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<metadata xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/"><dc:title>Anomalous diffusion in the long-range Haken-Strobl-Reineker model</dc:title><dc:creator>Catalano,	A. G.	(Avtor)
	</dc:creator><dc:creator>Mattiotti,	F.	(Avtor)
	</dc:creator><dc:creator>Dubail,	J.	(Avtor)
	</dc:creator><dc:creator>Hagenmüller,	D.	(Avtor)
	</dc:creator><dc:creator>Prosen,	Tomaž	(Avtor)
	</dc:creator><dc:creator>Franchini,	F.	(Avtor)
	</dc:creator><dc:creator>Pupillo,	Guido	(Avtor)
	</dc:creator><dc:subject>quantum mechanics</dc:subject><dc:subject>quantum gases</dc:subject><dc:subject>condensed matter physics</dc:subject><dc:subject>atoms</dc:subject><dc:description>We analyze the propagation of excitons in a $d$-dimensional lattice with power-law hopping $\propto 1/r^{\alpha}$ in the presence of dephasing, described by a generalized Haken-Strobl-Reineker model. We show that in the strong dephasing (quantum Zeno) regime the dynamics is described by a classical master equation for an exclusion process with long jumps. In this limit, we analytically compute the spatial distribution, whose shape changes at a critical value of the decay exponent $\alpha_{cr}=(d+2)/2$. The exciton always diffuses anomalously: a superdiffusive motion is associated to a Lévy stable distribution with long-range algebraic tails for $\alpha \leq \alpha_{cr}$, while for $\alpha &gt; \alpha_{cr}$ the distribution corresponds to a surprising mixed Gaussian profile with long-range algebraic tails, leading to the coexistence of short-range diffusion and long-range Lévy flights. In the many-exciton case, we demonstrate that, starting from a domain-wall exciton profile, algebraic tails appear in the distributions for any $\alpha$, which affects thermalization: the longer the hopping range, the faster equilibrium is reached. Our results are directly relevant to experiments with cold trapped ions, Rydberg atoms, and supramolecular dye aggregates. They provide a way to realize an exclusion process with long jumps experimentally.</dc:description><dc:date>2023</dc:date><dc:date>2024-04-09 10:58:03</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>155629</dc:identifier><dc:identifier>UDK: 53</dc:identifier><dc:identifier>ISSN pri članku: 0031-9007</dc:identifier><dc:identifier>DOI: 10.1103/PhysRevLett.131.053401</dc:identifier><dc:identifier>COBISS_ID: 191422979</dc:identifier><dc:language>sl</dc:language></metadata>
