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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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Riemannian Space-Time, de Donder Conditions and Gravitational Field in Flat Space-Time 被引量:1
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作者 Gordon Liu 《International Journal of Astronomy and Astrophysics》 2013年第1期8-19,共12页
Let the coordinate system xi of flat space-time to absorb a second rank tensor field Φij of the flat space-time deforming into a Riemannian space-time, namely, the tensor field Φuv is regarded as a metric tensor wit... Let the coordinate system xi of flat space-time to absorb a second rank tensor field Φij of the flat space-time deforming into a Riemannian space-time, namely, the tensor field Φuv is regarded as a metric tensor with respect to the coordinate system xu. After done this, xu is not the coordinate system of flat space-time anymore, but is the coordinate system of the new Riemannian space-time. The inverse operation also can be done. According to these notions, the concepts of the absorption operation and the desorption operation are proposed. These notions are actually compatible with Einstein’s equivalence principle. By using these concepts, the relationships of the Riemannian space-time, the de Donder conditions and the gravitational field in flat space-time are analyzed and elaborated. The essential significance of the de Donder conditions (the harmonic conditions or gauge) is to desorb the tensor field of gravitation from the Riemannian space-time to the Minkowski space-time with the Cartesian coordinates. Einstein equations with de Donder conditions can be solved in flat space-time. Base on Fock’s works, the equations of gravitational field in flat space-time are obtained, and the tensor expression of the energy-momentum of gravitational field is found. They all satisfy the global Lorentz covariance. 展开更多
关键词 General Relativity gravitation RIEMANNIAN SPACE-TIME FLAT SPACE-TIME Einstein Equations Harmonic CONDITIONS energy-momentum tensor Significance of the Coordinates gravitational RED-SHIFT
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Note on Energy-Momentum Tensor for General Mixed Tensor-Spinor Fields
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作者 ZHANG Hong-Bao 《Communications in Theoretical Physics》 SCIE CAS CSCD 2005年第6X期1007-1010,共4页
This note provides an explicit proof of the equivalence of Belinfante's energy-momentum tensor and metric energy-momentum tensor for general mixed tensor-spinor fields.
关键词 Belinfante's energy-momentum tensor metric energy-momentum tensor general mixed tensorspinor fields
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Gravitational radiation fields in teleparallel equivalent of general relativity and their energies
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作者 Gamal G.L.Nashed 《Chinese Physics B》 SCIE EI CAS CSCD 2010年第11期132-139,共8页
We derive two new retarded solutions in the teleparallel theory equivalent to general relativity (TEGR). One of these solutions gives a divergent energy. Therefore, we use the regularized expression of the gravitati... We derive two new retarded solutions in the teleparallel theory equivalent to general relativity (TEGR). One of these solutions gives a divergent energy. Therefore, we use the regularized expression of the gravitational energymomentum tensor, which is a coordinate dependent. A detailed analysis of the loss of the mass of Bondi space-time is carried out using the flux of the gravitational energy-momentum. 展开更多
关键词 teleparallel equivalent of general relativity energy-momentum tensor Bondi mass gravitational radiation
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The Basic Concepts and Basic Laws Relating to Matter and Gravitational Fields in Physics
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作者 Fangpei Chen 《Journal of Modern Physics》 2017年第11期1784-1794,共11页
In this work, the author applied the universal gauge field theory and Noether theorem to prove that universality exists for the Lorentz and Levi-Civita law of conservation of energy momentum tensor density. We also fo... In this work, the author applied the universal gauge field theory and Noether theorem to prove that universality exists for the Lorentz and Levi-Civita law of conservation of energy momentum tensor density. We also found that this conservation law has profound implications in physics. For example, based on this law, one can explore the origin of the matter field, and propose a new view about what is “dark energy” and what is “dark matter”. 展开更多
关键词 LAGRANGIAN MATTER field gravitational field energy-momentum tensor Density Conservation Law Origin of MATTER field
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A Locally Conservative Energy-Momentum Tensor in the General Relativity Based on a Cosmological Model without Singularity 被引量:1
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作者 Shihao Chen 《Journal of Modern Physics》 2016年第3期277-280,共4页
