An optimization-based approach to calculating neutrino flavor evolution
Eve Armstrong, Amol V. Patwardhan, Lucas Johns, Chad T. Kishimoto,, Henry D.I. Abarbanel, George M. Fuller

TL;DR
This paper explores an optimization-based data assimilation method to model nonlinear neutrino flavor transformation in supernovae, demonstrating its effectiveness in capturing flavor evolution and analyzing parameter sensitivities.
Contribution
It introduces the application of data assimilation techniques to neutrino flavor evolution, offering a model-agnostic approach that handles nonlinear dynamics and parameter estimation.
Findings
D.A. captures key flavor evolution features from endpoint measurements.
Method identifies parameter sensitivities and degeneracies.
Approach works well with a simple steady-state neutrino model.
Abstract
We assess the utility of an optimization-based data assimilation (D.A.) technique for treating the problem of nonlinear neutrino flavor transformation in core collapse supernovae. D.A. uses measurements obtained from a physical system to estimate the state variable evolution and parameter values of the associated model. Formulated as an optimization procedure, D.A. can offer an integration-blind approach to predicting model evolution, which offers an advantage for models that thwart solution via traditional numerical integration techniques. Further, D.A. performs most optimally for models whose equations of motion are nonlinearly coupled. In this exploratory work, we consider a simple steady-state model with two mono-energetic neutrino beams coherently interacting with each other and a background medium. As this model can be solved via numerical integration, we have an independent…
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