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Nonlinear Spinor Field Equations in Gravitational Theory: Spherical Symmetric Soliton-Like Solutions 被引量:2
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作者 V. Adanhounme A. Adomou +1 位作者 F. P. Codo M. N. Hounkonnou 《Journal of Modern Physics》 2012年第9期935-942,共8页
This paper deals with an extension of a previous work [Gravitation & Cosmology, Vol. 4, 1998, pp 107-113] to exact spherical symmetric solutions to the spinor field equations with nonlinear terms which are arbitra... This paper deals with an extension of a previous work [Gravitation & Cosmology, Vol. 4, 1998, pp 107-113] to exact spherical symmetric solutions to the spinor field equations with nonlinear terms which are arbitrary functions of S=ψψ, taking into account their own gravitational field. Equations with power and polynomial nonlinearities are studied in detail. It is shown that the initial set of the Einstein and spinor field equations with a power nonlinearity has regular solutions with spinor field localized energy and charge densities. The total energy and charge are finite. Besides, exact solutions, including soliton-like solutions, to the spinor field equations are also obtained in flat space-time. 展开更多
关键词 Lagrangian Static SPHERICAL SYMmetric metric field equationS einstein equationS Dirac equation ENERGY-MOMENTUM Tensor Charge Density Current Vector SOLITON-LIKE Solution
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利用Mathematica软件表示真空Einstein场方程
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作者 周建峰 张福 蒋栋荣 《中国科学院上海天文台年刊》 2000年第21期106-110,共5页
介绍了如何从某种形式的度规出发 ,利用Mathematica软件计算联络、Ricci张量和总曲率 ,最终写出了真空Einstein场方程。并在附录中给出了相应的Mathematica程序 ,它可有效地协助用户进行与广义相对论有关的理论、观测研究。
关键词 mathematica软件 度规 einstein场方程 曲率 RICCI张量 广义相对论 天文学
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利用Mathematica软件表示真空Einstein场方程
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作者 周建峰 张福 蒋栋荣 《中国科学院上海天文台年刊》 2000年第0期106-110,共5页
介绍了如何从某种形式的度规出发 ,利用Mathematica软件计算联络、Ricci张量和总曲率 ,最终写出了真空Einstein场方程。并在附录中给出了相应的Mathematica程序 ,它可有效地协助用户进行与广义相对论有关的理论、观测研究。
关键词 mathematica软件 度规 einstein场方程
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The Singularities of Gravitational Fields of Static Thin Loop and Double Spheres Reveal the Impossibility of Singularity Black Holes 被引量:2
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作者 Xiaochun Mei 《Journal of Modern Physics》 2013年第7期974-982,共9页
In the classical Newtonian mechanics, the gravity fields of static thin loop and double spheres are two simple but foundational problems. However, in the Einstein’s theory of gravity, they are not simple. In fact, we... In the classical Newtonian mechanics, the gravity fields of static thin loop and double spheres are two simple but foundational problems. However, in the Einstein’s theory of gravity, they are not simple. In fact, we do not know their solutions up to now. Based on the coordinate transformations of the Kerr and the Kerr-Newman solutions of the Einstein’s equation of gravity field with axial symmetry, the gravity fields of static thin loop and double spheres are obtained. The results indicate that, no matter how much the mass and density are, there are singularities at the central point of thin loop and the contact point of double spheres. What is more, the singularities are completely exposed in vacuum. Space near the surfaces of thin loop and spheres are highly curved, although the gravity fields are very weak. These results are inconsistent with practical experience and completely impossible. By reasonable analogy, black holes with singularity in cosmology and astrophysics are something illusive. Caused by the mathematical description of curved space-time, they do not exist in real world actually. If there are black holes in the universe, they can only be the types of the Newtonian black holes without singularities, rather than the Einstein’s singularity black holes. In order to escape the puzzle of singularity thoroughly, the description of gravity should return to the traditional form of dynamics in flat space. The renormalization of gravity and the unified description of four basic interactions may be possible only based on the frame of flat space-time. Otherwise, theses problems can not be solved forever. Physicists should have a clear understanding about this problem. 展开更多
关键词 General Relativity The einstein’s equation of Gravity field Axially Symmetrical Solutions SINGULARITY Kerr metric Kerr-Newman metric GRAVITATIONAL field of Static Thin LOOP GRAVITATIONAL field of Double SPHERES Black Hole Quasar MECO
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Metric of a Slow Rotating Body with Quadrupole Moment from the Erez-Rosen Metric
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作者 Francisco Frutos-Alfaro Edwin Retana-Montenegro +1 位作者 Iván Cordero-García Javier Bonatti-González 《International Journal of Astronomy and Astrophysics》 2013年第4期431-437,共7页
A metric representing a slowly rotating object with quadrupole moment is obtained using a perturbation method to include rotation into the weak limit of the Erez-Rosen metric. This metric is intended to tackle relativ... A metric representing a slowly rotating object with quadrupole moment is obtained using a perturbation method to include rotation into the weak limit of the Erez-Rosen metric. This metric is intended to tackle relativistic astrometry and gravitational lensing problems in which a quadrupole moment has to be taken into account. 展开更多
关键词 General RELATIVITY einstein field equations QUADRUPOLE Moment Erez-Rosen metric
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高维时空中静态荷电球体的内解(英文) 被引量:1
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作者 谭振强 黄湘寒 +1 位作者 罗量锱 沈有根 《广西大学学报(自然科学版)》 CAS CSCD 2007年第3期285-287,共3页
在假设静态荷电球体内部物质密度为ρ=μr2,电荷密度为σ=σ0e-λ(r)/2的条件下,严格求解高维Einstein-Maxwell场方程,给出了一个精确的内部解.
