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An absolute $\nu$ mass measurement with the DUNE experiment

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arxiv 2203.00024 v2 pith:STCG5MVU submitted 2022-02-28 hep-ph astro-ph.HE

Federica Pompa , Francesco Capozzi , Olga Mena , Michel Sorel This is my paper · ORCID
classification hep-phastro-ph.HE
keywords neutrinomasstimeabsoluteduneelectronfuturesupernova
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abstract

Time of flight delay in the supernova neutrino signal offers a unique tool to set model-independent constraints on the absolute neutrino mass. The presence of a sharp time structure during a first emission phase, the so-called neutronization burst in the electron neutrino flavor time distribution, makes this channel a very powerful one. Large liquid argon underground detectors will provide precision measurements of the time dependence of the electron neutrino fluxes. We derive here a new $\nu$ mass sensitivity attainable at the future DUNE far detector from a future supernova collapse in our galactic neighborhood, finding a sub-eV reach under favorable scenarios. These values are competitive with those expected for laboratory direct neutrino mass searches.

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Cited by 3 Pith papers

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    Binary neutron star merger neutrinos will require a megaton-scale detector and decades of operation to detect, but a single detected neutrino could set a sub-eV (~0.1 eV) limit on the lightest neutrino mass via gravit...

  3. Individual Neutrino Masses From a Supernova

    hep-ph 2024-11 conditional novelty 6.0 of 10

    Using time-of-flight delays of the three neutrino mass eigenstates across sharp supernova features, a galactic supernova at 10 kpc could individually constrain or measure neutrino masses at JUNO, with precision that d...

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