Superconducting and charge-density-wave orders in the spin-fermion model: a comparative analysis

TL;DR

This paper compares superconducting and charge-density-wave orders in the spin-fluctuation model for cuprates, showing that charge order can arise beyond conventional approximations and depends on Fermi surface nesting conditions.

Contribution

It demonstrates that anti-nesting does not prevent charge order formation and highlights the importance of going beyond Eliashberg approximation in this context.

Findings

Charge-density-wave order can occur with anti-nesting conditions.

Superconducting and charge-density-wave onset temperatures are comparable in ideal nesting.

Charge order disappears as magnetic correlation length decreases in non-ideal nesting cases.

Abstract

We present comparative analysis of superconducting and charge-density-wave orders in the spin-fluctuation scenario for the cuprates. That spin-fluctuation exchange gives rise to d-wave superconductivity is well known. Several groups recently argued that the same spin-mediated interaction may also account for charge-density-wave order with momenta $(Q,0)$ or $(0,Q)$, detected in underdoped cuprates. This has been questioned on the basis that charge-density-wave channel mixes fermions from both nested and anti-nested regions on the Fermi surface, and fermions in the anti-nested region do not have a natural tendency to form a bound state, even if the interaction is attractive. We show that anti-nesting is not an obstacle for charge order, but to see this one needs to go beyond the conventional Eliashberg approximation. We show that in the prefect nesting/antinesting case, when the velocities of hot fermions are either parallel or antiparallel, the onset temperatures in superconducting and charge-density-wave channels are of comparable strength for any magnetic correlation length $\xi$. The superconducting $T_{\rm sc}$ is larger than $T_{\rm cdw}$, but only numerically. When the velocities of hot fermions are not strictly parallel/antiparallel, $T_{\rm cdw}$ progressively decreases as $\xi$ decreases and vanishes at some critical $\xi$.