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Is nuclear structure relevant to non-mesonic hypernuclear weak decay? 核结构与非介子超核弱衰变有关吗?
Pub Date : 2002-03-01 DOI: 10.1556/APH.16.2002.1-4.37
H. C. Wu, M. Aristizábal, W. Ponce
This work studies the relevance of nuclear structure in the nonmesonic weak decay of Λ-hypernuclei, with the mechanism of ΛN → NN transition being restricted to one pion exchange (OPE) only. As an application, for the hypernucleus Λ 12 C a comparison between the L-S coupling and the j-j coupling gives an estimate of the range of nuclear structure effects. A considerable dependence is found of the total decay rate and the ratio Г n /qG p on the single particle properties of nuclear models. The possible contribution from the ΔI = 3/2 channel is investigated in a phenomenological manner.
本文研究了Λ-hypernuclei非介子弱衰变中核结构的相关性,其中ΛN→NN跃迁机制仅限于一次介子交换(OPE)。作为一个应用,对于超核Λ 12c, L-S耦合和j-j耦合的比较给出了核结构效应范围的估计。发现总衰变率和比值Г n /qG p与核模型的单粒子性质有相当大的关系。以现象学的方式研究了ΔI = 3/2通道的可能贡献。
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引用次数: 0
Λ0 polarization in ultrarelativistic nucleus-nucleus collisions Λ0超相对论性核-核碰撞中的极化
Pub Date : 2002-03-01 DOI: 10.1556/APH.16.2002.1-4.16
A. Ayala, E. Cuautle, Luis Manuel Monta o, G. Herrera
We study the polarization of Λ0’s produced in ultrarelativistic heavy-ion collisions. We argue that when the density of participants in the reaction is below the critical value for the production of a Quark-Gluon Plasma (QGP), recombination processes dominate the Λ0 production cross section and hence, Λ0’s are polarized. However, when the density of participants is above the critical value for QGP formation, coalescence processes dominate Λ0 production, giving rise to a reduction in the Λ0 polarization. For densities below the critical density for QGP production, we describe Λ0 polarization in terms of the DeGrand-Miettinen model and correct for the effects introduced by multiple scattering of the produced Λ0 within the nuclear environment.
我们研究了在超相对论性重离子碰撞中产生的Λ0 's的极化。我们认为,当反应参与者的密度低于产生夸克-胶子等离子体(QGP)的临界值时,重组过程主导了Λ0的产生截面,因此Λ0是极化的。然而,当参与者的密度高于QGP形成的临界值时,聚结过程主导Λ0的产生,导致Λ0极化降低。对于密度低于QGP产生的临界密度,我们用DeGrand-Miettinen模型描述Λ0极化,并校正了在核环境中产生的Λ0的多次散射所带来的影响。
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引用次数: 0
Spin Transfer Measurements in $(vec{p},vec{n})$ Reactions $(vec{p},vec{n})$反应中的自旋转移测量
Pub Date : 2002-03-01 DOI: 10.1556/aph.16.2002.1-4.12
J. Rapaport
The measurement of complete sets of spin transfer coefficients in nuclear transitions, induced via charge-exchange (((vec p, vec n))) reactions at intermediate energies, is a unique form of separating the spin-dependent and spin-independent contributions to the differential cross section. The two components of the spin-dependent contribution, the spin-longitudinal and spin-transverse components may equally be separated. This is extremely important in cases where the target nuclei has a non-integer ground state spin. In this study and as an example of the above, we present differential cross section and complete set of polarization transfer coefficients obtained in the ((^{13} C(vec p, vec n))) 13N reaction studied at angles between 0° and 33° and at 197 MeV incident proton energy. Polarization transfer coefficients are used to obtain the fraction of the Gamow-Teller (GT) component in the mirror ground state transition, which is a combination of the spin-independent Fermi (F) and spin-dependent GT components. Data are also presented for the transition to the first excited state in 13N at 2.34 MeV. This is a (1/2)− → (1/2)+ transition and the cross section is an incoherent admixture of ΔJ π = 1− and ΔJ π = 0− components. The complete set of polarization transfer coefficients are used to obtain differential cross section data for both components. The empirical results are compared with Distorted Wave Impulse Approximation calculations, DWIA.
