The “critical density” is the average density of matter required for the Universe to just halt its expansion, but only after an infinite amount of time. This means that the universe’s expansion would come to a halt, and not recollapse. A universe with…

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A perfect fluid can be completely characterized by its rest frame mass density and isotropic pressure .  Specifically, perfect fluids have no shear stresses, viscosity, or heat conduction. Real fluids are “sticky” and contain (and conduct) heat. Perfect fluids are idealized models…

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