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

Gersdorff, G; Irges, N; Quirós, M

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