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Optical conductivity of a two-dimensional metal at the onset of spin-density-wave order

Andrey V. Chubukov, Dmitrii L. Maslov, and Vladimir I. Yudson
Phys. Rev. B 89, 155126 – Published 21 April 2014

Abstract

We consider the optical conductivity of a clean two-dimensional metal near a quantum spin-density-wave transition. Critical magnetic fluctuations are known to destroy fermionic coherence at “hot spots” of the Fermi surface but coherent quasiparticles survive in the rest of the Fermi surface. A large part of the Fermi surface is not really “cold” but rather “lukewarm” in a sense that coherent quasiparticles in that part survive but are strongly renormalized compared to the noninteracting case. We discuss the self-energy of lukewarm fermions and their contribution to the optical conductivity σ(Ω), focusing specifically on scattering off composite bosons made of two critical magnetic fluctuations. Recent study [S. A. Hartnoll et al., Phys. Rev. B 84, 125115 (2011)] found that composite scattering gives the strongest contribution to the self-energy of lukewarm fermions and suggested that this may give rise to a non-Fermi-liquid behavior of the optical conductivity at the lowest frequencies. We show that the most singular term in the conductivity coming from self-energy insertions into the conductivity bubble σ(Ω)ln3Ω/Ω1/3 is canceled out by the vertex-correction and Aslamazov-Larkin diagrams. However, the cancellation does not hold beyond logarithmic accuracy, and the remaining conductivity still diverges as 1/Ω1/3. We further argue that the 1/Ω1/3 behavior holds only at asymptotically low frequencies, well inside the frequency range affected by superconductivity. At larger Ω, up to frequencies above the Fermi energy, σ(Ω) scales as 1/Ω, which is reminiscent of the behavior observed in the superconducting cuprates.

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  • Received 7 January 2014
  • Revised 31 March 2014

DOI:https://doi.org/10.1103/PhysRevB.89.155126

©2014 American Physical Society

Authors & Affiliations

Andrey V. Chubukov1, Dmitrii L. Maslov2, and Vladimir I. Yudson3

  • 1Department of Physics, University of Wisconsin-Madison, 1150 Univ. Ave., Madison, Wisconsin 53706-1390, USA
  • 2Department of Physics, University of Florida, P. O. Box 118440, Gainesville, Florida 32611-8440, USA
  • 3Institute for Spectroscopy, Russian Academy of Sciences, Troitsk, Moscow region, 142190, Russia

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Issue

Vol. 89, Iss. 15 — 15 April 2014

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