“School of Physic”
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| Paper IPM / Physic / 6935 |
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| Abstract: | |
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Spherical, time-dependent geometrical structures in an
inflationary RW background are derived from the Einstein
equations, using a constraint on the energy-momentum tensor which
is an extension of the one expected for inflation. The possibility
of dynamical wormholes and other spherical structures are explored
in the framework of the solutions.
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