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An obstacle to populating the string theory landscape

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arxiv 0809.2604 v2 pith:CNZA72TF submitted 2008-09-16 hep-th astro-phgr-qc

An obstacle to populating the string theory landscape

classification hep-th astro-phgr-qc
keywords solutionsstringtheorycontaindomaineternalinflationlandscape
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We construct domain walls and instantons in a class of models with coupled scalar fields, determining, in agreement with previous studies, that many such solutions contain naked timelike singularities. Vacuum bubble solutions of this type do not contain a region of true vacuum, obstructing the ability of eternal inflation to populate other vacua. We determine a criterion that potentials must satisfy to avoid the existence of such singularities, and show that many domain wall solutions in Type IIB string theory are singular. This has profound implications for applying the program of eternal inflation to making predictions in the string theory landscape.

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Cited by 1 Pith paper

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  1. The Lorentzian Geometry of Tunneling in Global de Sitter at Late Time

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    A late-time Lorentzian Hamiltonian/WKB calculation of bubble nucleation in de Sitter reproduces the CDL decay exponent for all tunneling types, with gravity-dominated bubbles going on-shell at the parent horizon.