According to the conventional theory it is difficult to define the energy-momentum tensor which is locally conservative. The energy-momentum tensor of the gravitational field is defined. Based on a cosmological model ... According to the conventional theory it is difficult to define the energy-momentum tensor which is locally conservative. The energy-momentum tensor of the gravitational field is defined. Based on a cosmological model without singularity, the total energy-momentum tensor is defined which is locally conservative in the general relativity. The tensor of the gravitational mass is different from the energy-momentum tensor, and it satisfies the gravitational field equation and its covariant derivative is zero. 展开更多
关键词 energy-momentum tensor of gravitational field Locally Conservative energy-momentum tensor in General Relativity tensor of the gravitational Mass Quasi-Local energy-momentum tensor
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Curvature Energy and Their Spectrum in the Spinor-Twistor Framework: Torsion as Indicium of Gravitational Waves
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作者 Francisco Bulnes Yuri Stropovsvky Igor Rabinovich 《Journal of Modern Physics》 2017年第10期1723-1736,共14页
The twistor kinematic-energy model of the space-time and the kinematic-energy tensor as the energy-matter tensor in relativity are considered to demonstrate the possible behavior of gravity as gravitational waves that... The twistor kinematic-energy model of the space-time and the kinematic-energy tensor as the energy-matter tensor in relativity are considered to demonstrate the possible behavior of gravity as gravitational waves that derive of mass-energy source in the space-time and whose contorted image is the spectrum of the torsion field acting in the space-time. The energy of this field is the energy of their second curvature. Likewise, it is assumed that the curvature energy as spectral curvature in the twistor kinematic frame is the curvature in twistor-spinor framework, which is the mean result of this work. This demonstrates the lawfulness of the torsion as the indicium of the gravitational waves in the space-time. A censorship to detect gravitational waves in the space-time is designed using the curvature energy. 展开更多
关键词 CENSORSHIP Condition Contorted Surface CURVATURE ENERGY gravitational Waves Matter-Energy tensor 3-Dimensional Sphere SPINOR fields Twistor Kinematic-Energy Model WEYL CURVATURE
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Fourth Rank Energy-Momentum Tensor
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作者 Vu B. Ho 《Journal of Applied Mathematics and Physics》 2022年第12期3684-3692,共9页
In this work, we introduce the new concept of fourth rank energy-momentum tensor. We first show that a fourth rank electromagnetic energy-momentum tensor can be constructed from the second rank electromagnetic energy-... In this work, we introduce the new concept of fourth rank energy-momentum tensor. We first show that a fourth rank electromagnetic energy-momentum tensor can be constructed from the second rank electromagnetic energy-momentum tensor. We then generalise to construct a fourth rank stress energy-momentum tensor and apply it to Dirac field of quantum particles. Furthermore, since the established fourth rank energy-momentum tensors have mathematical properties of the Riemann curvature tensor, thus it is reasonable to suggest that quantum fields should also possess geometric structures of a Riemannian manifold. 展开更多
关键词 Fourth Rank energy-momentum tensor Riemannian Manifold Riemann Curvature tensor Electromagnetic field Dirac field
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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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Representation of Physical Fields as Einstein Manifold
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作者 Vu B. Ho 《Journal of Applied Mathematics and Physics》 2023年第3期599-607,共9页
In this work we investigate the possibility to represent physical fields as Einstein manifold. Based on the Einstein field equations in general relativity, we establish a general formulation for determining the metric... In this work we investigate the possibility to represent physical fields as Einstein manifold. Based on the Einstein field equations in general relativity, we establish a general formulation for determining the metric tensor of the Einstein manifold that represents a physical field in terms of the energy-momentum tensor that characterises the physical field. As illustrations, we first apply the general formulation to represent the perfect fluid as Einstein manifold. However, from the established relation between the metric tensor and the energy-momentum tensor, we show that if the trace of the energy-momentum tensor associated with a physical field is equal to zero then the corresponding physical field cannot be represented as an Einstein manifold. This situation applies to the electromagnetic field since the trace of the energy-momentum of the electromagnetic field vanishes. Nevertheless, we show that a system that consists of the electromagnetic field and non-interacting charged particles can be represented as an Einstein manifold since the trace of the corresponding energy-momentum of the system no longer vanishes. As a further investigation, we show that it is also possible to represent physical fields as maximally symmetric spaces of constant scalar curvature. 展开更多