关键词 高维时空 einstein—Maxwell场方程 静态荷电球体 度规
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Gdel宇宙模型在理想流体条件下的一个近似解
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作者 杨淑敏 张伟 周向玲 《四川理工学院学报(自然科学版)》 CAS 2009年第3期18-20,共3页
在引力源为理想流体条件下,通过对Gdel宇宙基本性质的分析求解了Einstein场方程,给出了一个Gdel宇宙时空度规的近似解。并且对此解进行了分析。结果表明,在参量f(x)的两种不同情况下,Gdel宇宙将分别表现出静态与膨胀的特征。对于膨... 在引力源为理想流体条件下,通过对Gdel宇宙基本性质的分析求解了Einstein场方程,给出了一个Gdel宇宙时空度规的近似解。并且对此解进行了分析。结果表明,在参量f(x)的两种不同情况下,Gdel宇宙将分别表现出静态与膨胀的特征。对于膨胀宇宙,H的取值主要依赖于λ、k以及σ等模型参数。 展开更多
关键词 度规 Gdel 宇宙模型 einstein场方程
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荷电柱状天体外部度规的计算
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作者 吕君丽 周启煌 《湖南师范大学自然科学学报》 CAS 1989年第1期28-35,共8页
本文从静态轴对称度规的一般表达式ds^2=-e^(2u)(dx^0)~2+e^(-2u)[e^(2k)(dx^1)~2+e^(2k)(dx^2)~2+ρ~2(dx^3)~2]出发,结合Einstein-Maxwell方程组,应用渐近平直条件求出弯曲空间中的静电场,解出了荷电柱状天体(静态)外部度规的四级近... 本文从静态轴对称度规的一般表达式ds^2=-e^(2u)(dx^0)~2+e^(-2u)[e^(2k)(dx^1)~2+e^(2k)(dx^2)~2+ρ~2(dx^3)~2]出发,结合Einstein-Maxwell方程组,应用渐近平直条件求出弯曲空间中的静电场,解出了荷电柱状天体(静态)外部度规的四级近似解。 展开更多
关键词 柱状天体 引力场 度规 计算
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一类具有ReisSner-Nordstrom度规的SU(5)双荷解
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作者 余洪伟 王永久 《长沙铁道学院学报》 CSCD 1992年第1期56-60,共5页
本文研究弯曲时空中耦合Yang-Mills-Higgs系统的球对称双荷解.通过求解场方程,我们得到一类具有Reissner-Nordstrom度规的SU(5)双荷解.
关键词 R-N度规 SU(5)双荷 场方程
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荷电流体球的内部度规
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作者 吴亚波 《辽宁师范大学学报(自然科学版)》 CAS 1994年第4期288-293,共6页
对Mehra的荷电流体球的内部度规进行了深入讨论,指出该度规在某种限制条件下具有无奇性,且满足Robson条件.
关键词 荷电 流体球 E-M场方程 S度规 R-N度规
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Gdel宇宙模型在真空条件下的一个近似解
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作者 杨淑敏 张伟 周向玲 《喀什师范学院学报》 2009年第3期32-33,共2页
在真空情况下,通过求解Einstein场方程,给出了一个关于膨胀的Gdel宇宙时空度规的近似解.并且对此解进行了分析.
关键词 度规 Gdel 宇宙模型 einstein场方程
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Gdel宇宙模型的一个近似解
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作者 杨淑敏 李新克 +2 位作者 全条芬 姚乾凯 宋友林 《河南教育学院学报(自然科学版)》 2007年第1期30-32,共3页
通过对Gdel宇宙基本性质的分析,求得了弱场条件下其Einstein方程近似解,并对该解进行了分析.
