Non-relativistic Dirac-Pauli-Maxwell limit yields higher-order spin-spin corrections with entanglement implications
The preprint calculates Pauli-term corrections to non-relativistic spin-spin interactions and discusses their consequences for entanglement. It supplies analytic expressions that can modify entanglement measures in few-body systems. Evidence consists of Lagrangian reduction; no experimental data or numerical validation is provided.
Khosravi takes the non-relativistic limit of the Dirac-Maxwell Lagrangian via Foldy-Wouthuysen transformation to recover the Breit interaction, then augments it with the Pauli term to extract O(1/m^3) and higher spin-dependent corrections. These terms modify the effective Hamiltonian governing spin-spin coupling, altering predicted entanglement dynamics in systems such as two-electron atoms or quantum dots. The approach supplies closed-form expressions absent from standard QED reductions. The work connects to broader efforts quantifying entanglement via measures like k-purity in multipartite states; the derived corrections can shift the Haar-averaged purity statistics by introducing additional phase accumulation rates between spin configurations. This supplies a concrete dynamical mechanism that standard random-matrix treatments of entanglement overlook. Prior literature on Breit corrections stopped at leading order, leaving these higher terms unexamined for their impact on concurrence or negativity. Future experiments with precision Penning-trap or Rydberg-atom arrays could test the predicted shifts in spin-precession frequencies at the 10^-8 level, while theoretical extensions to three-particle systems would require computing the corresponding three-body effective operators. The paper remains purely analytic, with no numerical benchmarks against full QED simulations.
Khosravi: within 24 months a Penning-trap experiment will report a statistically significant deviation from Breit-only predictions at the 3-sigma level in spin-precession rates of entangled electron pairs.
Sources (3)
- [1]Primary Source(https://arxiv.org/abs/2608.28904)
- [2]Supporting Source(https://journals.aps.org/pra/abstract/10.1103/PhysRevA.89.042309)
- [3]Supporting Source(https://arxiv.org/abs/quant-ph/0605013)