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Matching conditions in Locally Rotationally Symmetric spacetimes and radiating stars

2020/11/02 by Pretty N. Khambule, Khambule, Pretty N., Rituparno Goswami +3
Physics and Astronomy · #Advanced Differential Geometry Research #Astrophysical Phenomena and Observations #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Solar and Stellar Astrophysics (astro-ph.SR) #astro-ph.SR #gr-qc

paper · pdf · doi:10.48550/arxiv.2011.00853

20 pages, Revtex4

arxiv created 2020/11/02 · openalex publication_date 2020/11/02 · arxiv updated 2020/11/03 · openalex created_date 2022/07/25 · openalex updated_date 2026/07/28

Abstract

We recast the well known Israel-Darmois matching conditions for Locally Rotationally Symmetric (LRS-II) spacetimes using the semitetrad 1+1+2 covariant formalism. This demonstrates how the geometrical quantities including the volume expansion, spacetime shear, acceleration and Weyl curvature of two different spacetimes are related at a general matching surface inheriting the symmetry, which can be timelike or spacelike. The approach is purely geometrical and depends on matching the Gaussian curvature of 2-dimensional sheets at the matching hypersurface. This also provides the constraints on the thermodynamic quantities on each spacetime so that they can be matched smoothly across the surface. As an example we regain the Santos boundary conditions and model of a radiating star matched to a Vaidya exterior in general relativity.

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