2007
DOI: 10.1088/0264-9381/24/17/007
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Canonical wave packets in quantum cosmology

Abstract: We discuss the construction of wave packets resulting from the solutions of a class of Wheeler-DeWitt equations in Robertson-Walker type cosmologies, for arbitrary curvature. We show that there always exists a "canonical initial slope" for a given initial wave function, which optimizes some desirable properties of the resulting wave packet, most importantly good classical-quantum correspondence. This can be properly denoted as a canonical wave packet. We introduce a general method for finding these canonical i… Show more

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Cited by 13 publications
(45 citation statements)
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“…(1) in some cosmological cases. We show that the resulting wave packets completely correspond to their classical counterparts and peak on the classical paths [3][4][5][6]. So, these wave packets follow the classical trajectories from big-bang to big-crunch.…”
Section: The Modelmentioning
confidence: 71%
“…(1) in some cosmological cases. We show that the resulting wave packets completely correspond to their classical counterparts and peak on the classical paths [3][4][5][6]. So, these wave packets follow the classical trajectories from big-bang to big-crunch.…”
Section: The Modelmentioning
confidence: 71%
“…It is worth to mention that this method has been used previously for some other similar cases [64,66,74,75].…”
Section: The Spectral Methodsmentioning
confidence: 99%
“…However, since we are interested to construct wave packet with classical properties, we need to assume a specific relationship between these coefficients. The prescription is that the coefficients have the same functional form [25][26][27] i.e.…”
Section: The Modelmentioning
confidence: 99%
“…To fix the expansion coefficients, we will apply the prescription used in Refs. [25][26][27] for the case of hyperbolic PDEs which also appear in the context of quantum cosmology.…”
Section: Introductionmentioning
confidence: 99%