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D3-brane vacua in stabilized compactifications
Author(s) -
Oliver DeWolfe,
Liam McAllister,
Gary Shiu,
Bret Underwood
Publication year - 2007
Publication title -
journal of high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.998
H-Index - 261
eISSN - 1126-6708
pISSN - 1029-8479
DOI - 10.1088/1126-6708/2007/09/121
Subject(s) - physics , conifold , brane , brane cosmology , moduli , supersymmetry , theoretical physics , moduli space , extra dimensions , inflation (cosmology) , classical mechanics , mathematical physics , quantum mechanics , geometry , mathematics
D3-branes feel no force in no-scale flux compactifications of type IIB stringtheory, but the nonperturbative effects required to stabilize the Kahler modulibreak the no-scale structure and generate a potential for D3-brane motion,confining the branes to certain loci. D3-branes away from these loci breaksupersymmetry spontaneously, by an F-term. We present the general conditionsfor supersymmetric D3-brane vacua in models with a single Kahler modulus, thenexplicitly calculate these vacua for D3-branes moving on the tip of the warpeddeformed conifold. We find both continuous moduli spaces and isolated vacua. Inaddition, we show that anti-D3-branes and D3-branes are localized to the sameregions by the nonperturbative potential, avoiding a potential obstacle tobrane inflation. We apply these results to determine whether angular motion ofa brane in a throat could play an important role in inflation, and find thatany inflation along the angular directions is short-lived because the fieldspace is very small.Comment: 30 pages, LaTeX. v2: references added, typos fixe

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