In many of the diverse reincarnations of the problem of finite density fermions with the interactions mediated by gapless bosonic excitations the propagator of the latter conforms to the general expression
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\ Among the practically important examples of this ’Mother of all NFLs’ are such seemingly disjoint topics as electromagnetic (i.e., Abelian gauge field) skin effect in metals [1] and quark-gluon (non-Abelian) plasmas [2], spin [3] and charge [4] fluctuations in itinerant ferromagnets and Ising quantum nematics, as well as compressible Quantum Hall effect with screened repulsive interactions [5], in all of which situations ξ = 1 and ρ = 2. By contrast, normal skin effect and antiferromagnetic fluctuations in doped Mott insulators are described by ξ = 0, ρ = 2, while compressible Quantum Hall Effect with the unscreened Coulomb interactions corresponds to ξ = 1, ρ = 1.
\ Over several decades much effort has been made towards ascertaining the effects of the interaction (1) on the FL propagator with a finite chemical potential µ
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\ whose Fourier transform in the spacetime domain reads
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\ Previous diagrammatic approaches to this problem sought out to investigate the stability of the first-order self-energy
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\ against higher-order corrections. For a choice of parameters conspiring to yield η = 1 the self-energy (4) acquires an extra factor ln ω.
\ In the early analyses it was argued that the self-energy retains its functional form (4) to all orders in perturbation theory for any finite N, provided that the FS curvature is properly accounted for [6–8]. This conclusion was drawn on the basis of self-consistent Eliashberg-type diagrammatics which, in turn, relies on the generalized Migdal theorem to control vertex corrections.
\ Utilizing the conjectured all-orders result (4) one arrives at the expression
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\ where the self-energy is a power-law function of energy with only a weak momentum dependence. To account for a FS curvature κ the fermion dispersion can be expanded in the vicinity of the (Luttinger) FS traced by the unit normal n
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\ Upon Fourier transforming (5) one finds that at the largest spatial separations the equal-time propagator demonstrates a power-law behavior
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\ Moreover, in the complementary limit of large temporal separations the leading term in the all-orders ’nearfield’ propagator retains its non-interacting form [7]
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\ although the sub-leading corrections bear some nontrivial τ-dependence (see next sections).
\ It has also noted that the algebraic behaviors (7,8) hold due to the presence of a pole in the integration over ǫk in (5) while in its absence a different functional behavior sets in. However, the latter was predicted to occur only in the (arguably, unphysical) limit N → 0.
\ Contrary to the earlier expectations, though, the refined analyses of higher-order corrections to (4) found them to be singular, albeit suppressed by extra powers of 1/N [9]. A number of attempts to get an analytic handle on the higher-order effects has been made [10] but their full bearing on the problem of interest remains unclear.
\ Furthermore, a naive generalization of the above calculations to finite temperatures appears to be problematic as (4) picks up a singular contribution Σ(0) [4]. This problem is particularly severe in those situations where gauge invariance prevents the mediating transverse gauge field A⊥ = A × k/k from developing a thermal mass (no magnetostatic screening in normal metals).
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\ A simpler - yet, questionable - practical recipe for dealing with this harmonic would be to ignore it altogether - as an artifact of the gauge-non-invariant nature of the fermion propagator- or, more formally, have it absorbed into the renormalized chemical potential.
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:::info Author:
(1) D. V. Khveshchenko, Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599.
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:::info This paper is available on arxiv under CC BY 4.0 DEED license.
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