共查询到20条相似文献,搜索用时 140 毫秒
1.
夸克胶子物质内的从夸克-夸克-反夸克到夸克-夸克-反夸克的散射过程会影响夸克物质和反夸克物质的热平衡化,其散射振幅是研究热平衡化的一个基础.依据微扰QCD理论,编制Fortran程序,推导了αs^4阶的各个qq-↑q→qq-↑q散射费曼图的振幅平方和不同费曼图间的干涉项. 相似文献
2.
3.
4.
利用“夸克产生律”与“夸克组合律”计算了e+e-湮没中重夸克喷注事例的带电粒子多重数,结果与实验符合.并与轻夸克喷注事例及平均夸克味道喷注事例的多重数做了比较. 相似文献
5.
从亚夸克物理中允许存在的编外粒子出发,探索了可能存在的双夸克态,双轻子态以及轻子夸克等新物质态,给出了它们的结构性和SU(3)对称表示。 相似文献
6.
最近在德国汉堡发现了一种轻子与夸克相结合的新物质--轻子夸克。本文根据焦--宫亚夸克模型及亚夸克对的产生与重组合机制,探讨了可能存在的轻子型夸克态。 相似文献
7.
基于夸克传播子的Dyson-Schwinger方程,计算了夸克胶子混合真空凝聚和夸克真空凝聚. 这些凝聚不仅联系着夸克在真空态中的虚度,而且也表征了真空中夸克分布的空间宽度. 真空凝聚的存在直接反映着QCD真空的非微扰结构. 计算表明:上夸克与下夸克的虚度为λ2u,d=0.7GeV2,奇异夸克的虚度为λ2s=1.6GeV2. 这些结果与许多用完全不同的方法得到的结果一致. 相似文献
8.
9.
10.
给出了一种超越阿贝尔优势近似求解夸克胶子等离子体输运方程的方法,并用它计算了夸克、反夸克等离子体的输运系数,讨论了输运系数的非阿贝尔修正. 相似文献
11.
Properties of hybrid stars with a mixed phase composed of asymmetric nuclear matter and strange quark matter are studied. The quark phase is investigated by the quark quasiparticle model with a self-consistent thermodynamic and statistical treatment. We present the stability windows of the strange quark matter with respect to the interaction coupling constant versus the bag constant. We find that the appearance of the quark–hadron mixed phases is associated with the meta-stable or unstable regions of the pure quark matter parameters. The mass–radius relation of the hybrid star is dominated by the equation of state of quark matter rather than nuclear matter. The contour plots of the maximum mass of the hybrid star are shown in the plane of the coupling constant and the bag constant. 相似文献
12.
Based on an extensive study of the Dyson-Schwinger equations for a fully
dressed quark propagator in the “rainbow” approximation, a parametrized form of the
quark propagator is suggested. The corresponding quark self-energy
Σf and the
structure of non-local quark vacuum condensate <0|:\bar{q}(x)q(0):|0>
are investigated. The algebraic form of the quark propagator proposed in this work describes a confining quark propagation, and is quite convenient
to be used in any numerical calculations. 相似文献
13.
We study vacuum of QCD in this work. The structure of non-local
quark vacuum condensate, values of various local quark and gluon
vacuum condensates, quark-gluon mixed vacuum condensate, quark and
gluon virtuality in QCD vacuum state, quark dynamical mass and
susceptibility of QCD vacuum state to external field are predicted by use of the solutions of Dyson-Schwinger equations in “rainbow”
approximation with a modeling gluon propagator and three different
sets of quark-quark interaction parameters. Our theoretical
predictions are in good agreement with the correspondent empirical
values used widely in literature, and many other theoretical
calculations. The quark propagator and self-energy functions are
also obtained from the numerical solutions of Dyson-Schwinger
equations. This work is centrally important for studying
non-perturbative QCD, and has many important applications both in
particle and nuclear physics. 相似文献
14.
