胶子有效质量对重夸克势的影响

本文采用椭球袋模型讨论胶子有效质量对重夸克势的影响.我们分别计算了胶子有效质量0,0.2,0.4,0.6和1.0GeV时的重夸克势.计算结果表明,除汤川势外,势仍近似地呈线性,随着胶子有效质量的增加,斜率逐渐减小.     

通过基矢光前量子化方法研究K介子

为研究K介子的性质，通过基矢光前量子化(BLFQ)方法获得K介子的光前波函数(LFWF)。使用的光前哈密顿量中包含了动能项、横向与纵向禁闭势以及夸克-胶子相互作用，其中横向禁闭势借鉴了光前全息量子色动力学(LFHQCD)模型的禁闭势。基矢空间包括领头阶与次领头阶的Fock空间。在前期工作的基础上，只引入了奇异夸克的质量作为唯一额外参数，使K>介子的质量与实验值相匹配。基于K介子领头阶Fock空间的LFWF，计算了K介子的部分子分布振幅(PDA)，其结果与量子色动力学(QCD)微扰论在零夸克质量近似下计算的结果相近。本工作得到的K介子的电磁形状因子(FF)与欧洲核子中心(CERN)超级质子同步加速器 (SPS)以及费米国家加速器实验室(FNAL)的实验结果一致。从领头阶Fock空间的LFWF计算出的电磁半径与粒子物理数据表(PDG)的实验值相近。计算出的K介子部分子分布函数(PDF)，QCD演化后，在实验能标下的K介子和$ \pi $介子中价夸克u的PDF之比与CERN-NA-003的实验数据在整体趋势上大体相符。此外，在计算出的K介子PDF中，价夸克携带的纵向动量之比，$ \langle x_{uv}\rangle/\langle x_{sv}\rangle $，约为$ 2/3 $，这个数值与Bethe-Salpeter equation(BSE)模型以及密西根州立大学格点QCD(MSULat)模型的计算结果相近。还计算了K介子的结构函数，发现与BLFQ考虑有效 Nambu–Jona-Lasinio相互作用(BLFQ-NJL)模型的结果有显著差别。K介子的结构函数有望在将来的电子离子对撞机(EIC)实验中得到观测与检验。     

单胶子交换正反夸克对产生模型中的自旋轨道耦合力

从单胶子交换正反夸克对产生模型出发,研究了核子间等效ρω介子交换势.计算结果表明这个模型能得到强子层次核力介子交换理论中ρ,ω介子交换势的各个部分,并且定性性质与传统的介子交换势也是相同的.     

相对论夸克模型和N–Δ能量劈裂

基于相对论夸克模型,在夸克层次上研究了N-Δ的质量和二者的能量劈裂,通过引入了赝标量π介子云效应,得到了π和核子之间的耦合常数g_πNN,以及单胶子交换势和单π介子交换势分别对N-Δ能量劈裂的贡献,计算结果较好地与实验值得到了吻合.另外我们还比较了相对论与非相对论夸克模型在处理上的不同.     

相对论夸克模型和N—△能量劈裂

基于相对论夸克模型，在夸克层次上研究了N-△的质量和二者的能量劈裂，通过引入了赝标量π介子云效应，得到了π和核子宰的耦合常数gxNN，以及单胶子交换势和单π介子交换势分别对N-△能量劈裂的贡献，计算结果较好地与实验值得到了吻合。另外我们还比较了相对论与非对论夸克模型在处理上的不同。     

重夸克偶素质量谱的相对论夸克模型研究（已撤稿）

使用量子场论中准势途径的相对论夸克模型,计算了重夸克偶素的质量谱.所采用的同味正反夸克间的有效相互作用包括通常的直接单胶子交换、单胶子湮没及具有相对论修正的标量和矢量线性禁闭的混合.得到了与实验上肯定的数据符合较好的拟合计算结果，并讨论了湮没项和相对论修正各项对能谱超精细分裂的作用. 关键词： 重夸克偶素 质量谱 相对论修正 湮没势     

双胶子交换模型中J/ψ的衍射产生

利用双胶子交换模型并结合重夸克偶素的色八重态产生机制,计算了π与p碰撞过程中J/ψ的衍射产生总截面.结果发现:随着质心系能量的增加,J/ψ衍射产生的总截面逐渐增大;并且,不同的π介子中的胶子分布函数给出的总截面偏离也逐渐加大.计算结果与未来的实验数据比较,可以检验π介子中的胶子分布函数及双胶子交换模型.     

在非拓扑孤立子模型中核子的电磁形状因子

从Friedberg-李政道的非拓扑孤立子模型出发得到一个新的夸克禁闭势.利用这个新的禁闭势,预言了核子的静态性质,并与实验数据进行了比较.理论很好地解释了实验结果.     

洛伦兹规范条件下对单胶子夸克势的QCD非微扰修正形式

在洛伦兹规范条件下,导出了具有平移不变性的双胶子两点函数真空平均值.利用所获得的双胶子真空期待值,给出了对微扰单胶子交换夸克–夸克势、夸克–反夸克对湮没和夸克–反夸克对激发势的最低阶非微扰QCD修正形式.     

