Insight into electronic and magnetic properties of Ba2NiOsO6 double perovskite: A Monte Carlo study and a comparative investigation between TB-mBJ and GGA plus U
被引:12
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作者:
Kerrai, H.
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Moulay Ismail Univ, Fac Sci, Unite Associee CNRST URAC 08, LP2MS, Meknes 11201, MoroccoMoulay Ismail Univ, Fac Sci, Unite Associee CNRST URAC 08, LP2MS, Meknes 11201, Morocco
Kerrai, H.
[1
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Zaim, N.
[1
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Kerouad, M.
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Moulay Ismail Univ, Fac Sci, Unite Associee CNRST URAC 08, LP2MS, Meknes 11201, MoroccoMoulay Ismail Univ, Fac Sci, Unite Associee CNRST URAC 08, LP2MS, Meknes 11201, Morocco
Kerouad, M.
[1
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Zaim, A.
[1
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机构:
[1] Moulay Ismail Univ, Fac Sci, Unite Associee CNRST URAC 08, LP2MS, Meknes 11201, Morocco
Monte Carlo study;
Double perovskite;
Hysteresis loops;
DFT;
Reentrant phenomenon;
Magnetic properties;
LOCALIZATION;
D O I:
10.1016/j.commatsci.2024.113404
中图分类号:
T [工业技术];
学科分类号:
08 ;
摘要:
The structural, electronic, and magnetic properties of the Ba2NiOsO6 double perovskite were comprehensively studied using density functional theory (DFT) and Monte Carlo simulations. Based on DFT calculations, we found that the double perovskite is stable in the ferromagnetic phase. The compound exhibited thermodynamic stability, confirmed by its negative formation energy and phonon spectrum. The electronic and magnetic properties were analyzed using various approximations, including the Generalized Gradient Approximation (GGA), modified Becke-Johnson approximation (mBJ), and Hubbard correction (GGA+U). The electronic profile indicated a metallic nature with GGA and a half-metallic nature with GGA+U and mBJ. The total magnetic moment was approximately 4 mu B across all approximations. The Monte Carlo simulations revealed intriguing phenomena, such as a tri-critical point, second-order and first-order phase transitions, a reentrant phenomenon, and both simple and double hysteresis loops.
机构:
Mohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, Morocco
Mohamed V Univ, Fac Sci, LPHE Modeling & Simulat, Rabat, MoroccoMohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, Morocco
Ahmed, S. Sidi
Boujnah, M.
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Mohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, MoroccoMohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, Morocco
Boujnah, M.
Bahmad, L.
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Mohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, MoroccoMohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, Morocco
Bahmad, L.
Benyoussef, A.
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Mohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, MoroccoMohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, Morocco
Benyoussef, A.
El Kenz, A.
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Mohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, MoroccoMohamed V Univ, Fac Sci, Phys Dept, Lab Magntism & Phys High Energies, Rabat, Morocco