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Emergent Symmetry

An emergent symmetry is a symmetry of an effective low-energy, long-wavelength, or large-scale description that is not an exact symmetry of the microscopic Hamiltonian. It is one of the main reasons very different microscopic systems can share the same long-distance physics.

The careful statement is not

microscopic Hamiltonian has symmetry G.\text{microscopic Hamiltonian has symmetry }G.

Instead it is often

effective theory near a scale or fixed point has symmetry Geff.\text{effective theory near a scale or fixed point has symmetry }G_{\mathrm{eff}}.

The symmetry may become exact only in a limiting description, such as energy E/Λ→0E/\Lambda\to0, correlation length ξ/a→∞\xi/a\to\infty, or system size L/a→∞L/a\to\infty, where aa is a microscopic scale and Λ\Lambda is a cutoff.

Suppose a microscopic Hamiltonian has only a smaller symmetry GmicroG_{\mathrm{micro}}. At low energies, one may describe the relevant degrees of freedom by an effective Hamiltonian or action

Heff=H∗+∑igi Oi.H_{\mathrm{eff}} = H_* + \sum_i g_i\,O_i.

Here H∗H_* has a larger symmetry GeffG_{\mathrm{eff}}, while the operators OiO_i may break it. If the coefficients gig_i become less important at long distances, the physics can approach the more symmetric description.

Schematic scaling language writes

gi(E)∼gi(Λ)(EΛ)Δi,Δi>0,g_i(E) \sim g_i(\Lambda) \left( \frac{E}{\Lambda} \right)^{\Delta_i}, \qquad \Delta_i>0,

for an irrelevant symmetry-breaking correction. Then the breaking becomes small as E/Λ→0E/\Lambda\to0.

This formula is only a signpost, not a substitute for renormalization-group analysis. Its purpose here is to emphasize the scale dependence: emergent symmetry is a statement about an effective regime.

Emergent symmetry is closely related to Approximate Symmetry, but the emphasis differs.

An approximate symmetry usually begins with a small breaking term:

H=Hsym+ϵVbreak,ϵ≪1.H=H_{\mathrm{sym}}+\epsilon V_{\mathrm{break}}, \qquad \epsilon\ll1.

An emergent symmetry may begin with no small microscopic number. Instead, the effective low-energy description suppresses symmetry-breaking operators. The small parameter can be

EΛ,aξ,aL,\frac{E}{\Lambda}, \qquad \frac{a}{\xi}, \qquad \frac{a}{L},

or another scale ratio.

In practice the concepts overlap. A symmetry can be both approximate and emergent in a given regime. The important habit is to state the scale and the corrections.

Emergent symmetry is one mechanism behind universality. Many microscopic Hamiltonians can share the same effective description, critical exponents, scaling forms, and symmetry structure even though their short-distance details differ.

This is why a continuum field theory can describe a lattice model near a critical point. The lattice remembers the microscopic spacing aa, but long-wavelength observables may depend primarily on fields, symmetries, dimensionality, and relevant perturbations. Lattice Models Overview states the microscopic model data that must be matched before such a universality claim is made.

The word “universal” should still be used carefully. Nonuniversal quantities such as microscopic velocities, cutoff-dependent constants, and amplitudes can remain model-dependent.

A crystal or lattice does not have continuous spatial rotation symmetry microscopically. It has a discrete space group. Nevertheless, long-wavelength excitations can have approximately rotational dispersion:

E(k)=E0+α∣k∣2+O(k4a4),E(\mathbf k) = E_0 + \alpha|\mathbf k|^2 + O(k^4a^4),

where the leading term depends only on ∣k∣|\mathbf k| and lattice anisotropy enters at higher order.

Similarly, some low-energy systems have an emergent Lorentz-like symmetry. A lattice Hamiltonian is not microscopically Lorentz invariant, but near a low-energy point the dispersion may take the form

E2≈v2∣p∣2+m2v4,E^2 \approx v^2|\mathbf p|^2 + m^2v^4,

with a common effective velocity vv. Corrections appear at higher powers of momentum or from interactions that distinguish time and space. The statement is therefore a low-energy approximation, not evidence that the microscopic lattice obeys special relativity.

Internal symmetries can also emerge. A microscopic model may allow anisotropic couplings, but near a fixed point the anisotropy can become irrelevant. The effective theory then has a larger internal symmetry than the lattice Hamiltonian.

For example, a spin model may have only a discrete or axial microscopic symmetry, while its long-distance critical theory is described by fields with a larger continuous symmetry in a suitable universality class. Whether this happens is model-dependent; anisotropies can be relevant, irrelevant, or dangerously irrelevant.

