Computational Techniques for the Analysis of Small Signals in High-Statistics Neutrino Oscillation Experiments
IceCube Collaboration: M. G. Aartsen, M. Ackermann, J. Adams, J. A., Aguilar, M. Ahlers, M. Ahrens, I. Al Samarai, D. Altmann, K. Andeen, T., Anderson, I. Ansseau, G. Anton, C. Arg\"uelles, T. C. Arlen, J. Auffenberg,, S. Axani, H. Bagherpour, X. Bai, A. Balagopal V.

TL;DR
This paper introduces a staged computational approach combining integration and smoothing techniques to analyze small signals in high-statistics neutrino experiments efficiently, reducing the need for extensive simulations.
Contribution
It presents a novel staged method for generating binned event distributions that overcomes computational challenges in neutrino oscillation analysis.
Findings
Reliable analysis results achieved with modest computational resources
Effective handling of limited simulation statistics
Potential application to subtle effects like neutrino mass ordering
Abstract
The current and upcoming generation of Very Large Volume Neutrino Telescopes---collecting unprecedented quantities of neutrino events---can be used to explore subtle effects in oscillation physics, such as (but not restricted to) the neutrino mass ordering. The sensitivity of an experiment to these effects can be estimated from Monte Carlo simulations. With the high number of events that will be collected, there is a trade-off between the computational expense of running such simulations and the inherent statistical uncertainty in the determined values. In such a scenario, it becomes impractical to produce and use adequately-sized sets of simulated events with traditional methods, such as Monte Carlo weighting. In this work we present a staged approach to the generation of binned event distributions in order to overcome these challenges. By combining multiple integration and smoothing…
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