The Third Quantization: To Tunnel or Not to Tunnel?
Mariam Bouhmadi-López, Manuel Krämer, João Morais and 1 more
Galaxies · 2018
doi:10.3390/galaxies6010019 (opens in a new tab)
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Abstract
Within the framework of the third quantization, we consider the possibility that an initially recollapsing baby universe can enter a stage of near de Sitter inflation by tunnelling through a Euclidean wormhole that connects the recollapsing and inflationary geometries. We present the solutions for the evolution of the scale factor in the Lorentzian and Euclidean regions as well as the probability that the baby universe indeed crosses the wormhole when it reaches its maximum size.
Abstract licence: CC BY
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