Critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented)

The critical exponents of the second-order ferromagnetic-paramagnetic phase transition of (Formula presented) (Formula presented) compounds are obtained. The results (Formula presented) (Formula presented) and (Formula presented) are qualitatively different than those reported in the literature for...

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Publicado: 1999
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_10980121_v59_n1_p123_Mira
http://hdl.handle.net/20.500.12110/paper_10980121_v59_n1_p123_Mira
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spelling paper:paper_10980121_v59_n1_p123_Mira2025-07-30T18:43:04Z Critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented) The critical exponents of the second-order ferromagnetic-paramagnetic phase transition of (Formula presented) (Formula presented) compounds are obtained. The results (Formula presented) (Formula presented) and (Formula presented) are qualitatively different than those reported in the literature for parent manganites, and are taken as the indication of the absence of long-range interactions below the Curie point. Electronic phase segregation in hole-rich ferromagnetic and hole-poor (Formula presented)-like regions is supposed to explain the observations. The hole-poor regions would dilute the magnetic lattice and prevent the occurrence of long-range order. Also, a spin transition of the (Formula presented) ions at (Formula presented) or the hole-poor regions (acting equivalently to missed spin clusters in amorphous ferromagnets) could be the reason for the high β value in the framework of a Heisenberg model. © 1999 The American Physical Society. 1999 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_10980121_v59_n1_p123_Mira http://hdl.handle.net/20.500.12110/paper_10980121_v59_n1_p123_Mira
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description The critical exponents of the second-order ferromagnetic-paramagnetic phase transition of (Formula presented) (Formula presented) compounds are obtained. The results (Formula presented) (Formula presented) and (Formula presented) are qualitatively different than those reported in the literature for parent manganites, and are taken as the indication of the absence of long-range interactions below the Curie point. Electronic phase segregation in hole-rich ferromagnetic and hole-poor (Formula presented)-like regions is supposed to explain the observations. The hole-poor regions would dilute the magnetic lattice and prevent the occurrence of long-range order. Also, a spin transition of the (Formula presented) ions at (Formula presented) or the hole-poor regions (acting equivalently to missed spin clusters in amorphous ferromagnets) could be the reason for the high β value in the framework of a Heisenberg model. © 1999 The American Physical Society.
title Critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented)
spellingShingle Critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented)
title_short Critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented)
title_full Critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented)
title_fullStr Critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented)
title_full_unstemmed Critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented)
title_sort critical exponents of the ferromagnetic-paramagnetic phase transition of (formula presented) (formula presented)
publishDate 1999
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_10980121_v59_n1_p123_Mira
http://hdl.handle.net/20.500.12110/paper_10980121_v59_n1_p123_Mira
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