Kähler corrections for the volume modulus of flux compactifications
By G. Gersdorff, A. Hebecker. 2005
159 citations recorded by the source corpus.
Abstract No-scale models arise in many compactifications of string theory and supergravity, the most prominent recent example being type IIB flux compactifications. Focussing on the case where the no-scale field is a single unstabilized volume modulus (radion), we analyse the general form of supergravity loop corrections that affect the no-scale structure of the Kahler potential. These corrections contribute to the 4d scalar potential of the radion in a way that is similar to the Casimir effect. We discuss the interplay of this loop effect with string-theoretic α ′ corrections and its possible role in the stabilization of the radion.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/622bc450956e2da698e6bc4668f856acebb97b32
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- D. Baumann
- Liam McAllister
- Eran Palti
- M. Cicoli
- F. Quevedo
- Anshuman Maharana
- A. Ringwald
- M. Goodsell
In Nuclear and High Energy Physics
- Eran Palti
- D. Baumann
- Liam McAllister
- M. Cicoli
- Anshuman Maharana
- F. Quevedo
- A. Ringwald
- I. Klebanov
Citations in the corpus
- Explicit de Sitter flux vacua for global string models with chiral matter (2013, background): “Further perturbative corrections arise due to string loop effects [67, 68].”
- Gaugino Condensates and D-terms from D7-branes (2006, unknown): “The inclusion of perturbative corrections to the Kähler potential, like the ones discussed in [50, 73, 74], would be interesting in view of the proposal of [26] which uses D-term potentials to uplift possible AdS minima obtained from balancing effects in the F -term potential due to perturbative cor”
- MODELS OF PARTICLE PHYSICS FROM TYPE IIB STRING THEORY AND F-THEORY: A REVIEW (2012, methodology): “Variations of the scenario by incorporating α′ and gs corrections were discussed in [44–47].”
- Systematics of string loop corrections in type IIB Calabi-Yau flux compactifications (2007, methodology): “– 27 – and Hebecker [ 14 ]. In addition, Parameswaran and Westphal [30] studied the possibility to have a consistent D-term uplifting to de Sitter in this scenario.”
- Flux compactifications in string theory: A Comprehensive review (2005, background): “[173, 189], that α′ corrections to the Kähler potential (tree level and string loop) should be enough to stabilize all moduli in a IIB orientifold compactification, without the need of non-perturbative corrections.”
- Inflation and String Theory (2014, background): “203), are those conjectured in [324] (see also [325, 782]) as generalizations of the explicit computations of [322,323] for the toroidal orientifold T (6)/(Z2 × Z2).”
- Kahler moduli inflation (2005, background): “(For other recent work on perturbative corrections in IIB flux compactifications see [18, 19, 20, 21, 22]).”
- On D3-brane Potentials in Compactifications with Fluxes and Wrapped D-branes (2006, background): “(3)Corrections to the Kähler potential provide one additional effect; see [20, 21].”
- The type IIB string axiverse and its low-energy phenomenology (2012, background): “Hence the remaining nax − 1 flat direction can be lifted at subleading order either by open string loops (if the corresponding cycle intersects a cycle wrapped by a brane or the cycle itself is wrapped by a brane with vanishing flux so that the axion is not eaten up) [24] or by closed string loops [”
- General analysis of LARGE Volume Scenarios with string loop moduli stabilisation (2008, background): “exhibits an extended no-scale structure, and the loop corrections contribute to the scalar potential at a level subleading to their contribution to the K¨ahler potential and subleading to the α ′ corrections [1 0, 11, 12].”