洛伦兹对称破缺框架下的广义克莱因-戈尔登谐振子

在洛伦兹对称破缺的背景下研究了广义克莱因-戈尔登谐振子,主要使用Nikiforov-Uvarov方法分析了有磁场和无磁场两种情况下的克莱因-戈尔登谐振子.在此基础上,详细分析了具有康奈尔势函数的克莱因-戈尔登谐振子的一些特殊情况.结果表明,广义克莱因-戈尔登谐振子的波函数和能量本征值明显依赖于洛伦兹对称破缺效应,另外,康奈尔势函数对克莱因-戈尔登谐振子也有着不可忽略的影响.     

超弦低能模型对称性的破缺

本文通过单圈辐射修正的方法,讨论了一个具有规范对称群SU(3)_C×SU(2)_L×SU(2)_R×SU(1)²的超弦低能模型在中间质量M₁处对称性的破缺.在唯象讨论的基础上,我们解决了一般超弦低能模型中存在的中微子质量问题,同时给出了软破缺参数A、m和M初值的取值范围.     

含磁单极电动力学的电磁对偶对称性自发破缺问题

首先提出了一种认为磁单极的存在将导致电动力学电磁对偶对称性自发破缺的新观点,指出了和这种对称性自发破缺相关联的零质量标量粒子即Goldstone玻子存在的可能性.然后通过对含磁单极电动力学作用量描述困难的分析,提醒读者磁单极的存在给电动力学带来的复杂性和不对称.最后为非高能物理背景的读者提供了两类磁单极即经典场扩展位形类磁单极和点粒子磁单极的概念.     

手征破缺模型与饱和核物质的热力学性质

本文在平均场理论框架下用手征破缺模型研究了不同温度区域饱和核物质的热力学性质.改进并推广了Chowdhury等人的结果,通过费米积分的数值积分确认了Chowdhury等处理核物质低温高密度系统近似方法的适用范围为βμ_eff>2.4,给出了(液)-(气)相变临界温度T_c≌23MeV,并得到核子-反核子等离子体相变区域为T=150～200MeV.     

高维de Sitter时空中宇宙视界处的Fermi子隧穿

运用半经典近似理论,本文研究了来自静态高维de Sitter时空和高维Schwarzschild-de Sitter时空宇宙视界处的Fermi子隧穿辐射.在文中,描述1/2自旋粒子行为的Dirac方程被简化为一个简单的形式,接着运用方程组有非平凡解的条件,可以得到了半经典的Hamilton-Jacobi方程,从而使得问题大大得以简化,最终得到了静态de Sitter时空中宇宙视界处的Fermi子隧穿率和Hawking温度.     

高维de Sitter时空中宇宙视界处的Fermi子隧穿

运用半经典近似理论,本文研究了来自静态高维deSitter时空和高维Schwarzschild-de Sitter时空宇宙视界处的Fermi子隧穿辐射.在文中,描述1/2自旋粒子行为的Dirac方程被简化为一个简单的形式,接着运用方程组有非平凡解的条件,可以得到了半经典的Hamilton-Jacobi方程,从而使得问题大大得以简化,最终得到了静态de Sitter时空中宇宙视界处的Fermi子隧穿率和Hawking温度.     

夸克与对称性自发破缺

用普通物理和原子物理的语言论述了对称性破缺机制和理论模型,介绍了2008年度诺贝尔物理学获奖者小林诚(Makoto Kobayashi)、益川敏英(Toshihide Maskawa)关于弱相互作用的理论模型(KM模型)和对称性破缺的起源,它是对电弱统一理论的完美补充;详细分析了在微观粒子世界系列实验中对称性自发破缺和夸克的发现.     

对称性、对称性破缺和相变

本文将扼要介绍物理学中对称性的分类及其特征,说明对称性破缺与一物理系统从无序到有序的相变过程间的关系,并讨论了对称性破缺出现的前提     

对称性自发破缺和希格斯机制

 众所周知,本世纪最辉煌的科学成就之一是弱电统一理论,然而历史上这一理论的重大突破有赖于对对称性自发破缺的研究,特别是希格斯机制的建立。     

关于对称破缺的一些体会

考察了对称破缺的数学形式及物理本质,说明了对称破缺、各态历经假设及序参量空间的一些简单联系,并希望通过这种联系能够更深刻地理解相变、亚平衡等概念,增加热力学和统计力学的统一性。     

ADM Mass for Asymptotically de Sitter Space-Time

In this paper, an ADM mass formula for asymptotically de Sitter（dS） space-time is derived from the energy-momentum tensor. We take the vacuum dS space as the background and investigate the ADM mass of the （d ＋ 3）-dimensional sphere-symmetric space with a positive cosmological constant, and find that the ADM mass of asymptotically dS space is based on the ADM mass of Schwarzschild field and the cosmological background brings some small mass contribution as well.     

