2017
DOI: 10.1039/c6ra28727a
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Wasp-waisted behavior in magnetic hysteresis curves of CoFe2O4 nanopowder at a low temperature: experimental evidence and theoretical approach

Abstract: We theoretically and experimentally investigated wasp-waisted magnetic hysteresis curves at a low temperature for CoFe2O4 nanopowders.

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Cited by 96 publications
(51 citation statements)
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“…3(c)), two spin-orbit doublets Fe 2p 3/2 (709.47 eV for B-sites and 710.55 eV for A-sites) and Fe 2p 1/2 (723.67 eV for B-sites and 725.86 eV for A-sites) were observed for Fe 3+ ions in the ferrite photocatalyst. The peaks at 718.42 eV, 723.67 eV, and 731.87 eV were satellite peaks 24 . The peak position of Fe 2p 3/2 B-sites and Fe 2p 1/2 B-sites coincided with the peak positions of Fe 2+ species 25 , indicating that Fe 2+ /Fe 3+ ions could occupy the octahedral sites.…”
Section: Resultsmentioning
confidence: 97%
“…3(c)), two spin-orbit doublets Fe 2p 3/2 (709.47 eV for B-sites and 710.55 eV for A-sites) and Fe 2p 1/2 (723.67 eV for B-sites and 725.86 eV for A-sites) were observed for Fe 3+ ions in the ferrite photocatalyst. The peaks at 718.42 eV, 723.67 eV, and 731.87 eV were satellite peaks 24 . The peak position of Fe 2p 3/2 B-sites and Fe 2p 1/2 B-sites coincided with the peak positions of Fe 2+ species 25 , indicating that Fe 2+ /Fe 3+ ions could occupy the octahedral sites.…”
Section: Resultsmentioning
confidence: 97%
“…SAED pattern ( Figure S3C, SI) of Fe 0.2 Ni 1.8 OH exhibited diffraction rings of (015), (018), (211) and (113) planes which were also observed in XRD pattern. Figure S4 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 of 711.55 eV, 713.97 eV, 719.18 eV, 725.78 eV, 711.55 eV and 719.18 eV should be related to Fe 3 + , [26,27] while others were related to Fe 2 + . [28,29] The amount of Fe 3 + was about 46.8% ( Figure S4A, SI).…”
Section: Characterization Of Fe X Ni Y Oh/egsimentioning
confidence: 98%
“…As seen, two characteristic peaks of Co 2p3/2 at around 779.2 and 781.5 eV were due to the Co 2+ in B-sites and Co 2+ in A-sites with the corresponding shake-up satellite peaks at 784.9 and 789.7 eV [30][31][32][33]. Similarly, the Fe 2p3/2 spectrum shown in Figure 5e is composed of two characteristic peaks at 709.4 and 710.8 eV, assigned to Fe 3+ at B-sites and Fe 3+ at A-sites along with shake-up satellites at 714.8 and 717.7 eV respectively [50][51][52][53][54][55]. Moreover, fitting peaks of O 1s reveal peaks at 529.6 and 530.8 eV, which coincide with the lattice oxygen and chemisorbed oxygen species, respectively, as displayed in Figure 5f [46,54].…”
Section: Resultsmentioning
confidence: 98%