Evaluating Approximate Flavor Instability Metrics in Neutron Star Mergers
Sherwood Richers

TL;DR
This paper evaluates the effectiveness of various moment-based neutrino flavor instability metrics in neutron star mergers, introducing a new maximum entropy test that improves prediction accuracy of flavor transformation regions.
Contribution
The study compares existing instability tests using realistic neutrino distributions and proposes a new maximum entropy test for better prediction of flavor instability in mergers.
Findings
Maximum entropy test predicts instability more accurately.
Resonant trajectory test also performs well.
All tests identify regions with significant flavor transformation.
Abstract
Neutrinos can rapidly change flavor in the inner dense regions of core-collapse supernovae and neutron star mergers due to the neutrino fast flavor instability. If the amount of flavor transformation is significant, the FFI could significantly affect how supernovae explode and how supernovae and mergers enrich the universe with heavy elements. Since many state of the art supernova and merger simulations rely on neutrino transport algorithms based on angular moments of the radiation field, there is incomplete information with which to determine if the distributions are unstable to the FFI. In this work we test the performance of several proposed moment-based instability tests in the literature. We perform time-independent general relativistic neutrino transport on a snapshot of a 3D neutron star merger simulation to generate reasonable neutrino distributions and check where each of these…
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Taxonomy
TopicsNeutrino Physics Research · Particle physics theoretical and experimental studies · High-Energy Particle Collisions Research
