Method to obtain shear-free two-fluid solutions of Einstein's equations
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Method to obtain shear-free two-fluid solutions of Einstein's equations

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Method to obtain shear-free two-fluid solutions of Einstein's equations

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dc.contributor.author Ferrando Bargues, Joan J.
dc.contributor.author Morales Lladosa, Juan Antonio
dc.contributor.author Portilla Moll, Miquel
dc.date.accessioned 2019-01-15T14:23:51Z
dc.date.available 2019-01-15T14:23:51Z
dc.date.issued 1989
dc.identifier.uri http://hdl.handle.net/10550/68479
dc.description.abstract We use the Einstein equations, stated as an initial-value problem (3+1 formalism), to present a method for obtaining a class of solutions which may be interpreted as the gravitational field produced by a mixture of two perfect fluids. The four-velocity of one of the components is assumed to be a shear-free, irrotational, and geodesic vector field. The solutions are given up to a set of a hyperbolic quasilinear system.
dc.language.iso eng
dc.relation.ispartof Physical Review D, 1989, vol. 40, num. 4, p. 1027-1032
dc.rights.uri info:eu-repo/semantics/openAccess
dc.source Ferrando Bargues, Joan J. Morales Lladosa, Juan Antonio Portilla Moll, Miquel 1989 Method to obtain shear-free two-fluid solutions of Einstein's equations Physical Review D 40 4 1027 1032
dc.subject Relativitat (Física)
dc.subject Gravitació
dc.title Method to obtain shear-free two-fluid solutions of Einstein's equations
dc.type info:eu-repo/semantics/article
dc.date.updated 2019-01-15T14:23:51Z
dc.identifier.doi https://doi.org/10.1103/PhysRevD.40.1027
dc.identifier.idgrec 129391

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