If the singular free-energy density is set by one correlated region, then . With reduced temperature , the definitions and therefore giveThis is the hyperscaling relation; it assumes that no dangerously irrelevant coupling introduces an additional scale.
For and , minimizing the -invariant potential givesThe free energy has the full symmetry, but choosing one point on this sphere leaves only the rotations fixing that point. This is spontaneous symmetry breaking, . The tangent directions along the sphere cost no potential energy and are the massless Goldstone modes predicted by the Goldstone theorem.
Choose the vacuum . The quadratic free energy contains a positive mass term for the radial field but no mass term for any transverse field :Thus the momentum-space correlation function is . Since a massive correlator has denominator , these Goldstone modes have and hence infinite correlation length.
The long-wavelength Goldstone fluctuation is proportional towhich diverges in the infrared for . These fluctuations destroy finite-temperature long-range order with a broken continuous symmetry, as formalized by the Mermin-Wagner theorem. Therefore the lower critical dimension is : conventional spontaneous order is possible for but not for .
The rotation symmetry requires the quadratic dependence on to be proportional to , soThe quartic terms involving only that pair must be proportional to , and the terms coupling it to must be proportional to . With the convention that the symmetric double sum counts off-diagonal terms twice, this giveswhile , , and the common mixed coupling are unrestricted. The stated symmetry imposes no further relation because every term is already even in .
Let , , and . With every , the uniform potential isFor , the minimum is the origin and is unbroken. If , then and ; the factor is broken, remains, and there is no Goldstone mode. If , then and ; the first remains while is broken to the reflection fixing the chosen direction, producing one Goldstone mode.
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