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Title: Features of de Sitter Vacua in M-Theory

Abstract

We compute the masses of all moduli in the unstable deSitter vacua arising in the toy model of cosmological M-theory flux compactifications on the G{sub 2} holonomy manifolds of [1]. The slow-roll parameters in the tachyonic directions are shown to be too large to be useful for conventional models of inflation. However, it appears that we can find fast roll regimes which could, under certain conditions, account for the current dark energy driven accelerated expansion of the universe.

Authors:
; ; ; ;
Publication Date:
Research Org.:
Stanford Linear Accelerator Center (SLAC)
Sponsoring Org.:
USDOE
OSTI Identifier:
878017
Report Number(s):
SLAC-PUB-11548
hep-th/0510254; TRN: US200609%%15
DOE Contract Number:
AC02-76SF00515
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of High Energy Physics
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; DE SITTER GROUP; INFLATIONARY UNIVERSE; MASS; COMPACTIFICATION; Theory-HEP,HEPTH

Citation Formats

Hsu, Jonathan P., Kallosh, Renata, /Stanford U., Phys. Dept., Sivanandam, Navin, and /Stanford U., Phys. Dept. /SLAC. Features of de Sitter Vacua in M-Theory. United States: N. p., 2005. Web.
Hsu, Jonathan P., Kallosh, Renata, /Stanford U., Phys. Dept., Sivanandam, Navin, & /Stanford U., Phys. Dept. /SLAC. Features of de Sitter Vacua in M-Theory. United States.
Hsu, Jonathan P., Kallosh, Renata, /Stanford U., Phys. Dept., Sivanandam, Navin, and /Stanford U., Phys. Dept. /SLAC. Wed . "Features of de Sitter Vacua in M-Theory". United States. doi:. https://www.osti.gov/servlets/purl/878017.
@article{osti_878017,
title = {Features of de Sitter Vacua in M-Theory},
author = {Hsu, Jonathan P. and Kallosh, Renata and /Stanford U., Phys. Dept. and Sivanandam, Navin and /Stanford U., Phys. Dept. /SLAC},
abstractNote = {We compute the masses of all moduli in the unstable deSitter vacua arising in the toy model of cosmological M-theory flux compactifications on the G{sub 2} holonomy manifolds of [1]. The slow-roll parameters in the tachyonic directions are shown to be too large to be useful for conventional models of inflation. However, it appears that we can find fast roll regimes which could, under certain conditions, account for the current dark energy driven accelerated expansion of the universe.},
doi = {},
journal = {Journal of High Energy Physics},
number = ,
volume = ,
place = {United States},
year = {Wed Nov 09 00:00:00 EST 2005},
month = {Wed Nov 09 00:00:00 EST 2005}
}
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