First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds

Oppeneer, P. M. ; Antonov, V. N. ; Kraft, T. ; Eschrig, H. ; Yaresko, A. N. ; Perlov, A. Ya.

[S.l.] : American Institute of Physics (AIP)
Published 1996
ISSN:
1089-7550
Source:
AIP Digital Archive
Topics:
Physics
Notes:
First-principles band-structure calculations of the magneto-optical Kerr spectra of MnBi and related compounds are reported. We find that band-structure theory, based on density-functional theory in the local spin-density approximation, explains the measured Kerr effect of MnBi very well. A giant Kerr rotation of about −1.75° at 1.8 eV photon energy is given by our ab initio calculations, in accordance with recent experiments. A second peak at 3.4 eV in the Kerr rotation spectrum, however, comes out smaller in our calculations than what was recently measured. It is discussed that this can be due to the Mn–Bi stoichiometry. The microscopic origin of the giant Kerr effect in MnBi is analyzed in detail. We find that the huge Kerr effect in MnBi is caused by the combination of a sizeable magnetic moment of 3.7 μB on manganese, the large spin-orbit coupling of bismuth, and a strong hybridization between the manganese d bands and the bismuth p states. The magneto-optically active states are mainly the p states of Bi. We pay further attention to the experimentally observed unusual temperature dependence of the MnBi Kerr spectra. We show that the observed temperature dependence can be explained by the reduction of the magnetic moment and the average lifetime with increasing temperature. The ab initio calculated Kerr effect in MnBi is furthermore compared to that calculated for the isoelectronic compounds MnAs and MnSb, and that of CrBi, CrTe, and Mn2Bi. © 1996 American Institute of Physics.
Type of Medium:
Electronic Resource
URL:
_version_ 1798289646146289664
autor Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
autorsonst Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
book_url http://dx.doi.org/10.1063/1.362847
datenlieferant nat_lic_papers
hauptsatz hsatz_simple
identnr NLZ218499582
issn 1089-7550
journal_name Journal of Applied Physics
materialart 1
notes First-principles band-structure calculations of the magneto-optical Kerr spectra of MnBi and related compounds are reported. We find that band-structure theory, based on density-functional theory in the local spin-density approximation, explains the measured Kerr effect of MnBi very well. A giant Kerr rotation of about −1.75° at 1.8 eV photon energy is given by our ab initio calculations, in accordance with recent experiments. A second peak at 3.4 eV in the Kerr rotation spectrum, however, comes out smaller in our calculations than what was recently measured. It is discussed that this can be due to the Mn–Bi stoichiometry. The microscopic origin of the giant Kerr effect in MnBi is analyzed in detail. We find that the huge Kerr effect in MnBi is caused by the combination of a sizeable magnetic moment of 3.7 μB on manganese, the large spin-orbit coupling of bismuth, and a strong hybridization between the manganese d bands and the bismuth p states. The magneto-optically active states are mainly the p states of Bi. We pay further attention to the experimentally observed unusual temperature dependence of the MnBi Kerr spectra. We show that the observed temperature dependence can be explained by the reduction of the magnetic moment and the average lifetime with increasing temperature. The ab initio calculated Kerr effect in MnBi is furthermore compared to that calculated for the isoelectronic compounds MnAs and MnSb, and that of CrBi, CrTe, and Mn2Bi. © 1996 American Institute of Physics.
package_name American Institute of Physics (AIP)
publikationsjahr_anzeige 1996
publikationsjahr_facette 1996
publikationsjahr_intervall 8004:1995-1999
publikationsjahr_sort 1996
publikationsort [S.l.]
publisher American Institute of Physics (AIP)
reference 80 (1996), S. 1099-1105
search_space articles
shingle_author_1 Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
shingle_author_2 Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
shingle_author_3 Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
shingle_author_4 Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
shingle_catch_all_1 Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
First-principles band-structure calculations of the magneto-optical Kerr spectra of MnBi and related compounds are reported. We find that band-structure theory, based on density-functional theory in the local spin-density approximation, explains the measured Kerr effect of MnBi very well. A giant Kerr rotation of about −1.75° at 1.8 eV photon energy is given by our ab initio calculations, in accordance with recent experiments. A second peak at 3.4 eV in the Kerr rotation spectrum, however, comes out smaller in our calculations than what was recently measured. It is discussed that this can be due to the Mn–Bi stoichiometry. The microscopic origin of the giant Kerr effect in MnBi is analyzed in detail. We find that the huge Kerr effect in MnBi is caused by the combination of a sizeable magnetic moment of 3.7 μB on manganese, the large spin-orbit coupling of bismuth, and a strong hybridization between the manganese d bands and the bismuth p states. The magneto-optically active states are mainly the p states of Bi. We pay further attention to the experimentally observed unusual temperature dependence of the MnBi Kerr spectra. We show that the observed temperature dependence can be explained by the reduction of the magnetic moment and the average lifetime with increasing temperature. The ab initio calculated Kerr effect in MnBi is furthermore compared to that calculated for the isoelectronic compounds MnAs and MnSb, and that of CrBi, CrTe, and Mn2Bi. © 1996 American Institute of Physics.
