Role of dense matter in collective supernova neutrino transformations
By A. Esteban-Pretel, A. Mirizzi, Sergio Pastor, R. Tomàs, G. Raffelt, P. Serpico, G. Sigl. 2008
136 citations recorded by the source corpus.
For neutrinos streaming from a supernova core, dense matter suppresses self-induced flavor transformations if the electron density n{sub e} significantly exceeds the neutrino density n{sub {nu}} in the conversion region. If n{sub e} is comparable to n{sub {nu}}, one finds multiangle decoherence, whereas the standard self-induced transformation behavior requires that in the transformation region n{sub {nu}} is safely above n{sub e}. This condition need not be satisfied in the early phase after the supernova core bounce. Our new multiangle effect is a subtle consequence of neutrinos traveling on different trajectories when streaming from a source that is not pointlike.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/08cdaf090d5d9f4b9a7a3074117a2519d0f5aa53
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In Nuclear and High Energy Physics
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Citations in the corpus
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- Self-induced neutrino flavor conversion without flavor mixing (2016, background): “For example, during the supernova accretion phase, this instability would be suppressed in analogy to the “slow” instabilities [41–45].”
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- SELF-SUSTAINED ASYMMETRY OF LEPTON-NUMBER EMISSION: A NEW PHENOMENON DURING THE SUPERNOVA SHOCK-ACCRETION PHASE IN THREE DIMENSIONS (2014, background): “…in the dense region below the stalledshock wave is the so-called multi-angle matter effect, which tends to suppress self-induced flavor conversion (Esteban-Pretel et al. 2008; Sarikas et al. 2012; Raffelt et al. 2013; Chakraborty et al. 2011; Saviano et al. 2012; Chakraborty et al. 2014).”
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