Inspired by the answers in a past question I asked on techniques for computing integrals using the Feynman parametrization, I became interested in computing integrals over Feynman parameters like so:
- $$\int_0^1\int_{0}^{1-u_1} \frac{u_1u_2\sqrt{u_1u_2(1-u_1-u_2)}}{(u_1(1-u_1)\|\textbf{a}\|^2-2u_1u_2\textbf{a}\cdot\textbf{b}+u_2(1-u_2)\|\textbf{b}\|^2)^3} \,du_2du_1$$
- $$\int_0^1\int_{0}^{1-u_1} \frac{u_1(u_1-1)\sqrt{u_1u_2(1-u_1-u_2)}}{(u_1(1-u_1)\|\textbf{a}\|^2-2u_1u_2\textbf{a}\cdot\textbf{b}+u_2(1-u_2)\|\textbf{b}\|^2)^3} \,du_2du_1$$
- $$\int_0^1\int_{0}^{1-u_1} \frac{u_2(u_2-1)\sqrt{u_1u_2(1-u_1-u_2)}}{(u_1(1-u_1)\|\textbf{a}\|^2-2u_1u_2\textbf{a}\cdot\textbf{b}+u_2(1-u_2)\|\textbf{b}\|^2)^3} \,du_2du_1$$
...where $\textbf{a},\textbf{b}\in\mathbb{R}^3$ are generic vectors.
My question: Does anyone know how to compute the integrals 1. 2. or 3. above or have any useful techniques to share possibly using some of the symmetries present?
Solution Attempt: As these are integrals over a simplex, I have seen related integrals (like the one in the linked question above) performed by making a change of variables like so: $u_1=s(1-t),u_2=(1-s)(1-t), du_2du_1=(1-t)dtds$, so that the integrals are transformed to integrals over a unit square:
1'. $$\int_0^1\int_{0}^{1} \frac{s(1-s)(1-t)\sqrt{ts(1-s)}}{\big(\left(s(1-s)\|\textbf{a}-\textbf{b}\|^2+t\|s\textbf{a}+(1-s)\textbf{b}\|^2 \right)\big)^3} \,dtds$$
2'. $$\int_0^1\int_{0}^{1} \frac{s\big(1-s(1-t)\big)\sqrt{ts(1-s)}}{\big(\left(s(1-s)\|\textbf{a}-\textbf{b}\|^2+t\|s\textbf{a}+(1-s)\textbf{b}\|^2 \right)\big)^3} \,dtds$$
3'. $$\int_0^1\int_{0}^{1} \frac{(1-s)(s(1-t)+t)\sqrt{ts(1-s)}}{\big(\left(s(1-s)\|\textbf{a}-\textbf{b}\|^2+t\|s\textbf{a}+(1-s)\textbf{b}\|^2 \right)\big)^3} \,dtds$$
Mathematica can compute the $t$ integrals in a fairly straightforward way, however it struggles with the $s$ integrals. I tried as well to make a change of variables $s=\frac{u^2}{1+u^2}$ and attempted applying some residue calculations like I've seen applied elsewhere, however I wasn't able to get too far.
Any clues or leads on how Feynman parameters like these are integrated over would be very much appreciated!
(P.S. I can also summarize how I came to these integrals if anyone is interested. It ultimately comes from the Feynman parametrization with multiple denominators where $\alpha_1=\alpha_2=\alpha_3=3/2$)