1089-7550
10897550
American Institute of Physics (AIP)
shingle_catch_all_2 Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
First-principles band-structure calculations of the magneto-optical Kerr spectra of MnBi and related compounds are reported. We find that band-structure theory, based on density-functional theory in the local spin-density approximation, explains the measured Kerr effect of MnBi very well. A giant Kerr rotation of about −1.75° at 1.8 eV photon energy is given by our ab initio calculations, in accordance with recent experiments. A second peak at 3.4 eV in the Kerr rotation spectrum, however, comes out smaller in our calculations than what was recently measured. It is discussed that this can be due to the Mn–Bi stoichiometry. The microscopic origin of the giant Kerr effect in MnBi is analyzed in detail. We find that the huge Kerr effect in MnBi is caused by the combination of a sizeable magnetic moment of 3.7 μB on manganese, the large spin-orbit coupling of bismuth, and a strong hybridization between the manganese d bands and the bismuth p states. The magneto-optically active states are mainly the p states of Bi. We pay further attention to the experimentally observed unusual temperature dependence of the MnBi Kerr spectra. We show that the observed temperature dependence can be explained by the reduction of the magnetic moment and the average lifetime with increasing temperature. The ab initio calculated Kerr effect in MnBi is furthermore compared to that calculated for the isoelectronic compounds MnAs and MnSb, and that of CrBi, CrTe, and Mn2Bi. © 1996 American Institute of Physics.
1089-7550
10897550
American Institute of Physics (AIP)
shingle_catch_all_3 Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
First-principles band-structure calculations of the magneto-optical Kerr spectra of MnBi and related compounds are reported. We find that band-structure theory, based on density-functional theory in the local spin-density approximation, explains the measured Kerr effect of MnBi very well. A giant Kerr rotation of about −1.75° at 1.8 eV photon energy is given by our ab initio calculations, in accordance with recent experiments. A second peak at 3.4 eV in the Kerr rotation spectrum, however, comes out smaller in our calculations than what was recently measured. It is discussed that this can be due to the Mn–Bi stoichiometry. The microscopic origin of the giant Kerr effect in MnBi is analyzed in detail. We find that the huge Kerr effect in MnBi is caused by the combination of a sizeable magnetic moment of 3.7 μB on manganese, the large spin-orbit coupling of bismuth, and a strong hybridization between the manganese d bands and the bismuth p states. The magneto-optically active states are mainly the p states of Bi. We pay further attention to the experimentally observed unusual temperature dependence of the MnBi Kerr spectra. We show that the observed temperature dependence can be explained by the reduction of the magnetic moment and the average lifetime with increasing temperature. The ab initio calculated Kerr effect in MnBi is furthermore compared to that calculated for the isoelectronic compounds MnAs and MnSb, and that of CrBi, CrTe, and Mn2Bi. © 1996 American Institute of Physics.
1089-7550
10897550
American Institute of Physics (AIP)
shingle_catch_all_4 Oppeneer, P. M.
Antonov, V. N.
Kraft, T.
Eschrig, H.
Yaresko, A. N.
Perlov, A. Ya.
First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
First-principles band-structure calculations of the magneto-optical Kerr spectra of MnBi and related compounds are reported. We find that band-structure theory, based on density-functional theory in the local spin-density approximation, explains the measured Kerr effect of MnBi very well. A giant Kerr rotation of about −1.75° at 1.8 eV photon energy is given by our ab initio calculations, in accordance with recent experiments. A second peak at 3.4 eV in the Kerr rotation spectrum, however, comes out smaller in our calculations than what was recently measured. It is discussed that this can be due to the Mn–Bi stoichiometry. The microscopic origin of the giant Kerr effect in MnBi is analyzed in detail. We find that the huge Kerr effect in MnBi is caused by the combination of a sizeable magnetic moment of 3.7 μB on manganese, the large spin-orbit coupling of bismuth, and a strong hybridization between the manganese d bands and the bismuth p states. The magneto-optically active states are mainly the p states of Bi. We pay further attention to the experimentally observed unusual temperature dependence of the MnBi Kerr spectra. We show that the observed temperature dependence can be explained by the reduction of the magnetic moment and the average lifetime with increasing temperature. The ab initio calculated Kerr effect in MnBi is furthermore compared to that calculated for the isoelectronic compounds MnAs and MnSb, and that of CrBi, CrTe, and Mn2Bi. © 1996 American Institute of Physics.
1089-7550
10897550
American Institute of Physics (AIP)
shingle_title_1 First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
shingle_title_2 First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
shingle_title_3 First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
shingle_title_4 First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
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titel First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
titel_suche First-principles study of the giant magneto-optical Kerr effect in MnBi and related compounds
topic U
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