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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:

Testing emission models on the extreme blazar 2WHSP J073326.7+515354 detected at very high energies with the MAGIC teles... - Interacting dark energy after the latest Planck, DES, and $H_0$ measurements: an excellent solution to the $H_0$ and cos... - The Cherenkov Telescope Array Performance in Divergent Mode - Gravity-mediated Scalar Dark Matter in Warped Extra-Dimensions - Dark sectors with dynamical coupling - Constraints on gamma-ray and neutrino emission from NGC 1068 with the MAGIC telescopes - Constraining the primordial black hole abundance with 21-cm cosmology - Neutrino Mass Ordering at DUNE: an Extra $\nu$-Bonus - Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout - Neutrino tomography of the earth - Comprehensive 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 $N_c$ - Is it Mixed dark matter or neutrino masses? - Leptogenesis from oscillations 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

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