A fully quantum model of Big Bang
Sergei P. Maydanyuk, Antonino Del Popolo, Vladislav S. Olkhovsky

TL;DR
This paper develops a fully quantum model of the Big Bang within a closed FRW universe, introducing a new wave propagation definition, calculating tunneling probabilities, and accounting for wave interference effects, aligning with semiclassical results.
Contribution
It presents a novel quantum approach to cosmological tunneling, including interference effects, and extends the method to models with arbitrary potential barriers.
Findings
Tunneling probability closely matches semiclassical results.
First calculation of reflection coefficient in quantum cosmology.
Method applicable to models with arbitrary potential barriers.
Abstract
In the paper the closed Friedmann-Robertson-Walker model with quantization in the presence of the positive cosmological constant and radiation is studied. For analysis of tunneling probability for birth of an asymptotically deSitter, inflationary Universe as a function of the radiation energy a new definition of a "free" wave propagating inside strong fields is proposed. On such a basis, tunneling boundary condition is corrected, penetrability and reflection concerning to the barrier are calculated in fully quantum stationary approach. For the first time non-zero interference between the incident and reflected waves has been taken into account which turns out to play important role inside cosmological potentials and could be explained by non-locality of barriers in quantum mechanics. Inside whole region of energy of radiation the tunneling probability for the birth of the inflationary…
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Taxonomy
TopicsCosmology and Gravitation Theories · advanced mathematical theories · Material Science and Thermodynamics
