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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>Normal weak eigenstate thermalization</dc:title><dc:creator>Łydżba,	Patrycja	(Avtor)
	</dc:creator><dc:creator>Świętek,	Rafał	(Avtor)
	</dc:creator><dc:creator>Mierzejewski,	Marcin	(Avtor)
	</dc:creator><dc:creator>Rigol,	Marcos	(Avtor)
	</dc:creator><dc:creator>Vidmar,	Lev	(Avtor)
	</dc:creator><dc:subject>quantum chaos</dc:subject><dc:subject>thermalization</dc:subject><dc:subject>localization</dc:subject><dc:description>Eigenstate thermalization has been numerically shown to occur for few-body observables in a wide range of nonintegrable models. For intensive sums of few-body observables, a weaker version of eigenstate thermalization known as weak eigenstate thermalization has been proved to occur in general. Here, we unveil a stricter weak eigenstate thermalization phenomenon that occurs in quadratic models exhibiting quantum chaos in the single-particle sector (quantum-chaotic quadratic models) and in integrable interacting models. In such models, we argue that few-body observables that have a properly defined system-size independent norm are guaranteed to exhibit at least a polynomially vanishing variance (over the entire many-body energy spectrum) of the diagonal matrix elements, a phenomenon we dub normal weak eigenstate thermalization. We prove that normal weak eigenstate thermalization is a consequence of single-particle eigenstate thermalization, i.e., it can be viewed as a manifestation of quantum chaos at the single-particle level. We report numerical evidence of normal weak eigenstate thermalization for quantum-chaotic quadratic models such as the three-dimensional Anderson model in the delocalized regime and the power-law random banded matrix model, as well as for the integrable interacting spin-1/2 XYZ and XXZ models.</dc:description><dc:date>2024</dc:date><dc:date>2024-12-12 12:20:38</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>165854</dc:identifier><dc:identifier>UDK: 538.9</dc:identifier><dc:identifier>ISSN pri članku: 2469-9950</dc:identifier><dc:identifier>DOI: 10.1103/PhysRevB.110.104202</dc:identifier><dc:identifier>COBISS_ID: 217686275</dc:identifier><dc:language>sl</dc:language></metadata>
