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CERN Accelerating science

 
Snowmass Neutrino Frontier Report - Huber, Patrick et al - arXiv:2211.08641FERMILAB-FN-1215-ND-PPD-SCD
 
Summary plot of experiments indicating rough time scale and range of physics topics addressed by each. The information is provided by the collaborations. Details and references are found in Tab.~\ref{tab:experiments}.
Summary plot of experiments indicating rough time scale and range of physics topics addressed by each. The information is provided by the collaborations. Details and references are found in Tab.~\ref{tab:experiments}.
The best-fit values of $\sinst{23}$ and $\deltacp$ to NOvA and T2K data for the normal neutrino mass ordering (top), and the inverted neutrino mass ordering (bottom)~\cite{NOvA:2021nfi}.
The best-fit values of $\sinst{23}$ and $\deltacp$ to NOvA and T2K data for the normal neutrino mass ordering (top), and the inverted neutrino mass ordering (bottom)~\cite{NOvA:2021nfi}.
90\% confidence intervals for $\sinstt{13} - \deltacp$ (left), and $\sin^2{23} - \dm{32}$ (right) after a range of exposures in kt-MW-years, for a projected measurement with assumed true parameter values near the current global best fit. Yellow regions indicate recent global fits from NuFIT 4.0.
90\% confidence intervals for $\sinstt{13} - \deltacp$ (left), and $\sin^2{23} - \dm{32}$ (right) after a range of exposures in kt-MW-years, for a projected measurement with assumed true parameter values near the current global best fit. Yellow regions indicate recent global fits from NuFIT 4.0.
90\% confidence intervals for $\sinstt{13} - \deltacp$ (left), and $\sin^2{23} - \dm{32}$ (right) after a range of exposures in kt-MW-years, for a projected measurement with assumed true parameter values near the current global best fit. Yellow regions indicate recent global fits from NuFIT 4.0.
90\% confidence intervals for $\sinstt{13} - \deltacp$ (left), and $\sin^2{23} - \dm{32}$ (right) after a range of exposures in kt-MW-years, for a projected measurement with assumed true parameter values near the current global best fit. Yellow regions indicate recent global fits from NuFIT 4.0.
HK sensitivity to exclude $\sin\delta (cp) = 0$, plotted as a function of the true value of \deltacp, assuming the mass ordering is unknown. A combined fit of HK beam and atmospheric neutrinos significantly enhances the HK sensitivity to \deltacp.
HK sensitivity to exclude $\sin\delta (cp) = 0$, plotted as a function of the true value of \deltacp, assuming the mass ordering is unknown. A combined fit of HK beam and atmospheric neutrinos significantly enhances the HK sensitivity to \deltacp.
``Grand Unified Neutrino Spectrum" of natural neutrinos arriving at Earth (reactor neutrinos also shown). Figure from Ref.~\cite{Vitagliano:2019yzm}.
``Grand Unified Neutrino Spectrum" of natural neutrinos arriving at Earth (reactor neutrinos also shown). Figure from Ref.~\cite{Vitagliano:2019yzm}.
Neutrino beam power vs. energy for current and future long-baseline neutrino beams. The energy range shown here is the approximate width to half-max around the beam peak energy.
Neutrino beam power vs. energy for current and future long-baseline neutrino beams. The energy range shown here is the approximate width to half-max around the beam peak energy.