title: Neutrino signal of electron-capture supernovae from core collapse to cooling.
abstract: An 8.8M{⊙} electron-capture supernova was simulated in spherical symmetry consistently from collapse through explosion to essentially complete deleptonization of the forming neutron star. The evolution time (∼9  s) is short because high-density effects suppress our neutrino opacities. After a short phase of accretion-enhanced luminosities (∼200  ms), luminosity equipartition among all species becomes almost perfect and the spectra of ν{e} and ν{μ,τ} very similar, ruling out the neutrino-driven wind as r-process site. We also discuss consequences for neutrino flavor oscillations.
authors.affiliation: Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, D-85748 Garching, Germany.
authors.forename: L
authors.initials: L
authors.lastname: Hüdepohl
authors.forename: B
authors.initials: B
authors.lastname: Müller
authors.forename: H-T
authors.initials: HT
authors.lastname: Janka
authors.forename: A
authors.initials: A
authors.lastname: Marek
authors.forename: G G
authors.initials: GG
authors.lastname: Raffelt