Quantum Simulation of Collective Neutrino Oscillations using Dicke States
arXiv QuantumArchived Apr 10, 2026✓ Full text saved
arXiv:2604.07452v1 Announce Type: new Abstract: In dense neutrino gases, which exist for instance in supernovae, the flavour states of different neutrinos may become entangled with one another. The theoretical description of such systems may therefore call for simulations on a quantum computer. Existing quantum simulations of simple toy systems are not optimal in the sense that they do not fully exploit the symmetries of the system. Here, we propose a new class of qubit-efficient algorithms base
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Quantum Physics
[Submitted on 8 Apr 2026]
Quantum Simulation of Collective Neutrino Oscillations using Dicke States
Katarina Bleau, Nikolina Ilic, Joachim Kopp, Ushak Rahaman, Xin Yue Yu
In dense neutrino gases, which exist for instance in supernovae, the flavour states of different neutrinos may become entangled with one another. The theoretical description of such systems may therefore call for simulations on a quantum computer. Existing quantum simulations of simple toy systems are not optimal in the sense that they do not fully exploit the symmetries of the system. Here, we propose a new class of qubit-efficient algorithms based on Dicke states and the su(2) spin algebra. We demonstrate the excellent performance of these algorithms both on classical and on quantum hardware.
Comments: 13 pages, 13 figures
Subjects: Quantum Physics (quant-ph); High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics - Phenomenology (hep-ph)
Cite as: arXiv:2604.07452 [quant-ph]
(or arXiv:2604.07452v1 [quant-ph] for this version)
https://doi.org/10.48550/arXiv.2604.07452
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Submission history
From: Katarina Bleau [view email]
[v1] Wed, 8 Apr 2026 18:00:06 UTC (1,549 KB)
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