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Wormholes are considered both from the Wheeler deWitt equation, as well as from the field equations in the Euclidean background of Robertson Walker mini-superspace in Formula: see text gravity. Quantum wormhole satisfies Hawking Page wormhole boundary condition in the Euclidean background of mini-superspace, however, in the Lorentzian background wave functional turns to the usual oscillatory function. The Euclidean field equations for Formula: see text lead to the wormhole configuration, as well as oscillating universe in Euclidean time Formula: see text. The oscillating universe in Euclidean time Formula: see text transforms to an expanding universe only for Formula: see text in Lorentz time Formula: see text under analytic continuation Formula: see text and asymptotically leads to an exponential solution. An Euclidean wormhole in the very early era evolves to an oscillating universe in Formula: see text, thereafter crossing deSitter radius transition to an inflationary era is evident at later epoch only for Formula: see text.
Modak et al. (Thu,) studied this question.