Temporal instability enables neutrino flavor conversions deep inside supernovae

Basudeb Dasgupta and Alessandro Mirizzi
Phys. Rev. D 92, 125030 – Published 28 December 2015

Abstract

We show that a self-interacting neutrino gas can spontaneously acquire a nonstationary pulsating component in its flavor content, with a frequency that can exactly cancel the “multiangle” refractive effects of dense matter. This can then enable homogeneous and inhomogeneous flavor conversion instabilities to exist even at large neutrino and matter densities, where the system would have been stable if the evolution were strictly stationary. Large flavor conversions, especially close to a supernova core, are possible via this novel mechanism. This may have important consequences for the explosion dynamics, nucleosynthesis, as well as for neutrino observations of supernovae.

  • Figure
  • Figure
  • Received 17 September 2015

DOI:https://doi.org/10.1103/PhysRevD.92.125030

© 2015 American Physical Society

Authors & Affiliations

Basudeb Dasgupta1 and Alessandro Mirizzi2

  • 1Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India
  • 2Dipartimento Interateneo di Fisica “Michelangelo Merlin,” Via Amendola 173, 70126 Bari, Italy; Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Via Amendola 173, 70126 Bari, Italy

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Issue

Vol. 92, Iss. 12 — 15 December 2015

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