Phonons and Spin Excitations in Fe-Based Superconductor Ca10Pt4As8 (Fe1−xPtxAs)10 (x ∼ 0.2)
Author(s) -
Kazuhiko Ikeuchi,
Masatoshi Sato,
Ryoichi Kajimoto,
Yoshiaski Kobayashi,
Kazunori Suzuki,
Masayuki Itoh,
Philippe Bourges,
A. D. Christianson,
Hiroki Nakamura,
Masahiko Machida
Publication year - 2014
Publication title -
proceedings of the international conference on strongly correlated electron systems (sces2019)
Language(s) - English
Resource type - Conference proceedings
DOI - 10.7566/jpscp.3.015043
Subject(s) - condensed matter physics , omega , phonon , physics , inelastic neutron scattering , superconductivity , inelastic scattering , scattering , quantum mechanics , optics
By means of neutron inelastic scattering, magnetic excitations and phonons were measured for a single crystal of slightly overdoped superconductor Ca10Pt4As8(Fe1-xPtxAs)10 (x ~ 0.2) with the transition temperature Tc of ~33 K. Below Tc, magnetic excitation spectra \{chi}"(Q, {\omega}) measured at Q = QM [magnetic {\Gamma} points] are gapped, and in the relatively higher {\omega} region, the \{chi}"(QM, {\omega})-increase was observed with decreasing T, where the maximum of the increase was found at ~18 meV at 3 K (<< Tc). These characteristics are favorable to orbital-fluctuation-mediated superconductivity with the so-called S++symmetry of the order parameter. The energy dependence of {\delta}Q-temperature(T) curve of the magnetic excitations seems to have anomalous behavior in rather wide T region above Tc, {\delta}Q being the width of the Q scan profile. In the phonon measurements, we observed softening of the in-plane TA mode, which corresponds to the elastic constant C66. This softening seems to start at rather high temperature T, as T is lowered. Additionally, anomalous increase in spectral weights of the TO-phonons at around QM in the region 35 < {\omega} < 40 meV was found even above Tc, as T is lowered from ambient T . Because the spectral weights in this {\omega} region mainly correspond to the in-plane motions of Fe atoms and because orbital fluctuations are expected to be strong at around QM, the result may present clues to investigate a possible coupling between the fluctuations of the orbitals and lattice system.
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