Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2010/iii/paper-41/2/solution

Use the connected correlation function . Away from criticality its large-distance envelope decays exponentially on the correlation length , often with an algebraic prefactor. At criticality diverges and a short-range scalar model instead has the power law , with anomalous dimension .
A blocking kernel assigns coarse spins to each block of side lattice spacings, with . Define the coarse Hamiltonian by
The operator basis must be sufficiently complete to include interactions generated by blocking. Summing over coarse spins preserves the partition function, while the physical lattice spacing and site count change to , . After steps they are and . Exact blocking preserves the long-distance predictions; truncating the generated interaction space introduces an approximation.
Define the dimensionless free energy per site . Preservation of gives . For one step, removing the explicitly additive constant gives
The function records the additive free-energy density generated by eliminated degrees of freedom; it is usually regular near a finite blocking step's critical point. Iteration proves
This is the additive free-energy recursion under blocking. After removing regular backgrounds, its singular part obeys homogeneous scaling.
A renormalization-group fixed point satisfies . Linearizing the map gives scaling coordinates . A relevant operator has , an irrelevant operator has , and a marginal operator has and needs nonlinear analysis. The critical surface consists of points flowing into the critical fixed point after all relevant directions are tuned. An outgoing or repulsive trajectory lies in the unstable manifold and describes perturbations that grow under coarse-graining.
With relevant thermal and magnetic coordinates , the singular free-energy density obeys . Choose to obtain
Here are the positive scaling eigenvalues, and refer to the signs of . Since , the correlation-length exponent is . Two temperature derivatives of give , establishing the hyperscaling relation
The magnetization exponent similarly is . These expressions assume no additional dangerous scaling variables.
For the Gaussian field theory, decompose the field into low and high Fourier modes, integrate out , and restore the cutoff using and . The gradient coefficient remains fixed, the mass coefficient transforms as , and the uniform source as . Hence , , and the Gaussian momentum-shell scaling gives
The sign convention reverses the magnetization's sign but not these exponents. For , these are Gaussian scaling predictions, not the exponents of a generic interacting scalar critical point: the quartic interaction is relevant there. The free quadratic Hamiltonian also has no stable ordered phase at negative , so the quoted is its formal order-parameter scaling index, not a spontaneously magnetized state of the unstabilized Gaussian integral. The relevance distinction is also explained in Tong's renormalization-group lecture notes.

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