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Huchan Lee (Seoul National University of Science and Technology)19/08/2026, 14:30Parallel talks: 17'+3'
We investigate the phenomenology of a minimally extended scotogenic model motivated by the observed active neutrino masses, viable dark matter (DM) candidates, and the high-energy behavior of the Standard Model (SM) quartic coupling constant. The neutrino mass generation mechanism is briefly reviewed, covering both normal and inverted mass hierarchies, along with a concise discussion of DM...
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Arghyajit Datta (Chung-Ang University)19/08/2026, 14:50Parallel talks: 17'+3'
In this talk, we will present a possibility of realising successful cogenesis of baryon asymmetry of the Universe, dark matter and neutrino masses within the minimal scotogenic model with low-mass right handed neutrinos (RHN). In the conventional thermal scotogenic leptogenesis setup, there exists a viable parameter space with smaller masses for RHNs as compared to Type-I seesaw case, because...
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Mr Bruno M. S. Oliveira (Centro de Física Teórica de Partículas (CFTP), Instituto Superior Técnico (IST), Universidade de Lisboa (UL))19/08/2026, 15:10Parallel talks: 17'+3'
Symmetry-protected low-scale seesaw models can account for the observed neutrino flavour oscillations without fine-tuning, while yielding collider-accessible signatures through pseudo-Dirac heavy neutral leptons (HNLs). Seesaw frameworks generically predict lepton number (LN) violation, which provides a powerful discovery channel. In symmetry-protected realisations, however, the amplitudes for...
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Avelino Vicente (IFIC, CSIC-UV)19/08/2026, 15:30Parallel talks: 17'+3'
The gauge principle is a cornerstone of model building, yet most constructions gauge only the $SU(N)$ factors while leaving the associated $U(1)$ phase redundancies global. I take the gauge principle to its logical extreme and promote all $SU(N)$ groups to $U(N)$, proposing that the underlying symmetry of the strong and electroweak interactions is not $SU(3)_c \times SU(2)_L \times U(1)_Y$ but...
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