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Feynman diagram
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=== Scalar propagator === Each mode is independently Gaussian distributed. The expectation of field modes is easy to calculate: :<math> \left\langle \phi_k \phi_{k'}\right\rangle = 0 \,</math> for {{math|''k'' ≠ ''k''′}}, since then the two Gaussian random variables are independent and both have zero mean. :<math> \left\langle\phi_k \phi_k \right\rangle = \frac{V}{k^2} </math> in finite volume {{mvar|V}}, when the two {{mvar|k}}-values coincide, since this is the variance of the Gaussian. In the infinite volume limit, :<math> \left\langle\phi(k) \phi(k')\right\rangle = \delta(k-k') \frac{1}{k^2} </math> Strictly speaking, this is an approximation: the lattice propagator is: :<math>\left\langle\phi(k) \phi(k')\right\rangle = \delta(k-k') \frac{1}{2\big(d - \cos(k_1) + \cos(k_2) \cdots + \cos(k_d)\big) }</math> But near {{math|''k'' {{=}} 0}}, for field fluctuations long compared to the lattice spacing, the two forms coincide. The delta functions contain factors of 2{{pi}}, so that they cancel out the 2{{pi}} factors in the measure for {{mvar|k}} integrals. :<math>\delta(k) = (2\pi)^d \delta_D(k_1)\delta_D(k_2) \cdots \delta_D(k_d) \,</math> where {{math|''δ<sub>D</sub>''(''k'')}} is the ordinary one-dimensional Dirac delta function. This convention for delta-functions is not universal—some authors keep the factors of 2{{pi}} in the delta functions (and in the {{mvar|k}}-integration) explicit.
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