α-particle spectrum in the reaction p + 11B → α + 8Be* → 3α

Using a simple phenomenological parametrization of the reaction amplitude we calculated α-particle spectrumin the reaction p + ¹¹B → α + ⁸Be* → 3α at the resonance proton energy of 675 keV. The parametrization includes Breit-Wigner factor with an energy-dependent width for intermediate ⁸Be* state and the Coulomb and the centrifugal factors in α-particle-emission vertices. The shape of the spectrum consists of a well-defined peak corresponding to emission of the primary α and a flat shoulder going down to very low energy. We found that below 1.5MeV there are 17.5% of α’s and below 1MeV there are 11% of them. The text was submitted by the author in English.     

双幻核100Sn的基态性质

用Skyrme—Hartree—Fock方法计算了双幻核¹⁰⁰Sn基态的一些性质.计算表明,由于库仑排斥,¹⁰⁰Sn存在一个质子皮.     

100Sn核墓态性质的微观研究

用相对论平均场理论和非相对论平均场理论计算了双幻核¹⁰⁰Sn的结合能,核物质分布半径,中子分布半径和质子分布半径等,并对这两种理论计算结果进行了比较和讨论.这是对¹⁰⁰Sn核的第一个微观计算.     

Resonance states in 16O+16O, 12C+16O, α+16O and α+12C with modified Morse potentials

The resonance states in ¹⁶O+¹⁶O, ¹²C+¹⁶O, α+¹⁶O and α+¹²C are described using modified Morse potential proposed earlier whose success has already been demonstrated in the case of ¹²C+¹²C system. The general validity of such a potential with long range, shallow depth and repulsive soft core determined from the resonance data itself is being examined through the present study of the resonances in the above four systems. In each system, the experimental data of a large number of states have been successfully described with a modified Morse potential. The success points out a common mechanism of the origin of these states, and reaffirms authentically the diatomic-like rotational and vibrational picture of the nuclear molecular resonances proposed previously. The close resemblance between the physics of diatomic molecules and nuclear molecular resonances extending to the level of potential which is Morse type in both the cases — although belong to two different areas of physics — is further strengthened through the present study.      

Reaction e + e ? → π + π ? π + π ? at energies of √ s ≤ 1 GeV

The e ⁺ e ⁻ → π ⁺ π ⁻ π ⁺ π ⁻ cross section is calculated for energies of 0.65 ≤ √s ≤ 1 GeV in the framework of the generalized hidden local symmetry model. The calculations are compared with the data of CMD-2 and BaBaR. It is shown that the inclusion of heavy isovector resonances ρ(1450) and ρ(1700) is necessary for reconciling calculations with the data. It is found that, at √s ≈ 1 GeV, the contributions of the above resonances are much larger, by a factor of 30, than the ρ(770) one, and amount to a considerable fraction ∼0.3–0.6 of the latter at √s ∼ m _ρ. The text was submitted by the authors in English.     

16O+94Zr和16O+116Sn的弹性散射角分布测量

用北京Q3D磁谱仪及其重离子焦面探测器系统测量了两个体系的14个弹性散射角分布,即¹⁶O+⁹⁴Zr体系在52,57,59,62,72,82和92MeV 7个能量点及¹⁶O+¹¹⁶Sn体系在57,59,62,67,72,82和92MeV 7个能量点的弹性散射角分布.用耦合道理论的ECIS计算程序拟合数据,初步观察到了“阈反常”现象.     

35MeV/u 40Ar+112Sn/124Sn反应中热核的同位旋对热核发射机制的影响

作为放射性束物理的延伸,热核的同位旋效应引起了理论和实验研究的广泛重视.给出35MeV/u ⁴⁰Ar+¹¹²Sn/¹²⁴Sn实验中,热核的同位旋对热核衰变出射道机制的影响:由于库仑不稳定性和库仑力作用,丰质子热核达到系统平衡前,很容易出现大量有利于增加余核中质比的高能粒子出射(如p.3He、a等);该类轻粒子在热核的衰变链中发射几率较大而且衰变链很长.这样,传统的热核测量量(如能谱斜率温度)将受到测量粒子种类的较大影响.     

