Lowest-lying spin-1/2 and spin-3/2 baryon magnetic moments in chiral perturbation theory

We review some recent progress in our understanding of the lowest-lying spin-1/2 and spin-3/2 baryon magnetic moments （MMs） in terms of Chiral Perturbation Theory （ChPT）.In particular,we show that at next-to-leading-order ChPT can describe the MMs of the octet baryons quite well.We also make predictions for the decuplet MMs at the same chiral order.Among them,the MMs of the Δ＋＋ and Δ ＋ are found to agree well with data within the experimental uncertainties.     

K0 Condensation in Hyperonic Neutron Star Matter

In the framework of the relativistic mean field theory, we investigate K^0 condensation along with K^- condensation in neutron star matter including the baryon octet. The results show that both K^0 and K^- condensations can occur well in the core of the maximum mass stars for relatively shallow optical potentials of K^- in the range of-100 MeV～ -160 MeV. With the increasing optical potential of K^-, the critical densities of K^- decrease and the species of baryons appearing in neutron stars become fewer. The main role of K^0 condensation is to make the abundances of particles become identical leading to isospin saturated symmetric matter including antikaons, nucleons and hyperons. K^- condensation is chiefly responsible for the softening of the corresponding equation of state, which leads to a large reduction in the maximum masses of neutron stars. In the core of massive neutron stars, neutron star matter including rich particle species, such as antikaons, nucleons and hyperons, may exist.     

宇宙中的暗物质

 十多年来,宇宙中暗物质的研究已成为天体物理、粒子物理和宇宙学的交叉热点,其中的冷暗物质的观测研究也已成为当今非加速器物理实验最热门的课题之一.     

PNJL模型下手征相变的临界指数

在PNJL模型下研究了临界点和旋节线边界上的临界指数。计算表明四个标准的临界指数$\alpha,\,\beta,\,\gamma,\,\delta$在 平均场近似下与朗道-金斯堡理论的预言一致。重子数涨落分布峰态的临界指数$\eta(\approx2)$大于偏态的 临界指数$\zeta(\approx1)$,这表明,如果在重离子碰撞实验中可以达到临界区域,峰态的测量比偏态的测量更加敏感。计算结果还表明,偏态(峰态)在旋节线边界上的临界指数与在临界点的临界指数具有相同的发散强度。根据重子数在不稳定相和亚稳相的剧烈涨落及峰态和偏态在旋节线边界上发散的特点,在将来的实验中用于鉴别一阶相变的信号在一定程度上会被干扰,一些偏离标准一阶相变的信号或许会在观测中发现。     

(S_(NN))~(1/2)=130GeV时Au Au碰撞中的反重子与重子比率

按照夸克随机组合的简单组合模型,本文通过分析得出重子反重子比率与夸克反夸克平均产生几率的关系．进一步计算了相对论重离子碰撞过程中各种反粒子与粒子的比率,不需要任何额外假定, 预言的比率与RHIC加速器时Au Au碰撞STAR实验的结果基本一致．表明夸克组合模型能够解释相对论重离子碰撞过程的反粒子与粒子比率．     

Sigma Terms and Strangeness Contents of Baryon Octet in Modified Chiral Perturbation Theory

In the frame work of chiral perturbation theory, a modified effective Lagrangian for meson-baryon system is constructed, where the SU（3） breaking effect for meson is considered. The difference between physical and chiral limlt decay constants is taken into account. Calculated to one 1ooi） at O（p^3）, the sigma terms and strangeness contents of baryon octet are obtained.     

非奇异重子谱的非微扰效应

在组态混合下,通过解三夸克系统的薛定谔方程,研究了N和△的能谱.考虑的夸克-夸克相互作用位,除通常的微扰单胶子交换位外,还包括两个具有非微扰效应的位,即具有色屏蔽效应的禁闭位和由手征破缺产生的π和σ交换位.所得到的重子谱表明非微扰效应改进了理论与实验的符合程度,从而给出了N和△体系较好的描述.     

五夸克态04国际专题研讨会文集

2003年日本的Spfing-8实验组宣布找到了五夸克态存在的第一个实验证据。这一消息在粒子物理实验和理论家中间引起了强烈的反响，掀起了五夸克研究的空前热潮。2004年7月-20-23日由Spring-8所在的日本大阪大学举办了“Pentaquark 04”国际专题研讨会。会议共收到了64篇报告，126位代表就这种奇物重子态展开了热烈的讨论。     

在e+e－湮没中粲重子介子比

根据e⁺e^－湮没中夸克产生规律和夸克组合规律,本文计算了e⁺e^－湮没中粲重子与粲介子的比值.我们得到的粲重子介子比同能量s有关,并且同实验相符.