from 30 November 2017 to 3 December 2017 (Europe/Warsaw)
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Radiative alignment in 2HDM

Presented by Pedro FERREIRA on 3 Dec 2017 from 10:00 to 10:30
Session: session 11

Content

The possibility that alignment arises in 2HDM as a consequence of the high-scale behaviour of the theory is discussed here. Requiring the 2HDM to be bounded from below and perturbative up to scales as low as a few TeV forces the lightest CP-even scalar to have SM-like properties for model Type II. Analogous conclusions are found for model I, if the charged higgs mass is larger than about 400 GeV. We therefore argue that alignment my arise "naturally" in the 2HDM, as a consequence from radiative corrections to the model.

Place

Location: Faculty of Physics
Room: Lecture Hall 0.06

Primary authors

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