English
español
Please use this identifier to cite or link to this item:
http://hdl.handle.net/10261/60319
Share/Impact:
Statistics  SHARE CORE MendeleyBASE 


Visualizar otros formatos: MARC  Dublin Core  RDF  ORE  MODS  METS  DIDL  

Title:  Pathintegral quantum cosmology: A class of exactly soluble scalarfield minisuperspace models with exponential potentials 
Authors:  Garay, Luis Javier ; Halliwell, J. J.; Mena Marugán, Guillermo A. 
Issue Date:  1991 
Publisher:  American Physical Society 
Citation:  Physical Review D  Particles, Fields, Gravitation and Cosmology 43: 2572 2589 (1991) 
Abstract:  We study a class of minisuperspace models consisting of a homogeneous isotropic universe with a minimally coupled homogeneous scalar field with a potential cosh(2+2sinh(2), where and 2 are arbitrary parameters. This includes the case of a pure exponential potential exp(2), which arises in the dimensional reduction to four dimensions of fivedimensional KaluzaKlein theory. We study the classical Lorentzian solutions for the model and find that they exhibit exponential or powerlaw inflation. We show that the WheelerDeWitt equation for this model is exactly soluble. Concentrating on the two particular cases of potentials cosh(2) and exp(2), we consider the Euclidean minisuperspace path integral for a propagation amplitude between fixed scale factors and scalarfield configurations. In the gauge N=0 (where N is the rescaled lapse function), the path integral reduces, after some essentially trivial functional integrations, to a single nontrivial ordinary integral over N. Because the Euclidean action is unbounded from below, N must be integrated along a complex contour for convergence. We find all possible complex contours which lead to solutions of the WheelerDeWitt equation or Green's functions of the WheelerDeWitt operator, and we give an approximate evaluation of the integral along these contours, using the method of steepest descents. The steepestdescent contours may be dominated by saddle points corresponding to exact solutions to the full Einsteinscalar equations which may be real Euclidean, real Lorentzian, or complex. We elucidate the conditions under which each of these different types of solution arise. For the exp(2) potential, we evaluate the path integral exactly. Although we cannot evaluate the path integral in closed form for the cosh(2) potential, we show that for particular N contours the amplitude may be written as a given superposition of exact solutions to the WheelerDeWitt equation. By choosing certain initial data for the pathintegral amplitude we obtain the amplitude specified by the >noboundary> proposal of Hartle and Hawking. We discuss the nature of the geometries corresponding to the saddle points of the noboundary amplitude. We identify the set of classical solutions this proposal picks out in the classical limit. © 1991 The American Physical Society. 
URI:  http://hdl.handle.net/10261/60319 
DOI:  10.1103/PhysRevD.43.2572 
Identifiers:  doi: 10.1103/PhysRevD.43.2572 issn: 05562821 
Appears in Collections:  (CFMACIO) Artículos 
Files in This Item:
File  Description  Size  Format  

Garay,.pdf  812,19 kB  Adobe PDF  View/Open 
Show full item record
Review this work
Review this work
Related articles:
WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.