Perturbativity Constraints in BSM Models
Manuel E. Krauss, Florian Staub

TL;DR
This paper investigates the limitations of perturbative calculations in BSM models, specifically the Georgi-Machacek model, highlighting the importance of radiative corrections and proposing criteria to identify non-perturbative regions.
Contribution
It introduces perturbativity conditions applicable to BSM models and demonstrates their significance in accurately analyzing the Georgi-Machacek model's parameter space.
Findings
Radiative corrections can invalidate perturbative assumptions in the Georgi-Machacek model.
Tree-level vacuum stability constraints may be misleading without loop corrections.
Perturbativity conditions help identify regions where perturbation theory breaks down.
Abstract
Phenomenological studies performed for non-supersymmetric extensions of the Standard Model usually use tree-level parameters as input to define the scalar sector of the model. This implicitly assumes that a full on-shell calculation of the scalar sector is possible - and meaningful. However, this doesn't have to be the case as we show explicitly at the example of the Georgi-Machacek model. This model comes with an appealing custodial symmetry to explain the smallness of the parameter. However, the model cannot be renormalised on-shell without breaking the custodial symmetry. Moreover, we find that it can often happen that the radiative corrections are so large that any consideration based on a perturbative expansion appears to be meaningless: counter-terms to quartic couplings can become much larger than and/or two-loop mass corrections can become larger than the one-loop…
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