Cosmological solution of Einstein's equations with uniform density and nonuniform pressure

Details Cosmological solution of Einstein's equations with uniform density and nonuniform pressure Cosmological solution of Einstein's equations with uniform density and nonuniform pressure

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvd..39..420w&link_type=abstract

Physical Review D (Particles and Fields), Volume 39, Issue 2, 15 January 1989, pp.420-422

Mathematics

Logic

12

Exact Solutions

Scientific paper

An exact solution of the equations of general relativity is given that is most appropriately interpreted cosmologically and has some unusual properties. The solution is a perfect-fluid, spherically symmetric, nonstatic one in which the density is uniform but the pressure is nonuniform. A brief investigation, both algebraic and numerical, is made of the solution's main physical attributes. It may be used to model a localized inhomogeneity such as a bubble in the early Universe.

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