scholarly journals Unified field theory in a curvature-free five-dimensional manifold

Instead of identifying fields with the curvature of a metric, the present theory shows that they may be identified with the manner in which the four-way measuring system of the physical observer O is embedded in a flat five-dimensional manifold provided that due accouut is taken of the imperceptibility of the fifth dimension. In this system fields are introduced by treating the direction cosines, k l j , of the four directions of measurement and of the imperceptible direction as variable functions of position in the manifold. The track of an unconstrained body P is taken as a straight line (cosmodesic) in the manifold, but the ‘projection’ of it which O observes in his four-co-ordinate system is in general curved. Thus the equation describing the element ds of P 's cosmodesic in O 's four-co-ordinate system (∆ x µ ) is ds 2 cos 2 λ-2 ds sinλ{(∑ v =1 4 v l 5 v l µ ) ∆ x µ }={ 5 l µ 5 l v -2 5 l v ∑ k =1 5 k l 5 k l µ +∑ k =1 5 k l µ k l v }∆ x µ ∆ x v . When O applies the variational condition to ds which expresses the fact that the cosmodesic is straight, he concludes that it has a space-time curvature with two distinct components, one dependent upon λ which is the angle between the cosmodesic and an universal direction 5 Q and upon v l 5 , the other acting equally on all P bodies whatever the value of λ and depending only on 5 l µ . These ‘accelerations’ are shown to correspond to electromagnetic and gravitational fields respectively, and the inverse square law of force is shown to hold for spherically sym­metrical fields of both types as a consequence of the condition of coherence of the measuring system. When the cause of the positional variation of the k l µ is a heavy body, having a constrained rotation, it is shown to give rise to the magnetic field that a body of charge equal to its gravi­tation mass would have, without the corresponding electrostatic field. The k l j 's are restricted by the requirement that the angles between the absolute fifth direction, the direction imperceptible for O , and the direction orthogonal to O 's four measuring directions, are all null.

1962 ◽  
Vol 14 ◽  
pp. 568-576 ◽  
Author(s):  
J. R. Vanstone

In 1947 Einstein and Strauss (2) proposed a unified field theory based on a four-dimensional manifold characterized by a nonsymmetric tensor gij and a non-symmetric connection , where(1)Using a variational principle in which gij and are independently varied, the above authors obtain the equivalent of the following field equations:(2a)(2b)In these equations a comma denotes partial differentiation with respect to the co-ordinates of the manifold, Wij is the Ricci tensor formed from and the notationfor the symmetric and skew-symmetric parts of geometric objects Q is employed.


2020 ◽  
Author(s):  
Mrittunjoy Guha Majumdar

In this paper, the statistics of excitation-tangles in a postulated background ideal-superfluid field is studied. The structure of the Standard Model is derived in terms of tangle vortex-knots and soliton. Gravity is observed in terms of torsion and curvature in the continuum. In this way, non-linear dynamics and excitations give rise to a unified field theory as well as a Theory of Everything. As a result of this unification, spacetime and matter are shown to be fundamentally equivalent, while gauge fields arise from reorientation and excitations of the the fundamental underlying field. Finally, the equivalence of topological and quantum entanglement is explored to posit a theory of everything in terms of long- and short-range entanglement between fundamental quantum units (bits) of information.


2007 ◽  
Vol 38 (1) ◽  
pp. 38-46 ◽  
Author(s):  
Friedrich W. Hehl ◽  
Yuri N. Obukhov

Author(s):  
D. W. Sciama

ABSTRACTIt is suggested, on heuristic grounds, that the energy-momentum tensor of a material field with non-zero spin and non-zero rest-mass should be non-symmetric. The usual relationship between energy-momentum tensor and gravitational potential then implies that the latter should also be a non-symmetric tensor. This suggestion has nothing to do with unified field theory; it is concerned with the pure gravitational field.A theory of gravitation based on a non-symmetric potential is developed. Field equations are derived, and a study is made of Rosenfeld identities, Bianchi identities, angular momentum and the equations of motion of test particles. These latter equations represent the geodesics of a Riemannian space whose contravariant metric tensor is gij–, in agreement with a result of Lichnerowicz(9) on the bicharacteristics of the Einstein–Schrödinger field equations.


1978 ◽  
Vol 18 (12) ◽  
pp. 4802-4805
Author(s):  
J. Balog ◽  
P. Hraskó

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