关键词 度规 einstein场方程 Godel宇宙模型
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轴对称荷电天体外部度规的研究——爱因斯坦-麦克斯韦方程组的精确解
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作者 周启煌 《湖南师范大学自然科学学报》 CAS 1991年第2期117-120,共4页
本文在作者发表于J.Math.Phys.29(1988)杂志中的文章的基础上,通过一系列变量和函数的变换的处理方法,得到了轴对称荷电天体的爱因斯坦—麦克斯韦方程组的一组精确解,此解适用于那些轴对称且平面(垂直于对称轴的平面)对称的所有天体。
关键词 天体 轴对称 度规 E-M方程组
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New Way to Calculate Ricci Tensor and Ricci Scalar
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作者 Abed El Karim S. Abou Layla 《Journal of High Energy Physics, Gravitation and Cosmology》 2019年第3期850-867,共18页
In the theory of general relativity, the finding of the Einstein Field Equation happens in a complex mathematical operation, a process we don’t need any more. Through a new theory in vector analysis, we’ll see that ... In the theory of general relativity, the finding of the Einstein Field Equation happens in a complex mathematical operation, a process we don’t need any more. Through a new theory in vector analysis, we’ll see that we can calculate the components of the Ricci tensor, Ricci scalar, and Einstein Field Equation directly in an easy way without the need to use general relativity theory hypotheses, principles, and symbols. Formulating the general relativity theory through another theory will make it easier to understand this relativity theory and will help combining it with electromagnetic theory and quantum mechanics easily. 展开更多
关键词 General Relativity RICCI TENSOR RICCI SCALAR einstein field equation Stress-Energy TENSOR Robertson-Walker metric SCHWARZSCHILD metric
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Gravitational Space-Time Curve Generation via Accelerated Charged Particles
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作者 Edward A. Walker 《Journal of Modern Physics》 2016年第9期863-874,共12页
A force with an acceleration that is equal to multiples greater than the speed of light per unit time is exerted on a cloud of charged particles. The particles are resultantly accelerated to within an infinitesimal fr... A force with an acceleration that is equal to multiples greater than the speed of light per unit time is exerted on a cloud of charged particles. The particles are resultantly accelerated to within an infinitesimal fraction of the speed of light. As the force or acceleration increases, the particles’ velocity asymptotically approaches but never achieves the speed of light obeying relativity. The asymptotic increase in the particles’ velocity toward the speed of light as acceleration increasingly surpasses the speed of light per unit time does not compensate for the momentum value produced on the particles at sub-light velocities. Hence, the particles’ inertial mass value must increase as acceleration increases. This increase in the particles’ inertial mass as the particles are accelerated produce a gravitational field which is believed to occur in the oscillation of quarks achieving velocities close to the speed of light. The increased inertial mass of the density of accelerated charged particles becomes the source mass (or Big “M”) in Newton’s equation for gravitational force. This implies that a space-time curve is generated by the accelerated particles. Thus, it is shown that the acceleration number (or multiple of the speed of light greater than 1 per unit of time) and the number of charged particles in the cloud density are surjectively mapped to points on a differential manifold or space-time curved surface. Two aspects of Einstein’s field equations are used to describe the correspondence between the gravitational field produced by the accelerated particles and the resultant space-time curve. The two aspects are the Schwarzchild metric and the stress energy tensor. Lastly, the possibility of producing a sufficient acceleration or electromagnetic force on the charged particles to produce a gravitational field is shown through the Lorentz force equation. Moreover, it is shown that a sufficient voltage can be generated to produce an acceleration/force on the particles that is multiples greater than the speed of light per unit time thereby generating gravity. 展开更多
关键词 Charged Particles Accelerated Particles Inertial Mass Gravitational Force einstein’s field equations Space-Time Manifold Schwardchild metric Stress Energy Tensor Surjective Mapping Lorentz Force
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高维球对称时空静态荷电球体的Einstein-Maxwell场方程 被引量:1
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作者 刘云 沈有根 谭振强 《云南大学学报(自然科学版)》 CAS CSCD 北大核心 2008年第5期489-493,共5页
假设荷电球体内部电荷密度σ=σ0rbe-2λ,严格求解Einstein-Maxwell场方程,给出了高维球对称时空中静态荷电球体的一个精确内解,并得到了高维时空中荷电球体的电磁质量计算公式和总引力质量的计算公式.
关键词 度规 einstein—Maxwell场方程 静态荷电球体 高维时空
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一阶常微分方程的计算机辅助教学 被引量:6
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作者 桂占吉 宋作忠 《数学的实践与认识》 CSCD 北大核心 2004年第5期163-167,共5页
利用计算机软件 Mathematica探讨了一阶常微分方程的计算机辅助教学 .
关键词 微分方程 mathematica软件 积分曲线 方向场
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