Inference solves a boundary-value collision problem, with relevance to neutrino flavor transformation
Eve Armstrong

TL;DR
This paper demonstrates that an inference-based approach can solve a boundary-value collision problem relevant to neutrino flavor transformation in dense astrophysical environments, overcoming limitations of traditional numerical integration methods.
Contribution
It introduces an inference formulation to solve a boundary-value collision problem in neutrino physics, enabling solutions without full initial condition knowledge.
Findings
Inference approach successfully solves the simple collision model.
The method recovers expected physical dynamics.
It offers a new way to handle boundary-value problems in neutrino physics.
Abstract
Understanding neutrino flavor transformation in dense environments such as core-collapse supernovae (CCSN) is critical for inferring nucleosynthesis and interpreting a detected neutrino signal. The role of direction-changing collisions in shaping the neutrino flavor field in these environments is important and poorly understood; it has not been treated self-consistently. There has been progress, via numerical integration, to include the effects of collisions in the dynamics of the neutrino flavor field. While this has led to important insights, integration is limited by its requirement that full initial conditions must be assumed known. On the contrary, feedback from collisions to the neutrino field is a boundary value problem. Numerical integration techniques are poorly equipped to handle that formulation. This paper demonstrates that an inference formulation of the problem can solve a…
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Taxonomy
TopicsNeutrino Physics Research · Particle accelerators and beam dynamics · Pneumonia and Respiratory Infections
