Suppose we have the L-loop amplitude of the form
IL=∫L∏i=1dDqi(2π)D1q2i1(p−∑Li=1qi)2.
Introducing Feynman parameters to merge the denominators as usual, we may write the amplitude in the form
IL=(N−1)!∫10L+1∏j=1dxjδ(L+1∑i=1xi−1)∫L∏i=1dDqi(2π)D[qiqjMij−2qjKj+J]−(L+1)
where M is a symmetric matrix. We can evaluate the q integrals using the formula
∫dDl(2π)D1(l2−Δ)N=(−1)Ni(4π)D/2Γ(N−D/2)Γ(N)(1Δ)N−D/2,
It can be shown that we can write IL as
IL=(−1)LΓ(L+1−D)(4π)D∫10L+1∏i=1dxiδ(L+1∑i=1xi−1)UL+1−3D/2FL+1−D,
where we have defined U=det and \mathcal{F}=\det M \left( K_i M^{-1}_{ij} K_j -J \right).
By setting D=4-2 \epsilon, my goal is to calculate the divergent part
\mathcal{I}_L = \frac{c_L}{\epsilon} + \mathcal{O}(\epsilon^0)
for any L. With that aim in mind, let's first look at L=2. Doing the above computations and calculating \mathcal{U} and \mathcal{F} explicitly, amounts to
c_L \propto \int dx_1 dx_2 dx_3 \delta \left( x_1+x_2+x_3-1\right) \frac{x_1 x_2 x_3}{(x_1 x_2 +x_2 x_3 + x_1 x_3)^3}.
The form for larger L follows a similar pattern (product of x_i in the numerator to some power, and sum of products of x_i with one missing in each term, just like above), so evaluating the integral for L=2 would probably lead the way for a more general result. However, how does one treat integrals such as this? Any ideas about how one might try to evaluate it completely?