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scienceFriday, November 6, 2026 at 09:52 AM
Möbius-Ingham protocols achieve single-cycle ground-state cooling in free-fermion and interacting models at strong system-bath coupling

Möbius-Ingham protocols achieve single-cycle ground-state cooling in free-fermion and interacting models at strong system-bath coupling

Strong-coupling Möbius-Ingham cooling protocols prepare ground and thermal states in one cycle for free-fermion and selected interacting systems. Exact scattering reduction yields optimal error-time trade-offs. Numerical tests on Hubbard and spin chains support the claims, but analytic proofs for general interactions are absent.

The work constructs time-dependent ancilla ramps and couplings that operate in the strong-coupling regime, bypassing the slow rates of weak-coupling Lindblad constructions. Exact mapping to resonant excitation transfer allows optimization that maximizes ground-state population transfer while minimizing non-adiabatic excitations within one cycle. Benchmarks on Ising, t-V, and 2D Fermi-Hubbard models show the protocols lie on the Pareto frontier for steady-state error versus cooling time.

Strong coupling enables faster thermalization relevant to near-term quantum simulators and fault-tolerant architectures where weak-coupling assumptions break down. Prior dissipative protocols typically required many cycles or weak baths; the new family trades controlled heating for dramatically reduced physical time. The single-cycle Gibbs-state extension further broadens applicability to finite-temperature preparation.

A central limitation remains the free-fermion exact solvability used for protocol design; interacting cases rely on numerical verification without the same analytic guarantees. Scaling to larger system sizes and experimental noise models will determine whether the Pareto gains survive hardware imperfections. Follow-on experiments on superconducting or trapped-ion platforms could test the predicted exponential suppression within 18 months.

Sources (3)

  • [1]
    Primary Source(https://arxiv.org/abs/2611.07021)
  • [2]
    Supporting Source(https://arxiv.org/abs/2305.08891)
  • [3]
    Supporting Source(https://journals.aps.org/prx/abstract/10.1103/PhysRevX.13.041016)