The safe rule is:

larger effective symmetryrequires a stability statement.\text{larger effective symmetry} \quad \text{requires a stability statement}.

One must check whether symmetry-breaking perturbations grow or shrink at the scale being studied.

Emergent symmetry and spontaneous symmetry breaking are different ideas, but they can coexist.

An effective long-distance theory may have an emergent continuous symmetry. That emergent symmetry may then be spontaneously broken in the effective description, producing collective modes or order-parameter structure. However, if the symmetry is only emergent, microscopic symmetry-breaking terms can eventually gap or split the would-be low-energy structures.

This is one reason pseudo-Goldstone modes occur: the effective theory has an approximate or emergent continuous symmetry, but the microscopic theory contains terms that weakly break it.

Emergent symmetry is tested through scaling and robustness, not through a single exact equality at one finite scale.

Useful evidence includes:

  • spectra whose low-energy levels organize into larger multiplets;
  • correlation functions approaching symmetric scaling forms;
  • velocities or couplings flowing toward common values;
  • symmetry-breaking observables shrinking with scale;
  • different microscopic models sharing the same long-distance exponents.

Finite systems and finite experimental windows can mimic or obscure emergence. A claimed emergent symmetry should always state the observable, scale range, and expected corrections.

  • Treating an emergent symmetry as exact at microscopic scales.
  • Forgetting the limiting procedure or scale ratio.
  • Assuming every approximate symmetry is emergent.
  • Assuming every low-energy theory has more symmetry than the microscopic model.
  • Ignoring relevant symmetry-breaking perturbations.
  • Calling a numerical near-degeneracy emergent without a scaling analysis.
  • Confusing emergent Lorentz-like symmetry with microscopic relativistic invariance.
  • Presenting universality as if all quantities become universal.
  • K. G. Wilson and J. Kogut, “The renormalization group and the epsilon expansion”, Physics Reports 12, 75-199, 1974.
  • J. Cardy, Scaling and Renormalization in Statistical Physics, Cambridge University Press, 1996.
  • S. Sachdev, Quantum Phase Transitions, 2nd ed., Cambridge University Press, 2011.
  • A. Altland and B. Simons, Condensed Matter Field Theory, 2nd ed., Cambridge University Press, 2010.
  • P. Coleman, Introduction to Many-Body Physics, Cambridge University Press, 2015.
  • S. Weinberg, The Quantum Theory of Fields, Volume I, Cambridge University Press, 1995.
  1. Scale-suppressed breaking.

Suppose a symmetry-breaking coupling scales as

g(E)=g(Λ)(EΛ)2.g(E) = g(\Lambda) \left( \frac{E}{\Lambda} \right)^2.

What happens to the breaking as E/Λ→0E/\Lambda\to0?

Solution

The factor (E/Λ)2(E/\Lambda)^2 tends to zero. Thus the symmetry-breaking correction becomes less important at low energy. The effective low-energy theory can have a larger symmetry than the microscopic theory, up to corrections controlled by E2/Λ2E^2/\Lambda^2.

  1. Lattice dispersion.

Assume a one-dimensional lattice excitation has

E(k)=v∣k∣+αa2∣k∣3+⋯ .E(k) = v|k| + \alpha a^2|k|^3 + \cdots .

Why can the low-energy theory look scale invariant or Lorentz-like even though the lattice is microscopic?

Solution

For ∣k∣a≪1|k|a\ll1, the correction term satisfies

αa2∣k∣3v∣k∣∼∣k∣2a2\frac{\alpha a^2|k|^3}{v|k|} \sim |k|^2a^2

up to constants. It becomes small at long wavelength. The leading dispersion is linear, E≈v∣k∣E\approx v|k|, which is the form used in many emergent relativistic or conformal low-energy descriptions. The lattice corrections remain present but are suppressed.

  1. Approximate or emergent?

A microscopic Hamiltonian is exactly GG-symmetric except for a small known term ϵV\epsilon V. Is this automatically an emergent symmetry?

Solution

No. It is at least an approximate symmetry when ϵ\epsilon is small in the relevant regime. To call it emergent, one should identify a scale-dependent mechanism by which the symmetry becomes better in a low-energy, long-distance, or limiting description. Small explicit breaking alone is not enough.

  1. Relevant anisotropy.

Why does an anisotropy that grows at long distances prevent an emergent larger rotational symmetry?

Solution

Emergent larger symmetry requires the symmetry-breaking perturbation to become less important in the regime of interest. If the anisotropy grows under coarse graining or dominates long-distance observables, the effective theory is not approaching the larger symmetric fixed point. The anisotropy is then relevant for the long-distance physics.