2. Background and Ancillary Results
In mathematical number theory, the Chebyshev function
is defined as
where the summation includes all prime numbers
p less than or equal to
x, and log denotes the natural logarithm. In contrast, the prime counting function
, which tallies the number of primes up to
x, is expressed as
with the sum similarly ranging over all primes
. Together, these functions furnish essential tools for exploring the distribution of primes and related functions, bridging elementary definitions to deeper analytical insights.
In 1734, Leonhard Euler made a seminal contribution to mathematics by evaluating the Riemann zeta function at
, a result tied to his resolution of the Basel problem [
2]. This work not only showcased his ingenuity but also laid foundational insights into number theory.
Proposition 1.
The value of the zeta function at 2 is defined as [2]:
where denotes the k-th prime number (often written as for the n-th prime), n is a natural number, and is the ubiquitous mathematical constant bridging number theory, geometry, and beyond. Euler’s proof elegantly unifies the infinite series with the infinite product over primes, culminating in the exact value .
Another constant of profound significance, the Euler-Mascheroni constant
, emerges in analytic number theory and is defined through two equivalent expressions:
where
denotes the floor function, yielding the greatest integer less than or equal to
x. This constant frequently appears in studies of harmonic sums and integral approximations.
Definition 1.
We say that the condition holds if:
where p ranges over all primes less than or equal to x, is the base of the natural logarithm, and is the Chebyshev function.
Finally, a primorial number of order
n, denoted
, is the product of the first
n prime numbers:
For example, . This construction is pivotal in exploring properties of primes and their distributions, often intersecting with conjectures like the Riemann Hypothesis. Together, these concepts weave a rich tapestry of mathematical relationships, illuminating the intricate structure of numbers.
In number theory, the Dedekind psi function is defined as , where the product is taken over all distinct prime numbers p dividing n. Similarly, Euler’s totient function, which counts the integers up to n that are coprime to n, is given by . These functions play a crucial role in analyzing arithmetic properties of numbers, particularly primorials-products of the first k primes, denoted .
Proposition 2.
For all natural numbers , as established by Choie et al. [3], the following inequality holds:
where is the Euler-Mascheroni constant. Furthermore, we can relate Ψ and φ through the primorial as follows:
Since is the product of the first k primes, and the infinite product over all primes satisfies (from Proposition 1), we derive:
This connects the growth of and to fundamental constants.
A pivotal result linking primorials to the Riemann Hypothesis is Nicolas’ Theorem:
Proposition 3.
The condition , defined as , holds for all if and only if the Riemann Hypothesis is true [4,5]. Empirical verification confirms holds for [4,5]. Nicolas further demonstrated that the Riemann Hypothesis is equivalent to the inequality:
holding for all natural numbers , where is the k-th primorial and relates the Chebyshev function to the primorial logarithm [4]. Equivalently, this implies holds for each k-th prime . Conversely, if the Riemann Hypothesis is false, Nicolas proved there exist infinitely many k for which:
highlighting a breakdown in the expected growth pattern [5].
By synthesizing these results, we construct a robust framework for disproving the Riemann Hypothesis, leveraging the interplay between arithmetic functions, primorials, and deep number-theoretic constants to illuminate this enduring conjecture.