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Flavor and Origin of Matter - Sabor y Origen de la Materia

SOM (We are) is one of the leading theoretical particle physics groups in Spain, and includes IFIC members from the University of Valencia and CSIC. Our group has a broad research program in flavor physics with active work in Lattice QCD, neutrino phenomenology and leptogenesis. Members of the group also carry out research in cosmology and fundamental physics. While we have a strong theoretical component to our research, some of us are involved in large collaborations in neutrino physics ( Euronu ) and cosmology (SDSSIII ).

SOM is the most active group at IFIC organizing about half of the IFIC collloquia and IFIC seminars (see La Trobada and Invisibles webinar).

 

Latest 10 Publications in INSPIRE

More publications:

Neutrino Mass Ordering at DUNE: an Extra $\nu$-Bonus - Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout - First numerical study of Neutrino-Dark Matter Mixed Damping - Cosmology-marginalized approaches in Bayesian model comparison: The neutrino mass as a case study - Dark matter microphysics and 21 cm observations - Majorana vs Pseudo-Dirac Neutrinos at the ILC - Follow-up on non-leptonic kaon decays at large $N_c$ - Low-scale leptogenesis and dark matter - Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects - The dispirited case of gauged U(1)$_{B-L}$ dark matter - EDGES result versus CMB and low-redshift constraints on ionization histories - Probing the sterile neutrino portal to Dark Matter with $\gamma$ rays - A fresh look into the interacting dark matter scenario - Neutrino tomography of Earth - Axion Searches with Microwave Filters: the RADES project - Reconciling tensor and scalar observables in G-inflation - Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z) \geq -1$ are tighter than those... - Non-Standard Interactions with High-energy Atmospheric Neutrinos at IceCube - Neutrino masses and their ordering: Global Data, Priors and Models - Robustness of cosmological thermal axion mass bounds

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