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IssuesArchive of Issues2002-2pp.70-81

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G. N. Chernyshev, "Mutual generalization of elastic and gravitational field equations on the basis of solid mechanics," Mech. Solids. 37 (2), 70-81 (2002)
Year 2002 Volume 37 Number 2 Pages 70-81
Title Mutual generalization of elastic and gravitational field equations on the basis of solid mechanics
Author(s) G. N. Chernyshev (Moscow)
Abstract By extending the phenomenon of deformation of time known from the general relativity to the elastic space, we construct refined equations of dynamic elasticity taking into account the deformation of the time coordinate. In terms of mechanics, this deformation is interpreted as the dynamic expansion-compression deformation of the substance similar to the thermal deformation. This generalization makes it possible to take into account the force interaction between particles of the medium in the inertial terms of the equilibrium equations and in the continuity relations. This interaction is ignored in the classical theory of elasticity. The new model of an elastic body is validated by means of the comparison of the theoretical solutions of a number of dynamic problems constructed on the basis of the relations obtained with experimental results. On the other hand, by extending the model of an elastic space to the model of the gravitational space, we equip the familiar equations of the gravitational field in the linear approximation with the generalized Hooke's law and equilibrium equations.

The material of this paper is presented in the following order. By generalizing the linearized mathematical model of the gravitational space to the elastic body we construct the dynamic equations of elasticity in which the time coordinate is deformed as is the case for the gravitational field theory. Unlike the gravitational field theory (the general relativity), when deriving the equations of elasticity we do not introduce in advance a fixed velocity of propagation of excitations equal to the velocity of light, sound, or some other velocity determining a four-dimensional metric of the elastic space. As shown in the present paper, there is no necessity for introducing such a velocity. Instead, an arbitrary constant having the dimension of velocity is introduced. This is necessary for forming a four-dimensional metric utilized when determining the strain state of an elastic space. The velocities of propagation of excitations and waves in an elastic body are determined by the elastic moduli and the density.

Then we validate the obtained equations by comparing theoretical solutions with experimental results. The confidence in the correctness of these equations suggested us to perform a reciprocal generalization of the constructed model of an elastic body to the gravitational space. The deformability of this space similar to the deformability of an elastic body is in fact recognized in the general relativity by introducing a metric tensor depending on the stress state. Therefore, by analogy with the theory of elasticity, the half-difference of the perturbed and unperturbed metric tensors of the gravitational space is referred to as the strain tensor.
References
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13.  C. Moller, "Trionfi e limiti della teoria di Einstein della relativita e gravitazione," in Astrofisica e Cosmologia, Gravitazione, Quanti e Relativita. Sentenario di Einstein, pp. 25-26, Giunti Barbera, Firenze, 1979.
14.  E. Almadi and G. Pizella, "La ricerca delle onde gravitazionali," in Astrofisica e Cosmologia, Gravitazione, Quanti e Relativita. Sentenario di Einstein, pp. 281-458, Giunti Barbera, Firenze, 1979.
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Received 23 December 1999
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