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No-boundary measure in the regime of eternal inflation
Hartle J., Hawking S.W., Hertog T.
Physical Review D 82 (2010) 063510 - http://hal.in2p3.fr/in2p3-00722560
Physique/Astrophysique/Cosmologie et astrophysique extra-galactique
Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique
Physique/Physique des Hautes Energies - Théorie
Physique/Relativité Générale et Cosmologie Quantique
No-boundary measure in the regime of eternal inflation
J. Hartle, S.W. Hawking1, T. Hertog2, 3
1 :  DAMTP/CMS - Department of Applied Mathematics and Theoretical Physics / Centre for Mathematical Sciences
http://www.damtp.cam.ac.uk/
Université de Cambridge
DAMTP, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA
Royaume-Uni
2 :  APC - UMR 7164 - AstroParticule et Cosmologie
http://www.apc.univ-paris7.fr/
CNRS : UMR7164 – IN2P3 – Observatoire de Paris – Université Paris VII - Paris Diderot – CEA : DSM/IRFU
APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13
France
3 :  International Solvay Institutes
International Solvay Institutes
Boulevard du Triomphe ULB-C.P.231, B-1050 Brussels
Belgique
APC - THEORIE
The no-boundary wave function (NBWF) specifies a measure for prediction in cosmology that selects inflationary histories and remains well behaved for spatially large or infinite universes. This paper explores the predictions of the NBWF for linear scalar fluctuations about homogeneous and isotropic backgrounds in models with a single scalar field moving in a quadratic potential. We treat both the spacetime geometry of the universe and the observers inhabiting it quantum mechanically. We evaluate top-down probabilities for local observations that are conditioned on the NBWF and on part of our data as observers of the universe. For models where the most probable histories do not have a regime of eternal inflation, the NBWF predicts homogeneity on large scales, a spectrum of observable fluctuations with a small non-Gaussian component, and a small amount of inflation in our past. By contrast, for models where the dominant histories have a regime of eternal inflation, the NBWF predicts significant inhomogeneity on scales much larger than the present horizon, a Gaussian spectrum of observable fluctuations, and a long period of inflation in our past. The absence or presence of non-Gaussianity in our observable universe therefore provides information about its global structure, assuming the NBWF.

Articles dans des revues avec comité de lecture
09/2010
Physical Review D (Phys. Rev. D)
Publisher American Physical Society
ISSN 1550-7998 (eISSN : 1550-2368)
82
063510

Quantum cosmology – Quantum gravity – Origin and formation of the Universe – Particle-theory and field-theory models of the early Universe
Lien vers le texte intégral : 
http://fr.arXiv.org/abs/1001.0262