2008
DOI: 10.1103/physrevd.77.123537
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Classical universes of the no-boundary quantum state

Abstract: 46 pages, 24 figures, revtex4We analyze the origin of the quasiclassical realm from the no-boundary proposal for the universe's quantum state in a class of minisuperspace models. The models assume homogeneous, isotropic, closed spacetime geometries, a single scalar field moving in a quadratic potential, and a fundamental cosmological constant. The allowed classical histories and their probabilities are calculated to leading semiclassical order. We find that for the most realistic range of parameters analyzed a… Show more

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Cited by 172 publications
(393 citation statements)
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“…It does not follow from the above analysis that the tuning (4.8) is possible with regularity conditions at the origin and therefore that the saddle points actually exist. However [25] have shown they do. In the neighbourhood of the SP at τ = τ 0 the O(4) invariant saddle point solutions take the form…”
Section: Jhep12(2015)025mentioning
confidence: 99%
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“…It does not follow from the above analysis that the tuning (4.8) is possible with regularity conditions at the origin and therefore that the saddle points actually exist. However [25] have shown they do. In the neighbourhood of the SP at τ = τ 0 the O(4) invariant saddle point solutions take the form…”
Section: Jhep12(2015)025mentioning
confidence: 99%
“…Classical histories correspond to curves in the complex τ -plane along which both the scale factor and field are real. It was found in [25] that in the above parameterisation all curves corresponding to classical histories asymptote to a constant value z f . 6 This can also be seen from the asymptotic expansions (4.5) and (4.6), which to leading order in u can be written as…”
Section: Ds Representation Of Saddle Pointsmentioning
confidence: 99%
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“…See Table ( 1) for the first several terms of a n sequences. Hence, equation (21) presents the most probable cosmological solutions.…”
Section: Deformation Quantization Of Flrw Cosmologymentioning
confidence: 99%
“…Therefore, predicting classical cosmology is a constraint on the theory of the state [1]. In minisuperspace models of cosmology, the classical gravitational field equations are often non-linear and the quantization procedure is not unique.…”
Section: Introductionmentioning
confidence: 99%