Junction equations for two spherically symmetric spacetimes and the distributional method

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dc.creatorKhakshournia, S.
dc.creatorMansouri, R.
dc.date1999-11-11
dc.date.accessioned2026-07-07T04:27:18Z
dc.date.available2026-07-07T04:27:18Z
dc.descriptionApplying the distributional formalism to study the dynamics of thin shells in general relativity, we regain the junction equations for matching of two spherically symmetric spacetimes separated by a singular hypersurface. In particular, we have shown how to define and insert the relevant sign functions in the junction equations corresponding to the signs of the extrinsic curvature tensor occurred in the Darmois-Israel method.
dc.description14 pages, no figure, Latex file
dc.identifierhttps://arxiv.org/abs/hep-th/9911076
dc.identifierhttp://arxiv.org/abs/hep-th/9911076
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/56372
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleJunction equations for two spherically symmetric spacetimes and the distributional method
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