TY - JOUR
T1 - Ultrafast optical excitation of coherent magnons in antiferromagnetic NiO
AU - Tzschaschel, Christian
AU - Otani, Kensuke
AU - Iida, Ryugo
AU - Shimura, Tsutomu
AU - Ueda, Hiroaki
AU - Günther, Stefan
AU - Fiebig, Manfred
AU - Satoh, Takuya
N1 - Funding Information:
T.S. was supported by KAKENHI (Grants No. 15H05454 and No. 26103004), JST-PRESTO, JSPS Core-to-Core Program, A. Advanced Research Networks, and thanks ETH Zurich for hosting him on a guest Professorship. C.T. and M.F. acknowledge support from the SNSF project 200021/147080 and by FAST, a division of the SNSF NCCR MUST.
Publisher Copyright:
© 2017 American Physical Society.
PY - 2017/5/5
Y1 - 2017/5/5
N2 - In experiment and theory, we resolve the mechanism of ultrafast optical magnon excitation in antiferromagnetic NiO. We employ time-resolved optical two-color pump-probe measurements to study the coherent nonthermal spin dynamics. Optical pumping and probing with linearly and circularly polarized light along the optic axis of the NiO crystal scrutinizes the mechanism behind the ultrafast magnon excitation. A phenomenological symmetry-based theory links these experimental results to expressions for the optically induced magnetization via the inverse Faraday effect and the inverse Cotton-Mouton effect. We obtain striking agreement between experiment and theory that, furthermore, allows us to extract information about the spin domain distribution. We also find that in NiO the energy transfer into the magnon mode via the inverse Cotton-Mouton effect is about three orders of magnitude more efficient than via the inverse Faraday effect.
AB - In experiment and theory, we resolve the mechanism of ultrafast optical magnon excitation in antiferromagnetic NiO. We employ time-resolved optical two-color pump-probe measurements to study the coherent nonthermal spin dynamics. Optical pumping and probing with linearly and circularly polarized light along the optic axis of the NiO crystal scrutinizes the mechanism behind the ultrafast magnon excitation. A phenomenological symmetry-based theory links these experimental results to expressions for the optically induced magnetization via the inverse Faraday effect and the inverse Cotton-Mouton effect. We obtain striking agreement between experiment and theory that, furthermore, allows us to extract information about the spin domain distribution. We also find that in NiO the energy transfer into the magnon mode via the inverse Cotton-Mouton effect is about three orders of magnitude more efficient than via the inverse Faraday effect.
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U2 - 10.1103/PhysRevB.95.174407
DO - 10.1103/PhysRevB.95.174407
M3 - Article
AN - SCOPUS:85024388096
SN - 2469-9950
VL - 95
JO - Physical Review B
JF - Physical Review B
IS - 17
M1 - 174407
ER -