M(10^24) = 7,189,337,839 and M(10^25) = -258,560,632,948 are computed using an optimized O(x^{2/3+epsilon}) algorithm, extending the record by two orders of magnitude.
Computing $\pi(N)$: An elementary approach in $\tilde{O}(\sqrt{N})$ time
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
We present an efficient and elementary algorithm for computing the number of primes up to $N$ in $\tilde{O}(\sqrt N)$ time, improving upon the existing combinatorial methods that require $\tilde{O}(N ^ {2/3})$ time. Our method has a similar time complexity to the analytical approach to prime counting, while avoiding complex analysis and the use of arbitrary precision complex numbers. While the most time-efficient version of our algorithm requires $\tilde{O}(\sqrt N)$ space, we present a continuous space-time trade-off, showing, e.g., how to reduce the space complexity to $\tilde{O}(\sqrt[3]{N})$ while slightly increasing the time complexity to $\tilde{O}(N^{8/15})$. We apply our techniques to improve the state-of-the-art complexity of elementary algorithms for computing other number-theoretic functions, such as the the Mertens function (in $\tilde{O}(\sqrt N)$ time compared to the known $\tilde{O}(N^{0.6})$), summing Euler's totient function, counting square-free numbers and summing primes. Implementation code is provided.
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Practical Computations of the Mertens Function: $M(10^{24})$ and $M(10^{25})$
M(10^24) = 7,189,337,839 and M(10^25) = -258,560,632,948 are computed using an optimized O(x^{2/3+epsilon}) algorithm, extending the record by two orders of magnitude.