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The Unravelling of Flavor Coherence

arunavam edited this page Nov 24, 2020 · 2 revisions

Speaker: Basudeb DasGupta (TIFR, Mumbai)

Date/Time: 1 December 2020 (Tuesday) 3:30 PM IST

Abstract:

A supernova natively emits neutrinos and antineutrinos of all flavors with different luminosities and energy spectra. I will show how the different neutrino flavors are brought closer to each other due to irreversible decoherence-like processes occurring at a Tera-Hz rate, determined by the large neutrino density. This new result allows detailed implementation of flavor-dependent neutrino transport in supernova simulations and paves the way for supernova neutrino phenomenology. From a more conceptual perspective, this concrete example will show how collective behaviour can be parametrically faster than that of its constituents, and how "coarse-graining" leads to irreversible "relaxation" even though the microscopic dynamics remains perfectly time-reversal invariant.

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