Statistics of M theory vacua

dc.contributor.areaPhysicsen_US
dc.contributor.authorAcharya, Bobby Samiren_US
dc.contributor.authorDenef, Frederiken_US
dc.contributor.authorValandro, Robertoen_US
dc.contributor.departmentElementary Particle Theoryen_US
dc.date.accessioned2005en_US
dc.date.accessioned2011-09-07T20:27:45Z
dc.date.available2005en_US
dc.date.available2011-09-07T20:27:45Z
dc.date.issued2005en_US
dc.description.abstractWe study the vacuum statistics of ensembles of M theory compactifications on G2 holonomy manifolds with fluxes, and of ensembles of Freund-Rubin vacua. We discuss similarities and differences between these and Type IIB flux landscapes. For the G2 ensembles, we find that large volumes are strongly suppressed, and for both, unlike the IIB case, the distribution of cosmological constants is non-uniform. We also argue that these ensembles typically have exponentially more non-supersymmetric than supersymmetric vacua, and show that supersymmetry is virtually always broken at a high scale.en_US
dc.format.extent692456 bytesen_US
dc.format.mimetypeapplication/pdfen_US
dc.identifier.citationJHEP 06(2005)056en_US
dc.identifier.urihttps://openscience.sissa.it/handle/1963/1716en_US
dc.language.isoen_USen_US
dc.relation.ispartofseriesSISSA;10/2005/EPen_US
dc.relation.ispartofseriesarXiv.org;hep-th/0502060en_US
dc.relation.uri10.1088/1126-6708/2005/06/056en_US
dc.titleStatistics of M theory vacuaen_US
dc.typePreprinten_US
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