12C+112Sn短寿命蒸发余核截面的研究

在束流能量范围52—71MeV中我们通过γ探测完成了¹²C+¹¹²Sn反应蒸发余核截面的测量.借助一个特别的装置将余核从靶室内传送到测量站后用一台Ge(Li)探测器探测了.最后仅得到了蒸发余核的相对生成截面.     

Signals of α clusters in 16O+16O collisions at the LHC from relativistic hydrodynamic simulations

In relativistic heavy ion collisions, the fluctuations of initial entropy density convert to the correlations of final state hadrons in momentum space through the collective expansion of strongly interacting QCD matter. Using a (3+1)D viscous hydrodynamic program, CLVisc, we consider whether the nuclear structure, which provides initial state fluctuations as well as correlations, can affect the final state of heavy ion collisions, and whether one can find signals of α cluster structures in oxygen using final state observables in \begin{document}$ ^{16}\text{O}+{}^{16}\text{O} $\end{document} collisions at the CERN Large Hadron Collider. For the initial nucleon distributions in oxygen nuclei, we compare three different configurations, a tetrahedral structure with four-α clusters, the deformed Woods-Saxon distribution, and a spherical symmetric Woods-Saxon distribution. Our results show that the charged multiplicity as a function of centrality and the elliptic flow at the most central collisions using the four-α structure differs from those with the Woods-Saxon and deformed Woods-Saxon distributions, which may help to identify α clustering structures in oxygen nuclei.     

Systematic study of the α decay preformation factors of the nuclei around the Z = 82, N = 126 shell closures within the generalized liquid drop model

In this study, we systematically investigate the \begin{document}$\alpha$\end{document} decay preformation factors, \begin{document}$P_{\alpha}$\end{document} , and the \begin{document}$\alpha$\end{document} decay half-lives of 152 nuclei around Z = 82, N = 126 closed shells based on the generalized liquid drop model (GLDM) with \begin{document}$P_{\alpha}$\end{document} being extracted from the ratio of the calculated \begin{document}$\alpha$\end{document} decay half-life to the experimental one. The results show that there is a remarkable linear relationship between \begin{document}$P_{\alpha}$\end{document} and the product of valance protons (holes) \begin{document}$N_p$\end{document} and valance neutrons (holes) \begin{document}$N_n$\end{document} . At the same time, we extract the \begin{document}$\alpha$\end{document} decay preformation factor values of the even–even nuclei around the Z = 82, N = 126 closed shells from the study of Sun \begin{document}${et\ al.}$\end{document} [J. Phys. G: Nucl. Part. Phys., 45: 075106 (2018)], in which the \begin{document}$\alpha$\end{document} decay was calculated by two different microscopic formulas. We find that the \begin{document}$\alpha$\end{document} decay preformation factors are also related to \begin{document}$N_pN_n$\end{document} . Combining with our previous studies [Sun \begin{document}${et\ al.}$\end{document} , Phys. Rev. C, 94: 024338 (2016); Deng \begin{document}${et\ al.}$\end{document} , ibid. 96: 024318 (2017); Deng \begin{document}${et\ al.}$\end{document} , ibid. 97: 044322 (2018)] and that of Seif \begin{document}${et\ al.,}$\end{document} [Phys. Rev. C, 84: 064608 (2011)], we suspect that this phenomenon of linear relationship for the nuclei around the above closed shells is model-independent. This may be caused by the effect of the valence protons (holes) and valence neutrons (holes) around the shell closures. Finally, using the formula obtained by fitting the \begin{document}$\alpha$\end{document} decay preformation factor data calculated by the GLDM, we calculate the \begin{document}$\alpha$\end{document} decay half-lives of these nuclei. The calculated results agree with the experimental data well.     

