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This research demonstrates how collective radiative kinetics in Dicke ladder systems enable the Mpemba effect, where a higher-energy state relaxes faster than a lower-energy one during superradiant emission. The study confirms that this anomalous ordering persists across system sizes up to N=60 and relies fundamentally on cooperative quantum dynamics rather than independent decay processes. These findings advance the theoretical understanding of non-equilibrium relaxation in collectively damped ensembles, which is relevant for optimizing coherence times in future quantum devices.
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Superradiant Mpemba Relaxation in a Dicke Ladder

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arXiv:2609.25359v1 Announce Type: new Abstract: The Mpemba effect occurs when a state initially farther from stationarity overtakes a closer one during relaxation. We show that this anomalous ordering can coexist with superradiant emission in a collectively damped ensemble of two-level systems. In the symmetric Dicke manifold, zero-temperature decay is a population cascade with rates $\Gamma n(N-n+1)$. We construct the sparse family $\rho_A=|\lceil2N/3\rceil\rangle\langle\lceil2N/3\rceil|$ and $\rho_B=(|0\rangle\langle0|+|N\rangle\langle N|)/2$. Although $A$ is initially more energetic and more distant from the stationary ground state, it crosses $B$ in both energy and trace distance because it starts in a more radiative region of the Dicke ladder. Both states develop emission peaks larger than their independent-emitter references. The crossing persists for all examined sizes from $N=6$ to $60$, while the peak intensities show an effective scaling close to $N^2$. The same pair has no crossing under independent decay, identifying collective radiative kinetics as the origin of the effect.

Abstract:The Mpemba effect occurs when a state initially farther from stationarity overtakes a closer one during relaxation. We show that this anomalous ordering can coexist with superradiant emission in a collectively damped ensemble of two-level systems. In the symmetric Dicke manifold, zero-temperature decay is a population cascade with rates $\Gamma n(N-n+1)$. We construct the sparse family $\rho_A=|\lceil2N/3\rceil\rangle\langle\lceil2N/3\rceil|$ and $\rho_B=(|0\rangle\langle0|+|N\rangle\langle N|)/2$. Although $A$ is initially more energetic and more distant from the stationary ground state, it crosses $B$ in both energy and trace distance because it starts in a more radiative region of the Dicke ladder. Both states develop emission peaks larger than their independent-emitter references. The crossing persists for all examined sizes from $N=6$ to $60$, while the peak intensities show an effective scaling close to $N^2$. The same pair has no crossing under independent decay, identifying collective radiative kinetics as the origin of the effect.

arXiv:2609.25359 [quant-ph]

(or arXiv:2609.25359v1 [quant-ph] for this version)

https://doi.org/10.48550/arXiv.2609.25359 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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