1974
DOI: 10.1143/jpsj.37.275
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Magnetic Structure of the Cubic Perovskite Type SrMnO3

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Cited by 181 publications
(94 citation statements)
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“…For the interplane distance we consider the two values c/a =1.005, 1.01, which are experimentally determined for the SBMO at different temperatures [14]. For all the above parameters SBMO is safely in an AFM (G-type) insulating state with a band gap of ∼ 0.4 eV with Mn magnetic moments M ∼ 2.6 µ b , in agreement with previous DFT calculations on CaMnO 3 and SrMnO 3 [12,13,21] and experiments on SrMnO 3 [22]. The valence band is predominantly majority-spin Mn t 2g and O 2p characther with strong p−d hybridization while the conduction band is formed by Mn e g orbital and empty minority t 2g states, which is consistent with Mn…”
Section: Pacs Numberssupporting
confidence: 88%
“…For the interplane distance we consider the two values c/a =1.005, 1.01, which are experimentally determined for the SBMO at different temperatures [14]. For all the above parameters SBMO is safely in an AFM (G-type) insulating state with a band gap of ∼ 0.4 eV with Mn magnetic moments M ∼ 2.6 µ b , in agreement with previous DFT calculations on CaMnO 3 and SrMnO 3 [12,13,21] and experiments on SrMnO 3 [22]. The valence band is predominantly majority-spin Mn t 2g and O 2p characther with strong p−d hybridization while the conduction band is formed by Mn e g orbital and empty minority t 2g states, which is consistent with Mn…”
Section: Pacs Numberssupporting
confidence: 88%
“…¦ÔÎË ÊÂÏÇÔÕËÕß Ä ÐÇÏ L Ð AEÄÖØÄÂÎÇÐÕÐÞÌ ÏÇÕÂÎÎ, ÐÂÒÓËÏÇÓ ³Â, ÕÑ Ä ÒÓÇAEÇÎÇ ÒÑÎÐÑÅÑ ÊÂÏÇÜÇÐËâ ÑÐ ÒÇÓÇÌAEÇÕ Ä CaMnO 3 .°Ã àÕË ÏÂÕÇÓËÂΠËÏÇáÕ ÔÕÓÖÍÕÖÓÖ ÒÇÓÑÄÔÍËÕ [32,33]. ³ÕÓÖÍÕÖÓÖ ËAEÇÂÎßÐÑÅÑ ÍÖÃËÚÇÔÍÑÅÑ ÒÇÓÑÄÔÍËÕ ABO 3 ÏÑÉÐÑ ÒÓÇAEÔÕÂÄËÕß ÍÂÍ ÔÑÄÑÍÖÒÐÑÔÕß ÒÓÂÄËÎßÐÞØ ÑÍÕÂàAEÓÑÄ BO 3 , ÍÑÕÑÓÞÇ ÍÂÔÂáÕÔâ AEÓÖÅ AEÓÖÅ ÄÇÓÛËÐÂÏË [34,35].…”
Section: ¬óëôõâîîñåóâ×ëúçôíëç ôäñìôõäâ ïâðåâðëõñä îâðõâðâ°ôunclassified
“…18 The cubic perovskite phase can be kept in a metastable state at 300 K, 19 and has a lattice parameter of 3.805Å. 20 Unstrained cubic SMO shows G-type AFM ordering with 2.6 ± 0.2 µ B magnetic moment per Mn 4+ atom below its Néel temperature (T N ), 21,22 which was reported between 233 K and 260 K, [20][21][22][23] this dispersion being probably caused by the variable oxygen stoichiometry in the samples. 22 Further studies showed how the magnetic ordering strongly depends on the tetragonality (c/a ratio) of the unit cell.…”
mentioning
confidence: 97%