Ramanujan tau function
The Ramanujan tau function, studied by Ramanujan (1916), is the function defined by the following identity:
where with
and
is the Dedekind eta function and the function
is a holomorphic cusp form of weight 12 and level 1, known as the discriminant modular form.

Contents
Values
The first few values of the tau function are given in the following table (sequence A000594 in OEIS):
![]() |
1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
![]() |
1 | −24 | 252 | −1472 | 4830 | −6048 | −16744 | 84480 | −113643 | −115920 | 534612 | −370944 | −577738 | 401856 | 1217160 | 987136 |
Ramanujan's conjectures
Ramanujan (1916) observed, but could not prove, the following three properties of :
if
(meaning that
is a multiplicative function)
for p prime and r > 0.
for all primes p.
The first two properties were proved by Mordell (1917) and the third one, called the Ramanujan conjecture, was proved by Deligne in 1974 as a consequence of his proof of the Weil conjectures.
Congruences for the tau function
For k ∈ Z and n ∈ Z>0, define σk(n) as the sum of the k-th powers of the divisors of n. The tau function satisfies several congruence relations; many of them can be expressed in terms of σk(n). Here are some:[1]
For p ≠ 23 prime, we have[1][7]
Conjectures on τ(n)
Suppose that is a weight
integer newform and the Fourier coefficients
are integers. Consider the problem: If
does not have complex multiplication, prove that almost all primes
have the property that
. Indeed, most primes should have this property, and hence they are called ordinary. Despite the big advances by Deligne and Serre on Galois representations, which determine
for
coprime to
, we do not have any clue as to how to compute
. The only theorem in this regard is Elkies' famous result for modular elliptic curves, which indeed guarantees that there are infinitely many primes
for which
, which in turn is obviously
. We do not know any examples of non-CM
with weight
for which
mod
for infinitely many primes
(although it should be true for almost all
). We also do not know any examples where
mod
for infinitely many
. Some people had begun to doubt whether
indeed for infinitely many
. As evidence, many provided Ramanujan's
(case of weight
). The largest known
for which
is
. The only solutions to the equation
are
and
up to
.[9]
Lehmer (1947) conjectured that for all
, an assertion sometimes known as Lehmer's conjecture. Lehmer verified the conjecture for
(Apostol 1997, p. 22). The following table summarizes progress on finding successively larger values of
for which this condition holds.
n | reference |
---|---|
3316799 | Lehmer (1947) |
214928639999 | Lehmer (1949) |
![]() |
Serre (1973, p. 98), Serre (1985) |
1213229187071998 | Jennings (1993) |
22689242781695999 | Jordan and Kelly (1999) |
22798241520242687999 | Bosman (2007) |
982149821766199295999 | Zeng and Yin (2013) |
816212624008487344127999 | Derickx, van Hoeij, and Zeng (2013) |
Notes
<templatestyles src="Reflist/styles.css" />
Cite error: Invalid <references>
tag; parameter "group" is allowed only.
<references />
, or <references group="..." />
References
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 1.0 1.1 Page 4 of Swinnerton-Dyer 1973
- ↑ 2.0 2.1 2.2 2.3 Due to Kolberg 1962
- ↑ 3.0 3.1 Due to Ashworth 1968
- ↑ Due to Lahivi
- ↑ 5.0 5.1 Due to D. H. Lehmer
- ↑ Due to Ramanujan 1916
- ↑ Due to Wilton 1930
- ↑ Due to J.-P. Serre 1968, Section 4.5
- ↑ Due to N. Lygeros and O. Rozier 2010