A dynamic model of the wormhole and the Multiverse model
A.A. Shatskii a,
I.D. Novikov b, a, c,
N.S. Kardashev a
a Astro Space Centre, Lebedev Physical Institute, Russian Academy of Sciences, ul. Profsoyuznaya 84/32, Moscow, 117997, Russian Federation
b National Research Centre ‘Kurchatov Institute’, pl. akad. Kurchatova 1, Moscow, 123182, Russian Federation
c Niels Bohr Institute, Blegdamsvej 17, Copenhagen, DK-2100, Denmark
An analytic solution methodology for general relativity (GR) equations describing the hypothetical phenomenon of
wormholes is presented and the analysis of wormholes in terms
of their physical properties is discussed. An analytic solution of
the GR equations for static and dynamic spherically symmetric
wormholes is given. The dynamic solution generally describes a
‘traversable’ wormhole, i.e., one allowing matter, energy, and
information to pass through it. It is shown how the energy-momentum tensor of matter in a wormhole can be represented in
a form allowing the GR equations to be solved analytically,
which has a crucial methodological importance for analyzing
the properties of the solution obtained. The energy-momentum
tensor of wormhole matter is represented as a superposition of a
spherically symmetric magnetic (or electric) field and negative-
density dust matter, serving as exotic matter necessary for a
‘traversable’ wormhole to exist. The dynamics of the model are
investigated. A similar model is considered (and analyzed in
terms of inflation) for the Einstein equations with a Λ term.
Superposing enough dust matter, a magnetic field, and a Λ term
can produce a static solution, which turns out to be a spherical
Multiverse model with an infinite number of wormhole-connected spherical universes. This Multiverse can have its total
energy positive everywhere in space, and in addition can be out
of equilibrium (i.e., dynamic).
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