测量中间能量下电荷交换(((vec p, vec n)))反应引起的核跃迁中自旋转移系数的完整集合,是分离微分截面中自旋依赖和自旋独立贡献的一种独特形式。自旋相关贡献的两个组成部分,自旋纵向和自旋横向组成部分可以平等地分开。这在目标原子核具有非整数基态自旋的情况下是非常重要的。在本研究中,作为上述的一个例子,我们给出了((^{13} C(vec p, vec n))) 13N反应在0°和33°之间的角度和197 MeV入射质子能量下的微分截面和完整的极化传递系数集。利用极化传递系数得到了镜面基态跃迁中独立于自旋的费米(F)和依赖于自旋的GT分量的组合——伽莫夫-泰勒(GT)分量的分数。本文还给出了在13N以2.34 MeV跃迁到第一激发态的数据。这是一个(1/2)−→(1/2)+跃迁,截面是ΔJ π = 1−和ΔJ π = 0−分量的非相干混合。利用完整的极化传递系数集来获得两组分的微分截面数据。实验结果与畸变波脉冲近似计算(DWIA)进行了比较。
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引用次数: 0
Searching for gluonic excitations —The Hall D project at Jlab 寻找胶子激发态- Jlab的D厅项目
Pub Date : 2002-03-01 DOI: 10.1556/APH.16.2002.1-4.21
E. Smith
Hybrid mesons are produced when the gluonic degrees of freedom are excited within normal mesons. A large fraction of these gluonic excitations can be identified using unique combinations of spin, parity and charge conjugation (J PC ) quantum numbers which are not allowed for ordinary (qbar q) bound states. Photon beams are expected to be particularly favorable for the production of such states, which are required by the quark confining mechanism of QCD. Mapping out the spectrum and decay modes of these hybrid mesons is the necessary first step in understanding the nature of confinement. Plans are underway at Jefferson Lab to upgrade the energy of the electron accelerator to 12 GeV. With 12 GeV electrons, a 9 GeV linearly polarized photon beam will be produced using the coherent bremsstrahlung technique. Along with this energy upgrade, a hermetic detector housed in new experimental hall (Hall D) will be used to collect data on photoproduced mesons with unprecedented statistics.
混合介子是在正常介子内激发胶子自由度时产生的。这些胶子激发的很大一部分可以用自旋、宇称和电荷共轭(jpc)量子数的独特组合来识别,这些量子数在普通(qbar q)束缚态中是不允许的。光子束被认为特别有利于产生这种状态,这是量子cd的夸克约束机制所需要的。绘制出这些混合介子的光谱和衰变模式是理解约束本质的必要的第一步。杰斐逊实验室正在计划将电子加速器的能量提升到12 GeV。利用相干轫致辐射技术,利用12 GeV的电子产生9 GeV的线极化光子束。伴随着这次能量升级,安置在新实验大厅(D厅)的一个密封探测器将用于收集光产生介子的数据,其统计数据前所未有。
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引用次数: 0
Enhancement of pionic modes in the quasielastic region 准弹性区域中子模式的增强
Pub Date : 2002-03-01 DOI: 10.1556/APH.16.2002.1-4.6
M. Ichimura, K. Kawahigashi
We report an evidence for the precursor phenomena of the pion condensation, which is found in the enhancement of the spin longitudinal cross sections ID q of the quasielastic 12C, (^{40} Ca(vec p, vec n)), reactions at the incident energy 494 and 346 MeV around the momentum transfer q ≈ q c , the critical momentum of the pion condensation. We utilized the distorted wave impulse approximation incorporated with the continuum random phase approximation. We adjusted the Landau-Migdal parameters, g′ NN and g′ NΔ, and obtained g′ NN ≈ 0.6–0.7 and g′ N Δ ≈ 0.3–0.4, which are consistent with those obtained from the energy of the Gamov-Teller giant resonance and the quenching factor of the Gamov-Teller sum rule.
我们报道了介子凝聚前驱现象的证据,发现在入射能量为494和346 MeV的准弹性12C, (^{40} Ca(vec p, vec n))反应的自旋纵向截面ID q在介子凝聚的临界动量q≈q c附近增强。我们采用了结合连续统随机相位近似的畸变波脉冲近似。我们调整了Landau-Migdal参数g ' NN和g ' NΔ,得到了g ' NN≈0.6-0.7和g ' NΔ≈0.3-0.4,这与从Gamov-Teller巨共振能量和Gamov-Teller求和规则的猝灭因子得到的结果一致。
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引用次数: 1
Barrett moments and rms charge radii 巴雷特力矩和均方根电荷半径
Pub Date : 2002-01-01 DOI: 10.1556/APH.15.2002.1-2.4
I. Angeli
An empirical relation is established between Barrett equivalent radii Rk,α and rms charge radii 1/2 based on the results of model-independent and Fermi model analyses of 2p → 1s transitions in muonic atoms. This relation follows simple Z dependence, and can be usefully applied to derive rms radii 1/2 or differences δAA′ 1/2 in cases where only Rk,α data or isotope shifts δAA′ Rk,α are published. The atomic number dependence of the Barrett parameters k(Z) and α(Z) is also given by empirical formulae. It is shown that the Barrett moment can be expanded in a sum of integer moments (m ≥ 2) using an effective exponential parameter αeff(Z). The moments and isotopic differences δ of the two-parameter Fermi distribution expressed in terms of the parameters c and a are given in the Appendix for m = 1 – 10.
