Systematic analysis of radiative symmetry breaking in models with extended scalar sector

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 approx...

Descrizione completa

Salvato in:
Dettagli Bibliografici
Autori principali: Chataignier, Leonardo (Autore) , Schmidt, Michael G. (Autore)
Natura: Article (Journal)
Lingua:inglese
Pubblicazione: 14 August 2018
In: Journal of high energy physics
Year: 2018, Fascicolo: 8
ISSN:1029-8479
DOI:10.1007/JHEP08(2018)083
Accesso online:Verlag, Volltext: https://doi.org/10.1007/JHEP08(2018)083
Testo
Note sull'autore:Leonardo Chataignier, Tomislav Prokopec, Michael G. Schmidt and Bogumiła Świeżewska
Descrizione
Riassunto: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)X 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 ref. [1], 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.
Descrizione del documento:Gesehen am 11.04.2019
Descrizione fisica:Online Resource
ISSN:1029-8479
DOI:10.1007/JHEP08(2018)083