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000643120 1001_ $$0P:(DE-H253)PIP1111196$$aFiorillo, Damiano Francesco Giuseppe$$b0$$eCorresponding author
000643120 245__ $$aNeutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae
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000643120 520__ $$aCollective neutrino flavor conversions in core-collapse supernovae begin with instabilities, initially triggered when the dominant νe outflow concurs with a small antineutrino flux of opposite lepton number, with $\bar{ν}_e$ dominating over  $\bar{ν}_μ$. When these “flipped” neutrinos emerge in the energy-integrated angular distribution (angular crossing), they initiate a fast instability. However, before such conditions arise, spectral crossings typically appear within 20 ms of collapse, i.e., local spectral excesses of $\bar{ν}_e$ over $\bar{ν}_μ$ along some direction. Therefore, postprocessing supernova simulations cannot consistently capture later fast instabilities because the early slow ones have already altered the conditions.
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000643120 7001_ $$00000-0002-0831-3330$$aJanka, Hans-Thomas$$b1
000643120 7001_ $$00000-0002-0199-9560$$aRaffelt, Georg G.$$b2
000643120 773__ $$0PERI:(DE-600)1472655-5$$a10.1103/jbmx-rbzt$$gVol. 135, no. 23, p. 231003$$n23$$p231003$$tPhysical review letters$$v135$$x0031-9007$$y2025
000643120 7870_ $$0PUBDB-2025-03940$$aFiorillo, Damiano Francesco Giuseppe et.al.$$d2025$$iIsParent$$rarXiv:2507.22985$$tWhen First Beats Fast: Early Neutrino-Mass-Driven Flavor Instabilities in Supernovae
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