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Physical review. B, Condensed matter

Critical properties of the random hierarchical model

Alba Theumann

Published Apr 1, 1980• 13 citations
Publisher

Abstract

The random hierarchical model is defined by introducing random couplings between spin blocks in Dyson's original hierarchical model for continuous spins. The spin-distribution functions are now site dependent and functions of random parameters that we take to be a quadratic and quartic potential, $r_{l}^{}{}_{}{}^{(m)}$ and $U_{l}^{}{}_{}{}^{(m)}$, respectively, for the mth spin at the $l$ level of the hierarchy. Renormalization-group recursion relations for the cumulant averages are derived in an expansion in ${\ensuremath{\epsilon}}^{\ensuremath{'}}=(2\ensuremath{\sigma}\ensuremath{-}1)\mathrm{ln}(2)$, where $\ensuremath{\sigma}$ is a parameter of the model and a measure of the interaction range. We find that only ${r}_{l}=〈r_{l}^{}{}_{}{}^{(m)}〉$, ${\ensuremath{\Delta}}_{l}=〈{[r_{l}^{}{}_{}{}^{(m)}\ensuremath{-}{r}_{l}]}^{2}〉$, and ${U}_{l}=〈U_{l}^{}{}_{}{}^{(m)}〉$ are relevant physical quantities within the ${\ensuremath{\epsilon}}^{\ensuremath{'}}$ expansion. By solving the equations for ${U}_{l}$ and ${\ensuremath{\Delta}}_{l}$ to $O({\ensuremath{\epsilon}}^{\ensuremath{'}})$ we obtain in general four fixed points of the recursion relations. For $\ensuremath{\sigma}>\frac{1}{2}$, there is no stable fixed point in the physical region $\ensuremath{\Delta}>~0$, $U>~0$; thus the behavior of the system is still open to study. In the particular case of uniform block coupling but random spin distributions, we find a fixed point with ${U}^{*}\ensuremath{\approx}O({|{\ensuremath{\epsilon}}^{\ensuremath{'}}|}^{\frac{1}{2}})$, ${\ensuremath{\Delta}}^{*}\ensuremath{\approx}O({|{\ensuremath{\epsilon}}^{\ensuremath{'}}|}^{\frac{1}{2}})$ for ${\ensuremath{\epsilon}}^{\ensuremath{'}}<0$, but it is unstable.

