K-原子体系与强相互作用

K-原子体系满足KleinGordon方程,通过考虑K-介子与核子之间的强相互作用,引入相应的光学模型势,经求解并数值计算得到的一组K-原子能级,与实验数据吻合得很好,其结果支持了光学模型势描述强相互作用的正确性     

Σ-原子能级的理论计算与分析

通过对Σ-原子的理论分析,数值求解了相应的Dirac方程,得到 了一组Σ-原子的能级值,与实验数据相当吻合;其结果连同K-原子的情况支持了Batty 光学模型势在奇异原子中应用的正确性,进而表明核子间的强相互作用力为吸引力.     

温度相关的核子相对论微观光学势

本文将Walecka模型和热场动力学理论应用在核物质和有限核中,研究了核子在各种温度下的相对论微观光学势以及相应的薛定谔等效势和平均自由程.对于核物质,取核子的Hartree-Fock自能为光学势的实部,交换σ和ω介子的极化图为光学势的虚部.对于有限核的微观光学势通过定域密度近似获得.     

相对论微观光学势的自洽计算

本文以Walecka模型及非线性σ模型自洽计算了¹⁶O、⁴⁰Ca的相对论微观光学势.得到的标量势和矢量势符号相反,大小约为几百MeV,与核子的质量可以相比拟.为了与非相对论光学势比较,给出了Schrodinger等价势.这个等价势在很大的能量范围(E=200MeV以下)内适用,相对论计算自然地得到较强的能量相关的自旋-轨道耦合势,与唯象分析一致.本文用洽计算的实部势及最低级的虚部势计算了核子-核散射微分截面及极化率,得到与实验较好的符合.非线性σ模型给出合理的核的不可压缩系数,从而考虑了核的表面效应,改善了计算的光学势.     

6Li与核弹性散射的微观光学势

从基本的Dirac-Brueckner-Hartree-Fock微观理论出发,得到同时包含实部和虚部的核子-核散射的微观光学势,并利用折叠模型直接获得了核-核散射参数无关的整体微观光学势.考虑到核-核散射去弹过程高级项的贡献和⁶Li的碎裂效应,在微观光学势的实部和虚部中引入了修正因子N_R,N_I.系统研究了入射粒子⁶Li与靶核¹²C,²⁸Si,关键词： 弹性散射 Dirac-Brueckner-Hartree-Fock方法 折叠模型 微观光学势     

核势和核子有效质量的同位旋相关性

在Dirac Brueckner Hartree-Fock (DBHF)理论框架下研究了核子光学势和核子有效质量的同位旋相关性. 非对称核物质的计算采用了DBHF的核子自能的Dirac结构的新的分解方法, 核子自能的实部是用G矩阵在Hartree-Fock近似下计算得到, 而虚部从极化图得到. 用核子的薛定谔等价势可以得到核子矢量有效质量. 研究表明考虑了核势的能量相关性在丰中子核物质情况下核子矢量有效质量比质子的大.     

6Li与核弹性散射的微观光学势

从基本的Dirac-Brueckner-Hartree-Fock微观理论出发,得到同时包含实部和虚部的核子-核散射的微观光学势,并利用折叠模型直接获得了核一核散射参数无关的整体微观光学势.考虑到核.核散射去弹过程高级项的贡献和6Li的碎裂效应,在微观光学势的实部和虚部中引入了修正因子NR,N1.系统研究了入射粒子6Li与靶核12C,28Si,40Ca,58Ni,90Zr和208Pb散射的微观光学势,计算中虚部增强因子取N1≈3.0,而实部修正因子NR对于给定的碰撞系统几乎是一个常数.理论很好地再现了所有被研究靶核和入射能量的弹性散射实验数据.参数无关的微观理论对核.核散射,尤其是对不稳定核.核系统反应的描述是有价值的.     

