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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

Other publications:

Micro-orbits in a many-branes model and deviations from module/r^2$ Newton's law - Non-standard interactions with high-energy atmospheric neutrinos at IceCube - Search for sharp and smooth spectral signatures of $\mu\nu$SSM gravitino dark matter with Fermi-LAT - Dark matter interpretations of ATLAS searches for the electroweak production of supersymmetric particles in $\sqrt{s} = ... - Test of Lorentz Violation with Astrophysical Neutrino Flavor - Non-leptonic kaon decays at large $N_c$ - Dark energy from the motions of neutrinos - Sterile Neutrino portal to Dark Matter II: Exact Dark symmetry - Testable Baryogenesis in Seesaw Models - Sterile neutrino portal to Dark Matter I: The $U(1)_{B-L}$ case - A New Approach to Nuclear Form Factors for Direct Dark Matter Searches - Primordial power spectrum features in phenomenological descriptions of inflation - Higgs lepton flavour violation: UV completions and connection to neutrino masses - On the improvement of cosmological neutrino mass bounds - The BSM-AI project: SUSY-AI - Generalizing LHC limits on Supersymmetry with Machine Learning - Searches for Sterile Neutrinos with the IceCube Detector - Analysis of the 4-year IceCube high-energy starting events - Implications of solar wind measurements for solar models and composition - Naturalness of MSSM dark matter - The 21 cm signal and the interplay between dark matter annihilations and astrophysical processes

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