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arXiv:1602.02087 · Physical review. E

Comment on “Nonlocal quartic interactions and universality classes in perovskite manganites”

Hans Werner Diehl

Published Sep 6, 2016• 0 citations
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Abstract

In a recent paper [Phys. Rev. E 92, 012123 (2015)], a modified $d$-dimensional ${\mathrm{\ensuremath{\Phi}}}^{4}$ model was investigated that differs from the standard one in that the ${\mathrm{\ensuremath{\Phi}}}^{4}$ term was replaced by a nonlocal one with a potential $u(\mathbit{x}\ensuremath{-}{\mathbit{x}}^{\ensuremath{'}})$ that depends on a parameter $\ensuremath{\sigma}$ and decays exponentially as $|\mathbit{x}\ensuremath{-}{\mathbit{x}}^{\ensuremath{'}}|\ensuremath{\rightarrow}\ensuremath{\infty}$ on a scale ${|m|}^{\ensuremath{-}1}<\ensuremath{\infty}$. The authors claim the upper critical dimension of this model to be ${d}_{\ensuremath{\sigma}}=4+2\ensuremath{\sigma}$. Performing a one-loop calculation, they arrive at expansions in powers of ${\ensuremath{\epsilon}}_{\ensuremath{\sigma}}={d}_{\ensuremath{\sigma}}\ensuremath{-}d$ for critical exponents such as $\ensuremath{\eta}$ and related ones to $O({\ensuremath{\epsilon}}_{\ensuremath{\sigma}})$ whose $O({\ensuremath{\epsilon}}_{\ensuremath{\sigma}})$ coefficients depend on $\ensuremath{\sigma}$ and the ratio $w={m}^{2}/{\mathrm{\ensuremath{\Lambda}}}^{2}$, where $\mathrm{\ensuremath{\Lambda}}$ is the uv cutoff. It is shown that these claims are unfounded and based on misjudgments and an ill-conceived renormalization-group calculation.

DOI
10.1103/physreve.94.036101

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Reply to Comment on Nonlocal quartic interactions and universality classes in perovskite manganites

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Comment [arXiv:cond-mat.stat.mech., 1602.02087v1 (2016)] has raised questions claiming that the nonlocal model Hamiltonian presented in [Phys. Rev. E 92, 012123 (2015)] is equivalent to the standard (short-ranged) Φ^4 theory. These claims are based on a low momentum expansion of the interaction vertex that cannot be applied to the vertex factors containing both low and high momenta inside the loop-integrals. Elaborating upon the important steps of the momentum shell decimation scheme, employed in the renormalization-group calculation, we explicitly show the interplay of internal (high) and external (low) momenta determining the loop integrals for self-energy and vertex functions giving rise to corrections (to the bare parameters) different from those of the standard (short-ranged) Φ^4 theory. Employing explicit mathematical arguments, we show that this difference persists when the range of interaction is assumed to be long (short) ranged with respect to the lattice constant (correlation-length), yielding the critical exponents as given in the original paper.

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Critical Exponents from Other Expansions

It is useful to compare the results obtained so far with other approaches to the critical exponents. One is a similar field-theoretic approach based on perturbation expansions of φ 4-theories. But instead of working in D = 4−ε dimensions and continuing the results to ε = 1 to obtain critical exponents in the physical dimension D = 3, perturbation expansions can be derived directly in three dimensions, and studied in the regime of small masses. Fundamentally, this approach is less satisfactory than the previous one since there is no small parameter analogous to ε which permits us to prove the existence of a scaling limit at least for small ε. Another disadvantage is that it is impossible to calculate the expansion coefficients analytically, except for one- and two loop-diagrams. In one respect the three-dimensional approach has, however, an advantage: the power series have long been available up to six loops for ω, η, and ν, and there exist recent results up to seven loops for the critical exponents η and ν. Although numerical expansions are not as esthetic as the exact expansions derived in this book, their increased order leads to a higher accuracy in the critical exponents, as we shall see below in Section 20.4. Another approach is based on high-temperature expansions for lattice models of the O(N)symmetric classical Heisenberg model with the energy of Eq. (1.52). The critical exponents will be derived from such expansions in Section 20.8. Finally we take advantage of the fact that the O(N)-symmetric classical Heisenberg model is exactly solvable in the limit of large N, where it reduces to the spherical model [recall the remark after Eq. (1.69)]. It is therefore possible to expand the φ 4-theory around this limit in powers of 1/N. The results will be compared with those from the perturbation expansions in

