The first real progress towards the prime number theorem was achieved by
Chebyshev in 1850. In a flash of inspiration, he saw that
instead of simply counting primes, it might
be easier to count them with ``weights". In other words, take a function
and consider sums like
, where again
denotes the set of primes not greater than
. As we have seen, Abel
summation can then be used to relate such quantities to
itself.
In particular, Chebyshev considered the function
defined
in this way, with
chosen to be
:
The notation
is now standard. Another way to describe it is:
if
are the primes not greater than
, then
Proposition 1.6.1. For all
, we have
.
Proof. With the above notation,
and
for each
.
The relationship is expressed more exactly by Abel's summation formula.
Recall that
is 1 if
is prime and 0 otherwise. By 1.3.6, we have
Conversely, we can express
in terms of
.
Clearly,
,
where
Since
, version 1.3.7 of Abel's summation formula gives
Theorem 1.6.2. Suppose that for some constants
we have
Proof. Integration by parts, with 1 as one factor, gives
| (2) |
Note. A similar proof using discrete Abel summation delivers a variant of
the theorem in terms of ls
instead of li
.
A numerical example.
Some actual numbers will help to illustrate how
proceeds in ``jerks", and the limits to how well it
can be expected to approximate to
. Computation gives
. There are no primes between 181 and 191, so
remains constant at this value for
. The
numbers 191, 193, 197, 199 are all prime, each adding slightly more than 5
to
, with the result that
.
This value then persists until we reach 211, the next prime.
Since the jumps
in the value of
become increasingly
large, it is clear that the difference
is unbounded, even
if (as we hope) it is ultimately small compared to
.
To prove the prime number theorem, we will have to show that
satisfies
the hypothesis of Theorem 1.6.2 with
and
(for any given
). Apart from diversions, this task will occupy
most of the next two chapters. However, one can
show by much more direct methods that the stated inequalities
hold for some
and
. This is what Chebyshev did.
Our first proof of the prime number theorem does not actually need these
results, while our second and third proofs require the upper estimate
but not the lower one. However, the estimates (particularly the upper one) have
numerous other applications. Also, their proofs are both ingenious and
instructive. Here we prove the upper estimate, leaving the lower one
until later (section 2.4), when we will have the machinery to prove it
much more neatly.
The proof is rather more number-theoretic in nature than anything we have encountered yet. In particular, we need to recall two statements from elementary number theory.
(NT1) If
is prime and
, then
or
.
(NT2) If
and the greatest common divisor of
and
is 1 (in particular, if
are distinct primes),
then
.
These statements are easy consequences of unique prime factorization, but in the usual approach they are actually used in proving it.
Note that by (NT1), if
, then
for some
,
so certainly
.
Theorem 1.6.3. For all
, we have
Note.
: our constant
is not much bigger than 1.
Proof. It is sufficient to consider integers
. Fix
, and let
Let
be the primes
such that
,
so that
| (3) |
The statement for
follows, by 1.6.2, since
.
Corollary 1.6.4. There is a constant
such that
Proof. This follows at once from 1.6.3 and 1.5.5.
Short alternative proofs of this theorem will appear in sections 2.4 and 6.1; however, they do not yield such a good value for the constant.
We finish this section by showing how the last result, combined with
Abel summation, can be used to give an upper estimate for
.
(More accurate estimates, both upper and lower, will be obtained in sections 2.1
and 2.6.)
Proposition 1.6.5. Let
be as in 1.6.4. Then for another constant
,
Proof. Denote the sum by
. With
defined as before,
we have by Abel's summation formula,
1. Modify the proof of 1.6.5 to show that
is convergent.
2. Let
be such that
for all
. Show that
3. Write
as
, where
4. Show that there is a constant
such that for all
,