Non-tachyonic Scherk-Schwarz compactifications, cosmology and moduli stabilization
arXiv:hep-th/0401201 · doi:10.1088/1126-6708/2004/03/060
Abstract
It is well-known that Scherk-Schwarz compactifications in string theory have a tachyon in the closed string spectrum appearing for a critical value of a compact radius. The tachyon can be removed by an appropriate orientifold projection in type II strings, giving rise to tachyon-free compactifications. We present explicit examples of this type in various dimensions, including six and four-dimensional chiral examples, with softly broken supersymmetry in the closed sector and non-BPS configurations in the open sector. These vacua are interesting frameworks for studying various cosmological issues. We discuss four-dimensional cosmological solutions and moduli stabilization triggered by nonperturbative effects like gaugino condensation on D-branes and fluxes.
36 pages, LaTeX; added references
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- Spin-field Interaction Effects and Loop Dynamics in AdS/CFT Duality
- An Alternative for Moduli Stabilisation
- On exponential suppression of the cosmological constant in non-SUSY strings at two loops and beyond
- Scherk-Schwarz Breaking and Intersecting Branes
- Stability and vacuum energy in open string models with broken supersymmetry
- On interpolations from SUSY to non-SUSY strings and their properties
- Geometry of orientifold vacua and supersymmetry breaking
- Moduli Stabilization with Long Winding Strings
- A Dynamical Mechanism for Large Volumes with Consistent Couplings
- Tachyons and Misaligned Supersymmetry in Closed String Vacua