Methodology for simulating collective neutrino oscillations using quantum computing — comparing quantum kinetic frameworks with many-body Hamiltonian calculations, analyzing Trotter error scaling, and designing efficient fermion-to-qubit encodings for astrophysical quantum simulations. arXiv:2606.12404
Scanned 9/11/2026
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---
name: many-body-neutrino-quantum-simulation
description: "Methodology for simulating collective neutrino oscillations using quantum computing — comparing quantum kinetic frameworks with many-body Hamiltonian calculations, analyzing Trotter error scaling, and designing efficient fermion-to-qubit encodings for astrophysical quantum simulations. arXiv:2606.12404"
category: "quantum-physics"
metadata:
arxiv_id: "2606.12404"
authors: "Julien Froustey, Ermal Rrapaj, Yuhao Liu"
published: "2026-06-10"
---
## Context
Collective neutrino oscillations in dense astrophysical environments (supernovae, neutron star mergers) involve many-body quantum correlations that are challenging to simulate classically. This paper compares quantum kinetic frameworks with full many-body Hamiltonian calculations and analyzes the quantum computing resources required.
## Core Methodology
1. **Two-approach comparison**: Quantum kinetic framework (neglects multi-body correlations) vs. simplified many-body calculations (allows entanglement development)
2. **Non-forward scattering**: Incorporated via collision term (kinetic) or full neutrino-neutrino many-body Hamiltonian
3. **Trotter error scaling**: Analyzed for neutrino many-body evolution — found to be on the low end of high-energy physics problems
4. **Resource analysis**: Entangling gate and non-Clifford gate costs quantified relative to quantum chemistry benchmarks
5. **Fermion-to-qubit encoding**: Identified as essential for reducing computational resources
## Implementation Steps
1. Set up neutrino-gas configuration with simplified geometry
2. Implement quantum kinetic equation with collision term for non-forward scattering
3. Construct full many-body Hamiltonian with neutrino-neutrino interactions
4. Compare characteristic timescales and asymptotic behavior between approaches
5. Map to quantum circuits using efficient fermion-to-qubit encoding (Jordan-Wigner or Bravyi-Kitaev)
6. Analyze Trotter error scaling for time evolution
7. Count entangling and non-Clifford gate requirements
## Pitfalls
- **Truncated vs. full Hamiltonian**: Full Hamiltonian requires significantly more resources than truncated version
- **Encoding choice**: Fermion-to-qubit encoding critically impacts resource requirements — choose based on interaction locality
- **Timescale mismatch**: Kinetic and many-body approaches show different characteristic timescales
## Verification
- Verify Trotter error scales correctly with time step size
- Compare asymptotic behavior between kinetic and many-body approaches
- Validate gate counts against known quantum chemistry benchmarks
## Activation
many-body neutrino, quantum kinetic, neutrino oscillation, fermion-to-qubit encoding, Trotter error scaling, astrophysical quantum simulation

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