关键词 General Relativity Einstein Manifold energy-momentum tensor Electromagnetic field Perfect Fluid Maximally Symmetric Spaces
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Forward Modeling of Gravity,Gravity Gradients,and Magnetic Anomalies due to Complex Bodies 被引量:6
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作者 骆遥 姚长利 《Journal of China University of Geosciences》 SCIE CSCD 2007年第3期280-286,共7页
On the basis of the results of improved analytical expression of computation of gravity anomalies due to a homogeneous polyhedral body composed of polygonal facets, and applying the forward theory with the coordinate ... On the basis of the results of improved analytical expression of computation of gravity anomalies due to a homogeneous polyhedral body composed of polygonal facets, and applying the forward theory with the coordinate transformation of vectors and tensors, we deduced both the analytical expressions for gravity gradient tensors and for magnetic anomalies of a polygon, and obtained new analytical expressions for computing vertical gradients of gravity anomalies and vertical component of magnetic anomalies caused by a polyhedral body. And also we developed explicitly the complete unified expressions for the calculation of gravity anomalies, gravity gradient, and magnetic anomalies due to the homogeneous polyhedron. Furthermore, we deduced new analytical expressions for computing vertical gradients of gravity anomalies due to a finite rectangular prism by applying the newly obtained expressions for gravity gradient tensors due to a polyhedral target body. Comparison with forward calculation of models shows the correctness of these new expressions. It will reduce forward calculation time of gravity-magnetic anomalies and improve computational efficiency by applying our unified expressions for joint forward modeling of gravity-magnetic anomalies due to homogeneous polyhedral bodies. 展开更多
关键词 polyhedral body gravitational field and magnetic field gravity gradient tensor forward calculation coordinate transformation
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Plane Symmetric Solutions to the Nonlinear Spinor Field Equations in General Relativity Theory 被引量:5
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作者 A. Adomou Jonas Edou Siaka Massou 《Journal of Modern Physics》 2019年第10期1222-1234,共13页
We have obtained exact static plane-symmetric solutions to the spinor field equations with nonlinear terms which are arbitrary functions of invariant , taking into account their own gravitational field. It is shown th... We have obtained exact static plane-symmetric solutions to the spinor field equations with nonlinear terms which are arbitrary functions of invariant , taking into account their own gravitational field. It is shown that the initial set of the Einstein and spinor field equations with a power-law nonlinearity have regular solutions with a localized energy density of the spinor field only if m=0 (m is the mass parameter in the spinor field equations). Equations with power and polynomial nonlinearities are studied in detail. In this case, a soliton-like configuration has negative energy. We have also obtained exact static plane-symmetric solutions to the above spinor field equations in flat space-time. It is proved that in this case soliton-like solutions are absent. 展开更多
关键词 LAGRANGIAN Static Plane-Symmetric Metric field EQUATIONS energy-momentum tensor Charge Density Current Vector SOLITON-LIKE Solution
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Time-Machine Solutions of Einstein's Equations with Electromagnetic Field
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作者 沈明 孙庆有 《Communications in Theoretical Physics》 SCIE CAS CSCD 2011年第1期69-71,共3页
In this paper we investigate the time-machine problem in the electromagnetic field. Based on a metric which is a more general form of Ori's, we solve the Einstein's equations with the energy-momentum tensors for ele... In this paper we investigate the time-machine problem in the electromagnetic field. Based on a metric which is a more general form of Ori's, we solve the Einstein's equations with the energy-momentum tensors for electromagnetic field, and construct the time-machine solutions, which solve the time machine problem in electromagnetic field. 展开更多
关键词 time-machine solutions closed timelike curves Einstein's equations energy-momentum tensor electromagnetic field energy conditions
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On Quasi-Einstein Field Equation
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作者 赵培标 杨孝平 《Northeastern Mathematical Journal》 CSCD 2005年第4期411-420,共10页
