aiqbench analysis
This study establishes a universal upper bound for fermionic non-Gaussianity, identifying it as a critical resource for universal quantum computation within many-body systems. By analyzing evolution under the Sachdev-Ye-Kitaev Hamiltonian, the authors reveal a first-order phase transition in magic density that occurs independently of thermal free energy changes. These findings provide fundamental theoretical limits on how interaction-generated resources scale in large quantum systems.
Universal Bound and Phase Transition in Many-Body Fermionic Non-Gaussianity
arXiv:2610.02075v1 Announce Type: new Abstract: Fermionic non-Gaussianity is a resource for universal quantum computation that can be generated by interactions in quantum many-body systems. Using the magic R\'enyi entropy (MRE) as a measure of non-Gaussianity, we derive its universal upper bound and Haar mean, proving that typical Haar-random states attain the maximal MRE density of $\ln(4/3)$ per Majorana in the large-system limit. We also show that the MRE can differ extensively between states with identical covariance matrices. To investigate how non-Gaussianity grows toward this maximal density, we evolve a Gaussian state in imaginary and real time under the Sachdev-Ye-Kitaev Hamiltonian. By varying the imaginary- and real-time durations, we identify a first-order transition marked by a kink in the MRE density and spontaneous breaking of the permutation symmetry among the four copies used to evaluate the MRE. This transition represents a qualitative change in the non-Gaussianity of the state that is not reflected in the thermal free energy.
Abstract:Fermionic non-Gaussianity is a resource for universal quantum computation that can be generated by interactions in quantum many-body systems. Using the magic Rényi entropy (MRE) as a measure of non-Gaussianity, we derive its universal upper bound and Haar mean, proving that typical Haar-random states attain the maximal MRE density of $\ln(4/3)$ per Majorana in the large-system limit. We also show that the MRE can differ extensively between states with identical covariance matrices. To investigate how non-Gaussianity grows toward this maximal density, we evolve a Gaussian state in imaginary and real time under the Sachdev-Ye-Kitaev Hamiltonian. By varying the imaginary- and real-time durations, we identify a first-order transition marked by a kink in the MRE density and spontaneous breaking of the permutation symmetry among the four copies used to evaluate the MRE. This transition represents a qualitative change in the non-Gaussianity of the state that is not reflected in the thermal free energy.
Quantum Physics (quant-ph); Statistical Mechanics (cond-mat.stat-mech); Strongly Correlated Electrons (cond-mat.str-el)
arXiv:2610.02075 [quant-ph]
(or arXiv:2610.02075v1 [quant-ph] for this version)
https://doi.org/10.48550/arXiv.2610.02075 Focus to learn more arXiv-issued DOI via DataCite (pending registration)
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