核子–核子散射过程的研究和矢量介子交换势

在推广的手征SU(3)夸克模型下讨论了核子–核子散射过程和矢量介子交换势.给出了赝标π介子和矢量ρ和ω介子的GCM中心力的交换势和NN散射14个分波的相移.研究表明,矢量介子交换势可以替代单胶子交换势以解释核力的短程排斥.     

The AdS5 Black Hole Space-time with the Perturbed?Dilaton Field Background

The AdS ₅ black hole space-time with perturbed dilaton field background considered. We use the holographic AdS/QCD soft-wall model to investigate the wave functions and the effective potential. In this model, glueballs are described by a massless scalar field in an AdS ₅ black hole with a dilaton soft-wall background. For the first time we use modified dilaton field and discuss the consequence of the perturbation. In order to obtain the effective potential we rewrite the equation of motion in the Schr?dinger like equation, then try to find corresponding solution.     

String theory and cosmology

We discuss the main cosmological implications of considering string-loop effects and a potential for the dilaton in the lowest order string effective action. Our framework is based on the effective model arising from regarding homogeneous and isotropic dilaton, metric and Yang-Mills field configurations. The issues of inflation, entropy crisis and the Polonyi problem as well as the problem of the cosmological constant are discussed.     

Equation of state and chiral transition in soft-wall AdS/QCD with a more realistic gravitational background

We construct an improved soft-wall AdS/QCD model with a cubic coupling term of the dilaton and the bulk scalar field. The background fields in this model are solved by the Einstein-dilaton system with a nontrivial dilaton potential, which has been shown to reproduce the equation of state from the lattice QCD with two flavors. The chiral transition behaviors are investigated in the improved soft-wall AdS/QCD model with the solved gravitational background, and the crossover transition can be realized. Our study provides the possibility to address the deconfining and chiral phase transitions simultaneously in the bottom-up holographic framework.     

Potentials of pointlike particles in gauge theory with a dilaton

I examine the potential of a pointlike particle carrying SU (N _c) charge in a gauge theory with a dilaton. The potential depends on boundary conditions imposed on the dilaton: For a dilaton that vanishes at infinity the resulting potential is a regulatized Coulomb potential of the form (r+r _ϕ)⁻¹, withr _ϕ, inversely proportional to the decay constant of the dilaton. Another natural constraint on the dialaton ϕ is independence of (1/g ²) exp(ϕ/f_ϕ) from the gauge couplingg. This requirement yields a confining potential proportional tor.     

Charged rotating dilaton black branes in AdS universe

We present the metric for the (n + 1)-dimensional charged rotating dilaton black branes with cylindrical or toroidal horizons in the background of anti-de Sitter spacetime. We find the suitable counterterm which removes the divergences of the action in the presence of the dilaton potential in all higher dimensions. We plot the Penrose diagrams of the spacetime and reveal that the spacetime geometry crucially modifies in the presence of the dilaton field. The conserved and thermodynamic quantities of the black branes are also computed.     

Emergent universe scenario in the Einstein–Gauss–Bonnet gravity with dilaton

We obtain cosmological solutions which admit emergent universe (EU) scenario in the framework of Einstein Gauss–Bonnet (GB) gravity coupled with a dilaton field in 4-dimensions. The coupling parameter of the GB terms and the dilaton in the theory are determined for obtaining an EU scenario. The corresponding dilaton potential which admits such scenario is determined. It is found that the GB terms coupled with a dilaton field plays an important role in describing the dynamics of the evolution of the early as well as the late universe. We note an interesting case where the GB term dominates initially in the asymptotic past regime, subsequently it decreases and thereafter its contribution in determining the dynamics of the evolution dominates once again. We note that the Einstein’s static universe solution permitted here is unstable which the asymptotic EU might follow. We also compare our EU model with supernova data.     

黑洞背景下费米物质能量密度涨落的计算

应用泛函积分方法推导了量子Thirring模型中的传播子和有效势,计算了二维点物质黑洞和dilaton黑洞模型中费米物质的能量密度涨落,在相同的物理条件下,发现dilaton黑洞外费米物质的能量密度涨较大.     

Letter: Inflationary Dilatonic de Sitter Universe from Super Yang-Mills Theory Perturbed by Scalars and Spinors

In this paper a quantum N = 4 super Yang-Mills theory perturbed by dilaton-coupled scalars and spinor fields, is considered. The induced effective action for such a theory is calculated on a dilaton-gravitational background using the conformal anomaly found via the AdS/CFT correspondence. Considering such an effective action (using the large N method) as a quantum correction to the classical gravity action with cosmological constant, we study the effect from the dilaton on the scale factor (this corresponds to an inflationary universe without dilaton). It is shown that, depending on the initial conditions for the dilaton, the dilaton may slow down, or accelerate, the inflation process. At late times, the dilaton is decaying exponentially. Different possible cases corresponding to a dilatonic dS Universe are analyzed with respect to the equations of motion.     

Numerical calculation of the entanglement entropy for scalar field in dilaton spacetimes

Using coupled harmonic oscillators model, we numerical analyze the entanglement entropy of massless scalar field in Gafinkle–Horowitz–Strominger (GHS) dilaton spacetime and Gibbons–Maeda (GM) dilaton spacetime. By numerical fitting, we find that the entanglement entropy of the dilaton black holes receive contribution from dilaton charge and is proportional to the area of the event horizon. It is interesting to note that the results of numerical fitting are coincide with ones obtained by using brick wall method and Euclidean path integral approach.