对称能表征了同位旋非对称强相互作用物质状态方程的同位旋相关部分,它对于理解核物理和天体物理中的许多问题有重要意义。简要总结了关于核物质和夸克物质对称能研究的最新进展。对于核物质对称能,通过对核结构,核反应以及中子星的研究,目前对其亚饱和密度的行为已有比较清楚的认识,同时,对饱和密度附近对称能的约束也取得了很好的研究进展。但如何确定核物质对称能的高密行为仍然是一个挑战。另一方面,在极端高重子数密度条件下,强相互作用物质将以退禁闭的夸克物质状态存在。同位旋非对称夸克物质可能存在于致密星内部,也可能产生于极端相对论重离子碰撞中。对最近关于夸克物质对称能对夸克星性质的影响以及重夸克星的存在对夸克物质对称能的约束的研究工作进行了介绍,结果表明同位旋非对称夸克物质中上夸克和下夸克可能感受到很不一样的相互作用,这对于研究极端相对论重离子碰撞中部分子动力学的同位旋效应有重要启发。The symmetry energy characterizes the isospin dependent part of the equation of state of isospin asymmetric strong interaction matter and it plays a critical role in many issues of nuclear physics and astrophysics. In this talk, we briefly review the current status on the determination of the symmetry energy in nucleon (nuclear) and quark matter. For nuclear matter, while the subsaturation density behaviors of the symmetry energy are relatively well-determined and significant progress has been made on the symmetry energy around saturation density, the determination of the suprasaturation density behaviors of the symmetry energy remains a big challenge. For quark matter, which is expected to appear in dense matter at high baryon densities, we briefly review the recent work about the effects of quark matter symmetry energy on the properties of quark stars and the constraint of possible existence of heavy quark stars on quark matter symmetry energy. The results indicate that the u and d quarks could feel very different interactions in isospin asymmetric quark matter, which may have important implications on the isospin effects of partonic dynamics in relativistic heavy-ion collisions. 相似文献
15.
16.
The adiabatic effective baryon-baryou interactions and dibaryon candidates are studied systematically with three constituent quark models based on different effective degrees of freedom:Glozman-Riska-Brown Goldstone boson exchange model based on constituent quark and Goldstone boson coupling;Fujiwara model based on constituent quark gluon coupling and Nijmegen one-boson exchange;QDCSM based on constituent quark and gluon coupling with quark delocalization and color screening.We find that the three models predicted the similar effective baryon-baryon interactions for roughly two thirds among the 64 states consisted of octet and decuplet baryons.The differences among three models and their separate characteristics are also studied. 相似文献
17.
研究夸克的质量是QCD研究中的一个非常重要问题。因为, 夸克质量是标准模型的基本输入参数, 准确地确定这些参数无论对于唯象的应用还是对于理论的应用都是极其重要的。基于参数化的完全穿衣服的夸克传播子, 研究了自能函数和夸克的动力学质量。理论预言了夸克质量和自能函数, 其结果与文献中的经验值相符合, 也与Dyson Schwinger方程解一致。反过来这也说明了参数化的夸克传播子是成功和可靠的。Study of mass of quark is one of the most important issues in the investigation of QCD. Because masses of quarks are fundamental QCD input parameters of standard Model, and an accurate determination of these parameters is extremely important for both phenomenological and theoretical applications. Based on the parameterized fully dressed quark propagator proposed by us, the theoretical predictions of the masses of quarks are predicted in this short note. The effective quark mass is defined by the scalar self energy function Bf(p2) and vector self energy function Af(p2). The results of our calculations are in agreement with the empirical values used widely in literature and also show that the parameterized form of quark propagator is an applicable and reliable approximation. 相似文献
18.
在MTT口袋模型的基础上采用密度依赖口袋常数,给出了奇异夸克物质的热力学关系,并用于描述奇异夸克物质及混合星内的夸克相,研究了奇异星、混合星的性质.结果表明,密度依赖口袋常数下,奇异夸克物质的压强公式中有一个附加项,而能量密度中则没有,从而保证了系统的热力学自洽性.在新的热力学关系下,奇异夸克物质的状态方程变软,相应的奇异星的引力质量和对应的半径均变小;混合星的状态方程也变软,其质量变小,而对应的半径也变小.说明经热力学自洽处理后该模型对中子星的状态方程及相应的质量-半径关系等都有显著的影响. 相似文献
19.
SUN Wei-Min ZONG Hong-Shi 《理论物理通讯》2008,49(2):435-438
In equilibrium statistical field theory, the partition function has fundamental importance. In this paper we propose a direct and general method for calculating the partition function and equation of state of QCD at finite chemical potential. It is found that the partition function is totally determined by the dressed quark propagator at finite chemical potential up to a multiplicative constant. From this a criterion for the phase transition between the Nambu and the Wigner phases is obtained. This general method is applied to two specific cases: the free quark theory and QCD with a model dressed quark propagator having confinement features. In the first case, the standard Fermi distribution at T = 0 is reproduced. In the second case, we apply the conclusion in previous works to obtain the dressed quark propagator at finite chemical potential and find the unphysical result that the baryon number density vanishes for all values of chemical potential. The reason for this result is discussed. 相似文献
20.
提出一种新的包含三代已知轻子与夸克的SU(5)大统—模型.按本模型,强子可看作由夸克形成的非拓扑孤粒子;轻子与夸克本质上是相同的,它们之间的差别是由对称性自发破缺造成的;在强子内部,夸克质量很小,其性质与已知夸克相同;在强子外部,夸克的性质与已知轻子相同,只是质量很重,并将很快衰变.本文除了定义严格守恒的电荷Q0、费米子数F0外,还在孤粒子内部定义了近似守恒的内色荷、内电荷、内费米子数.已知SU(5)大统—模型的(L-B)守恒相应于本模型的F0守恒。 相似文献