Edit: I'm not sure if this is better suited to StatsStackexchange.
I thought of this question after reading about quasi-random sequences (and quasi-random numbers) in the context of Monte Carlo integration.
Introduction and definitions
Quasi-random numbers are different from pseudo-random numbers, because they are deterministically constructed to have **low discrepancy**.Discrepancy is defined as follows,
Let $x_1, x_2, \cdots x_N$ be $N$ numbers in $I=[0,1]^s$, let $E \subset I$. Define a function $A(E;N)$ such that, it counts the number of $n$, $ 1\leq n\leq N$, for $x_n \in E.$ The discrepancy $D_n$ of the $N$ numbers in $I$ is then given by, \begin{align*} D_n=\sup_J \left| \frac{A(J;N)}{N}-\lambda_s(J) \right| \end{align*} Where, $J$ is any sub-interval of $I$, and $\lambda_s(J)$ denotes its $s$ dimensional Lebesgue measure.
The star discrepancy ($D_N^*$) is a more commonly used definition which is as follows. \begin{align*} D_N^*=\sup_{0\leq t \leq 1} \left | \frac{A([0,t); N)}{N} - \lambda_s([0,t)) \right| \end{align*} $D_n$ and $D_n^*$ are related by the following inequality \begin{align*} D_n^* \leq D_n \leq 2^s D_n^* \label{starrelation} \end{align*}
Question
What is the discrepancy for a uniformly distributed random variate (or even pseudorandom numbers)?
Through the definition of star discrepancy it seems intuitively to me that a UD random variate probably has a high discrepancy. However I couldn't prove this, neither could I find any references online.
Update: There is a mistake in my bounty text (I misread the notation). The method described, to use the CDF of a Uniform Distribution times $N$ in place of $A([0,t),N)$ is correct and it gives the discrepancy of the uniformly distributed random variate as exactly $0$ for the single dimensional case. However the question to prove it for $s$-dimensional case is still open.
Thanks for any and all help!