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28 March 2024
 
  » arxiv » astro-ph/9702201

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On classical anisotropies in models of Open Inflation
Jaume Garriga ; V.F. Mukhanov ;
Date 23 Feb 1997
Journal Phys.Rev. D56 (1997) 2439-2441
Subject astro-ph gr-qc
AbstractIn the simplest model of open inflation there are two inflaton fields decoupled from each other. One of them, the tunneling field, produces a first stage of inflation which prepares the ground for the nucleation of a highly symmetric bubble. The other, a free field, drives a second period of slow roll inflation inside the bubble. However, the second field also evolves during the first stage of inflation, which to some extent breaks the needed symmetry. We show that this generates large supercurvature anisotropies which, together with the results of Tanaka and Sasaki, rule out this class of simple models (unless, of course, $Omega_0$ is sufficiently close to one.) The problem does not arise in modified models where the second field does not evolve in the first stage of inflation.
Source arXiv, astro-ph/9702201
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