Mathematical Anatomy of Neutrino Decoherence in Red Turbulence: A Fractional Calculus Approach
Yiwei Bao, Andrea Addazi, Shuai Zha

TL;DR
This paper develops an exact fractional calculus-based framework to describe neutrino decoherence in turbulent supernova matter, linking long-range correlations to anomalous diffusion phenomena.
Contribution
It introduces a novel fractional calculus approach with renormalization techniques to model non-Markovian neutrino decoherence in turbulent environments.
Findings
Exact non-Markovian master equation derived for neutrino density matrix.
Solution expressed via Mittag-Leffler functions, connecting to anomalous diffusion.
Clarifies the role of spectral index and renormalization in decoherence efficiency.
Abstract
We develop an exact framework for neutrino decoherence in power-law correlated turbulent matter, as encountered in core-collapse supernovae. Employing the Nakajima--Zwanzig projection technique, we derive an exact non-Markovian master equation for the neutrino density matrix. For kernels \( K(t) \propto t^{-\nu} \), the spectral index \(\nu\) characterizes the correlation structure: smaller (including negative) values of \(\nu\) correspond to stronger long-range correlations. To treat ultraviolet singularities for \( \nu \geq 1 \) without spoiling the fractional structure, we use a renormalization prescription based on Hadamard finite parts and analytic continuation. The exact Laplace-space solution for the survival probability is obtained. In the high-density matter basis relevant to supernovae, the solution is expressed through Mittag-Leffler functions, establishing a direct link to…
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