Gravity Cutoff in Theories with Large Discrete Symmetries

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dc.creatorDvali, Gia
dc.creatorRedi, Michele
dc.creatorSibiryakov, Sergey
dc.creatorVainshtein, Arkady
dc.date2008-04-04
dc.date2008-09-29
dc.date.accessioned2026-07-07T11:49:36Z
dc.date.available2026-07-07T11:49:36Z
dc.descriptionWe set an upper bound on the gravitational cutoff in theories with exact quantum numbers of large N periodicity, such as Z_N discrete symmetries. The bound stems from black hole physics. It is similar to the bound appearing in theories with N particle species, though a priori, a large discrete symmetry does not imply a large number of species. Thus, there emerges a potentially wide class of new theories, that address the hierarchy problem by lowering the gravitational cutoff due to existence of large Z_{10^32}-type symmetries.
dc.descriptionexample and discussion added
dc.identifierhttps://arxiv.org/abs/0804.0769
dc.identifierhttp://arxiv.org/abs/0804.0769
dc.identifierPhys.Rev.Lett.101:151603,2008
dc.identifierdoi:10.1103/PhysRevLett.101.151603
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203293
dc.subjectHigh Energy Physics - Theory
dc.subjectHigh Energy Physics - Phenomenology
dc.titleGravity Cutoff in Theories with Large Discrete Symmetries
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