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- W2054379904 abstract "We address the question of unified description of dark ingredients in the Universe by a vacuum dark fluid with continuous density and pressures, which represents both distributed vacuum dark energy by a time evolving and spatially inhomogeneous cosmological term, and compact self-gravitating objects with de Sitter vacuum trapped inside. The existence of spherically symmetric globally neutral gravitationally bound vacuum objects without horizons (called G-lumps) asymptotically de Sitter at the center, is implied by the Einstein equations. Their masses are restricted by m<mcrit where mcrit=αmPlρPl/ρ0 with a coefficient α depending on the model. We introduce vacuum dark fluid and present the criterion of stability of G-lumps to external polar perturbations." @default.
- W2054379904 created "2016-06-24" @default.
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- W2054379904 date "2007-02-01" @default.
- W2054379904 modified "2023-10-18" @default.
- W2054379904 title "Vacuum dark fluid" @default.
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- W2054379904 doi "https://doi.org/10.1016/j.physletb.2006.12.047" @default.
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