Systematic analysis of radiative symmetry breaking in models with extended scalar sector
Abstract
Radiative symmetry breaking (RSB) is a theoretically appealing framework for the generation of mass scales through quantum effects. It can be successfully implemented in models with extended scalar and gauge sectors. We provide a systematic analysis of RSB in such models: we review the common approximative methods of studying RSB, emphasising their limits of applicability and discuss the relevance of the relative magnitudes of tree-level and loop contributions as well as the dependence of the results on the renormalisation scale. The general considerations are exemplified within the context of the conformal Standard Model extended with a scalar doublet of a new SU(2) gauge group, the so-called SU(2)cSM. We show that various perturbative methods of studying RSB may yield significantly different results due to renormalisation-scale dependence. Implementing the renormalisation-group (RG) improvement method recently developed in arXiv:1801.05258, which is well-suited for multi-scale models, we argue that the use of the RG improved effective potential can alleviate this scale dependence providing more reliable results.
Keywords
Cite
@article{arxiv.1805.09292,
title = {Systematic analysis of radiative symmetry breaking in models with extended scalar sector},
author = {Leonardo Chataignier and Tomislav Prokopec and Michael G. Schmidt and Bogumila Swiezewska},
journal= {arXiv preprint arXiv:1805.09292},
year = {2018}
}
Comments
31 pages, 8 figures; v2: comparison with the Gildener-Weinberg method extended with an analysis of the mixing angle, references added, minor modifications, v3: missing plot legends added, v4: minor changes, matches published version