Building a better racetrack

By Frederik Denef, Michael R Douglas, B. Florea. 2004

356 citations recorded by the source corpus.

We find IIb compactifications on Calabi-Yau orientifolds in which all Kahler moduli are stabilized, along lines suggested by Kachru, Kallosh, Linde and Trivedi.

Subfields: Geometry and Topology, Mathematical Physics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/0f89a5352f7bce1ec67e52d4cc4418c2ca05c0e2

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Citations in the corpus

Systematics of string loop corrections in type IIB Calabi-Yau flux compactifications (2007, background): “1, is that these are the only 4-cycles which get instanton contributions to W when fluxes are turned off [33].”
Gaugino Condensation and Nonperturbative Superpotentials in Flux Compactifications (2004, background): “While as discussed in [11] the D7s often have numerous matter fields in the most naive Kaluza-Klein analysis of their 4d N = 1 supersymmetric worldvolume gauge theory, the three-form flux can give masses to many or all of these matter fields.”
Stringy corrections to Kahler potentials, SUSY breaking, and the cosmological constant problem (2004, background): “For such F-theory compactifications every Kähler modulus will appear in the non-perturbative superpotential and the scenario of [1] can stabilize all moduli supersymmetrically at finite (and possibly large) volume [2].”
General analysis of LARGE Volume Scenarios with string loop moduli stabilisation (2008, background): “In this section we will briefly review – 3 – how moduli are typically stabilised in IIB string theory and then we will describe the general conditions under which an exponentially large volume Calabi-Yau compactification is obtained.”
Large-volume flux compactifications: Moduli spectrum and D3/D7 soft supersymmetry breaking (2005, methodology): “We also present results for the general case, illustrating our conclusions with a three Kähler moduli example (the F11 model of [16]).”
Systematics of moduli stabilisation in Calabi-Yau flux compactifications (2005, methodology): “As shown in [20], both D4 and D5 correspond to divisors which when lifted to Calabi-Yau fourfold X have arithmetic genus 1 and thus appear non-perturbatively in the superpotential.”
Enumerating flux vacua with enhanced symmetries (2004, methodology): “We initiate the study of the relative frequencies of vacua with vanishing superpotential W = 0 and with certain discrete symmetries.”
Gaugino Condensates and D-terms from D7-branes (2006, background): “For example such a model will generically feature several anomalous U(1)’s and the occurrence of condensing gauge groups might be nongeneric, see for instance [69].”
Les Houches Lectures on Constructing String Vacua (2008, methodology): “he existence of suitable nonperturbative corrections to the superpotential. The ﬁrst concrete models satisfying the necessary geometrical requirements for this (in the KKLT scenario) were proposed in [125], and a simpler and more explicit model was given in [126] and subsequently generalized in [127”
Fixing all moduli in a simple f-theory compactification (2005, methodology): “We used the algorithm outlined in appendix B of [37], which is essentially the procedure followed for the local model in section 2, with the following results.”
The statistics of supersymmetric D-brane models (2004, unknown): “11/2004”
Moduli Stabilisation versus Chirality for MSSM like Type IIB Orientifolds (2007, background): “The standard example primarily studied in the literature is the Calabi-Yau manifold IP[1,1,1,6,9][18] which has a codimension three Z3-singularity [11, 31, 32].”
Flux compactifications in string theory: A Comprehensive review (2005, background): “In the past year, explicit examples of type IIB orientifold compactifications were constructed with all moduli (also twisted and open string moduli) stabilized [179, 187, 37].”
Distributions of nonsupersymmetric flux vacua (2004, background): “acy of vacua comes from the diﬀerent choices of ﬂux. In particular, inclusion of Ka¨hler moduli typically only produces small shifts in the vacua found by ignoring them. This was made more precise in [12] section 4.1, and [16]. The constraint of small W ﬂux, needed to stabilize the model in a contro”