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On the Origin of Mass and Angular Momentum of Stellar Objects
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作者 Peter C. W. Fung K. W. Wong 《Journal of Modern Physics》 2015年第15期2303-2341,共39页
The consequence of the 5D projection theory [1] is extended beyond the Gell-Mann Standard Model for hadrons to cover astronomical objects and galaxies. The proof of Poincare conjecture by Pe-relman’s differential geo... The consequence of the 5D projection theory [1] is extended beyond the Gell-Mann Standard Model for hadrons to cover astronomical objects and galaxies. The proof of Poincare conjecture by Pe-relman’s differential geometrical techniques led us to the consequence that charged massless spinors reside in a 5D void of a galactic core, represented by either an open 5D core or a closed, time frozen, 3D × 1D space structure, embedded in massive structural stellar objects such as stars and planets. The open galactic core is obtained from Ricci Flow mapping. There exist in phase, in plane rotating massless spinors within these void cores, and are responsible for 1) the outward spiral motion of stars in the galaxy in the open core, and 2) self rotations of the massive stellar objects. It is noted that another set of eigen states pertaining to the massless charged spinor pairs rotating out of phase in 1D (out of the 5D manifold) also exist and will generate a relatively weak magnetic field out of the void core. For stars and planets, it forms the intrinsic dipole field. Due to the existence of a homogeneous 5D manifold from which we believe the universe evolves, the angular momentum arising from the rotation of the in-phase spinor pairs is proposed to be counter-balanced by the rotation of the matter in the surrounding Lorentz domain, so as to conserve net zero angular momentum. Explicit expression for this total angular momentum in terms of a number of convergent series is derived for the totally enclosed void case/core, forming in general the structure of a star or a planet. It is shown that the variables/parameters in the Lorentz space-time domain for these stellar objects involve the object’s mass M, the object’s Radius R, period of rotation P, and the 5D void radius Ro, together with the Fermi energy Ef and temperature T of the massless charged spinors residing in the void. We discovered three laws governing the relationships between Ro/R, T, Ef and the angular momentum Iω of such astronomical object of interest, from which we established two distinct regions, which we define as the First and Second Laws for the evolution of the stellar object. The Fermi energy Ef was found to be that of the electron mass, as it is the lightest massive elementary particle that could be created from pure energy in the core. In fact the mid-temperature of the transition region between the First and Second Law regions for this Ef value is 5.3 × 109 K, just about that of the Bethe fusion temperature. We then apply our theory to analyse observed data of magnetars, pulsars, pre-main-sequence stars, the NGC 6819 group, a number of low-to-mid mass main sequence stars, the M35 members, the NGC 2516 group, brown dwarfs, white dwarfs, magnetic white dwarfs, and members of the solar system. The ρ = (Ro/R) versus T, and ρ versus P relations for each representative object are analysed, with reference to the general process of stellar evolution. Our analysis leads us to the following age sequence of stellar evolution: pulsars, pre-main-sequence stars, matured stars, brown dwarfs, white dwarfs/magnetic white dwarfs, and finally neutron stars. For every group, we found that there is an increasing average mass density during their evolution. 展开更多
