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One new stationary axisymmetric solution of the vacuum Einstein equations is obtained. It depends on a particular form of the fifth Painlevé transcendent.  相似文献   

3.
It is shown that a collapsing (anticollapsing) plane desk consisting of incoherent dust can be the source of the Taub solution. The metric tensor inside the matter is found.  相似文献   

4.
A slice for the action of a group G on a manifold X at a point x ? X is, roughly speaking, a submanifold Sx which is transverse to the orbits of G near x. Ebin and Palais proved the existence of a slice for the diffeomorphism group of a compact manifold acting on the space of all Riemannian metrics. We prove a slice theorem for the group D of diffeomorphisms of spacetime acting on the space E of spatially compact, globally hyperbolic solutions of Einstein's equations. New difficulties beyond those encountered by Ebin and Palais arise because of the Lorentz signature of the spacetime metrics in E and because E is not a smooth manifold- it is known to have conical singularities at each spacetime metric with symmetries. These difficulties are overcome through the use of the dynamic formulation of general relativity as an infinite dimensional Hamiltonian system (ADM formalism) and through the use of constant mean curvature foliations of the spacetimes in E. (We devote considerable space to a review and extension of some special properties of constant mean curvature surfaces and foliations that we need.) The conical singularity structure of E, the sympletic aspects of the ADM formalism, and the uniqueness of constant mean curvature foliations play key roles in the proof of the slice theorem for the action of D on E. As a consequence of this slice theorem, we find that the space D = E/D of gravitational degrees of freedom is a stratified manifold with each stratum being a sympletic manifold. The spaces for homogeneous cosmologies of particular Bianchi types give rise to special finite dimensional symplectic strata in this space G. Our results should extend to such coupled field theories as the Einstein-Yang-Mills equations, since the Yang-Mills system in a given background spacetime admits a slice theorem for the action of the gauge transformation group on the space of Yang-Mills solutions, since there is a satisfactory Hamiltonian treatment of the Einstein-Yang-Mills system, and since the singularity structure of the solution set is known.  相似文献   

5.
The space of solutions of Einstein's vacuum equations is shown to have conical singularities at each spacetime possessing a compact Cauchy surface of constant mean curvature and a nontrivial set of Killing fields. Similar results are shown for the coupled Einstein-Yang-Mills system. Combined with an appropriate slice theorem, the results show that the space of geometrically equivalent solutions is a stratified manifold with each stratum being a symplectic manifold characterized by the symmetry type of its members.  相似文献   

6.
Huei Peng 《Physics letters. A》1984,103(3):113-115
By considering the relationship between a freely falling frame and a local Lorentz frame, we propose a new expression of Einstein's equivalence principle (EEP). According to it, some feasible experiments should be done to test EEP. We point out that the effect of the magnetic-type gravitational counterpart of the Aharonov-Bohm experiment is too small to be detected now.  相似文献   

7.
Kraitchman's method for the determination of the substitution (or rs) coordinates of an atom in a rotating molecule (asymmetric rotor) from the two sets of three principal moments of inertia of the common isotope of the molecule and the species where the particular atom has been isotopically substituted, has been extended to include the complete coordinate transformation between the principal axis systems of both molecular species. No additional information is required. Several applications are discussed, including a method which helps solve the problem of “small coordinates” by following an appropriate “substitution sequence.”  相似文献   

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New quantities have been found which are constants of motion in Newton's gravitational theory. Analogous but different quantities exist in Einstein's theory. The difference between the Newtonian and the relativistic quantities may be used to distinguish experimentally between the theories.  相似文献   

10.
In terms of the covariance of equations under a generalized galilean transformation, a general expression of Maxwell's equations in anistropic space is given here.  相似文献   

11.
A solution to the long-standing problem involving the incorporation of Mach's principle into general relativity is proposed in terms of a new scalar-tensor theory of gravity, which seems to introduce no change in the predictions of general ralativity for any of its existing tests.  相似文献   

12.
The nonlinear system of partial differential equations generalizing Plebanski's ω-equation is given for conformally self-dual spaces. It is then shown that solving this system is equivalent to the problem that the induced connection in a certain distinguished line bundle hasa self-dual curvature and self-dual “involuted” curvature.  相似文献   