通过对介子原子2p→1s跃迁的非模型分析和费米模型分析,建立了巴雷特等效半径Rk、α与rms电荷半径1/2之间的经验关系。这种关系遵循简单的Z依赖关系,在只有Rk,α数据或同位素位移δAA ' Rk,α的情况下,可以有效地应用于推导rms半径1/2或δAA ' Rk,α的差异。用经验公式给出了Barrett参数k(Z)和α(Z)与原子序数的关系。利用有效指数参数αeff(Z),可以将Barrett矩展开为整数矩(m≥2)的和。附录中给出了m = 1 - 10时用参数c和a表示的双参数费米分布的矩和同位素差δ。
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引用次数: 3
The percolation mechanism for fragmentation of nuclei using Monte Carlo technique 利用蒙特卡罗技术研究核破碎的渗透机制
Pub Date : 2002-01-01 DOI: 10.1556/APH.15.2002.1-2.8
A. El-Naghy, M. Mohery, K. Gad
A statistical bond-percolation model for the fragmentation has been applied to the proton-induced reactions assuming a lattice structure to the prefragment nucleus and using the Monte Carlo technique to determine the bond to be broken. The model succeeded to reproduce the essential features of the mass yield curves for the p-Cu reaction at 3.9 GeV and to describe qualitatively the charge and the multiplicity distributions of the projectile fragments for the 28Si interactions with the quasi-free emulsion nucleon at 3.7 AGeV.
断裂的统计键渗透模型已应用于质子诱导反应,假设断裂前核的晶格结构,并使用蒙特卡罗技术确定要断裂的键。该模型成功地再现了3.9 GeV下p-Cu反应的质量产率曲线的基本特征,并定性地描述了3.7 AGeV下28Si与准自由乳剂核子相互作用时抛射碎片的电荷和多重分布。
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引用次数: 2
Directed flow of baryons from high-energy heavy-ion collisions 高能重离子碰撞中重子的定向流动
Pub Date : 2002-01-01 DOI: 10.1556/APH.15.2002.1-2.6
W. Nörenberg, E. Nikonov, Y. Ivanov
The collective motion of nucleons from high-energy heavy-ion collisions is analyzed within a relativistic two-fluid model for different equations of state (EoS). As function of beam energy the theoretical slope parameter F y of the differential directed flow is in good agreement with experimental data, when calculated for the QCD-consistent EoS described by the statistical mixed-phase model. Within this model, which takes the deconfinement phase transition into account, the excitation function of the directed flow (P x ) turns out to be a smooth function in the whole range from SIS till SPS energies. This function is close to that for pure hadronic EoS and exhibits no minimum predicted earlier for a two-phase bag-model EoS. Attention is also called to a possible formation of nucleon antiflow (F y < 0) at energies ≳ 100 A·GeV.
在不同状态方程的相对论双流体模型中,分析了高能重离子碰撞中核子的集体运动。对于统计混合相模型描述的QCD-consistent EoS,微分定向流的理论斜率参数F作为光束能量的函数与实验数据吻合较好。在考虑解定义相变的模型中,定向流的激励函数(px)在从SIS到SPS的整个能量范围内都是平滑函数。这一函数接近于纯强子方程的函数,并且在两相袋模型方程中没有显示出先前预测的最小值。在能量约为100 a·GeV时,也有可能形成核子逆流(fy < 0)。
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引用次数: 3
Comparative study for nucleus-nucleus interactions and modified cascade evaporation model at (4.1 – 4.5) AGeV/c (4.1 ~ 4.5) AGeV/c下核-核相互作用与改进级联蒸发模型的比较研究
Pub Date : 2001-08-01 DOI: 10.1556/APH.15.2002.1-2.7
A. E. Naghy, S. Abdel-Aziz, S. Abou-Steit
The characteristics of the nucleus-nucleus collisions at high energy for the interactions of 1H, 4He, 12C, 16O, 22Ne, 28Si and 32S with emulsion at momentum (4.1 – 4.5) AGeV/c have been investigated. It has been found that the multiplicity distributions of the different emitted particles and their average values can be described by the modified cascade evaporation model. The model reproduces satisfactorily the multiplicity distributions of the shower, grey and black particles and the correlations between their multiplicities. It has been seen that the number of the produced shower particles increases with the increase of the projectile mass number. From the correlation between the average multiplicity of the evaporation particles and the number of the produced particles, it was found that a phase transition in the target system may occur. The calculated pseudo-rapidity distributions of the produced shower particles are typically Gaussian shaped in the mid-rapidity region and agree well with the experimental data. Also, the angular distributions of the grey and black particles have been investigated. The angular distributions of the grey particles show a universal shape independent of the type of projectile. The angular distributions of the black particles are nearly isotropic with a small asymmetry in the forward direction. The modified cascade evaporation model, reproduces the general characteristics of the nucleus-nucleus interactions and gives an explanation for the multiparticle production process.
