In the long-wavelength description of an antiferromagnet, is the antiferromagnetic spin wave velocity and controls the stiffness or strength of quantum fluctuations. The field is an auxiliary Lagrange multiplier enforcing the fixed-length constraint on the order parameter. At the translation-invariant saddle, shifts every propagator denominator and is the excitation gap, which explains the name gap equation.
The Large-N expansion makes fluctuations of the auxiliary field relatively small. Its leading saddle-point condition is then self-consistent and becomes the displayed gap equation.
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As , the Matsubara sum becomes . Put and . The factors of cancel from both sides, leaving
Using four-dimensional spherical coordinates,
At the onset of spontaneous symmetry breaking, the symmetric-phase gap closes. Thus
For the constraint is instead satisfied by an ordered condensate; a positive symmetric gap exists for .
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Subtracting the critical equation from the massive equation gives
As from above,
Therefore, up to constants inside the slowly varying logarithm,
The square-root mean-field power is modified by a logarithm. It is therefore not a pure quantum-critical power law; this is an upper-critical-dimension logarithmic correction.
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The first term is a gauge choice for the Spin coherent-state Berry phase. For a closed spin trajectory, changing the surface used to evaluate the solid angle changes the action by
The path-integral phase must be independent of that choice, so
Hence
and the spin is integer or half-integer.
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Write and . To quadratic order,
After dropping the total derivative , the quadratic Lagrangian density is
Its Euler--Lagrange equations are
For modes proportional to , nontrivial amplitudes require
Thus
At short wavelength the anisotropy is negligible and the quadratic dispersion is that of a conventional ferromagnetic magnon. At long wavelength, easy-plane anisotropy makes the out-of-plane fluctuation the conjugate density of the in-plane phase; eliminating it produces the linear Goldstone sound mode characteristic of a superfluid.
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