B ?→ K 1*? (1270)(→ ρ 0 K ?) ? + ? ? in LEET

Flavor changing neutral current (FCNC) decays of the B-meson are a very useful tool for studying possible physics scenarios beyond the standard model (SM), where of the many FCNC modes radiative, purely leptonic and semi-leptonic decays of the B-meson are relatively clean tests. Within this context, the BELLE collaboration has measured the process B→K ^* γ and also searched for the B→K ₁(1270)γ process. Theoretical analyses of these processes are yielding similar values of the relevant form factors. In this work we have used this upper bound in studying the angular correlations for the related semi-leptonic decay mode B ⁻→K ₁⁻(1270)(→ρ ⁰ K ⁻)ℓ ⁺ ℓ ⁻, where we have used the form factors that have already been estimated for the B→K ₁(1270)γ mode. Note that the additional form factors that are required were calculated using large energy effective theory (LEET).     

Rare decays of Λ b → Λ γ and Λ b → Λ l + l ? in universal extra-dimension model

The exclusive weak decay of Λ _b →Λ γ and Λ _b →Λ l ⁺ l ⁻ are investigated in the Appelquist–Cheng–Dobrescu model, which is an extension of the standard model in the presence of universal extra dimensions. Employing the transition form factors obtained in the light-cone sum rules, we analyze how the invariant-mass distribution, the forward–backward asymmetry and the polarization asymmetry of the Λ baryon of these decay modes can be used to constrain the only additional free parameter with respect to the standard model, namely, the radius, R, of the extra dimension. Our results indicate that the Kaluza–Klein modes can lead to approximately 25% suppression of the branching ratio of Λ _b →Λ γ; however, their contributions can bring about 10% enhancement to the decay rate of Λ _b →Λ l ⁺ l ⁻. It is shown that in the present scenario the zero position of the forward–backward asymmetry of Λ _b →Λ μ ⁺ μ ⁻ is sensitive to the compactification parameter R, while the measurement of polarizations of Λ baryon in the Λ _b decays are not a useful tool to provide any valuable information for the universal extra-dimension model.     

35MeV/u 36,40Ar+112,124Sn反应中同位旋自由度的弛豫

35MeV/u ^36,40Ar+^112,124Sn反应中,在前角5°和20°观测到丰中子核与稳定核的产额比随粒子出射动能的增加而减小,而缺中子核与稳定核的产额比随动能的增加而增加.对于某种元素,随着动能的减小,其平均中质比逐渐由弹核N/Z向靶核N/Z过渡.这些现象表明在这样的入射能量下,周边或近周边碰撞过程中同位旋自由度没有完全达到平衡.这种行为对两个靶核系统是相似的,但是同位素产额比的绝对值在5°没有靶核相关性,而在20°处却表现出明显的靶核相关性.     

α-decay study of 218Ac and 221Th in 40Ar+186W reaction

In this study,²¹⁸Ac and ²²¹Th nuclides were produced via the heavy-ion induced fusion evaporation reaction ⁴⁰Ar+¹⁸⁶W.Their decay properties were studied with the help of the gas-filled recoil spectrometer SHANS and a digital data acquisition system.The cross section ratio between ²²²Pa and ²¹⁸Ac was extracted experimentally,withmeasured value 0.69(9).Two new possible α decay branches to ²²¹Th are suggested.The valence neutron configurations for the daughter ²¹⁷Ra are discussed in terms of the hindrance factors.     

Measurement of inclusive π 0 production in hadronic Z 0 decays

An analysis is presented of inclusiveπ ⁰ production inZ ⁰ decays measured with the DELPHI detector. At low energies,π ⁰ decays are reconstructed by using pairs of converted photons and combinations of converted photons and photons reconstructed in the barrel electromagnetic calorimeter (HPC). At high energies (up to ) the excellent granularity of the HPC is exploited to search for two-photon substructures in single showers. The inclusive differential cross section is measured as a function of energy forqq andbb events. The number ofπ ⁰’s per hadronicZ ⁰ event isN(π ⁰)/Z _had ⁰ =9.2±0.2(stat)±1.0(syst) and forbb events the number ofπ ⁰’s is N(π ⁰)/bb=10.1±0.4(stat)±1.1(syst). The ratio of the number ofπ ⁰’s inbb events to hadronicZ ⁰ events is less affected by the systematic errors and is found to be 1.09±0.05±0.01. The measuredπ ⁰ cross sections are compared with the predictions of different parton shower models. For hadronic events, the peak position in theξ _p=ln(1/x_p) distribution isξ* _p =3.90 _−0.14 ^+0.24 . The average number ofπ ⁰’s from the decay of primary B hadrons is found to be N(B→π ⁰ X)/B hadron=2.78±0.15(stat)±0.60(syst).     

