作者: C. R. Almeida , J. C. Fabris , F. Sbisá , Y. Tavakoli
DOI: 10.1007/978-3-319-69164-0_25
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摘要: A class of k-Essence cosmological models, with a power law kinetic term, is quantised in the mini-superspace. It shown that for specific configuration, corresponding to pressureless fluid, Schrodinger-type equation obtained scalar field playing role time. The resulting quantum scenario reveals bounce, classical behaviour being recovered asymptotically.