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Three-flavor supernova neutrino simulation using a hybrid quantum-classical algorithm with qutrits

2026/05/31 by Daniel J. Heimsoth, A. Baha Balantekin, Pooja Siwach · 4 citations
Physics and Astronomy · #astro-ph.HE #astro-ph.SR #hep-ph #nucl-th #quant-ph

paper · pdf · doi:10.1103/8kcg-l79c

13 pages, 6 figures; accepted to Phys. Rev. D

arxiv created 2026/08/05 · arxiv updated 2026/08/07

Abstract

We simulate a self-interacting three-flavor neutrino system within a core-collapse supernova using a hybrid classical-quantum algorithm on a qutrit computer. Based on the Dirac-Frenkel evolution equations, we employ a variation of the quantum-assisted simulator to calculate the system's time evolution operator by performing qutrit Hadamard tests to find expectation values of unitary operators in the Hamiltonian. The time evolution simulation is then done classically. We find that the hybrid algorithm produces results comparable to an exact numerical integration out to times of t ≈ 30 ω0-1 with time step δt = 0.005 ω0-1, where ω0 is the energy scale of the single neutrino vacuum oscillations. We discuss the lessons learned in simulating neutrino systems using this hybrid quantum-classical algorithm, along with the advantages it offers over quantum Trotterization.

Citations