Ab Initio Calculations of New Full Heusler Alloys Rh{sub 2}ZrX (X = Al, Ga, In, Si, Ge, Sn)

In recent years, Heusler alloys have attracted extensive attention because of their usefulness in spintronic devices. In this paper, the structural, electronic, and magnetic properties of full Heusler alloys Rh{sub 2}ZrX (X = Al, Ga, In, Si, Ge, Sn) have been studied using Quantum Espresso software...

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Bibliographic Details
Published inJournal of superconductivity and novel magnetism Vol. 32; no. 8
Main Authors Abadi, Ahmad Asadi Mohammad, Forozani, Ghasem, Baizaee, Seyyed Mahdy, Gharaati, Abdolrasoul
Format Journal Article
LanguageEnglish
Published United States 15.08.2019
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Summary:In recent years, Heusler alloys have attracted extensive attention because of their usefulness in spintronic devices. In this paper, the structural, electronic, and magnetic properties of full Heusler alloys Rh{sub 2}ZrX (X = Al, Ga, In, Si, Ge, Sn) have been studied using Quantum Espresso software package based on density functional theory. Calculations have been done by GGA and GGA+U methods. The investigations on the structural properties of the alloys showed that the Rh{sub 2}ZrSi alloy had the most stable structure (E{sub coh} = − 1.807 eV) among the six compounds reviewed. The results of GGA calculation on electronic properties of Rh{sub 2}ZrX alloys show that while the Rh{sub 2}ZrX (X = Al, Ga, In) alloys had metallic nature due to overlapping between conduction and valance band at Fermi level for both spin directions, the Rh{sub 2}ZrX (X = Si, Ge, Sn) alloys had half-metal characteristic. Also, Rh{sub 2}ZrSi and Rh{sub 2}ZrGe alloys had 100% spin polarization. By studying the magnetic properties, it was found that the Rh{sub 2}ZrAl and Rh{sub 2}ZrSi alloys were antiferromagnetic, while the Rh{sub 2}ZrGa, Rh{sub 2}ZrIn, Rh{sub 2}ZrGe, and Rh{sub 2}ZrSn alloys were ferromagnetic materials. Also, the total spin magnetic moment of alloys was found in accordance with the Slater-Pauling rule. The results obtained using GGA+U calculation are slightly different from the results of GGA calculation.
ISSN:1557-1939
1557-1947