Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2004-05-28
Phys.Rev.D70:063528,2004
Physics
High Energy Physics
High Energy Physics - Theory
10 pages including 1 figure and two appendices. V2: Final version accepted for publication in PRD. The content and conclusions
Scientific paper
10.1103/PhysRevD.70.063528
Cosmic inflation is envisioned as the ``most likely'' start for the observed universe. To give substance to this claim, a framework is needed in which inflation can compete with other scenarios and the relative likelihood of all scenarios can be quantified. The most concrete scheme to date for performing such a comparison shows inflation to be strongly disfavored. We analyze the source of this failure for inflation and present an alternative calculation, based on more traditional semiclassical methods, that results in inflation being exponentially favored. We argue that reconciling the two contrasting approaches presents interesting fundamental challenges, and is likely to have a major impact on ideas about the early universe.
Albrecht Andreas
Sorbo Lorenzo
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