Orientifolds of Gepner models

We systematically construct and study Type II Orientifolds based on Gepner models which have ##IMG## [http://ej.iop.org/icons/Entities/calN.gif] Script N = 1 supersymmetry in 3+1 dimensions. We classify the parity symmetries and construct the crosscap states. We write down the conditions that a conf...

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Hauptverfasser: Brunner, Ilka (VerfasserIn) , Walcher, Johannes (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: February 1, 2007
In: Journal of high energy physics
Year: 2007, Heft: 02
ISSN:1029-8479
DOI:10.1088/1126-6708/2007/02/001
Online-Zugang:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1088/1126-6708/2007/02/001
Verlag, kostenfrei, Volltext: http://stacks.iop.org/1126-6708/2007/i=02/a=001
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Verfasserangaben:Ilka Brunner (CERN Theory Division, Geneva, Switzerland, and King’s College, London, United Kingdom), Kentaro Hori and Kazuo Hosomichi (University of Toronto, Toronto, Ontario, Canada), Johannes Walcher (Kavli Institute for Theoretical Physics, University of California, Santa Barbara, U.S.A)

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520 |a We systematically construct and study Type II Orientifolds based on Gepner models which have ##IMG## [http://ej.iop.org/icons/Entities/calN.gif] Script N = 1 supersymmetry in 3+1 dimensions. We classify the parity symmetries and construct the crosscap states. We write down the conditions that a configuration of rational branes must satisfy for consistency (tadpole cancellation and rank constraints) and spacetime supersymmetry. For certain cases, including Type IIB orientifolds of the quintic and a two parameter model, one can find all solutions in this class. Depending on the parity, the number of vacua can be large, of the order of 10 10 −10 13 . For other models, it is hard to find all solutions but special solutions can be found — some of them are chiral. We also make comparison with the large volume regime and obtain a perfect match. Through this study, we find a number of new features of Type II orientifolds, including the structure of moduli space and the change in the type of O-planes under navigation through non-geometric phases. 
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