Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/950
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dc.contributor.authorMilošević, Savaen
dc.contributor.authorSpasojević, Đorđeen
dc.date.accessioned2022-07-12T17:56:39Z-
dc.date.available2022-07-12T17:56:39Z-
dc.date.issued1990-11-15en
dc.identifier.issn0378-4371en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/950-
dc.description.abstractWe prove that the free energy per spin of the nearest-neighbour classical n-vector spin model situated on the Sierpinski gasket (SG) family of fractals tends to the free energy per spin of the same model situated on the standard triangular lattice, when the linear size b of the SG fractal generator tends to infinity. This finding can be regarded as the first step in the analytical investigation of the spin system thermodynamics at the fractal to Euclidean crossover. © 1990.en
dc.relation.ispartofPhysica A: Statistical Mechanics and its Applicationsen
dc.titleFree energy of magnetic model systems at the fractal to Euclidian crossoveren
dc.typeArticleen
dc.identifier.doi10.1016/0378-4371(90)90163-Men
dc.identifier.scopus2-s2.0-44949290299en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/44949290299en
dc.relation.issue2en
dc.relation.volume169en
dc.relation.firstpage139en
dc.relation.lastpage146en
item.openairetypeArticle-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.orcid0000-0003-2177-530X-
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