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The possible effect on the flavour spectra of astronomical neutrinos from aneutrino-dark matter interaction has been investigated for decoherentneutrinos. In this work, we report results calculated for coherent neutrinos.This was done with two different models for the neutrino dark-matterinteractions: a flavour state interaction,as for the weak interaction in theStandard Model, and a mass state interaction, which is predicted by certainnon-Standard Models (specifically Scotogenic models). It was found that using acoherent analysis dramatically increased the explorable parameter space for theneutrino-dark matter interaction. However, the detection of coherentastronomical neutrinos presents a significant challenge to experimentalists,because such a detection would require an improvement in energy resolution byat least six orders of magnitude, with similar improvements in astronomicaldistance determinations.

Meaningful Details: The value of adding baseline dependence to the Neutrino-Dark Matter Effect