Negative pressure in the early universe and its effect on cosmological evolution.

Computer Science

Scientific paper

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Scientific paper

For various reasons the description of matter in terms of a negative
pressure (or state of tension) may be a realistic possibility in the
early universe. The effect of such a state of decompression on the
evolution of the scale factor in a homogeneous and isotropic universe
admitting energy-dependent bulk viscosity is briefly discussed.

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