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Dynamic Scaling and Critical Slowing Down

Near a continuous transition, the equilibrium correlation length diverges and the longest relaxation time scales as τrelξz\tau_{\mathrm{rel}}\sim\xi^z. The dynamic exponent zz depends on the slow-variable dynamics, not only on the static fixed point. For a finite-rate ramp, evolution freezes out when the relaxation time becomes comparable to the time remaining to the critical point.

Required background. Use critical exponents and hyperscaling and correlations, susceptibilities, and correlation lengths.

Helpful background. Dynamic universality classes determine which zz should be used.

Let the reduced control parameter be ϵ=(ggc)/gc\epsilon=(g-g_c)/g_c. In the scaling regime,

ξ=ξ0ϵν,τrel=τ0(ξξ0)z=τ0ϵνz.\xi=\xi_0|\epsilon|^{-\nu}, \qquad \tau_{\mathrm{rel}}=\tau_0\left(\frac{\xi}{\xi_0}\right)^z =\tau_0|\epsilon|^{-\nu z}.

A two-point dynamic structure factor has the scaling form

S(k,ω;ϵ)=k2+ηzΦ ⁣(ωkz,kξ),S(k,\omega;\epsilon) =k^{-2+\eta-z}\, \Phi\!\left(\frac{\omega}{k^z},k\xi\right),

up to operator normalization and additional scaling fields. This form assumes one dominant relaxation scale. Propagating and diffusive modes, multiple conserved fields, or dangerously irrelevant variables can require several frequency variables or crossover exponents.

Critical slowing down means local equilibration fails first at the largest wavelengths. Finite size cuts off ξ\xi at LL, giving τLLz\tau_L\sim L^z. A measured saturation can therefore be a box effect rather than a microscopic relaxation time.

The last box of the schematic is a testable scaling claim, not an automatic consequence of writing a Langevin equation. The dynamic exponent and scaling function depend on the complete set of slow variables, conservation laws, and reversible couplings.

Flow from declared slow fields and noise calculus through a Langevin equation, Fokker–Planck probability current, and an MSRJD response action to dynamic scaling or aging tests; a dashed equilibrium branch says detailed balance and fluctuation–dissipation must be derived rather than assumed.

Dynamic scaling follows only after the stochastic process and its slow-variable content have been specified and the corresponding response theory has a controlled scaling regime. Detailed balance is optional and must be checked; nonequilibrium fixed points can have different scaling. Kibble–Zurek freeze-out further requires a declared ramp and a comparison between relaxation and driving timescales. The diagram is schematic and not to scale.

The sections Dynamic scaling, Kibble–Zurek freeze-out, and Failure tests provide the text and equation equivalent of the scaling endpoint and its assumptions.

For a linear ramp ϵ(t)=t/τQ\epsilon(t)=t/\tau_Q through t=0t=0, the freeze-out argument of Zurek 1985 compares

τrel(ϵ)withϵϵ˙=t.\tau_{\mathrm{rel}}(\epsilon) \quad\text{with}\quad \left|\frac{\epsilon}{\dot\epsilon}\right|=|t|.

The freeze-out condition gives

ϵ^=(τ0τQ)1/(1+νz),ξ^=ξ0(τQτ0)ν/(1+νz),|\hat\epsilon| =\left(\frac{\tau_0}{\tau_Q}\right)^{1/(1+\nu z)}, \qquad \hat\xi =\xi_0\left(\frac{\tau_Q}{\tau_0}\right)^{\nu/(1+\nu z)},

and

t^=τ01/(1+νz)τQνz/(1+νz).\hat t =\tau_0^{1/(1+\nu z)} \tau_Q^{\nu z/(1+\nu z)}.

These are scaling estimates, not exact switching times. The adiabatic–impulse picture compresses a smooth crossover, and amplitudes depend on the ramp, initial state, and operational definition.

For defects of codimension cc whose initial separation is controlled by ξ^\hat\xi, one often estimates ndefξ^cn_{\mathrm{def}}\sim\hat\xi^{-c}. Defect annihilation after crossing, inhomogeneous fronts, topology, gauge fields, and finite detection time can change the observed exponent.

For a Gaussian nonconserved order parameter, ν=1/2\nu=1/2 and the relaxation rate is Γ(k2+ξ2)\Gamma(k^2+\xi^{-2}), so z=2z=2. The formulas give

ξ^τQ1/4,t^τQ1/2.\hat\xi\propto\tau_Q^{1/4}, \qquad \hat t\propto\tau_Q^{1/2}.

Directly, at k=0k=0 the relaxation time is proportional to ϵ1|\epsilon|^{-1}; equating τ0/ϵ\tau_0/|\epsilon| with τQϵ\tau_Q|\epsilon| gives ϵ^(τ0/τQ)1/2|\hat\epsilon|\sim(\tau_0/\tau_Q)^{1/2} and the same ξ^\hat\xi scaling.

  • Demonstrate the static and dynamic scaling windows separately.
  • Identify all conserved and reversible slow modes before assigning zz.
  • Repeat at several sizes and ramp shapes.
  • Vary the initial distance from criticality and initial correlations.
  • Test for crossover between multiple dynamic exponents.
  • Separate freeze-out scaling from post-crossing coarsening and defect annihilation.

For a power-law ramp ϵ(t)=sgn(t)t/τQr\epsilon(t)=\operatorname{sgn}(t)|t/\tau_Q|^r, derive the scaling of ϵ^|\hat\epsilon|.

Solution

ϵ/ϵ˙=t/r|\epsilon/\dot\epsilon|=|t|/r. With t=τQϵ1/r|t|=\tau_Q|\epsilon|^{1/r}, the condition τ0ϵνz=τQϵ1/r/r\tau_0|\epsilon|^{-\nu z}=\tau_Q|\epsilon|^{1/r}/r gives ϵ^(rτ0/τQ)r/(1+rνz)|\hat\epsilon|\sim(r\tau_0/\tau_Q)^{r/(1+r\nu z)}.

Classify the slow variables on dynamic universality classes and distinguish freeze-out from later coarsening and aging.

  • Kibble, T. W. B. (1976). “Topology of Cosmic Domains and Strings.” Journal of Physics A 9, 1387–1398. DOI.
  • Zurek, W. H. (1985). “Cosmological Experiments in Superfluid Helium?” Nature 317, 505–508. DOI.