6Li与核弹性散射的微观光学势

从基本的Dirac-Brueckner-Hartree-Fock微观理论出发，得到同时包含实部和虚部的核子-核散射的微观光学势，并利用折叠模型直接获得了核-核散射参数无关的整体微观光学势.考虑到核-核散射去弹过程高级项的贡献和⁶Li的碎裂效应，在微观光学势的实部和虚部中引入了修正因子N_R，N_I.系统研究了入射粒子⁶Li与靶核¹²C，²⁸Si，相似文献   

相对论微观光学势中相互作用力程的效应

从关于相对论的核子-介子场理论的Walecka模型出发,利用由Walecka模型得到的二核子的相互作用势,对定域密度近似下的光学势进行折叠,来考虑相互作用力程在核——有限核的相对论微观光学势中的效应,并用所得到的光学势分析核子与有关核的弹性散射微分截面和有关自旋可观测量,与定域密度近似计算相比,本文的计算结果同实验值有更好的符合.     

自洽半经典方法与有限温度微观光学势——Ⅰ.实部

从扩展Skyrme力出发,利用自洽半经典(Scsc)方法确定了热核~(40)Ca和~(208)Pb的核子密度_(ρq)(q=n,p);由核物质近似及定域密度近似(LDA)推导了有限温度微观光学势的计算公式.利用这些公式及上述密度,具体计算了不同能量和温度下的核子-核光学势.这样得到的光学势是完全自洽和微观的,并且较完整地考虑了温度对光学势的影响.本文仅讨论光学势的实部.     

Kaon absorption from kaonic atoms and formation spectra of kaonic nuclei

We considered the kaon absorption from atomic states into the nucleus. We found that the nuclear density probed by the atomic kaon significantly depends on the kaon orbit. Then, we re-examined the meanings of the observed strengths of one-body and two-body kaon absorption, and investigated the effects to the formation spectra of kaon bound states by in-flight (K ^-, p) reactions. As a natural consequence, if the atomic kaon probes a smaller nuclear density, the ratio of the two-body absorption at nuclear center is larger than the observed value in kaonic atoms, and the depth of the imaginary potential is deeper even at smaller kaon energies as in kaonic nuclear states because of the large phase space for the two-body processes. This deeper imaginary potential makes the signals of kaonic nucleus formation more unclear in the (K ^-, p) spectra.     

重离子碰撞中K介子和π介子产生的统一动力学模拟

用RVUU模型统一地研究了重离子碰撞中产生的K介子和π介子的动力学过程.考虑了K产生和输运过程的介质效应,同时,计入了π在核物质中的传播.用它模拟了每核子1GeV入射能量的重离子碰撞中π产生和阈下K产生过程.讨论了核介质效应对π末态性质的影响,以及对K末态性质的联带影响.计算结果表明,吸引的π光学势,影响了末态π动量分布,使横动量分布中具有小动量的π产额增大,同时明显增大了K的产额,改变了K的动量分布.这说明要合理地评价重离子碰撞的探测信息,需要统一地研究K和π的这些末态动力学作用.     

Kaon flow in heavy ion collisions

Using transport models that include explicitly the kaon degree of freedom, we have studied kaon flow, i.e., the average kaon transverse momentum as a function of rapidity, and the associated flow parameter in heavy ion collisions at both SIS and AGS energies. It is found that the pattern of kaon flow in heavy ion collisions is sensitive to the kaon potential used in the model and thus provides a useful means for studying the kaon properties in nuclear medium.     

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。     

重离子碰撞中产生的K介子的末态作用

推广了RVUU模型,计入了K介子的平均场势和K与核子的末态重散射.并用它模拟了每核子1GeV入射能量的两个Ca核碰撞的阈下K⁺产生.讨论了K⁺矢量势和K⁺末态重散射效应对K介子的末态性质的影响.计算结果表明,排斥的矢量势,与K⁺的末态重散射相似,明显地影响了末态K⁺动能谱,导致了实验室系中具有大动量的K⁺产额的增大.然而,排斥的K⁺矢量势的计入可观地减少了K⁺的末态重散射的影响.这说明,为了合理地评价K⁺能谱和角分布,K⁺同核子的这些末态作用都是不能忽略的.     