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In a recent paper [Phys. Rev. E 92, 012123 (2015)], a modified ddd-dimensional \ensuremathΦ4{\mathrm{\ensuremath{\Phi}}}^{4}\ensuremathΦ4 model was investigated that differs from the standard one in that the \ensuremathΦ4{\mathrm{\ensuremath{\Phi}}}^{4}\ensuremathΦ4 term was replaced by a nonlocal one with a potential u(\mathbitx\ensuremath−\mathbitx\ensuremath′)u(\mathbit{x}\ensuremath{-}{\mathbit{x}}^{\ensuremath{'}})u(\mathbitx\ensuremath−\mathbitx\ensuremath′) that depends on a parameter \ensuremathσ\ensuremath{\sigma}\ensuremathσ and decays exponentially as ∣\mathbitx\ensuremath−\mathbitx\ensuremath′∣\ensuremath→\ensuremath∞|\mathbit{x}\ensuremath{-}{\mathbit{x}}^{\ensuremath{'}}|\ensuremath{\rightarrow}\ensuremath{\infty}∣\mathbitx\ensuremath−\mathbitx\ensuremath′∣\ensuremath→\ensuremath∞ on a scale ∣m∣\ensuremath−1<\ensuremath∞{|m|}^{\ensuremath{-}1}<\ensuremath{\infty}∣m∣\ensuremath−1<\ensuremath∞. The authors claim the upper critical dimension of this model to be d\ensuremathσ=4+2\ensuremathσ{d}_{\ensuremath{\sigma}}=4+2\ensuremath{\sigma}d\ensuremathσ​=4+2\ensuremathσ. Performing a one-loop calculation, they arrive at expansions in powers of \ensuremathϵ\ensuremathσ=d\ensuremathσ\ensuremath−d{\ensuremath{\epsilon}}_{\ensuremath{\sigma}}={d}_{\ensuremath{\sigma}}\ensuremath{-}d\ensuremathϵ\ensuremathσ​=d\ensuremathσ​\ensuremath−d for critical exponents such as \ensuremathη\ensuremath{\eta}\ensuremathη and related ones to O(\ensuremathϵ\ensuremathσ)O({\ensuremath{\epsilon}}_{\ensuremath{\sigma}})O(\ensuremathϵ\ensuremathσ​) whose O(\ensuremathϵ\ensuremathσ)O({\ensuremath{\epsilon}}_{\ensuremath{\sigma}})O(\ensuremathϵ\ensuremathσ​) coefficients depend on \ensuremathσ\ensuremath{\sigma}\ensuremathσ and the ratio w=m2/\ensuremathΛ2w={m}^{2}/{\mathrm{\ensuremath{\Lambda}}}^{2}w=m2/\ensuremathΛ2, where \ensuremathΛ\mathrm{\ensuremath{\Lambda}}\ensuremathΛ is the uv cutoff. It is shown that these claims are unfounded and based on misjudgments and an ill-conceived renormalization-group calculation.
Comment [arXiv:cond-mat.stat.mech., 1602.02087v1 (2016)] has raised questions claiming that the nonlocal model Hamiltonian presented in [Phys. Rev. E 92, 012123 (2015)] is equivalent to the standard (short-ranged) Φ^4 theory. These claims are based on a low momentum expansion of the interaction vertex that cannot be applied to the vertex factors containing both low and high momenta inside the loop-integrals. Elaborating upon the important steps of the momentum shell decimation scheme, employed in the renormalization-group calculation, we explicitly show the interplay of internal (high) and external (low) momenta determining the loop integrals for self-energy and vertex functions giving rise to corrections (to the bare parameters) different from those of the standard (short-ranged) Φ^4 theory. Employing explicit mathematical arguments, we show that this difference persists when the range of interaction is assumed to be long (short) ranged with respect to the lattice constant (correlation-length), yielding the critical exponents as given in the original paper.
