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Accepted Answer

In binary neutron star merger remnants, fast flavor instability occurs transiently and locally with high sensitivity to the central compact object, whereas collisional flavor instability occurs persistently and widespread throughout the accretion disk. Novelty: ClaimNovelty.INCREMENTAL. Consensus alignment: ConsensusAlignment.SUPPORTS_CONSENSUS.

Neutrino flavor instabilities in a binary neutron star merger remnant: Roles of a long-lived hypermassive neutron star

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