Direct observable regressor for fermionic shadow spectroscopy on linear-H4 /
STO-3G. Predicts time-evolved expectation values of 120 Majorana observables
(\Gamma_\mu(t) = e^{iH(R)t}\Gamma_\mu e^{-iH(R)t}) as a function of equal
nearest-neighbor bond length (R) and time (t), to feed downstream
shadow-spectroscopy post-processing.
Heads-up. v10 H4 has uneven accuracy across the PES — strong at (R \geq 1.5) Å
but degraded at (R < 1.0) Å where low-lying singlet avoided crossings drive
non-analytic eigenvector rotation. Use this model with awareness of the
short-R regime; see "Known limitations" below.
Short-R (R < 1.0 Å) accuracy is structurally weaker. Linear H4 has a
multi-reference singlet manifold whose eigenvectors rotate near-discontinuously
through avoided crossings as the chain compresses. The current freq_net
correctly tracks energy-gap motion (eigenvalues are smooth), but the trunk
struggles to encode the rapid amplitude rotation that lives in the eigenvector
sector. H2 v10 (single-reference, no avoided crossings) confirms the recipe is
sound on simpler chemistry — the bottleneck is H4-specific.
Resource-experiment guidance: trust v10 H4 most strongly for (R \geq 1.5) Å;
treat short-R predictions as exploratory. A v11 release with adaptive Fourier
bandwidth is in development to address part of this.
Files in this repo
File
Purpose
regressor.pt
torch payload (state_dict + config + R/t grids)
observable_regressor.py
architecture
inference.py
loader
orbital_energies.npz
R-grid + HF orbital-energy table
eval_results.json
per-R held-out metrics (50 geoms)
eval_summary.json
aggregate
history.json
training curves
README.md
this file
Versioning
v10 (current): HF orbital-energy freq_net + dense R-grid + 6×768 trunk.
Mean Pearson 0.834 (R≥1.5 Å strong, R<1.0 Å weak).
Future versions will be pushed as new commits with new tags. Pin via
revision="v10" to preserve loading across architecture changes.