2012
DOI: 10.1088/0264-9381/29/9/095005
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The no-boundary measure in scalar–tensor gravity

Abstract: In this article, we study the no-boundary wave function in scalar-tensor gravity with various potentials for the non-minimally coupled scalar field. Our goal is to calculate probabilities for the scalar field -and hence the effective gravitational coupling and cosmological constant -to take specific values. Most calculations are done in the minisuperspace approximation, and we use a saddle point approximation for the Euclidean action, which is then evaluated numerically.We find that for potentials that have se… Show more

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Cited by 29 publications
(45 citation statements)
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“…Then, we can paste the Lorentzian manifold t = 0 at the η = η 0 surface. This is possible only for the caseρ(η 0 ) =Φ(η 0 ) = 0, because of the Cauchy-Riemann theorem of complex analysis; otherwise, the Lorentzian manifold should be complex valued functions (for exceptional cases, we might be able to consider complex valued instantons, the so-called fuzzy instantons [55,56]). In this procedure, an event shows a spontaneous creation of the universe from 'nothing' [2], in which nothing means a state without the concept of classical spacetime [57].…”
Section: Oscillating Fubini Instantonsmentioning
confidence: 99%
“…Then, we can paste the Lorentzian manifold t = 0 at the η = η 0 surface. This is possible only for the caseρ(η 0 ) =Φ(η 0 ) = 0, because of the Cauchy-Riemann theorem of complex analysis; otherwise, the Lorentzian manifold should be complex valued functions (for exceptional cases, we might be able to consider complex valued instantons, the so-called fuzzy instantons [55,56]). In this procedure, an event shows a spontaneous creation of the universe from 'nothing' [2], in which nothing means a state without the concept of classical spacetime [57].…”
Section: Oscillating Fubini Instantonsmentioning
confidence: 99%
“…We use the steepest-descent method and consider only the on-shell solutions to count the probability from the path-integral [11,12,25,26]. We solve the classical equations of motion for Euclidean as well as Lorentzian time directionsφ…”
Section: Hawking-moss Instantonsmentioning
confidence: 99%
“…where I denotes the index of the canonical variables, then the wave function describes an almost classical behavior [11,12,25,26].…”
Section: Generalization To Fuzzy Instantonsmentioning
confidence: 99%
See 1 more Smart Citation
“…2. Hwang, Sahlmann and Yeom [4] and Hwang, Lee, Sahlmann and Yeom [5] discussed that complexvalued instantons are useful to explain the initial condition for the stabilization of dilaton or moduli fields. 3.…”
Section: Perspectivesmentioning
confidence: 99%