研究了1H、4He、12C、16O、22Ne、28Si和32S与乳化液在动量(4.1 ~ 4.5)AGeV/c下相互作用的高能核-核碰撞特性。研究发现,改进的串级蒸发模型可以描述不同发射粒子的多重分布及其平均值。该模型较好地再现了雨粒、灰粒和黑粒的多重分布及其多重度之间的相关性。可以看出,随着抛射物质量数的增加,产生的阵雨粒子的数量也随之增加。从蒸发粒子的平均多重数与生成粒子数之间的关系可以看出,目标体系可能发生相变。计算得到的阵雨粒子的伪快度分布在中快度区域呈典型的高斯分布,与实验数据吻合较好。此外,还研究了灰色和黑色粒子的角分布。灰色粒子的角分布与抛射体的类型无关,呈现出一种普遍的形状。黑色粒子的角分布几乎是各向同性的,在正向上有较小的不对称性。修正的级联蒸发模型再现了核-核相互作用的一般特征,并给出了多粒子产生过程的解释。
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引用次数: 3
KeV astrophysics with GeV beams; blazing a new trail on the summit of Nuclear Astrophysics GeV光束的KeV天体物理学;在核天体物理学的顶峰上开辟了一条新路
Pub Date : 2001-07-12 DOI: 10.1556/APH.15.2002.3-4.21
M. Gai
GeV beams of light ions and electrons are used for creating a high flux of real and virtual photons, with which some problems in Nuclear Astrophysics are studied. GeV 8B beams are used to study the Coulomb dissociation of 8B and thus the 7Be(p,γ)8B reaction. This reaction is one of the major source of uncertainties in estimating the 8B solar neutrino flux and a critical input for calculating the 8B solar neutrino flux. The Coulomb dissociation of 8B appears to provide a viable method for measuring the 7Be(p,γ)8B reaction rate, with a weighted average of the RIKEN1, RIKEN2, GSI1 and MSU published results of S 17(0)=18.9±1.0 eV-b. This result, however, does not include a theoretical error estimated to be ±10%. GeV electron beams on the other hand, are used to create a high flux of real and virtual photons at TUNL-HIGS and MIT-Bates, respectively, and we discuss two new proposals to study the 12C(α,γ)16O reaction with real and virtual photons. The 12C(α,γ)16O reaction is essential for understanding Type II and Type Ia supernova. It is concluded that virtual and real photons produced by GeV light ions and electron beams are useful for studying some problems in Nuclear Astrophysics.
利用GeV光离子和电子束产生高通量的实光子和虚光子,研究了核天体物理学中的一些问题。GeV 8B光束用于研究8B的库仑解离,从而研究7Be(p,γ)8B反应。该反应是估算8B太阳中微子通量的主要不确定性来源之一,也是计算8B太阳中微子通量的关键输入。8B的库仑解离似乎为测量7Be(p,γ)8B的反应速率提供了一种可行的方法,RIKEN1、RIKEN2、GSI1和MSU公布的结果的加权平均值为s17(0)=18.9±1.0 eV-b。然而,该结果不包括估计为±10%的理论误差。另一方面,GeV电子束在TUNL-HIGS和MIT-Bates分别产生了高通量的实光子和虚光子,我们讨论了用实光子和虚光子研究12C(α,γ)16O反应的两种新方案。12C(α,γ)16O反应对于理解II型和Ia型超新星至关重要。结论认为,GeV光离子和电子束产生的虚光子和实光子对研究核天体物理中的一些问题是有用的。
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引用次数: 0
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Acta Physica Hungarica
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