A note on the mass splitting of K(892)

Belle Collaboration reported a new observed value of K^*－(892) mass by studying τ^－→ K_Sπ－ν_τ decay, which is significantly different from the current world average value given by Particle Data Group 2006. Motivated by this new data, we revisit the issue on the K^*0(892)－K^*±(892) mass splitting. Our theoretical estimation favors the new measurement by Belle Collaboration. Therefore further experimental efforts are urgently needed to improve our understanding of these issues.     

Evidence for special relativity with de Sitter space-time symmetry

I show the formulation of de Sitter Special Relativity (dS-SR) based on Dirac-Lu-Zou-Guo's discussions. dS-SR quantum mechanics is formulated, and the dS-SR Dirac equation for hydrogen is suggested. The equation in the earth-QSO framework reference is solved by means of the adiabatic approach. It's found that the fine-structure "constant" α in dS-SR varies with time. By means of the t-z relation of the ΛCDM model, α's time-dependency becomes redshift z-dependent. The dS-SR's predictions of Δα/α agree with data of spectra of 143 quasar absorption systems, the dS-space-time symmetry is SO(3,2) (i.e., anti-dS group) and the universal parameter R (de Sitter ratio) in dS-SR is estimated to be R≈2.73×10¹² ly. The effects of dS-SR become visible at the cosmic space-time scale (i.e., the distance ≥ 10⁹ ly). At that scale, dS-SR is more reliable than Einstein SR. The α-variation with time is evidence of SR with de Sitter symmetry.     

变加速直线运动黑洞中Weyl中微子的Hawking辐射

利用推广的乌龟坐标变换法研究了作变加速直线运动的Kinnersley黑洞中Weyl中微子的量子 热效应，导出了局部的事件视界面方程和Hawking温度以及中微子的热辐射谱.结果表明视界 的位置和温度不仅随时间变化，而且明显依赖于方位角. 关键词： Hawking辐射 Weyl中微子 动态Kinnersley黑洞 广义乌龟坐标变换     

U(2)L×U(2)R介子手征理论中对衰变ρ→ππ的重求和研究

把U(2)_L×U(2)_R介子手征理论中对矢量介子的O(p⁴)计算用重求和方法进行了改进,并重新研究了衰变ρ→ππ.由此得到了f_ρππ(p²)直到O(p^∞)的完整表达式,并基于收敛性条件和么正性条件给出了一个重要的非微扰结论.     

K*(892)电磁质量反常(英文)

电中性的 K* (892 )电磁质量可以大于带电荷的 K* (892 ) .这是异乎寻常的现象 ,将被称为K* -电磁质量反常 .评述了这个课题 ,并指出 K* 的质量劈裂可以在北京谱仪 (BES)上作精密测量. Electromagnetic masses of neutral K *(892) may be larger than one of charged K *(892). It is unusual and is called K *-EM-mass anomaly. We review the studies on this issue, and point out that K *-mass splitting can be measured in BES accurately.     

One Electron Atom in Special Relativity with de Sitter Space-Time Symmetry(Ⅱ): ——Higher Order Contributions

This is a follow of previous work entitled "One Electron Atom in Special Relativity with de Sitter SpaceTime Symmetry" [Commun. Theor. Phys. 57(2012) 930]. In this paper, we consider the higher order calculations and contributions in the previous framework to solve one electron atoms in de Sitter invariant relativistic quantum mechanics. The next-to-leading-order calculations in 1/R2-expansions show that the fine-structure constant α is variant with cosmologic time going by in the de Sitter invariant special relativistic quantum mechanics with standard FRW cosmologic model.     

在BEPCⅡ/BESⅢ上测量K((892)质量劈裂的Monte Carlo研究

对BEPCⅡ BESⅢ上的J ψ→K±K (892 ) 和J ψ→K0 K (892 ) 0 过程进行了MonteCarlo模拟,对测量K (892 )的质量劈裂的可行性进行了研究.在BESⅢ探测器的设计指标下,采用6×10 8J ψ数据,若输入K (892)0 和K(892)±的质量差为6 0 0MeV ,经过BESⅢ模拟和拟合后的质量差则是5 79±0 16±0 13MeV ,其中第一项误差为统计误差,第二项误差为系统误差.这表明,BESⅢ的建造将为精确测量K (892 )质量劈裂提供极佳机遇.     

＇t Hooft黑洞量子态理论的一个推论

从＇t Hooft将黑洞作为高度简并的量子态的理论出发，考虑黑洞的量子效应，由于海森堡测不准原理，导出视界面上的时空坐标是非对易的．利用非对易场论的办法，研究了大的远离极端情况的Reissner-Nordstrom黑洞，成功的同时推导出黑洞的温度和熵．而且预言了场的动力学自由度的数目该数目支持了最小超对称标准模型．     

关于零质量粒子力学的教学

相对论力学的非真空零质量极限是与光量子的力学，是经典力学过渡到量子力学的桥梁。本研讨力学课程中讲授这种零质量粒子力学的必要性与可能性；在普通力学和理论力学两个层次上分别给出了教案；从科学和教学法两方面对现行的大学普物力学、理论力学、相对论和量子力学教学做了若干批评性述评。最后指出在力学课程中讲授零质量粒子力学的优点。     

用量子色动力学描绘现代核物理的蓝图——评何汉新所著《核色动力学导论》

在2009年科技出版物物理学类著作中,中国科学技术大学出版社出版的何汉新教授的<核色动力学导论--量子色动力学及其对核子和核结构体系的应用>(以下简称<核色动力学导论>)以其新颖的题材引人注目.