2014
DOI: 10.1103/physrevb.90.024307
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Infrared-active optical phonons and magnetic excitations in the hexagonal manganites RMnO3 ( R=Ho , Er, Tm, Yb, and Lu)

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Cited by 20 publications
(17 citation statements)
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“…[1][2][3][4][5][6] Owing to the different ionic radii of R 3+ (R: rare-earth), RMnO 3 can naturally form two different types of structures: one is a perovskite orthorhombic (R ¼ La-Dy) structure [7][8][9] and the other is a hexagonal (R ¼ Ho-Lu, Y, Sc) structure. [10][11][12][13] In particular, the hexagonal structure RMnO 3 can be stabilized into the perovskite orthorhombic phase for small R 3+ (R ¼ Ho-Lu, Y) ion sizes under high temperature and high pressure.…”
Section: Introductionmentioning
confidence: 99%
“…[1][2][3][4][5][6] Owing to the different ionic radii of R 3+ (R: rare-earth), RMnO 3 can naturally form two different types of structures: one is a perovskite orthorhombic (R ¼ La-Dy) structure [7][8][9] and the other is a hexagonal (R ¼ Ho-Lu, Y, Sc) structure. [10][11][12][13] In particular, the hexagonal structure RMnO 3 can be stabilized into the perovskite orthorhombic phase for small R 3+ (R ¼ Ho-Lu, Y) ion sizes under high temperature and high pressure.…”
Section: Introductionmentioning
confidence: 99%
“…Therefore, the general property of asymmetry of anti-Stokes to Stokes intensity ratio of bulk spin wave scattering should not be correlated with the anomalous asymmetry properties of surface spin wave. In recent years, magnetic excitations in magnetoelectric multiferroics have been attracted much research interests [76][77][78][79][80][81][82][83][84][85][86][87][88][89]. The magnetic excitations in multiferroic hexagonal manganites have been systematically investigated through resonance and polarization Raman scattering experiments [81,82,87,89].…”
Section: Anti-stokes To Stokes Intensity Ratiomentioning
confidence: 99%
“…Therefore, longwavelength optical phonons are sensitive to the changes in crystal symmetry and atom positions. The zone center phonon modes in h-RMnO 3 have been studied experimentally (using Raman, THz and IR spectroscopies), as well as theoretically (using shell model and first-principle calculations; Iliev et al, 1997;Litvinchuk et al, 2004;Fukumura et al, 2007;Vermette et al, 2008Vermette et al, , 2010Ghosh et al, 2009;Liu et al, 2012;Toulouse et al, 2014;Goian et al, 2010;Kadlec et al, 2011;Souchkov et al, 2003;Ková cs et al, 2012;Zaghrioui et al, 2008;Basistyy et al, 2014;Rushchanskii & Ležaić, 2012;Varignon et al, 2012).…”
Section: Phononsmentioning
confidence: 99%
“…A recent IR measurement on LuMnO 3 , however, may shed light on this problem, finding 13 E 1 modes out of 14 (Basistyy et al, 2014). Adopting the highest energy mode at 644 cm À1 found in Raman spectroscopy (Vermette et al, 2010), the energies of all the possible E 1 modes were determined.…”
Section: Phononsmentioning
confidence: 99%
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