Idea: when Gauss was a boy (by the dates found on his notes he was approximately 16) he noticed that the primes appear with density around . Then, instead of counting primes and looking at the function , lets weight by the natural density and look at . Since we are weighting by what we think is the density, we expect it to be asymptotic to be . This is the first Chebyshev function.
The second Chebyshev function, denoted by , is defined in terms of the von Mangoldt function:
where
This means that includes all prime powers, not just primes, but weights each one by .
Why Counts Prime Numbers
Although includes powers of primes (), those contribute very little compared to the primes themselves.
Most contributions to the sum come from , i.e., the actual primes.
Higher powers become rare as increases.
Every prime contributes to the sum via , and possibly a smaller number of contributions via .
So, behaves like a smoothed or weighted version of the prime counting function . While simply counts 1 for each prime , counts for each prime and its powers .
It turns out that this function is more natural in complex analysis than the prime counting function:
That is, the total weight of primes and their powers up to behaves like . Since powers contribute little, this tells us that the primes themselves are distributed with density .