In mathematics, the prime counting function is the function counting the number of prime numbers less than or equal to some real number x. It is denoted by (although it has no connection with the number π).
Of great interest in number theory is the growth rate of the prime counting function. It was conjectured in the end of the 18th century by Gauss and by Legendre to be approximately
in the sense that
This statement is the prime number theorem. An equivalent statement is
where li is the logarithmic integral function. This was first proved around 1896 by Hadamard and by de la Vallée Poussin (independently), using properties of the Riemann zeta function introduced by Riemann in 1859.
More precise estimates of are now known; for example
where the O is big O notation. Proofs of the prime number theorem not using the zeta function or complex analysis were found around 1948 by Atle Selberg and by Paul Erdős (for the most part independently).
Another conjecture about the growth rate for prime series involving PNT is:
Here is a table that shows how the three functions π(x), x / ln x and Li(x) compare:
The first column is sequence A006880 in OEIS; the second column is sequence A057835; and the third column is sequence A057752.
A simple way to find , if is not too large, is to use the sieve of Eratosthenes to produce the primes smaller or equal to and then to count them.
A more elaborate way of finding is due to Legendre: given , if , , …, are distinct prime numbers, then the number of integers smaller or equal to which are divisible by no is
(where denotes the floor function). This number is therefore equal to
when the numbers , , …, are the prime numbers smaller or equal to the square root of .
In a series of articles published between 1870 and 1885, Ernst Meissel described (and used) a practical combinatorial way of evaluating . Let , , …, be the first primes and denote by the number of natural numbers not greater than which are divisible by no . Then
Given a natural number , if and if , then
Using this approach, Meissel computed , for equal to 5×105, 106, 107, and 108.
In 1959, Derrick Henry Lehmer extended and simplified Meissel's method. Define, for real and for natural numbers , and , as the number of numbers not greater than m with exactly k prime factors, all greater than . Furthermore, set . Then
where the sum actually has only finitely many nonzero terms. Let denote an integer such that , and set . Then and when ≥ 3. Therefore
The computation of can be obtained this way:
On the other hand, the computation of can be done using the following rules:
Using his method and an IBM 701, Lehmer was able to compute .
Chinese mathematician Hwang Cheng, in a conference about prime number functions at the university of Burdeaux used the following identities:
and setting , Laplace-transforming both sides and applying a geometric sum on got the expression:
Other prime counting functions are also used because they are more convenient to work with. One is Riemann's prime counting function, denoted or . This has jumps of 1/n for prime powers pn, with it taking a value half-way between the two sides at discontinuities. That added detail is because then it may be defined by an inverse Mellin transform. Formally, we may define J by
where p is a prime.
We may also write
and knowing the relationship between log of the Riemann function and the von Mangoldt function , and the Perron formula we have:
except where we have discontinuities at prime powers, and hence π can be recovered from J by Möbius inversion.
The Chebyshev function weights primes or prime powers pn by ln p:
Apart from the discontinuities at prime powers, we have
where Λ(n) is the von Mangoldt function.
These come in two kinds, arithmetic formulas and analytic formulas. The latter are what allow us to prove the prime number theorem. They stem from the work of Riemann and von Mangoldt, and are generally known as explicit formulas.
We have the following expression for ψ:
For J we have a more complicated formula
The following simple approximation can be useful:
round*
where x=ln(powers of 10>2) , z=ln(x) ,A=1.007 , B= -.05245
Here are some inequalities for the nth prime, pn.
An approximation for the nth prime number is
The Riemann hypothesis is equivalent to a much tighter bound on the error in the estimate for , and hence to a more regular distribution of prime numbers,
if we had a sum of a function over all primes : and we wish to accelerate its convergence we can write it as:
for the series on the left we could apply Euler transform for alternating series, providing that f(n)>f(n+1) and that the 2 series converges, it also relates an alternating series to its prime sum counterpart, the main task of using this is that we can give a good approximation using only a few values of the prime number counting function.
Fonction de compte des nombres premiers | Funzione enumerativa dei primi | Funkcja π | Število praštevil
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"Prime counting function".
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