13.
Our account provides a local, realist and fully non-causal principle explanation for EPR correlations, contextuality, no-signalling, and the Tsirelson bound. Indeed, the account herein is fully consistent with the causal structure of Minkowski spacetime. We argue that retrocausal accounts of quantum mechanics are problematic precisely because they do not fully transcend the assumption that causal or constructive explanation must always be fundamental. Unlike retrocausal accounts, our principle explanation is a complete rejection of Reichenbach’s Principle. Furthermore, we will argue that the basis for our principle account of quantum mechanics is the physical principle sought by quantum information theorists for their reconstructions of quantum mechanics. Finally, we explain why our account is both fully realist and psi-epistemic.  相似文献   

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H.A Tolhoek 《Physica A》1977,86(2):278-302
In a previous paper wave propagation was studied according to a sixth-order partial differential equation involving a complex mass M. The corresponding Yang-Feldman integral equations (indicated as SM-YF-equations), were formulated using modified Green's functions GMR(x) and GMA(x), which then incorporate the partial differential equation together with certain boundary conditions. In this paper certain limit properties of these modified Green's functions are derived: (a) It is shown that for |M| → ∞ the Green's functions GMR(x) and GMA(x) approach the Green's functions ΔR(x) and ΔA(x) of the corresponding KG-equation (Klein-Gordon equation). (b) It is further shown that the asymptotic behaviour of GMA(x) and GMA(x) is the same as of ΔR(x) and ΔA(x) - and also the same as for DR(x) and DA(x) for t→ ± ∞, where DR and DA are the Green n's functions for the KG-equation with mass zero. It is essential to take limits in the sense of distribution theory in both cases (a) and (b). The property (b) indicates that the wave propagation properties of the SM-YF-equations, the KG-equation with finite mass and the KG-equation with mass zero are closely related in an asymptotic sense.  相似文献   

16.
In this paper, we study the Einstein’s photoemission from III–V, II–VI, IV–VI and HgTe/CdTe quantum well superlattices (QWSLs) with graded interfaces and quantum well effective mass superlattices in the presence of a quantizing magnetic field on the basis of newly formulated dispersion relations in the respective cases. Besides, the same has been studied from the afore-mentioned quantum dot superlattices and it appears that the photoemission oscillates with increasing carrier degeneracy and quantizing magnetic field in different manners. In addition, the photoemission oscillates with film thickness and increasing photon energy in quantum steps together with the fact that the solution of the Boltzmann transport equation will introduce new physical ideas and new experimental findings under different external conditions. The influence of band structure is apparent from all the figures and we have suggested three applications of the analyses of this paper in the fields of superlattices and microstructures.  相似文献   

17.
J.C. Caillon 《Physics letters. A》2018,382(46):3307-3312
We have considered electric charge as the fourth component of the particle momentum in five-dimensional space–time. The fifth dimension has been compactified on a circle with an extremely small radius determined from the fundamental physics constants. First, we have given equations in the framework of five-dimensional special relativity and determined the corresponding reduction to four-dimensional space–time. Then, in order to obtain an appropriate charge-to-mass ratio and to avoid the Fourier modes problem, we have considered the propagation of an off-mass shell particle in the five-dimensional space–time which can be interpreted as the motion of an on-mass shell particle in the four-dimensional world we experience. As an example, we have discussed the five-dimensional kinematic equations associated with the electron-positron annihilation process into two photons. Finally, the consequences on the gravitational interaction between two elementary charged particles has been studied. As a main result, we have obtained a unification of Newton's gravitational and Coulomb's electrostatic forces.  相似文献   

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N.L. Balazs 《Physica A》1980,102(2):236-254
According to Weyl one may associate a function with a dynamical operator; these functions depend on the parameters p and q and can be displayed in a p, q manifold, the W space. In the classical limit the W space becomes the phase space parametrised by the canonical variables. The function associated in this manner with the density operator is Wigner's function. It turns out that if Wigner's function is a delta function it cannot represent the density operator of a physically realisable state unless the argument of the delta-function is linear in the parameters a and q. In all other cases Wigner's function associated with a physically realisable state has a finite width, proportional to h23. Consequently straightness (linear combination of p and q) has a fundamental significance in the W space. Since this property is preserved under linear inhomogeneous transformations the W space will have a geometry generated by these transformations, the affine geometry of Euler, Moebius and Blaschke. In the present note we show how this comes about, how it simplifies the semiclassical approximations of Wigner's function, and makes one understand how in the classical limit this geometry is lost, allowing to be replaced by the geometry of canonical transformations.  相似文献   

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