There is no mathematical proof for the simple reason that a statement like the CLT (or even weaker conclusions such as "Arithmetic means will converge") is not true for pseudo random numbers. Nevertheless, there is theory available on how good you can approximate integrals by weighted sums of function evaluations. This is applicable to pseudo random numbers in particular but also to quasi random numbers or other designs such as grids.
In addition to integration, pseudo random numbers are used for other applications such as simulation. My answer does address only numerical integration not those other applications.
Counter example
The situation of the CLT is unique that it, among stronger conclusions, ensures the convergence of the estimate for the integral for every (square) integrable function. A similar statement is not possible for finite deterministic sequences (pseudo random or others). Here is a counter example:
- A function $f:[0,1]\rightarrow\mathbb{R}$ with $\int_0^1 f(x)dx=1$ but $\sum_i f(x_i)=0$ for all outputs from your random generator.
This is possible because your generator of pseudo random numbers will have a finite(!) number of possible outputs $x_1, \ldots, x_N$. This number is finite, because it is generated by a deterministic machine with finite memory. See this answer for further explanation. Now, given this finite set, it is a standard exercise in functional analysis to construct a function which is zero exactly on these points but sufficiently large everywhere else to make the integral one (see here). This function can actually be chosen to be infinitely differentiable, i.e. very smooth and "nice".
Error estimation
To rule out counterexamples as the above, error estimates have to take into account quantitative properties beyond smoothness. The best known example is the Koksma-Hlawka inequality:
$$ \left| \frac{1}{N}\sum_i f(x_i) - \int_0^1 f(x) dx \right|\leq V(f) \,D(x_1,\ldots,x_N).$$
$V(f)$ is the total variation of $f$ and $D(x_1,\ldots,x_N)$ the "star-discrepancy" of the set $\{x_1,\ldots,x_N\}$.
The star-discrepancy is a measure for the deviation of the points in the set from being uniform. It is defined as the largest difference between the relative number of points $x_i$ in any sub interval of $[0,1]$ and the Lebesgue measure of the interval, i.e. its length:
$$ D(x_1,\ldots,x_N) = \sup_{I\subset [0,1]} \left| \frac{\text{# of $x_i$ in }I}{N} - \lambda(I)\right|.$$
What does it mean in practice?
The Koksma-Hlawka inequality provides a nice split of the integration error into two distinct contributions. One part related to the functions you would like to integrate and one part related to the design, i.e. the choice of points used for integration.
The inequality shows the problem with the counter example. Since one had to force the function down to zero and then up again for each and every $x_i$, the graph of the function will wiggle a lot. This creates a very large Total Variation and drives up the error, even though the choice of design points might be nearly uniform.
On the other hand the inequality explains why pseudo random numbers work (in most cases). Ultimately your pseudo random numbers will fill up the whole interval nearly uniform and your star discrepancy will become very, very small.
Furthermore, it explains why people did not stop at pseudo random numbers but went further to quasi Monte Carlo. Choosing points "at random" will lead to areas of higher and lower concentrations of points, smoothing this out will lower the star discrepancy and increase approximation quality.