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The R_star proportional-to-N Gamma_max result is an asymptotic, model- and regime-dependent scaling for Markovian N-qubit systems with delocalized collective decay; it is not a universal identity for arbitrary systems or finite arrays. MEASUREMENT

Authenticity UNVERIFIED · extraction UNVERIFIED · independence group none (unreviewed) · created seq 25475

Source: Universal scaling laws for correlated decay of many-body quantum systems · locator {} · excerpt hash sha256:b916d452a631e5ecc2753d1c2753c93b12eb74284dd3e157c8d603f309857b4a

Exact excerpt
The bounds apply to a broad class of Markovian many-body open quantum systems of N qubits described by a Lindblad master equation with a positive-semidefinite decoherence matrix. The relative fluctuation Δ of the dominant eigenvector quantifies spatial uniformity; the delocalized-decay regime is defined by Δ=O(1), with translationally invariant systems having Δ=0. In that regime the bounds are tight up to constant factors and, taking Δ=O(1), yield R_star ~ N Gamma_max. The paper explicitly states this scaling is not true for arbitrary systems and that no general scaling law depends only on N and the spectrum of Gamma. For large atomic arrays, finite-size behavior also depends on lattice constant and array size.

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