Sensitivity to the ordering of neutrino masses at oscillation experiments

• Pilar Coloma (Virginia Tech)

Room: 132:028

Illuminating LMA-Dark solution and superlight sterile neutrinos by intermediate baseline reactor neutrino experiments

• Yasaman Farzan (IPM)

Room: 132:028

A non-SUSY SO(10) model for the physics below MGUT

• Davide Meloni (RomaTre University)

Room: 132:028

The search for leptonic CP violation

• Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)

Room: 132:028

The Zee-Babu revisited in the light of new data

• Juan Herrero (IFIC Valencia)

Room: 132:028

Interplay of flavour and CP symmetries

• Claudia Hagedorn (TU Munich)

Room: 132:028

Beyond tree-level Majorana neutrino masses: the two-loop case

• Diego Aristizabal (IFPA, Universite de Liege)

Room: 132:028

Cabibbo’s dream: dynamical origin of masses

• Belen Gavela (IFT Madrid)

Room: FA32 Are the seemingly random masses and mixings of the fundamental particles “just-so” numbers or may they have a dynamical origin? I will overview the status of the flavour puzzle, with special emphasis on the light that the neutrino sector is shedding on it. I will then discuss recent developments that could suggest a change of paradigm in our understanding of the masses of the visible matter, in a quite model-independent way, as well as the expected phenomenological and experimental consequences.

Running Masses at Various Energy Scales

• He Zhang (MPIK Heidelberg)

Room: 132:028

Low Scale Minimal Seesaw Models

• Jacobo Lopez Pavon (SISSA Trieste)

Room: 132:028

Sterile Neutrinos on Earth and in the Skies

• Joachim Kopp (MPIK Heidelberg)

Room: 132:028

Neutrino results from WiggleZ

• Signe Riemer-Sorensen (Institute of Theoretical Astrophysics, Oslo)

Room: 132:028

On neutrinos in E6 GUT

• Borut Bajc

Room: 132:028

Are GRBs the sources of the UHECRs?

• Walter Winter (Wurzburg university)

Room: 132:028

Neutrinos: Ghost particles of the universe

• Georg Raffelt (MPI Physik, Munich, Germany)

Room: Oskar Klein's auditorium

Atmospheric neutrinos from charm/leptons from charm

• Hallsie Reno (University of Iowa)

Room: 132:028

On the flavor composition of the high-energy neutrino events in IceCube

• Sergio Palomares-Ruiz (IFIC Valencia)

Room: 132:028

FIMP Realization of the Scotogenic Model

• Emiliano Molinaro (TU München)

Room: 132:028

Strong thermal leptogenesis and the absolute neutrino mass scale

• Pasquale Di Bari (University of Southampton)

Room: 132:028

Dips in the Diffuse Supernova Neutrino Background

• Yasaman FARZAN

Room: 132:028 Scalar (fermion) dark matter with mass in the MeV range coupled to ordinary neutrinos and another fermion (scalar) is motivated by scenarios that establish a link between radiatively generated neutrino masses and the dark matter relic density. With such a coupling, cosmic supernova neutrinos can resonantly interact with the background dark matter particles on their way to us, giving rise to a dip in their redshift-integrated spectra. Current and future neutrino detectors, such as Super-Kamiokande, LENA and Hyper- Kamiokande, might be able to detect this distortion.