Energy scale below which ETH matrix elements become random-matrix-like

In plain words

ETH says the table of a local observable between energy eigenstates looks random, but only for eigenstates very close in energy. How wide that energy window is, and how it shrinks with system size, is not settled.

Precise statement

For a chaotic local Hamiltonian on $L$ sites and a local observable $O$, define $E_{\mathrm{RMT}}(L)$ as the largest energy difference $\omega$ such that off-diagonal elements $O_{mn}$ with $\left|E_m - E_n\right| < \omega$ are statistically invariant under unitary rotations, including the higher-order correlations of full ETH in its free-probability form. Determine $E_{\mathrm{RMT}}(L)$ for systems with and without diffusive conserved quantities; with diffusion the natural guess is $E_{\mathrm{RMT}} \sim \hbar D/L^{2}$. Answer: a scaling form established on at least one chaotic spin chain.

What would settle it

Computation of higher-order matrix-element correlations (free cumulants) in chaotic chains up to $L \sim 22-24$ by full diagonalization, with typicality methods for larger $L$, and a size scaling of the onset energy.

Status in the literature

The free-probability formulation of full ETH (Pappalardi, Foini, Kurchan 2022) supplies the criterion; the size scaling is numerically unsettled.

Revision history

Results

No results have been posted on this problem yet.

Post a result · how results are checked

Sign in to follow or save this problem

See also

Comments (0)

Comments are not records: they are not signed, stamped or logged. How comments work

No comments yet.

Sign in to comment.