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Role of collective neutrino flavor oscillations in core-collapse supernova shock revival
Physical Review D
We explore the effects of collective neutrino flavor oscillations due to neutrino-neutrino interactions on the neutrino heating behind a stalled core-collapse supernova shock. We carry out axisymmetric (2D) radiation-hydrodynamic core-collapse supernova simulations, tracking the first 400 ms of the post-core-bounce evolution in 11.2 solar mass and 15 solar mass progenitor stars. Using inputs from these 2D simulations, we perform neutrino flavor oscillation calculations in multi-energydoi:10.1103/physrevd.85.065008 fatcat:t6cle6iezrg77lyr5qtbnkoctm