Two-beam Multiparticle Many-body simulations of Inhomogeneous FFI
Zoha Laraib, Sherwood Richers
TL;DR
The paper addresses the challenge of modeling nonlinear neutrino flavor evolution in dense astrophysical environments where many-body correlations exceed mean-field descriptions. It introduces a tensor-network framework based on matrix-product states to simulate two-beam, two-flavor fast flavor instabilities with spatial inhomogeneity, angular structure, and flexible boundary conditions, using a Hamiltonian $H[Z(t)]=H_{vac}+H_{SI}[Z(t)]$ and TEBD2 time evolution. The main findings show that many-body entanglement drives decoherence that suppresses FFIs and accelerates flavor equilibration relative to MF, with dynamics profoundly affected by inhomogeneity, boundary conditions, initial configurations, and bond-dimension convergence. This approach provides a scalable, physically faithful platform for benchmarking MB neutrino dynamics and informs astrophysical flavor transport and nucleosynthesis in core-collapse supernovae and neutron-star mergers, with clear pathways to extend to higher dimensions, multiple beams, and non-forward scattering terms. Overall, the work establishes a robust framework for systematically exploring MB effects in dense neutrino systems and for validating quantum simulators targeting entanglement-driven neutrino flavor dynamics.
Abstract
Neutrino flavor evolution in dense astrophysical environments is inherently nonlinear and sensitive to many-body (MB) quantum effects beyond the mean-field (MF) approximation. Existing MB studies are constrained by small system sizes, closed boundaries, and highly idealized symmetry assumptions. We present a unified tensor-network framework that enables simulations of inhomogeneous and anisotropic flavor evolution under conditions relevant to core-collapse supernovae and neutron-star mergers. Within this framework, we examine the effects of inhomogeneity, boundary conditions, and convergence with resolution for multiple neutrino distributions, allowing direct comparison of these setups under one consistent formulation. In our simulations, many-body systems equilibrate earlier than their mean-field counterparts while approaching similar final flavor states. Enlarging the interaction region allows open boundaries to reproduce closed-system behavior, but only when the beams begin superimposed and interact continuously. By contrast, initially separated configurations develop entanglement more slowly, interact over longer times, and equilibrate to a flavor content that differs from that obtained from initially superimposed calculations.