It is useful to compare the results obtained so far with other approaches to the critical exponents. One is a similar field-theoretic approach based on perturbation expansions of φ 4-theories. But instead of working in D = 4−ε dimensions and continuing the results to ε = 1 to obtain critical exponents in the physical dimension D = 3, perturbation expansions can be derived directly in three dimensions, and studied in the regime of small masses. Fundamentally, this approach is less satisfactory than the previous one since there is no small parameter analogous to ε which permits us to prove the existence of a scaling limit at least for small ε. Another disadvantage is that it is impossible to calculate the expansion coefficients analytically, except for one- and two loop-diagrams. In one respect the three-dimensional approach has, however, an advantage: the power series have long been available up to six loops for ω, η, and ν, and there exist recent results up to seven loops for the critical exponents η and ν. Although numerical expansions are not as esthetic as the exact expansions derived in this book, their increased order leads to a higher accuracy in the critical exponents, as we shall see below in Section 20.4. Another approach is based on high-temperature expansions for lattice models of the O(N)symmetric classical Heisenberg model with the energy of Eq. (1.52). The critical exponents will be derived from such expansions in Section 20.8. Finally we take advantage of the fact that the O(N)-symmetric classical Heisenberg model is exactly solvable in the limit of large N, where it reduces to the spherical model [recall the remark after Eq. (1.69)]. It is therefore possible to expand the φ 4-theory around this limit in powers of 1/N. The results will be compared with those from the perturbation expansions in
We investigate the nonconserved critical dynamics of a nonlocal model Hamiltonian incorporating screened long-range interactions in the quartic term. Employing dynamic renormalization group analysis at one-loop order, we calculate the dynamic critical exponent $z=2+\ensuremath{\epsilon}{f}_{1}(\ensuremath{\sigma},\ensuremath{\kappa},n)+O({\ensuremath{\epsilon}}^{2})$ and the linewidth exponent $w=\ensuremath{-}\ensuremath{\sigma}+\ensuremath{\epsilon}{f}_{2}(\ensuremath{\sigma},\ensuremath{\kappa},n)+O({\ensuremath{\epsilon}}^{2})$ in the leading order of $\ensuremath{\epsilon}$, where $\ensuremath{\epsilon}=4\ensuremath{-}d+2\ensuremath{\sigma}$, with ddd the space dimension, nnn the number of components in the order parameter, and $\ensuremath{\sigma}$ and $\ensuremath{\kappa}$ the parameters coming from the nonlocal interaction term. The resulting values of linewidth exponent www for a wide range of $\ensuremath{\sigma}$ is found to be in good agreement with the existing experimental estimates from spin relaxation measurements in perovskite manganite samples.
Employing Wilson's renormalization group scheme, we investigate the critical behaviour of a modified Ginzburg-Landau model with a nonlocal mode-coupling interaction in the quartic term. Carrying out the calculations at one-loop order, we obtain the critical exponents in the leading order of , where ρ is an exponent occurring in the nonlocal interaction term and d is the space dimension. Interestingly, the correlation exponent η is found to be non-zero at one-loop order and the expansion corresponds to an expansion about the tricritical mean-field theory in three dimensions, unlike the conventional theory. The ensuing critical exponents are in good agreement with experimental values for samples close to tricriticality. Our analysis indicates that tricriticality is a feature only in three dimensions.