Radiative brane-mass terms in D>5 orbifold gauge theories
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 A_i (brane scalars) might acquire (when allowed by the brane symmetries) quadratically divergent radiative masses and thus jeopardize the stability of the four-dimensional theory. We have analyzed Z_2 compactifications and identified the brane symmetries remnants of the higher dimensional gauge invariance. No mass term is allowed for D=5 while for D>5 a tadpole \epsilon^{ij}F_{ij}^\alpha can appear when there are U_\alpha(1) factors in H. A detailed calculation is done for the D=6 case and it is established that the tadpole is related, although does not coincide, with the U_\alpha(1) anomaly induced on the brane by the bulk fermions. In particular, no tadpole is generated from gauge bosons or fermions in real representations
Cite
@article{arxiv.hep-ph/0210134,
title = {Radiative brane-mass terms in D>5 orbifold gauge theories},
author = {G. v. Gersdorff and N. Irges and M. Quiros},
journal= {arXiv preprint arXiv:hep-ph/0210134},
year = {2010}
}
Comments
12 pages, 2 figures, axodraw.sty. v2: important typoes corrected and reference added. v3: logarithmic corrections to tadpole included