arXiv:1208.3483 · Physical Review B
First-Matsubara-frequency rule in a Fermi liquid. I. Fermionic self-energy
Andrey V. Chubukov, Dmitrii L. Maslov
Abstract
We analyze in detail the fermionic self-energy $\ensuremath{\Sigma}(\ensuremath{\omega},T)$ in a Fermi liquid (FL) at finite temperature $T$ and frequency $\ensuremath{\omega}$. We consider both canonical FLs, i.e., systems in spatial dimension $D>2$, where the leading term in the fermionic self-energy is analytic [the retarded $\mathrm{Im}{\ensuremath{\Sigma}}^{R}(\ensuremath{\omega},T)=C({\ensuremath{\omega}}^{2}+{\ensuremath{\pi}}^{2}{T}^{2})]$, and noncanonical FLs in $1<D<2$, where the leading term in $\mathrm{Im}{\ensuremath{\Sigma}}^{R}(\ensuremath{\omega},T)$ scales as ${T}^{D}$ or ${\ensuremath{\omega}}^{D}$. We relate the ${\ensuremath{\omega}}^{2}+{\ensuremath{\pi}}^{2}{T}^{2}$ form to a special property of the self-energy, ``the first-Matsubara-frequency rule,'' which stipulates that ${\ensuremath{\Sigma}}^{R}(i\ensuremath{\pi}T,T)$ in a canonical FL contains an $\mathcal{O}(T)$ but no ${T}^{2}$ term. We show that in any $D>1$, the next term after $\mathcal{O}(T)$ in ${\ensuremath{\Sigma}}^{R}(i\ensuremath{\pi}T,T)$ is of order ${T}^{D}$ (${T}^{3}\mathrm{ln}T$ in $D=3$). This ${T}^{D}$ term comes from only forward and backward scattering, and is expressed in terms of fully renormalized amplitudes for these processes. The overall prefactor of the ${T}^{D}$ term vanishes in the ``local approximation,'' when the interaction can be approximated by its value for the initial and final fermionic states right on the Fermi surface. The local approximation is justified near a Pomeranchuk instability, even if the vertex corrections are non-negligible. We show that the strength of the first-Matsubara-frequency rule is amplified in the local approximation, where it states that not only the ${T}^{D}$ term vanishes, but also that ${\ensuremath{\Sigma}}^{R}(i\ensuremath{\pi}T,T)$ does not contain any terms beyond $\mathcal{O}(T)$. This rule imposes two constraints on the scaling form of the self-energy: upon replacing $\ensuremath{\omega}$ by $i\ensuremath{\pi}T$, $\mathrm{Im}{\ensuremath{\Sigma}}^{R}(\ensuremath{\omega},T)$ must vanish and $\mathrm{Re}{\ensuremath{\Sigma}}^{R}(\ensuremath{\omega},T)$ must reduce to $\mathcal{O}(T)$. These two constraints should be taken into consideration in extracting scaling forms of ${\ensuremath{\Sigma}}^{R}(\ensuremath{\omega},T)$ from experimental and numerical data.