Improved uncertainty budget for optical frequency measurements with microkelvin neutral atoms: Results for a high-stability 40Ca optical frequency standard

Using a Ca optical frequency standard at 657 nm, we demonstrate a method that reduces uncertainties in absolute frequency measurements of optical transitions using freely expanding neutral atoms. Working with atoms that have been laser cooled to 10 μK, we have developed and employed a new technique that combines launching of cold atom clouds with atom interferometry to measure and optimise spectroscopy beam parameters. When applied to a frequency standard with laser beams of high spatial quality, this approach can potentially reduce residual Doppler effect uncertainties to well below one part in 10¹⁶. With Doppler uncertainties greatly suppressed, we investigate other potential shifts at the 1-Hz level with a multiplexed measurement system that takes advantage of the low instability of the calcium frequency standard (4×10^-15 at 1 s). The resultant fractional frequency uncertainty for the standard is 6.6×10^-15, the lowest uncertainty reported to date for a neutral atom optical standard. PACS 06.30.Ft; 32.30.-r; 39.20.+q     

Theory of kaonic atoms

A nonlocal energy-dependent self-consistent kaon-nucleus optical potential is derived for kaonic atoms. Energy level shifts and widths are calculated for several light nuclei, and the results are compared with experiment. The sensitivity of the results to changes in parameters of the nuclear matter distribution is studied. Nonlocality and off-energy-shell effects are examined.The optical potential is derived by means of a Brueckner-type many-body theory with the independent pair approximation for the kaon and the nucleon. The two-body interaction on which the optical potential depends is represented by separable potentials of the Yamaguchi form. Coupled channels ($\text{K}\text{N}$ and Σπ) are used for the I = 0 states, which are dominated by the $\text{Y}{}_0{}^1$ resonance, and only a single channel ($\text{K}\text{N}$) is used for the I = 1 state.Calculations are carried out in three levels of approximation of the nonlocal energy-dependent optical potential. In no approximation is the potential found to be proportional to the nuclear density. Indeed, the real part of the potential changes sign in the nuclear surface. Sensitivity of the results to variations in the nuclear matter distribution is investigated and found to be on the order of experimental error. Nonlocality and off-energy-shell effects are estimated to be at least as large as this error, so that these effects must be included if one wishes to extract information about the nuclear surface from the existing experimental data. The use of correct nucleon wavefunctions and binding energies is similarly found to be essential in the calculation.     

Kaon production at finite temperature and baryon density in an effective relativistic mean field model

We investigate the kaon production at finite temperature and baryon density by means of an effective relativistic mean-field model with the inclusion of the full octet of baryons. Kaons are considered taking into account of an effective chemical potential depending on the self-consistent interaction between baryons. The obtained results are compared with a minimal coupling scheme, calculated for different values of the anti-kaon optical potential.     

Towards more exoticness—X-ray spectroscopy of Ξ− atoms at J-PARC

Atoms with a doubly-strange hadron, namely Ξ^?, are really exotic and interesting objects. We are planning to measure X rays from Ξ^? atoms for the first time at J-PARC, where a high intensity and high quality kaon beam is available. Our purpose is to obtain the strength of the optical potential, and hence to provide information on the Ξ-N interaction which is currently very poorly known. We can accumulate several thousand counts of X rays and determine the level energy shift down to ~0.05 keV. This is sensitive enough to observe the expected level shift (~1 keV) with reasonable accuracy, while the sensitivities for the level width is somewhat weaker (measurable down to ~1 keV).     

Role of the Coulomb interaction in the flow and the azimuthal distribution of kaons from heavy ion reactions

Coulomb final-state interaction of positive charged kaons in heavy ion reactions and its impact on the kaon transverse flow and the kaon azimuthal distribution are investigated within the framework of QMD (quantum molecular dynamics) model. The Coulomb interaction is found to tend to draw the flow of kaons away from that of nucleons and lead to a more isotropic azimuthal distribution of kaons in the target rapidity region. The recent FOPI data have been analyzed by taking into account both the Coulomb interaction and a kaon in-medium potential of the strong interaction. Although the effect of the kaon Coulomb potential on the kaon flow and azimuthal distribution is much smaller than that of the strong potential, it is found to be visible, and therefore, should be taken into account if one wants to extract unambiguous information about the kaon strong potential in nuclear matter from the kaon flow and azimuthal distribution data.