Complexity with constant spectral gap and growing Hamiltonian variation
Determine the complexity of Berry phase estimation when the spectral gap is constant but the Hamiltonian variation bound B_1 grows polynomially with the system size, including constant-precision estimation with an accurate guiding state, and establish whether this regime remains classically tractable or permits BQP-hardness without a small spectral gap.
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Several open problems remain. First, what is the complexity of Berry phase estimation when the spectral gap remains constant but $B_1$ is allowed to grow polynomially in $n$, even at constant precision and with an accurate guiding state? Does this regime remain classically tractable, or can sufficiently large variation revive $\mathsf{BQP}$-hardness without a small gap?
Second, can our classical algorithms be extended to guiding states with smaller overlap? In particular, it remains open whether efficient classical estimation is possible with an arbitrary nonzero constant, or even inverse-polynomial, overlap with the initial ground state.
Third, what is the complexity of constant-precision Berry phase estimation without a guiding state? Previous work establishes $\mathsf{UQMA}\cap\mathsf{co}\text{-}\mathsf{UQMA}$-completeness at inverse-polynomial precision when an energy threshold that separates the ground energy and first excited energy is given. It is essential to clarify how this characterization changes under exact phase quantization or a constant spectral gap.
These results suggest analogous questions for Berry phase estimation. Can Berry phase estimation be performed faster than the complexity of $O(2{n/2})$, and can fine-grained upper and lower bounds characterize how the achievable speedup depends on the phase precision and spectral gap?