关键词 ORIGIN of MASS and Self Rotation of STELLAR Objects Angular momentum fermi-Dirac Distribution
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自旋轨道角动量耦合的超流费米气体
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作者 徐子威 杨明月 +1 位作者 纪安春 孙青 《首都师范大学学报(自然科学版)》 2024年第2期65-73,共9页
近年来,自旋轨道耦合的原子气体研究取得了许多重要的进展,其中一种新近实现的新类型自旋轨道耦合-自旋轨道角动量耦合由于其独特性质吸引了人们的兴趣。本文以费米气体为例,介绍自旋轨道角动量耦合的实现和特点,以及对单粒子谱特别是... 近年来,自旋轨道耦合的原子气体研究取得了许多重要的进展,其中一种新近实现的新类型自旋轨道耦合-自旋轨道角动量耦合由于其独特性质吸引了人们的兴趣。本文以费米气体为例,介绍自旋轨道角动量耦合的实现和特点,以及对单粒子谱特别是对费米超流的重要影响。结合平均场解析方法和数值模拟,分析了自旋轨道角动量耦合诱导的有限角动量配对和由此导致的不同类型的超流涡旋基态,并进一步讨论了相关的进展和未来可能的发展方向。 展开更多
关键词 费米气体 自旋轨道角动量耦合 费米超流 涡旋态
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一维接触排斥相互作用单自旋翻转费米气体的基态和淬火动力学性质
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作者 尹相国 于海如 +1 位作者 郝亚江 张云波 《物理学报》 SCIE EI CSCD 北大核心 2024年第2期76-88,共13页
基于严格解方法,研究了一维排斥相互作用单自旋翻转费米气体的基态和淬火动力学性质.借助Bethe波函数,基态和不同本征态之间的单体关联函数和两体关联函数可以表示为简单函数之和,这一简洁形式可以极大地降低计算难度.系统初始状态为无... 基于严格解方法,研究了一维排斥相互作用单自旋翻转费米气体的基态和淬火动力学性质.借助Bethe波函数,基态和不同本征态之间的单体关联函数和两体关联函数可以表示为简单函数之和,这一简洁形式可以极大地降低计算难度.系统初始状态为无相互作用的基态,当迅速把相互作用强度调节为有限大时,动量分布和关联函数出现周期性的振荡行为;当相互作用调节为比较弱时,振荡周期性好且振荡幅度小,系统可以用二能级模型近似;当相互作用调为非常强时,振荡周期性变差且振荡幅度大,但是依然存在主周期.此时整体偏离初态较远,但是在时间为mL^(2)/(2πh)时系统非常接近初态. 展开更多
关键词 一维费米气体 动量分布 关联函数 淬火动力学
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短程关联对核内核子动量分布的影响
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作者 李小华 李明 +2 位作者 吴喜军 向东 郑波 《西北大学学报(自然科学版)》 CAS CSCD 北大核心 2014年第6期890-892,903,共4页
原子核内核子的动量分布对于研究原子核结构的性质至关重要,核子关联是影响核内核子动量分布的一个重要因素。文中基于核内核子短程关联的性质,分析研究了核内核子的动量分布,并计算了一些原子核内核子处在费米面以上的几率,计算结果与... 原子核内核子的动量分布对于研究原子核结构的性质至关重要,核子关联是影响核内核子动量分布的一个重要因素。文中基于核内核子短程关联的性质,分析研究了核内核子的动量分布,并计算了一些原子核内核子处在费米面以上的几率,计算结果与实验数据符合得很好。 展开更多
关键词 短程关联 动量分布 费米动量
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Neutron Star Magnetic Field as for Nonzero Photon Mass
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作者 WANGQing-Wu LǖXiao-Fu 《Communications in Theoretical Physics》 SCIE CAS CSCD 2005年第4期704-708,共5页
We investigate the neutron star magnetic field by the relative mean-field theory, where the photon effective mass depending on baryon density of charged particles is nonzero. This field is produced by star itself, whi... We investigate the neutron star magnetic field by the relative mean-field theory, where the photon effective mass depending on baryon density of charged particles is nonzero. This field is produced by star itself, which is the function of baryon density. The result fits the observations. 展开更多
关键词 effective photon mass fermi momentum beta-equilibrium
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铁的γ射线康普顿轮廓
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作者 顾广颐 俞飞 宫竹芳 《淮南矿业学院学报》 1994年第3期83-86,共4页
摘要用活度为210mCi ^241Am放射源发出的γ射线测量铁的康普顿轮廓。由此求出铁的费米动量是0.98±0.04a.u.这一结果与自由电子气模型计算结果相一致。
关键词 γ 射线 康普顿轮廓 费米动量 实验误差 数据处理
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玻色统计和费米统计分布律的相对论修正
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作者 谢文杰 畅福善 《山西师范大学学报(自然科学版)》 2009年第4期46-49,共4页
本文分别给出了非相对论和相对论情况下玻色统计和费米统计的能量,动量以及速率分布函数,结果发现在考虑相对论情况时,玻色统计和费米统计的能量和动量分布的大体形状是不变的,但速率分布就有了较大的变化.
