Inference of neutrino flavor evolution through data assimilation and neural differential equations

E. Rrapaj, A. Patwardhan, Eve Armstrong, G. Fuller
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引用次数: 2

Abstract

The evolution of neutrino flavor in dense environments such as core-collapse supernovae and binary compact object mergers constitutes an important and unsolved problem. Its solution has potential implications for the dynamics and heavy-element nucleosynthesis in these environments. In this paper, we build upon recent work to explore inference-based techniques for estimation of model parameters and neutrino flavor evolution histories. We combine data assimilation, ordinary differential equation solvers, and neural networks to craft an inference approach tailored for non-linear dynamical systems. Using this architecture, and a simple two-neutrino, two-flavor model, we test various optimization algorithms with the help of four experimental setups. We find that employing this new architecture, together with evolutionary optimization algorithms, accurately captures flavor histories in the four experiments. This work provides more options for extending inference techniques to large numbers of neutrinos.
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基于数据同化和神经微分方程的中微子风味演化推断
中微子风味在致密环境中的演化,如核心坍缩超新星和双紧天体并合,是一个重要的尚未解决的问题。它的解决对这些环境中的动力学和重元素核合成具有潜在的意义。在本文中,我们以最近的工作为基础,探索基于推理的技术来估计模型参数和中微子风味演化历史。我们结合数据同化,常微分方程求解器和神经网络来制作适合非线性动力系统的推理方法。利用这种结构和一个简单的双中微子、双风味模型,我们在四个实验装置的帮助下测试了各种优化算法。我们发现,采用这种新架构,结合进化优化算法,可以准确地捕获四个实验中的风味历史。这项工作为将推理技术扩展到大量中微子提供了更多的选择。
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