The incorporation of matter into characteristic numerical relativity

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dc.creatorBishop, N. T.
dc.creatorGomez, R.
dc.creatorLehner, L.
dc.creatorMaharaj, M.
dc.creatorWinicour, J.
dc.date1999-01-20
dc.date.accessioned2026-07-07T11:34:26Z
dc.date.available2026-07-07T11:34:26Z
dc.descriptionA code that implements Einstein equations in the characteristic formulation in 3D has been developed and thoroughly tested for the vacuum case. Here, we describe how to incorporate matter, in the form of a perfect fluid, into the code. The extended code has been written and validated in a number of cases. It is stable and capable of contributing towards an understanding of a number of problems in black hole astrophysics.
dc.description15 pages + 4 (eps) figures
dc.identifierhttps://arxiv.org/abs/gr-qc/9901056
dc.identifierhttp://arxiv.org/abs/gr-qc/9901056
dc.identifierPhys.Rev.D60:024005,1999
dc.identifierdoi:10.1103/PhysRevD.60.024005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198248
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe incorporation of matter into characteristic numerical relativity
dc.typetext

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