Miroslav Abrashev

Prof. Dr. Miroslav Abrashev

Faculty of Physics, Sofia University
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Research Focus & Metrics

Academic Career Length

37Years (1990-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 February 1998 in Physical Review B
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Journal Article
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MIM. N. Iliev
M. N. Iliev
Miroslav AbrashevMiroslav Abrashev
Miroslav Abrashev
HLH.-G. Lee
H.-G. Lee
Valentin Nikolov PopovValentin Nikolov Popov
Valentin Nikolov Popov
YSY. Y. Sun
Y. Y. Sun
CCC. W. Chu
C. W. Chu
The Raman-active phonons in orthorhombic perovskitelike YMnO3 and LaMnO3 were studied by measuring Raman spectra in various scattering configurations. The experimental Raman line wave numbers and the expected shapes for the phonon modes were compared to those reported for other perovskitelike compounds with the Pnma structure and to the results of lattice dynamical calculations. The observed Raman lines in the spectra of YMnO3 and LaMnO3 were assigned to definite atomic motions. The much larger linewidths and strong variation of the Raman spectra with increasing laser power in the case of LaMnO3 provide evidence for a structural instability that may result in a phase transition under laser annealing.

1 February 1999 in Physical Review B
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Miroslav AbrashevMiroslav Abrashev
Miroslav Abrashev
ALA. P. Litvinchuk
A. P. Litvinchuk
MIM. N. Iliev
M. N. Iliev
RMR. L. Meng
R. L. Meng
Valentin Nikolov PopovValentin Nikolov Popov
Valentin Nikolov Popov
CTC. Thomsen
C. Thomsen
The Raman and infrared phonons of isostructural rhombohedral LaMnO3 and LaAlO3 are studied at room temperature. The experimental spectra are compared with the prediction of lattice-dynamical calculations and the lines observed are assigned to definite atomic vibrations. It is shown that the Raman mode of A1g symmetry in LaAlO3 and LaMnO3 (at 123 cm−1 and 236 cm−1, respectively) involves atomic motions that cause the rhombohedral distortion, i.e., it is a “soft” mode, and its position could be used as a measure of the degree of the distortion. It is also argued that the broad Raman bands in the high-frequency range of LaMnO3 are not proper modes of the rhombohedral R3¯c structure, but are rather induced by the dynamic Jahn-Teller effect.

16 February 2006 in Physical Review B
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MIM. N. Iliev
M. N. Iliev
Miroslav AbrashevMiroslav Abrashev
Miroslav Abrashev
JLJ. Laverdière
J. Laverdière
SJS. Jandl
S. Jandl
MGM. M. Gospodinov
M. M. Gospodinov
YSY.-Y. Sun
Y.-Y. Sun
The polarized Raman spectra of orthorhombic RMnO3 series (R=La,Pr,Nd,Sm,Eu,Gd,Tb,Dy,Ho,Y) were studied at room temperature. The variation of phonon frequencies with R ionic radius rR as a whole confirms the commonly accepted Raman line assignments with two noticeable exceptions: (1) with decreasing rR the stretching Ag(1) and bending Ag(3) modes strongly mix for R=Sm to Tb, while for further decrease or rR (R=Dy,Ho,Y) the Ag(3) mode is observed at higher frequency than Ag(1) mode; (2) similar distortion-dependent mode mixing takes place for the rotational Ag(2) and O1(x) [Ag(7)] modes. The mode mixing is particularly strong for the RMnO3 compounds with rR values close to the transition from A type to incommensurate sinusoidal antiferromagnetic ordering at low temperatures. The frequency of rotational Ag(2) and Ag(4) modes scales to the angles of MnO6 [101] and [010] rotations, respectively, and could be used as a measure of their value.

1 July 2010 in Journal of Magnetism and Magnetic Materials
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Journal Article
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LSL. Slavov
L. Slavov
Miroslav AbrashevMiroslav Abrashev
Miroslav Abrashev
TMT. Merodiiska
T. Merodiiska
CGCh. Gelev
Ch. Gelev
RVR.E. Vandenberghe
R.E. Vandenberghe
INI. Nedkov
I. Nedkov

30 March 2007 in Physical Review B
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Journal Article
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MIM. N. Iliev
M. N. Iliev
Miroslav AbrashevMiroslav Abrashev
Miroslav Abrashev
ALA. P. Litvinchuk
A. P. Litvinchuk
VHV. G. Hadjiev
V. G. Hadjiev
HGH. Guo
H. Guo
AGA. Gupta
A. Gupta
The Raman spectra of epitaxial thin films of La2CoMnO6 on (001)-oriented SrTiO3 substrates have been measured in several exact scattering configuration between 12 and 890K. The polarization dependence of the spectra provide clear evidence for ordered P121∕n1 structure, differing from its parent Fm3¯m structure by the presence of rotational distortions. The correlation between the phonon modes in Fm3¯m, R3¯, and P121∕n1 phases is analyzed and the corresponding types of atomic motions as well as their expected frequency range are determined by comparison to the predictions of lattice dynamical calculations. The ferromagnetic ordering and spin-phonon coupling below TC result in softening of some of the phonon modes. The evolution of the Raman spectra at high temperatures shows no indication for P121∕n1–R3¯ transition up to 800K.

1 August 1997 in Physical Review B
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Journal Article
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MIM. N. Iliev
M. N. Iliev
HLH.-G. Lee
H.-G. Lee
Valentin Nikolov PopovValentin Nikolov Popov
Valentin Nikolov Popov
Miroslav AbrashevMiroslav Abrashev
Miroslav Abrashev
AHA. Hamed
A. Hamed
CCC. W. Chu
C. W. Chu
Raman-scattering and far-infrared-transmission spectra of hexagonal YMnO3 (space group P63cm) are reported and discussed. In the Raman spectra measured in several exact scattering configurations, lines of A1 (at 148, 190, 257, ∼300, 433, 459, and 681 cm−1), E1 (at 376, 408, and 632 cm−1), and E2 (at 135, and ∼215 cm−1), symmetries have been observed. Maxima in the infrared absorption have been found at 211, 238, 265, 281, 308, 398, 428, 457, 491, 596, and 612 cm−1. An assignment of the phonon lines to definite atomic vibrations has been made on the basis of their symmetries in close comparison with results of lattice-dynamical calculations for YMnO3 in its ferroelectric (P63cm, Z=6) and high-temperature paraelectric (P63/mmc, Z=2) phases.