An inhomogeneous cosmology featuring a `stiff' fluid density wave

Details An inhomogeneous cosmology featuring a `stiff' fluid density wave An inhomogeneous cosmology featuring a `stiff' fluid density wave

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cqgra..15.2813d&link_type=abstract

Classical and Quantum Gravity, Volume 15, Issue 9, pp. 2813-2828 (1998).

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Scientific paper

An inhomogeneous (group on ) cosmological solution to Einstein's equations, derived by the method of progression from a vacuum to a stiff fluid solution, is presented. The solution is characterized by a density wave propagating parallel to the x-axis, initially of infinite amplitude in the fluid density, that peters out at spatial and temporal infinity. There are two singularities, t = 0 and x = 0. The physical and geometrical properties of the spacetime are discussed, with some reference to possible cosmological implications.

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