In this paper some properties of a symmetric tensor field T(X,Y) = g(A(X), Y) on a Riemannian manifold (M, g) without boundary which satisfies the S quasi-Einstein equation Rij-S/2gij=Tij+bξiξj are given. ... In this paper some properties of a symmetric tensor field T(X,Y) = g(A(X), Y) on a Riemannian manifold (M, g) without boundary which satisfies the S quasi-Einstein equation Rij-S/2gij=Tij+bξiξj are given. The necessary and sufficient conditions for this tensor to satisfy the quasi-Einstein equation are also obtained. 展开更多
关键词 Einstein field equation quasi-Einstein field equation Minkowski space Parallel field gravitational field “Ricci” symmetric tensor Lagrange equation
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The gravitational gradient tensor’s invariants and the related boundary conditions 被引量:7
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作者 YU JinHai1,2,3 & ZHAO DongMing4 1 College of Earth Science, Graduate University of Chinese Academy of Sciences, Beijing 100049, China 2 Institute of Geodesy and Geophysics, Chinese Academy of Sciences, Wuhan 430077, China +1 位作者 3 State Key Laboratory of Astronautic Dynamics, Xi’an 710043, China 4 Zhengzhou Institute of Surveying and Mapping, Zhengzhou 450052, China 《Science China Earth Sciences》 SCIE EI CAS 2010年第5期781-790,共10页
Here we report new approaches of recovering the Earth gravitational field from GOCE (Gravity field and steady-state Ocean Circulation Explorer) gradiometric data with the help of the gradient tensor’s invariants. Our... Here we report new approaches of recovering the Earth gravitational field from GOCE (Gravity field and steady-state Ocean Circulation Explorer) gradiometric data with the help of the gradient tensor’s invariants. Our results only depend on GOCE satellite’s position and gradiometry, in other words, they are completely independent of the satellite attitude. First, starting from the invariants, linearization models are established, which can be referred as the general boundary conditions on the satellite’s orbit. Then, the spherical approximation expressions for the models are derived, and the corresponding solving methods for them are discussed. Furthermore, considering effects of J2-term, the spherical approximation models are improved so that the accuracies of the boundary conditions can be theoretically raised to O ( J 2/2 T), which is approximately equivalent to O(T2). Finally, some arithmetic examples are constructed from EGM96 model based on the derived theories, and the computational results illustrate that the spherical models have accuracies of 10-7 and the order recovering the gravitational field can reach up to 200, and the models with regard to effect of J2-term have accuracies of 10-8 and the order can reach up to 280. 展开更多
关键词 the Earth’s gravitational field gravitational gravidiometry tensor’s INVARIANT
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复杂形体重力场、梯度及磁场计算方法 被引量:7
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作者 骆遥 姚长利 《地球科学(中国地质大学学报)》 EI CAS CSCD 北大核心 2007年第4期517-522,共6页
在改进均匀多面体重力场正演公式基础上,利用二阶张量的坐标变换实现对多面体重力场梯度的求解,推导了新的多面体重力梯度和磁场的正演公式,给出了新的统一的均匀多面体重力场、梯度及磁场正演表达式形式,并用理论模型进行了检验.同时,... 在改进均匀多面体重力场正演公式基础上,利用二阶张量的坐标变换实现对多面体重力场梯度的求解,推导了新的多面体重力梯度和磁场的正演公式,给出了新的统一的均匀多面体重力场、梯度及磁场正演表达式形式,并用理论模型进行了检验.同时,应用新的多面体重力场梯度正演公式推导出新的长方体重力场垂直梯度理论表达式.本文给出的均匀多面体重力场、梯度及磁场正演表达式形式统一,重磁场联合正演中可相互利用其计算过程中的结果,避免重复计算以提高正演计算效率. 展开更多
关键词 多面体 重磁场 梯度张量 正演 坐标变换
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有挠引力场之能动张量密度及自旋密度的再研究 被引量:5
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作者 陈方培 《大连理工大学学报》 CAS CSCD 北大核心 1998年第2期157-161,共5页
在有挠情况下对引力场的能动张量密度及自旋密度进行了再研究,肯定了定义T(G)μidefδLG/δhiμ及C(G)μijdef-2δLG/δΓijμ的合理性,导出了引力波虽存在但不携带能量、动量及自旋的结论.
关键词 引力场 能动张量密度 自旋密度 挠率
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荷磁矩中子星外部的电磁场能量动量张量 被引量:1
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作者 石东平 吴张晗 《重庆大学学报(自然科学版)》 EI CAS CSCD 北大核心 2004年第3期69-73,共5页
利用王永久等人所得到的具有磁矩的球对称质量外部的引力场度规和电磁势的表达式,计算出了球对称质量外部的电磁场量动量张量。数值计算结果和分布曲线表明,时空的弯曲将引起磁偶极子电磁场能量的增加。
关键词 磁矩 球对称质量 引力场度规 电磁势 电磁场能量动量张量 中子星
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引力场的运动方程及引力波的互作用 被引量:3
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作者 青心 《山东师范大学学报(自然科学版)》 CAS 1997年第1期40-45,共6页
在Vierbein表述的局域Lorentz群引力规范理论中,合理地定义了引力场的张力张量,给出了广义协变的引力场的运动方程,讨论了一般对角度规引力波情况以及Bondi引力平面波、引力孤立波各部分之间的互作用等有关问题.
关键词 引力场 运动方程 引力波 相互作用
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引力场能动张量定义的历史争论及重新研究 被引量:2
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作者 陈方培 《河北师范大学学报(自然科学版)》 CAS 2000年第3期326-329,共4页
引力场的能动张量是引力理论中一个极为重要的物理量 .八十多年前 Levi-Civita等人同爱因斯坦曾就这个量的定义及守恒律展开过一次重大争论 .后来虽然爱因斯坦的观点占了上风 ,但其定义的引力场能动张量 ,由于缺乏协变性 ,成了至今尚未... 引力场的能动张量是引力理论中一个极为重要的物理量 .八十多年前 Levi-Civita等人同爱因斯坦曾就这个量的定义及守恒律展开过一次重大争论 .后来虽然爱因斯坦的观点占了上风 ,但其定义的引力场能动张量 ,由于缺乏协变性 ,成了至今尚未完满解决的“老大难”问题 .文章对这场争论的前因后果和双方的观点进行了较详细叙述 ;且结合作者自己的研究对这场争论作了新的评论 ;并介绍了作者重新研究的成果 ,特别是引力波不传播能量的新观点及可能的实验验证 . 展开更多
关键词 引力场 能动张量 守恒定律 引力波 广义相对论
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