JOURNAL ARTICLE

Spin nematic fluctuations near a spin-density-wave phase

Hiroyuki YamaseRoland Zeyher

Year: 2015 Journal:   New Journal of Physics Vol: 17 (7)Pages: 073030-073030   Publisher: IOP Publishing

Abstract

We study an interacting electronic system exhibiting a spin nematic instability. Using a phenomenological form for the spin fluctuation spectrum near the spin-density-wave (SDW) phase, we compute the spin nematic susceptibility in energy and momentum space as a function of temperature and the magnetic correlation length ξ . The spin nematic instability occurs when ξ reaches a critical value ${\xi }_{\mathrm{cr}}$ , i.e., its transition temperature ${T}_{\mathrm{SN}}$ is always higher than the SDW critical temperature ${T}_{\mathrm{SDW}}$ . In particular, ${\xi }_{\mathrm{cr}}$ decreases monotonically with increasing ${T}_{\mathrm{SN}}$ . Concomitantly, low-energy nematic fluctuations are present in a wider temperature region as ${T}_{\mathrm{SN}}$ becomes higher. Approaching the spin nematic instability, the nematic spectral function at zero momentum exhibits a central peak as a function of energy for a finite temperature and a soft mode at zero temperature. These properties originate from the general feature that the imaginary part of the spin-fluctuation bubble has a term linear in energy and its coefficient is proportional to the square of temperature. Furthermore we find that the nematic spectral function exhibits a diffusive peak around zero momentum and zero energy without clear dispersive features. A possible phase diagram for the spin nematic and SDW transitions is also discussed.

Keywords:

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22
Cited By
1.66
FWCI (Field Weighted Citation Impact)
42
Refs
0.84
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Is in top 1%
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Citation History

Topics

Iron-based superconductors research
Physical Sciences →  Materials Science →  Electronic, Optical and Magnetic Materials
Physics of Superconductivity and Magnetism
Physical Sciences →  Physics and Astronomy →  Condensed Matter Physics
Advanced Condensed Matter Physics
Physical Sciences →  Physics and Astronomy →  Condensed Matter Physics

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