DOI
10.1103/physrevb.21.2984

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The random hierarchical model is defined by introducing random couplings between spin blocks in Dyson's original hierarchical model for continuous spins. The spin-distribution functions are now site dependent and functions of random parameters that we take to be a quadratic and quartic potential, rl(m)r_{l}^{}{}_{}{}^{(m)}rl​​(m) and Ul(m)U_{l}^{}{}_{}{}^{(m)}Ul​​(m), respectively, for the mth spin at the lll level of the hierarchy. Renormalization-group recursion relations for the cumulant averages are derived in an expansion in \ensuremathϵ\ensuremath′=(2\ensuremathσ\ensuremath−1)ln(2){\ensuremath{\epsilon}}^{\ensuremath{'}}=(2\ensuremath{\sigma}\ensuremath{-}1)\mathrm{ln}(2)\ensuremathϵ\ensuremath′=(2\ensuremathσ\ensuremath−1)ln(2), where \ensuremathσ\ensuremath{\sigma}\ensuremathσ is a parameter of the model and a measure of the interaction range. We find that only rl=〈rl(m)〉{r}_{l}=〈r_{l}^{}{}_{}{}^{(m)}〉rl​=〈rl​​(m)〉, \ensuremathΔl=〈[rl(m)\ensuremath−rl]2〉{\ensuremath{\Delta}}_{l}=〈{[r_{l}^{}{}_{}{}^{(m)}\ensuremath{-}{r}_{l}]}^{2}〉\ensuremathΔl​=〈[rl​​(m)\ensuremath−rl​]2〉, and Ul=〈Ul(m)〉{U}_{l}=〈U_{l}^{}{}_{}{}^{(m)}〉Ul​=〈Ul​​(m)〉 are relevant physical quantities within the \ensuremathϵ\ensuremath′{\ensuremath{\epsilon}}^{\ensuremath{'}}\ensuremathϵ\ensuremath′ expansion. By solving the equations for Ul{U}_{l}Ul​ and \ensuremathΔl{\ensuremath{\Delta}}_{l}\ensuremathΔl​ to O(\ensuremathϵ\ensuremath′)O({\ensuremath{\epsilon}}^{\ensuremath{'}})O(\ensuremathϵ\ensuremath′) we obtain in general four fixed points of the recursion relations. For \ensuremathσ>12\ensuremath{\sigma}>\frac{1}{2}\ensuremathσ>21​, there is no stable fixed point in the physical region \ensuremathΔ> 0\ensuremath{\Delta}>~0\ensuremathΔ> 0, U> 0U>~0U> 0; thus the behavior of the system is still open to study. In the particular case of uniform block coupling but random spin distributions, we find a fixed point with U∗\ensuremath≈O(∣\ensuremathϵ\ensuremath′∣12){U}^{*}\ensuremath{\approx}O({|{\ensuremath{\epsilon}}^{\ensuremath{'}}|}^{\frac{1}{2}})U∗\ensuremath≈O(∣\ensuremathϵ\ensuremath′∣21​), \ensuremathΔ∗\ensuremath≈O(∣\ensuremathϵ\ensuremath′∣12){\ensuremath{\Delta}}^{*}\ensuremath{\approx}O({|{\ensuremath{\epsilon}}^{\ensuremath{'}}|}^{\frac{1}{2}})\ensuremathΔ∗\ensuremath≈O(∣\ensuremathϵ\ensuremath′∣21​) for \ensuremathϵ\ensuremath′<0{\ensuremath{\epsilon}}^{\ensuremath{'}}<0\ensuremathϵ\ensuremath′<0, but it is unstable.
In quenched random-spin systems, the renormalization group can be used to develop recursion relations for the probability distribution for random potentials. Alternatively, recursion relations for the average values of potentials and their higher cumulants can be obtained. In this paper, the above technique is used to study phase transitions in quenched random nnn-component classical spin systems using the $\ensuremath{\epsilon}$ expansion to second order in $\ensuremath{\epsilon}$. It there are long-range correlations in the random potentials (e.g., all potentials along a line are equal), there are no stable physical fixed points within the $\ensuremath{\epsilon}$ expansion. This is interpreted as a smeared transition. If there are no long-range correlations in the random potentials, there is a sharp transition with pure system exponents if the specific-heat exponent ${\ensuremath{\alpha}}^{H}$ of the pure system is negative. If ${\ensuremath{\alpha}}^{H}>0$ and n>1n>1n>1, there is a sharp transition with new exponents $\ensuremath{\eta}=[\frac{(5{n}^{2}\ensuremath{-}8n)}{256{(n\ensuremath{-}1)}^{2}}]{\ensuremath{\epsilon}}^{2}$ and $\ensuremath{\nu}=\frac{1}{2}+[\frac{3n}{32(n\ensuremath{-}1)}]\ensuremath{\epsilon}+[\frac{n(127{n}^{2}\ensuremath{-}572n\ensuremath{-}32)}{4096{(n\ensuremath{-}1)}^{3}}]{\ensuremath{\epsilon}}^{2}$. For n=1n=1n=1, there is no stable fixed point, which is again interpreted as a smeared transition.
