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Radiative brane-mass terms in D>5 orbifold gauge theories

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dc.contributor.author Gersdorff, G en
dc.contributor.author Irges, N en
dc.contributor.author Quirós, M en
dc.date.accessioned 2014-03-01T01:52:51Z
dc.date.available 2014-03-01T01:52:51Z
dc.date.issued 2003 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/26745
dc.subject Fixed Point en
dc.subject Gauge Field en
dc.subject Gauge Invariance en
dc.subject Gauge Theory en
dc.subject Space Time en
dc.title Radiative brane-mass terms in D>5 orbifold gauge theories en
heal.type journalArticle en
heal.identifier.primary 10.1016/S0370-2693(02)03039-3 en
heal.identifier.secondary http://dx.doi.org/10.1016/S0370-2693(02)03039-3 en
heal.publicationDate 2003 en
heal.abstract A gauge theory with gauge group G defined in D>4 space–time dimensions can be broken to a subgroup H on four-dimensional fixed point branes, when compactified on an orbifold. Mass terms for extra-dimensional components of gauge fields Ai (brane scalars) might acquire (when allowed by the brane symmetries) quadratically divergent radiative masses and thus jeopardize the stability of the four-dimensional en
heal.journalName Physics Letters B en
dc.identifier.doi 10.1016/S0370-2693(02)03039-3 en


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