TY - JOUR
T1 - Anisotropic charge distribution induced by spin polarization in La0.6Sr0.4MnO3 thin films studied by X-ray magnetic linear dichroism
AU - Shibata, Goro
AU - Yoshimatsu, Kohei
AU - Ishigami, Keisuke
AU - Harano, Takayuki
AU - Takahashi, Yukio
AU - Sakamoto, Shoya
AU - Nonaka, Yosuke
AU - Kadono, Toshiharu
AU - Furuse, Mitsuho
AU - Fuchino, Schuichiro
AU - Okano, Makoto
AU - Fujihira, Junichi I.
AU - Uchida, Akira
AU - Watanabe, Kazunori
AU - Fujihira, Hideyuki
AU - Fujihira, Seiichi
AU - Tanaka, Arata
AU - Kumigashira, Hiroshi
AU - Koide, Tsuneharu
AU - Fujimori, Atsushi
N1 - Funding Information:
Acknowledgments We would like to thank Kenta Amemiya and Masako Sakamaki for valuable technical support at KEK-PF. We would also like to thank Hiroki Wadati for providing us with information about the XLD studies of LSMO thin films. This work was supported by a Grant-in-Aid for Scientific Research from the JSPS (22224005, 15H02109, 15K17696, and 16H02115). The experiment was done under the approval of the Photon Factory Program Advisory Committee (proposal Nos. 2016S2-005, 2013S2-004, 2016G066, 2014G177, 2012G667, and 2015S2-005). G.S. acknowledges support from Advanced Leading Graduate Course for Photon Science (ALPS) at the University of Tokyo and the JSPS Research Fellowships for Young Scientists (Project No. 26.11615). A.F. is an adjunct member of Center for Spintronics Research Network (CSRN), the University of Tokyo, under Spintronics Research Network of Japan (Spin-RNJ).
Funding Information:
We would like to thank Kenta Amemiya and Masako Sakamaki for valuable technical support at KEK-PF. We would also like to thank Hiroki Wadati for providing us with information about the XLD studies of LSMO thin films. This work was supported by a Grant-in-Aid for Scientific Research from the JSPS (22224005, 15H02109, 15K17696, and 16H02115). The experiment was done under the approval of the Photon Factory Program Advisory Committee (proposal Nos. 2016S2-005, 2013S2-004, 2016G066, 2014G177, 2012G667, and 2015S2-005). G.S. acknowledges support from Advanced Leading Graduate Course for Photon Science (ALPS) at the University of Tokyo and the JSPS Research Fellowships for Young Scientists (Project No. 26.11615). A.F. is an adjunct member of Center for Spintronics Research Network (CSRN), the University of Tokyo, under Spintronics Research Network of Japan (Spin-RNJ).
Publisher Copyright:
©2018 The Physical Society of Japan.
PY - 2018
Y1 - 2018
N2 - Magnetic anisotropy of epitaxially grown thin films is affected by the strain from the substrates due to a combined effect of distorted electronic structure and spin–orbit interaction (SOI). As an inverse process, one expects an anisotropy of the electronic structure induced by magnetization in the presence of SOI. We have studied the charge-density anisotropy induced by magnetization in thin films of the ferromagnetic metal La1−xSrxMnO3 via X-ray magnetic linear dichroism (XMLD). XMLD measurements on thin films with various thicknesses have shown that the XMLD intensity is proportional to the square of the ferromagnetic moment. Using the XMLD sum rule and cluster-model calculation, it has been shown that more Mn 3d electrons are distributed in orbitals elongated along the direction parallel to the spin polarization than in orbitals elongated in the direction perpendicular to it. The cluster-model calculation has shown that the effect of tensile strain from the SrTiO3 substrate on the XMLD spectra is also consistent with the observed XMLD spectral line shapes.
AB - Magnetic anisotropy of epitaxially grown thin films is affected by the strain from the substrates due to a combined effect of distorted electronic structure and spin–orbit interaction (SOI). As an inverse process, one expects an anisotropy of the electronic structure induced by magnetization in the presence of SOI. We have studied the charge-density anisotropy induced by magnetization in thin films of the ferromagnetic metal La1−xSrxMnO3 via X-ray magnetic linear dichroism (XMLD). XMLD measurements on thin films with various thicknesses have shown that the XMLD intensity is proportional to the square of the ferromagnetic moment. Using the XMLD sum rule and cluster-model calculation, it has been shown that more Mn 3d electrons are distributed in orbitals elongated along the direction parallel to the spin polarization than in orbitals elongated in the direction perpendicular to it. The cluster-model calculation has shown that the effect of tensile strain from the SrTiO3 substrate on the XMLD spectra is also consistent with the observed XMLD spectral line shapes.
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U2 - 10.7566/JPSJ.87.114713
DO - 10.7566/JPSJ.87.114713
M3 - Article
AN - SCOPUS:85056247060
SN - 0031-9015
VL - 87
JO - Journal of the Physical Society of Japan
JF - Journal of the Physical Society of Japan
IS - 11
M1 - 114713
ER -