Speaker
Yong Du
(ITP CAS)
Description
In this talk, we will firstly briefly review the type-II seesaw model that is responsible for non-vanishing neutrino masses and the baryon asymmetry of the Universe. Then after discussing its collider signatures, we will explain how to investigate this model using gravitational wave searches at future gravitational wave observatories such as BBO and DECIGO. Time permitting, the complementarity between collider and gravitational wave searches for this model will also be discussed.
This talk is based on: https://arxiv.org/abs/2203.01561
Primary author
Yong Du
(ITP CAS)
Co-authors
Dr
Ligong Bian
(ITP/KITPC)
Ruiyu Zhou
(CQUPT)
