AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France

Neutrino–neutrino refraction dominates the flavor evolution in core-collapse supernovae,
neutron star mergers, and the early Universe. Ordinary neutrino flavor conversions develop …

The sensitivity of the Deep Underground Neutrino Experiment (DUNE) to neutrino oscillation
is determined, based on a full simulation, reconstruction, and event selection of the far …

The preponderance of matter over antimatter in the early universe, the dynamics of the
supernovae that produced the heavy elements necessary for life, and whether protons …

Abstract The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose
underground liquid scintillator detector, was proposed with the determination of the neutrino …

Abstract The Deep Underground Neutrino Experiment (DUNE), a 40-kton underground
liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino …

We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a
broad range of progenitor masses. This is the largest collection of sophisticated 3D …

All ten LIGO/Virgo binary black hole (BH-BH) coalescences reported following the O1/O2
runs have near-zero effective spins. There are only three potential explanations for this. If the …

One of the greatest uncertainties in any modeling of the inner engine of core-collapse
supernova (CCSN) is neutrino-flavor conversions driven by neutrino self-interactions. We …

We return to interpreting the historical SN 1987A neutrino data from a modern perspective.
To this end, we construct a suite of spherically symmetric supernova models with the …