Magnetite Nanocrystals with a High Magnetic Anisotropy Constant due to the Particle Shape


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Abstract

Chemical solution deposition in the presence of arabinogalactan makes it possible to prepare magnetite nanocrystals in the form of square plates with a high aspect ratio (~1/9). The magnetic anisotropy constant of particles is several times higher than that of spherical magnetite particles, which enhances the hysteretic properties with a small particle volume retained.

About the authors

O. A. Bayukov

Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660036

D. A. Velikanov

Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660036

M. N. Volochaev

Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660036

E. V. Cheremiskina

Siberian Federal University

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660041

M. Sh. Bairmani

B.B. Gorodovikov Kalmyk State University; Al-Qasim Green University, College of Biotechnology

Email: stol@iph.krasn.ru
Russian Federation, Elista, 358000; Babylon

P. E. Eroshenko

Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660036

R. S. Iskhakov

Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660036

S. V. Stolyar

Siberian Federal University; Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences; Federal Research Krasnoyarsk Science Center, Siberian Branch of the Russian Academy of Sciences

Author for correspondence.
Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660041; Krasnoyarsk, 660036; Krasnoyarsk, 660036

S. V. Komogortsev

Siberian Federal University; Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences; Federal Research Krasnoyarsk Science Center, Siberian Branch of the Russian Academy of Sciences

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660041; Krasnoyarsk, 660036; Krasnoyarsk, 660036

L. A. Chekanova

Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660036

R. N. Yaroslavtsev

Siberian Federal University; Kirensky Institute of Physics, Subdivision of Federal Krasnoyarsk Science Center,
Siberian Branch of the Russian Academy of Sciences

Email: stol@iph.krasn.ru
Russian Federation, Krasnoyarsk, 660041; Krasnoyarsk, 660036

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