23–27 Oct 2023
Istituto Veneto di Scienze, Lettere ed Arti
Europe/Rome timezone
opening day available in streaming on the YouTube channel of the Physics and Astronomy Dpt. of the University of Padova: https://youtu.be/t_9s2ALOFGQ

The race for the Neutrino Mass Ordering

Not scheduled
20m
Palazzo Franchetti (Istituto Veneto di Scienze, Lettere ed Arti)

Palazzo Franchetti

Istituto Veneto di Scienze, Lettere ed Arti

Campo S. Stefano, 2945 S.Marco, Venezia
Contributed Parallel Talk Neutrino Properties

Speaker

Stephen Parke (Fermilab)

Description

On Friday, 5/12, I gave the Wine and Cheese seminar at Fermilab titled “The race to the Neutrino Mass Ordering”.
The slides are here https://indico.fnal.gov/event/59268/

In this talk I argued that when JUNO’s measurement of Delta m^2_atm (31 or 32 or ee) is 1\% or better (which will happen very quickly)
then when combined with Delta m^2_atm from T2K and NOvA disappearance will give us a Delta Chisq between the two mass orderings, IO and NO, will exceed 9, in a combined fit with JUNO, T2K, NOvA and SuperK. So by Neutrino 2026 (or maybe Neutel 2025) we should know the mass ordering at better than 3 sigma. A hint of this can be seen in the 2022 NuFit plot (bottom right panel). http://www.nu-fit.org/sites/default/files/v52.fig-chisq-dma.pdf Replacing Daya Bay which is a 2.4% measurement with a new 1% JUNO measurement will greatly effect this plot.

The comparison of nu_e disappearance to nu_mu disappearance as a way to determine the mass ordering was first discussed in our 2005 paper https://arxiv.org/abs/hep-ph/0503283 This paper also was the first to defined Delta m^2_{ee}. We will update this in a paper in the next month or so and certainly before Neutel 2023.

If there is interest I could give a version of this talk explaining this development as plenary talk at Neutel 2023. For now I would keep the same title “The race to the Neutrino Mass Ordering”.

Primary author

Stephen Parke (Fermilab)

Presentation materials

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