26–29 Oct 2021
Fully online format
Asia/Tokyo timezone

A model for tiny neutrino masses, dark matter, and baryon asymmetry and its phenomenology at the ILC

27 Oct 2021, 13:40
20m
Room #4 (Zoom Meeting ID: 840 3553 0145)

Room #4

Zoom Meeting ID: 840 3553 0145

Oral presentation using Zoom Session H: BSM particle production H-1: BSM particle production

Speakers

Kazuki Enomoto (Osaka University) Mayumi Aoki Shinya Kanemura (Osaka University)

Description

The origin of tiny neutrino masses, dark matter, and baryon asymmetry of the universe is still a mystery, and there is no doubt that there is new physics beyond the Standard Model. In a previous work, a new physics model at TeV-scale where all of them can be explained has been proposed, however the authors neglected CPV phases, and on the baryon asymmetry, they only showed the possibility of the strongly 1st order phase transition for the electroweak baryogenesis. We have extended this model to include CPV phases and evaluated neutrino masses, dark matter, and the baryon number asymmetry generated by the electroweak baryogenesis. In this talk, I will introduce this model and discuss the phenomenology at current and near future experiments including the ILC.

1st preferred time slot for your oral presentation 13:00-15:00 JST (6:00-8:00 CEST, 0:00-2:00 EDT, 21:00-23:00 PDT)
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Primary authors

Kazuki Enomoto (Osaka University) Mayumi Aoki Shinya Kanemura (Osaka University)

Presentation materials

There are no materials yet.