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Journal ArticleDOI

Junction conditions in general relativity

C. K. Raju
- 01 Jun 1982 - 
- Vol. 15, Iss: 6, pp 1785-1797
TLDR
In this paper, an analytical formalism is developed to deal with the occurrence of jump discontinuities in the gmu nu or their derivatives across a hypersurface Sigma, and it is shown that the equations of relativity remain meaningful at Sigma, even when Sigma does not inherit a unique intrinsic geometry, so that the gm nu are discontinuous across Sigma in natural coordinates.
Abstract
An analytical formalism is developed to deal with the occurrence of jump discontinuities in the gmu nu or their derivatives across a hypersurface Sigma . It is shown that the equations of relativity remain meaningful at Sigma , even when Sigma does not inherit a unique intrinsic geometry, so that the gmu nu are discontinuous across Sigma in natural coordinates. The spherically symmetric surface layer at the Schwarzschild-Minkowski junction is used to illustrate these techniques, and to establish rigorously the existence of C0 solutions of the Einstein equations and the conservation equations. The possible validity of relativity at the microscopic level is examined, and it is concluded that, if relativity is valid at the microscopic level, then it is likely that the gmu nu are not globally continuously differentiable.

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Citations
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The use of generalized functions and distributions in general relativity

TL;DR: In this paper, a mathematical theory of nonlinear generalized functions based on Colombeau algebras is described and applied in general relativity, and it is shown that certain solutions with weak singularities may be regarded as distributional solutions of Einstein's equations.
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Generalized functions and distributional curvature of cosmic strings

TL;DR: In this article, a new method is presented for assigning distributional curvature, in an invariant manner, to a spacetime of low differentiability, using the techniques of Colombeau's ''new generalized functions''.
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The use of Generalised Functions and Distributions in General Relativity

TL;DR: In this article, the authors review the extent to which one can use classical distribution theory in describing solutions of Einstein's equations and show that there are some physically interesting cases which cannot be treated using distribution theory but require a more general concept.
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The equivalence of Darmois‐Israel and distributional method for thin shells in general relativity

TL;DR: In this paper, a distributional method to solve the Einstein's field equations for thin shells is formulated and the familiar field equations and jump conditions of Darmois-Israel formalism are derived.
Journal ArticleDOI

The elastoplastic shock problem as an example of the resolution of ambiguities in the multiplication of distributions

TL;DR: In this paper, a general physicomathematical method, adapted to each particular case, is proposed to resolve the ambiguity inherent in such products, which can be achieved with the aid of a new mathematical theory of generalized functions, which permits dealing with mathematical phenomena of a microscopic nature that govern products of distributions having singularities at the same point.
References
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Journal ArticleDOI

Singular hypersurfaces and thin shells in general relativity

TL;DR: In this article, an approach to study the dynamics of thin shells of dust in general relativity is presented. But no mention of admissible or even any space-time co-ordinates is needed.
Journal ArticleDOI

An Extensible model of the electron

TL;DR: In this paper, it was proposed that the electron should be considered classically as a charged conducting surface, with a surface tension to prevent it from flying apart under the repulsive forces of the charge.
Journal ArticleDOI

Discontinuities in spherically symmetric gravitational fields and shells of radiation

TL;DR: In this article, the validity of the O'Brien-Synge junction conditions is established for co-ordinates derivable from Lichnerowicz's 'admissible coordinates' by a transformation which is uniformly differentiable across a 3-space of discontinuity.
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