I have an integral on the unit sphere as follows.
$$I(\mathbf{s}_1, \mathbf{s}_2) = \int_{\mathbb{S}^2} f(\mathbf{x} \cdot \mathbf{s}_1)f(\mathbf{x}\cdot\mathbf{s}_2)d\mathbf{x} $$ where the integral is on the whole unit sphere $\mathbb{S}^2$. $\mathbf{s}_1$ and $\mathbf{s}_2$ are also unit-length vectors on the unit sphere. For example, $\mathbf{s}_1$ is the vector from the origin to a point on the sphere $\vec{O s_1}$.
Intuitively, since the integral is over the whole sphere, $I(\mathbf{s}_1, \mathbf{s}_2)$ should only depend on the relative angle between $\mathbf{s}_1$ and $\mathbf{s}_2$. This is actually done here.
Now I want to go further and do a Taylor expansion in terms of the relative spherical angle between $\mathbf{s}_1$ and $\mathbf{s}_2$, say $\theta$, so that $\theta = \angle (\mathbf{s}_1, \mathbf{s}_2)$. When $\mathbf{s}_1$ is close to $\mathbf{s}_2$, $\theta$ will be small and I want to do an expansion in terms of $\theta$. The problem is that I don't know how to explicit write $I(\mathbf{s}_1, \mathbf{s}_2)$ as a function of $\theta$, so I am stuck.
I need help on write this $I(\mathbf{s}_1, \mathbf{s}_2)$ as an Taylor expansion in terms of $\theta$, the relative angle between vectors $\mathbf{s}_1$ and $\mathbf{s}_2$. Any comments will be greatly appreciated.