On the axisymmetric metric generated by a rotating perfect fluid with the vacuum boundary
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DOI: 10.1088/1361-6382/abfed3
Abstract: We consider the equations for the coefficients of stationary rotating axisymmetric metrics governed by the Einstein–Euler equations, that is, the Einstein equations together with the energy–momentum tensor of a barotropic perfect fluid. Although the reduced… read more here.
Keywords: metric generated; system; perfect fluid; vacuum boundary ... See more keywords