子分布函数演化方程的迭代求解。在次导对数近似中给出了正电子-电子型函数的结果。
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引用次数: 0
Study of the Temperature Stability of the High-Voltage DAC AD5535 for Powering Silicon Photomultipiers 用于为硅光电倍增器供电的高压 DAC AD5535 的温度稳定性研究
IF 0.5 Q3 Physics and Astronomy Pub Date : 2023-12-04 DOI: 10.1134/S154747712306033X
A. S. Selyunin, N. V. Anfimov, A. V. Rybnikov, D. V. Fedoseev, V. I. Sharov

In this paper we present the results of a study of a high-voltage 32-channel DAC AD5535 for powering silicon photomultipliers. Built-in high-voltage buffer amplifiers allow output voltage regulation in the range of up to 200 V which provides application for a broad SiPM types including their serial connection. The significant output current of 500 μA/ch allows biasing the SiPM arrays and assemblies. The documentation indicates a significant temperature dependence of (sim ~200~) ppm/C which limits the use of DAC for SiPM powering. This work demonstrates the excellent temperature stability of the chip. Still since the manufacturer does not guarantee this an express method of channel-by-channel measurement of temperature dependence has been developed for a mass use of the AD5535 DAC

本文介绍了用于为硅光电倍增管供电的 32 通道高压 DAC AD5535 的研究结果。内置高压缓冲放大器可实现高达 200 V 的输出电压调节,适用于各种类型的硅光电倍增管,包括其串行连接。输出电流高达 500 μA/ch,可为 SiPM 阵列和组件提供偏压。文件显示,该器件具有明显的温度依赖性(sim ~200~) ppm/C),这限制了 DAC 在 SiPM 供电中的使用。这项工作证明了芯片出色的温度稳定性。不过,由于制造商并不保证这一点,因此为了大规模使用 AD5535 DAC,我们开发了一种逐通道测量温度依赖性的明确方法。
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引用次数: 0
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Physics of Particles and Nuclei Letters
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