α-particle preformation for favoured transitions using proximity potential

α-particle preformation probability (P₀) is calculated for favoured transitions of all α-emitters. An indirect approach is employed in which P₀ is given by the ratio of the experimental values of α-decay constant and theoretically determined values of assault frequency and the penetrability. The proximity potential is used for determination of the penetrability, and the assault frequency is calculated through a modified formula. Analysis of the results show that P₀ is highest for the even–even type, and lowest for the odd–odd type α-emitter. Also, it is noted that P₀ is higher for transitions originating in the ground state, and lower for transitions originating in the isomeric state. This suggests that there is greater preformation of α-particle in the ground state than in the isomeric state. P₀ values show a distinct minima at the neutron magic number, N = 126. Also, it is noted that values of α-decay fraction (f_α) reported in the literature for a few α-emitters are, either, not consistent, or only limiting values are available. This raises the possibility of determining improved values of P₀ if accurate values of f_α are known in future.     

30MeV/u 40Ar+112,124Sn反应后角能谱温度的同位旋效应

在30MeV/u ⁴⁰Ar+^112,124Sn反应中用平行板雪崩计数器实现了前冲余核的测量.在不同的线性动量转移下用运动源模型拟合了后角的³He,α和⁶He能谱,发现³He的能谱斜率温度在¹²⁴Sn系统中高于¹¹²Sn系统,而⁶He的温度在¹¹²Sn系统中更高,α粒子在两个系统中没有明显差别.用热核粒子蒸发过程衰变道的选择性对这种同位旋相关性进行了解释.GEMINI的计算不能重现实验结果.     

30MeV/u 40Ar+ 112,124Sn反应中态布居核温度的同位旋效应

用13单元望远镜探测器阵列测量了30MeV/u ⁴⁰Ar +^112,124Sn反应中小角关联粒子,由两体符合事件提取了αα关联函数.用三体弹道理论模型MENEKA计算本底关联函数,用Monte Carlo方法计算探测效率函数,在扣除本底产额并考虑探测效率的修正后,对不同同位旋反应系统⁴⁰Ar +¹¹²Sn和⁴⁰Ar+¹²⁴Sn提取的相对态布居核温度分别是4.18±0.25 0.21MeV和4.10±0.22 0.20MeV ;考察态布居核温度和粒子能量的关系时,观察到两个系统的发射温度均随着粒子能量的增加而降低,缺中子系统⁴⁰Ar +¹¹²Sn中由低能时的5.13±0.30 0.2 6MeV降低到高能时的3.87±0.37 0.29MeV ,丰中子系统⁴⁰Ar+¹²⁴Sn中由低能时的5.39±0.30 0.26MeV降低到高能时的3.32±0.28 0.23MeV .用激发热核衰变过程的同位旋选择性对这种同位旋相关性进行了解释.     

Cross sections for 68Ge production in natural- and enriched-germanium targets irradiated with protons of energy 100 MeV and background in experiments devoted to searches for the 2β0ν decay of 76Ge

The rate of ⁶⁸Ge production at sea level under the effect of the nuclear component of cosmic rays is calculated. The calculation is based on the experimental values of the cross sections for ⁶⁸Ge production in natural- and enriched-germanium targets (enrichment in ⁷⁶Ge) irradiated with high-energy protons. The background from the decays of ⁶⁸Ge can be a serious problem in new-generation experiments devoted to searches for the 2β0ν decay of ⁷⁶Ge.