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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>Antiferromagnetic Barkhausen noise induced by weak random-field disorder</dc:title><dc:creator>Tadić,	Bosiljka	(Avtor)
	</dc:creator><dc:subject>antiferromagnets</dc:subject><dc:subject>magnetization dynamics</dc:subject><dc:subject>numerical techniques</dc:subject><dc:subject>spin lattice models</dc:subject><dc:subject>Barkhausen noise</dc:subject><dc:description>This study numerically investigates magnetization reversal processes driven by an external magnetic field in three-dimensional antiferromagnetic spin models with weak random-field disorder. Considering an extremely weak disorder and low temperature, we observe a stepwise hysteresis loop and the appearance of short magnetization bursts of a characteristic triangular shape; the number of bursts increases with disorder, indicative of Barkhausen-type noise. These phenomena are attributed to the simultaneous reversal at a given external field of segments composed of spins with identical neighborhoods. A local random field orients one or more spin neighbors, resulting in small, ferromagneticlike clusters distributed throughout the system. As disorder increases, these clusters may merge to form a labyrinthine structure within the antiferromagnetic background, facilitating brief avalanche propagation. The results demonstrate that, compared with familiar random-field ferromagnets, the observed antiferromagnetic Barkhausen noise and the related avalanche sequence have a profoundly different structure, organized into peaks associated with the transition between magnetization plateaus. They exhibit prominent cyclical trends and disorder-dependent multifractal fluctuations, with the singularity spectrum quantifying the degree of disorder. The activity avalanches exhibit scale invariance resembling that recently found in experiments with disordered ferr�⁢magnets and martensites, as well as in quantum Barkhausen noise, which are associated with active geometric regions rather than individual-spin dynamics. The observed scaling behavior is interpreted in terms of self-organized critical dynamics.</dc:description><dc:publisher>American Physical Society</dc:publisher><dc:date>2026</dc:date><dc:date>2026-03-24 14:21:47</dc:date><dc:type>Neznano</dc:type><dc:identifier>28583</dc:identifier><dc:identifier>UDK: 537</dc:identifier><dc:identifier>ISSN pri članku: 2469-9969</dc:identifier><dc:identifier>DOI: 10.1103/ym7r-kzdl</dc:identifier><dc:identifier>COBISS_ID: 272853507</dc:identifier><dc:source>ZDA</dc:source><dc:language>sl</dc:language><dc:rights>©2026 The authors</dc:rights></metadata>
