Surviving Eratosthenes sieve I: quadratic density and Legendre's conjecture

Abstract

We have been studying Eratosthenes sieve as a discrete dynamic system, obtaining exact models for the relative populations for small gaps (currently gaps g 82) in the cycle of gaps G(p\#) at each stage of the sieve. The gaps in the interval H(pk)=[pk2, pk+12] are fixed in G(p\#) and survive all subsequent stages of the sieve to be confirmed as gaps between primes. We have shown that samples of gaps between primes over these intervals of survival H(pk) have population distributions that reflect the relative population models wg(pk\#). This paper advances our study of the estimates of survival across stages of the sieve. Inspired by Legendre's conjecture, we introduce the concept of quadratic density ηs(pk), which is the expected population of the constellation s in the intervals [n2, (n+1)2] for pk n < pk+1. We show that once a gap occurs in G(p\#), its expected quadratic density increases across all subsequent stages of the sieve. Regarding Legendre's conjecture, beyond postulating one prime in the interval [n2,(n+1)2], the quadratic density predicts the populations of several prime gaps within this interval.

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