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arXiv:2411.02723 · Physical review. B./Physical review. B

Universal spin screening clouds in local moment phases

Minsoo Kim, Jeongmin Shim, H.-S. Sim, Dong-Hoon Kim

Published Jun 4, 2026• 0 citations
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Abstract

When a local impurity spin interacts with conduction electrons whose density of states (DOS) has a (pseudo)gap or diverges at the Fermi energy, a local moment (LM) phase can be favored over a Kondo phase. Theoretically studying quantum entanglement between the impurity and conduction electrons, we demonstrate that conduction electrons form an LM spin cloud in general LM phases, which corresponds to, but has a fundamental difference from, the Kondo cloud screening the impurity spin in the Kondo phase. The LM cloud algebraically decays over the distance from the impurity when the DOS has a pseudogap or divergence, and exponentially when it has a hard gap. We find an LM cloud length, a single length scale characterizing a universal form of the LM cloud. The findings are supported by both analytic theories and numerical computations.

DOI
10.1103/dxvl-kdlw

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When a local impurity spin interacts with conduction electrons whose density of states (DOS) has a (pseudo)gap or diverges at the Fermi energy, a local moment (LM) phase can be favored over a Kondo phase. Theoretically studying quantum entanglement between the impurity and conduction electrons, we demonstrate that conduction electrons form an LM spin cloud in general LM phases, which corresponds to, but has a fundamental difference from, the Kondo cloud screening the impurity spin in the Kondo phase. The LM cloud algebraically decays over the distance from the impurity when the DOS has a pseudogap or divergence, and exponentially when it has a hard gap. We find an LM cloud length, a single length scale characterizing a universal form of the LM cloud. The findings are supported by both analytic theories and numerical computations.
The screening of an impurity spin by conduction electrons is associated with the formation of a large Kondo screening cloud, of size ξ K . We study the quantum entanglement between a region of size r surrounding the impurity and the rest of the sample (of total size R ) using density matrix renormalization group and analytic methods. The corresponding ‘impurity entanglement entropy’, S imp , is shown to be a universal scaling function of r /ξ K and r / R . We calculate this universal function using Fermi liquid theory in the regime ξ K ≪ r .
A magnetic moment in a metal or in a quantum dot is, at low temperatures, screened by the conduction electrons through the mechanism of the Kondo effect. This gives rise to spin-spin correlations between the magnetic moment and the conduction electrons, which can have a substantial spatial extension. We study this phenomenon, the so-called Kondo cloud, by means of the density matrix renormalization group method for the case of the single-impurity Anderson model. We focus on the question whether the Kondo screening length, typically assumed to be proportional to the inverse Kondo temperature, can be extracted from the spin-spin correlations. For several mechanisms---the gate potential and a magnetic field---which destroy the Kondo effect, we investigate the behavior of the screening cloud induced by these perturbations.
The numerical renormalization group is used to study quantum entanglement in the Kondo impurity model with a density of states ρ(ϵ)∝|ϵ|^{r} (0<r<1/2) that vanishes at the Fermi energy ϵ=0. This nonintegrable model features a Kondo-destruction quantum critical point (QCP) separating a partially screened phase from a local-moment phase. The impurity contribution S_{e}^{imp} to the entanglement entropy between a region of radius R around the magnetic impurity and the rest of the system reveals a length scale R^{*} that distinguishes a region R≪R^{*} of strong critical entanglement from one R≫R^{*} of weak entanglement. Within each phase, S_{e}^{imp} is a universal function of R/R^{*} with a power-law decay for R/R^{*}≫1. The entanglement length R^{*} diverges on approach to the interacting QCP, showing that the critical Kondo screening cloud subsumes the entire system as the impurity becomes maximally entangled with the conduction band. This work has implications for entanglement calculations in other models and for the nature of heavy-fermion quantum criticality.
A magnetic moment in a metal or in a quantum dot is, at low temperatures, screened by the conduction electrons through the mechanism of the Kondo effect. This gives rise to spin-spin correlations between the magnetic moment and the conduction electrons, which can have a substantial spatial extension. We study this phenomenon, the so-called Kondo cloud, by means of the density matrix renormalization group method for the case of the single-impurity Anderson model. We focus on the question whether the Kondo screening length, typically assumed to be proportional to the inverse Kondo temperature, can be extracted from the spin-spin correlations. For several mechanisms -- the gate potential and a magnetic field -- that destroy the Kondo effect, we investigate the behavior of the screening cloud induced by these perturbations.
The existence of a length scale ${\ensuremath{\xi}}_{K}\ensuremath{\sim}1/{T}_{K}$ (with TK{T}_{K}TK​ the Kondo temperature) has long been predicted in quantum impurity systems. At low temperatures $T\ensuremath{\ll}{T}_{K}$, the standard interpretation is that a spin-12\frac{1}{2}21​ impurity is screened by a surrounding ``Kondo cloud'' of spatial extent ${\ensuremath{\xi}}_{K}$. We argue that renormalization group (RG) flow between any two fixed points (FPs) results in a characteristic length scale, observed in real space as a crossover between physical behavior typical of each FP. In the simplest example of the Anderson impurity model, three FPs arise, and we show that ``free orbital,'' ``local moment,'' and ``strong coupling'' regions of space can be identified at zero temperature. These regions are separated by two crossover length scales ${\ensuremath{\xi}}_{\text{LM}}$ and ${\ensuremath{\xi}}_{K}$, with the latter diverging as the Kondo effect is destroyed on increasing temperature through TK{T}_{K}TK​. One implication is that moment formation occurs inside the ``Kondo cloud'', while the screening process itself occurs on flowing to the strong coupling FP at distances $\ensuremath{\sim}{\ensuremath{\xi}}_{K}$. Generic aspects of the real-space physics are exemplified by the two-channel Kondo model, where ${\ensuremath{\xi}}_{K}$ now separates local moment and overscreening clouds.
We analyze the spatial correlation structure of the spin density of an electron gas in the vicinity of an antiferromagnetically coupled Kondo impurity. Our analysis extends to the regime of spin-anisotropic couplings, where there are no quantitative results for spatial correlations in the literature. We use an original and numerically exact method, based on a systematic coherent-state expansion of the ground state of the underlying spin-boson Hamiltonian. It has not yet been applied to the computation of observables that are specific to the fermionic Kondo model. We also present an important technical improvement to the method that obviates the need to discretize modes of the Fermi sea, and allows one to tackle the problem in the thermodynamic limit. As a result, one can obtain excellent spatial resolution over arbitrary length scales, for a relatively low computational cost, a feature that gives the method an advantage over popular techniques such as the numerical and density-matrix renormalization groups. We find that the anisotropic Kondo model shows rich universal scaling behavior in the spatial structure of the entanglement cloud. First, SU(2) spin-symmetry is dynamically restored in a finite domain in the parameter space in the vicinity of the isotropic line, as expected from poor man's scaling. More surprisingly, we are able to obtain in closed analytical form a set of different, yet universal, scaling curves for strong exchange asymmetry, which are parametrized by the longitudinal exchange coupling. Deep inside the cloud, i.e., for distances smaller than the Kondo length, the correlation between the electron spin density and the impurity spin oscillates between ferromagnetic and antiferromagnetic values at the scale of the Fermi wavelength, an effect that is drastically enhanced at strongly anisotropic couplings. Our results also provide further numerical checks and alternative analytical approximations for the Kondo overlaps that were recently computed by Lukyanov, Saleur, Jacobsen, and Vasseur [Phys. Rev. Lett. 114, 080601 (2015)].