关键词 玻色统计 费米统计 相对论修正 动量分布 速率分布
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费米动量对中能重离子碰撞椭圆流的影响
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作者 高波 王永佳 +1 位作者 李庆峰 李保春 《核技术》 CAS CSCD 北大核心 2023年第7期69-77,共9页
椭圆流(v_2)是利用重离子碰撞探究核物质性质最重要的观测量之一,它的大小除了受到动力学过程的影响外,还与初态核子的费米动量有关。基于极端相对论量子分子动力学(Ultrarelativistic Quantum Molecular Dynamics,UrQMD)模型,通过反向... 椭圆流(v_2)是利用重离子碰撞探究核物质性质最重要的观测量之一,它的大小除了受到动力学过程的影响外,还与初态核子的费米动量有关。基于极端相对论量子分子动力学(Ultrarelativistic Quantum Molecular Dynamics,UrQMD)模型,通过反向追踪反应末态处在中心快度区(|y0|<0.1)的核子的v_2随时间的演化过程。探究初始时无费米动量、有费米动量和有一半费米动量对v_2演化的影响。以束流能量为0.4A GeV和0.8A GeV、碰撞参数为6 fm的金与金(Au+Au)碰撞为例,计算结果表明有费米动量时中心快度区的核子数远多于无费米动量的情况,这是由于不考虑费米动量时,核子-核子碰撞数目减少而导致。而v_2却表现出相反的效应,不考虑费米动量时的v_2更大,因为旁观核子有更强的阻止效应。这表明核子动量的初始化需要在输运模型中细致考虑。 展开更多
关键词 重离子碰撞 费米动量 椭圆流
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Projectile Fragmentation in ^(20)Ne-^(165)Ho Reaction at 45 MeV/u 被引量:1
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作者 G.X.Dai J.B.Natowitz +9 位作者 R.Wada K.Hagel Q.Z.Luo Z.Y.He J.Blackadar S.Lee J.T.Li Y.N.Lou D.Utley B.Xiao 《Chinese journal of nuclear physics》 1995年第3期228-233,共6页
At 45 MeV/u an experiment on fragmentation of projectile(<sup>20</sup>Ne)on <sup>165</sup>Ho was performed.An average reduced width σ<sub>0</sub> of 84.3±6.6 MeV/c was obtaine... At 45 MeV/u an experiment on fragmentation of projectile(<sup>20</sup>Ne)on <sup>165</sup>Ho was performed.An average reduced width σ<sub>0</sub> of 84.3±6.6 MeV/c was obtained by separating the break=up of all com-plex fragments of <sup>20</sup>Ne from the evaporation part of compound nucleus in momentum spectra. 展开更多
关键词 Projectile FRAGMENTATION Reduced width of fermi momentum 20Ne+165Ho REACTION
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Correlation between Nucleon-Nucleon Interaction, Pairing Energy Gap and Phase Shift for Identical Nucleons in Nuclear Systems
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作者 Willy K. Koech Ken M. Muguro +1 位作者 Godfrey S. Murunga Kapil M. Khanna 《Journal of High Energy Physics, Gravitation and Cosmology》 2019年第2期321-331,共11页
Assuming some known nucleon-nucleon interactions, and using the relations between phase shift δ and nucleon-nucleon interaction potential V (r);the relation between nucleon-nucleon interaction and scattering length a... Assuming some known nucleon-nucleon interactions, and using the relations between phase shift δ and nucleon-nucleon interaction potential V (r);the relation between nucleon-nucleon interaction and scattering length a;the relation between energy gap Δ, and scattering length a;an equation is obtained between energy gap Δ and Fermi momentum kF via the phase shift δ (kF). Assuming 1s0 (singlet) pairing between the nucleons, the energy gap Δ has been calculated and it is found that Δ = 3.0 MeV at Fermi momentum kF = 0.8 fm-1. 展开更多
关键词 SCATTERING Length PAIRING Gap Phase SHIFT fermi momentum
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Spin-orbit coupling in Bose-Einstein condensate and degenerate Fermi gases 被引量:3
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作者 Peng-Jun Wang Jing Zhang 《Frontiers of physics》 SCIE CSCD 2014年第5期598-612,共15页
We review our recent experimental realization and investigation of a spin orbit (SO) coupled Bose Einstein condensate (BEC) and quantum degenerate Fermi gas. By using two counter-propagathlg Ranlan lasers and cont... We review our recent experimental realization and investigation of a spin orbit (SO) coupled Bose Einstein condensate (BEC) and quantum degenerate Fermi gas. By using two counter-propagathlg Ranlan lasers and controlling the different frequency of two R,aman lasers to engineer the atom light interaction, we first study the SO coupling in BEC. Then we study SO coupling in Fermi gas. We, observe the spin dephasing in spin dynamics and momentum distribution asymmetry of the equilibrium state as halhnarks of SO coupling in a Fermi gas. To clearly reveal the, property of SO coupling Fermi gas, we also study the momentmn-resolved radio-frequency spectroscopy which characterizes the energy momentum dispersion and spin composition of the quantum states. We observe the change of errmion surfaces in different helieity branches with different atomic density, which indicates that a Lifshitz transition of the Fermi surface topology change can be found by further cooling the system. At last, we study the momentum-resolved Raman spectroscopy of an ultracoht Fermi gas. 展开更多
关键词 spin-orbit coupling Bose Einstein condensate fermi gases topological change momentum-resolved radio-frequency spectroscopy momentum-resolved Raman spectroscopy
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原子核内的夸克分布 Ⅳ EMC效应的复合模型
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作者 王正本 《云南大学学报(自然科学版)》 CAS CSCD 1991年第3期214-218,共5页
本文建立了EMC效应的复合模型。计算表明,这一模型能较好地解释整个x_B区的测量数据,特别是与最新实验数据符合很好。
关键词 原子核 夸克分布 EMC效应 复合模型
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