N = 1 sigma models in AdS[subscript 4]

We study sigma models in AdS4 with global N = 1 supersymmetry and find that they differ significantly from their flat-space cousins - the target space is constrained to be a K¨ahler manifold with an exact K¨ahler form, the superpotential transforms under K¨ahler transformations, the space of supersy...

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Bibliographic Details
Main Authors: Adams, Allan (Contributor), Jockers, Hans (Author), Kumar, Vijay (Author), Lapan, Joshua M. (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: Springer-Verlag, 2012-08-06T19:36:06Z.
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Online Access:Get fulltext
LEADER 01722 am a22002293u 4500
001 71992
042 |a dc 
100 1 0 |a Adams, Allan  |e author 
100 1 0 |a Massachusetts Institute of Technology. Department of Physics  |e contributor 
100 1 0 |a Adams, Allan  |e contributor 
100 1 0 |a Adams, Allan  |e contributor 
700 1 0 |a Jockers, Hans  |e author 
700 1 0 |a Kumar, Vijay  |e author 
700 1 0 |a Lapan, Joshua M.  |e author 
245 0 0 |a N = 1 sigma models in AdS[subscript 4] 
260 |b Springer-Verlag,   |c 2012-08-06T19:36:06Z. 
856 |z Get fulltext  |u http://hdl.handle.net/1721.1/71992 
520 |a We study sigma models in AdS4 with global N = 1 supersymmetry and find that they differ significantly from their flat-space cousins - the target space is constrained to be a K¨ahler manifold with an exact K¨ahler form, the superpotential transforms under K¨ahler transformations, the space of supersymmetric vacua is generically a set of isolated points even when the superpotential vanishes, and the R-symmetry is classically broken by the cosmological constant. Remarkably, the exactness of the K¨ahler class is also required for the sigma model to arise as a decoupling limit of N = 1 supergravity, and ensures the vanishing of gravitational anomalies. As applications of these results, we argue that fields with AdS4 scale masses are ubiquitous in, for example, type IIB N = 1 AdS4 vacua stabilized near large volume; we also present a schematic argument that the Affleck-Dine- Seiberg runaway of Nf < Nc SQCD can be regulated by considering the theory in AdS4. 
520 |a United States. Dept. of Energy (contract DE-FC02-94ER40818) 
546 |a en_US 
655 7 |a Article 
773 |t Journal of High Energy Physics