The defining integral for the retarded Green function has support only at . If with , then supplies exponential damping. Under the usual tempered-growth condition on the thermal commutator, the integral and all its derivatives converge locally uniformly. Therefore
This is the frequency-space expression of causality.
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Let , , and take Hermitian. Inserting energy eigenstates gives
On the support of the delta function, and
This has the same sign as . Every remaining factor is nonnegative, hence
This thermal spectral-positivity statement also shows that is odd after pairing .
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A path integral is obtained by slicing an evolution operator into short time intervals and inserting complete sets of field eigenstates between successive factors. An operator inserted at a later slice therefore appears to the left of one inserted at an earlier slice. Summing over the intermediate fields preserves this ordering, so real-time path integrals generate time-ordered correlators and Euclidean thermal path integrals generate imaginary-time-ordered correlation functions.
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Let and . For , cyclicity of the trace gives
This is the bosonic Kubo--Martin--Schwinger condition. It identifies the two time orderings across the end of the thermal interval, so
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Periodicity on the interval gives the bosonic Matsubara frequencies
The Fourier coefficients are
The notation emphasizes that these data lie at imaginary real-time frequencies .
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The energy-eigenstate expansion of for is
Fourier integration and give
Comparing this with the spectral expression in part ii yields the spectral representation of a thermal correlation function
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The Drude response
has a pole at . Analyticity in the upper half plane therefore requires
For real frequency,
The sign condition from part ii then requires
so with a nonzero causal relaxation time the convention used in this question has . In conventions where the physical conductivity is defined with an additional minus sign, its static value is positive. The parameter is the relaxation time: after forcing is removed, the corresponding current or response decays as .
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The spectral density is
Substitution into the spectral representation, closing the contour in the half plane selected by the sign of , gives
In particular under the sign convention established in part vii. The absolute value is required because a bosonic Hermitian-operator Matsubara correlator is even in .
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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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