Journal
PHYSICAL REVIEW LETTERS
Volume 104, Issue 25, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.104.251101
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Funding
- DFG [SFB/TR 7, SFB/TR 27, EXC 153]
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An 8: 8M(circle dot) 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 (similar to 9 s) is short because high-density effects suppress our neutrino opacities. After a short phase of accretion-enhanced luminosities (similar to 200 ms), luminosity equipartition among all species becomes almost perfect and the spectra of (nu) over bar (e) and (nu) over bar (mu,tau) very similar, ruling out the neutrino-driven wind as r-process site. We also discuss consequences for neutrino flavor oscillations.
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