第五讲暗能量和德西特时空

最近的天文观测表明，宇宙是在加速膨胀，而不是原来认为的减速膨胀．为解释加速膨胀，必须在宇宙的物质能量中引入暗能量这一成分，文章讨论了暗能量的可能侯选者，特别强调了宇宙常数问题、德西特时空问题以及和德西特时空相关的一些基本问题．     

Cosmological Evolution of a Ghost Scalar Field

We consider a scalar field with a negative kinetic term minimally coupled to gravity. We obtain an exact non-static spherically symmetric solution which describes a wormhole in a cosmological setting. The wormhole is shown to connect two homogeneous spatially flat universes expanding with acceleration. Depending on the wormhole's mass parameter m the acceleration can be constant (the de Sitter case) or infinitely growing.     

How Far Can the Generalized Second Law Be Generalized?

Jacob Bekenstein's identification of black hole event horizon area with entropy proved to be a landmark in theoretical physics. In this paper we trace the subsequent development of the resulting generalized second law of thermodynamics (GSL), especially its extension to incorporate cosmological event horizons. In spite of the fact that cosmological horizons do not generally have well-defined thermal properties, we find that the GSL is satisfied for a wide range of models. We explore in particular the case of an asymptotically de Sitter universe filled with a gas of small black holes as a means of casting light on the relative entropic worth of black hole versus cosmological horizon area. We present some numerical solutions of the generalized total entropy as a function of time for certain cosmological models, in all cases confirming the validity of the GSL.     

Letter: A Twisting Electrovac Solution of Type II with the Cosmological Constant

An exact solution of the current–free Einstein–Maxwell equations with the cosmological constant is presented. It is of Petrov type II, and its double principal null vector is geodesic, shear–free, expanding, and twisting. The solution contains five constants. Its electromagnetic field is non–null and aligned. The solution admits only one Killing vector and includes, as special cases, several known solutions.     

Asymptotically de Sitter and anti-de Sitter black holes with confining electric potential

We study gravity interacting with a special kind of QCD-inspired nonlinear gauge field system which earlier was shown to yield confinement-type effective potential (the “Cornell potential”) between charged fermions (“quarks”) in flat space-time. We find new static spherically symmetric solutions generalizing the usual Reissner-Nordström-de Sitter and Reissner-Nordström-anti-de Sitter black holes with the following additional properties: (i) appearance of a constant radial electric field (in addition to the Coulomb one); (ii) novel mechanism of dynamical generation of cosmological constant through the non-Maxwell gauge field dynamics; (iii) appearance of confining-type effective potential in charged test particle dynamics in the above black hole backgrounds.     

Letter: Casimir Stress for Cylindrical Shell in de Sitter Space

The Casimir stress on a cylindrical shell in the de Sitter background for a massless scalar field satisfying Dirichlet boundary conditions on the cylinder is calculated. The metric is written in conformally flat form to make maximal use of the Minkowski space calculations. In the framework of a toy model, we have considered the quantum vacuum effect in the evolution of a domain wall between a cylindrical or in fact circle region around the z axis in which vacuum is _in and the remaining part of space where vacuum is _out .     

Spinning Particles in Reissner-Nordström-de Sitter Spacetime

We study the geodesic motion of pseudo-classical spinning particles in the Reissner-Nordström-de Sitter spacetime. We investigate the generalized Killing equations for spinning space and derive the constants of motion in terms of the solutions of these equations. We discuss bound state orbits in a plane.     

Interference Phase of Neutrino Oscillation in Schwarzschild-de Sitter Space-Time

We study the mass neutrino interference phase in Schwarzschild-de Sitter space time along the null trajectory and the geodesic line and obtain the effects of cosmological constant A on the neutrino oscillation. Firstly, in the high energy limit, we find that the phase along the geodesic keeps the double of that along the null. Secondly, we calculate the phase on the condition that the cosmological constant, A, is a small quantity. The correction of the phase due to A is given. Finally, we calculate the proper oscillation length in Schwarzschild-de Sitter space-time, which increases because of the existence of A, compared with the result in Schwarzschild space-time. All of our results can be reduced to those in Schwarzschild space-time as A approaches to zero.     

Thermodynamics of de Sitter Black Holes in Massive Gravity

In this paper, by taking de Sitter space-time as a thermodynamic system, we study the effective thermodynamic quantities of de Sitter black holes in massive gravity, and furthermore obtain the effective thermodynamic quantities of the space-time. Our results show that the entropy of this type of space-time takes the same form as that in Reissner-Nordstr¨om-de Sitter space-time, which lays a solid foundation for deeply understanding the universal thermodynamic characteristics of de Sitter space-time in the future. Moreover, our analysis indicates that the effective thermodynamic quantities and relevant parameters play a very important role in the investigation of the stability and evolution of de Sitter space-time.