Renormalization-group techniques are used to study a model of nnn-coupled mmm-component spin systems, in the limit of large dipole-dipole interactions. As recently shown by Emery, this model describes the critical behavior of a constrained dipolar system in the limit $n\ensuremath{\rightarrow}\ensuremath{\infty}$ and that of a dipolar system with a quenched random perturbation in the limit $n\ensuremath{\rightarrow}0$. In both cases, the unperturbed dipolar fixed point is unstable, and there is a crossover to a new behavior. For the constrained system, this leads to another dipolar fixed point (if $\ensuremath{\alpha}<0$, $\ensuremath{\alpha}$ being the dipolar specific-heat exponent) with the same thermodynamic critical exponents, or to one with renormalized dipolar exponents (if $\ensuremath{\alpha}>0$). These results are different from those of previous "spherical" dipolar models. For the random case, the crossover is either to a new fixed point, with very different exponents, e.g., $2\ensuremath{\nu}\ensuremath{\simeq}1+1.183\ensuremath{\epsilon}$ for $m=d=4\ensuremath{-}\ensuremath{\epsilon}$, or away from all the fixed points found to order $\ensuremath{\epsilon}$. One of the new fixed points in this case has complex eigenvalues of the linearized recursion relations. This is related to the fact that the recursion-relation flow is not of a gradient type for random systems.
For pt.II see ibid., vol.11, p.375 (1978). Exact renormalisation group equations (RGE) are obtained for the d-dimensional n-vector and spin-S Heisenberg versions of Dyson's hierarchical model. In the quantum mechanical case the fixed point and neighbourhood properties of the RGE are shown to be independent of S indicating universality of critical behaviour in spin magnitude. Expansions for critical exponents, analogous to the usual epsilon =4-d expansions, are obtained and the RGE solved numerically to obtain relevant scaling indices. The n to infinity or spherical limit is also discussed and 1/n corrections to critical exponents are calculated to first order in 1/n.
Critical properties of Dyson's hierarchical Ising model in one dimension with 'potential' falling off like r -(1+ sigma ) are examined in the range 0< sigma <1 where a phase transition is known to occur. A new exact renormalisation group recursion relation is derived for a 'dual' spin probability density function. Together with a scaling-type assumption the authors obtain eta =2- sigma and delta =(1+ sigma )/(1- sigma ) for all 0< sigma <1. Independent evidence, however, suggests that delta =3 for 0< sigma <or=1/2, along with other classical critical exponents in this region. In the non-classical region 1/2< sigma <1 accurate numerical values are obtained for the critical exponents nu and gamma and various Delta sigma = sigma -1/2 expansions to third order in Delta sigma .
The critical properties of a random Ising model with long-range isotropic interactions decaying as R -(d+ sigma ) are analysed by using renormalisation group methods in an expansion in epsilon '=2 sigma -d, where d is dimensionality. For epsilon '>O the critical behaviour is described by a stable fixed point O( epsilon 1 2/') in the physical region of parameter space. The crossover to short-range behaviour is analysed and takes place when sigma =2+ epsilon /106, epsilon =4-d>O. There is then a small region O< sigma -2<O( epsilon ) where the system is still dominated by long-range behaviour. The results for d=1 are compared with those obtained previously for the random hierarchical model and it is found that the two models do not show the same critical behaviour in the epsilon ' expansion.
We review recent results concerning the renormalization group (RG) transformation of Dyson's hierarchical model (HM). This model can be seen as an approximation of a scalar field theory on a lattice. We introduce the HM and show that its large group of symmetry simplifies drastically the blockspinning procedure. Several equivalent forms of the recursion formula are presented with unified notations. Rigourous and numerical results concerning the recursion formula are summarized. It is pointed out that the recursion formula of the HM is inequivalent to both Wilson's approximate recursion formula and Polchinski's equation in the local potential approximation (despite the very small difference with the exponents of the latter). We draw a comparison between the RG of the HM and functional RG equations in the local potential approximation. The construction of the linear and nonlinear scaling variables is discussed in an operational way. We describe the calculation of non-universal critical amplitudes in terms of the scaling variables of two fixed points. This question appears as a problem of interpolation between these fixed points. Universal amplitude ratios are calculated. We discuss the large- N limit and the complex singularities of the critical potential calculable in this limit. The interpolation between the HM and more conventional lattice models is presented as a symmetry breaking problem. We briefly introduce models with an approximate supersymmetry. One important goal of this review is to present a configuration space counterpart, suitable for lattice formulations, of functional RG equations formulated in momentum space (often called exact RG equations and abbreviated ERGE).