Skewes Number
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In
number theory Number theory (or arithmetic or higher arithmetic in older usage) is a branch of pure mathematics devoted primarily to the study of the integers and arithmetic function, integer-valued functions. German mathematician Carl Friedrich Gauss (1777â ...
, Skewes's number is any of several large numbers used by the
South Africa South Africa, officially the Republic of South Africa (RSA), is the southernmost country in Africa. It is bounded to the south by of coastline that stretch along the South Atlantic and Indian Oceans; to the north by the neighbouring countri ...
n mathematician
Stanley Skewes Stanley Skewes (; 1899–1988) was a South African mathematician, best known for his discovery of the Skewes's number in 1933. He was one of John Edensor Littlewood's students at Cambridge University. Skewes's numbers contributed to the refine ...
as upper bounds for the smallest
natural number In mathematics, the natural numbers are those numbers used for counting (as in "there are ''six'' coins on the table") and ordering (as in "this is the ''third'' largest city in the country"). Numbers used for counting are called ''Cardinal n ...
x for which :\pi(x) > \operatorname(x), where is the
prime-counting function 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 (''x'') (unrelated to the number ). History Of great interest in number theory is t ...
and is the
logarithmic integral function In mathematics, the logarithmic integral function or integral logarithm li(''x'') is a special function. It is relevant in problems of physics and has number theoretic significance. In particular, according to the prime number theorem, it is a ...
. Skewes's number is much larger, but it is now known that there is a crossing between \pi(x) < \operatorname(x) and \pi(x) > \operatorname(x) near e^ < 1.397 \times 10^. It is not known whether it is the smallest crossing.


Skewes's numbers

J.E. Littlewood John Edensor Littlewood (9 June 1885 – 6 September 1977) was a British mathematician. He worked on topics relating to analysis, number theory, and differential equations, and had lengthy collaborations with G. H. Hardy, Srinivasa Raman ...
, who was Skewes's research supervisor, had proved in that there is such a number (and so, a first such number); and indeed found that the sign of the difference \pi(x) - \operatorname(x) changes infinitely many times. All numerical evidence then available seemed to suggest that \pi(x) was always less than \operatorname(x). Littlewood's proof did not, however, exhibit a concrete such number x. proved that, assuming that the
Riemann hypothesis In mathematics, the Riemann hypothesis is the conjecture that the Riemann zeta function has its zeros only at the negative even integers and complex numbers with real part . Many consider it to be the most important unsolved problem in ...
is true, there exists a number x violating \pi(x) < \operatorname(x), below :e^<10^. In , without assuming the Riemann hypothesis, Skewes proved that there must exist a value of x below :e^<10^. Skewes's task was to make Littlewood's existence proof effective: exhibiting some concrete upper bound for the first sign change. According to
Georg Kreisel Georg Kreisel FRS (September 15, 1923 – March 1, 2015) was an Austrian-born mathematical logician who studied and worked in the United Kingdom and America. Biography Kreisel was born in Graz and came from a Jewish background; his family ...
, this was at the time not considered obvious even in principle.


More recent estimates

These upper bounds have since been reduced considerably by using large-scale computer calculations of zeros of the
Riemann zeta function The Riemann zeta function or Euler–Riemann zeta function, denoted by the Greek letter (zeta), is a mathematical function of a complex variable defined as \zeta(s) = \sum_^\infty \frac = \frac + \frac + \frac + \cdots for \operatorname(s) > ...
. The first estimate for the actual value of a crossover point was given by , who showed that somewhere between 1.53\times 10^ and 1.65\times 10^ there are more than 10^ consecutive
integer An integer is the number zero (), a positive natural number (, , , etc.) or a negative integer with a minus sign (−1, −2, −3, etc.). The negative numbers are the additive inverses of the corresponding positive numbers. In the language ...
s x with \pi(x) > \operatorname(x). Without assuming the Riemann hypothesis, proved an upper bound of 7\times 10^. A better estimate was 1.39822\times 10^ discovered by , who showed there are at least 10^ consecutive integers somewhere near this value where \pi(x) > \operatorname(x). Bays and Hudson found a few much smaller values of x where \pi(x) gets close to \operatorname(x); the possibility that there are crossover points near these values does not seem to have been definitely ruled out yet, though computer calculations suggest they are unlikely to exist. gave a small improvement and correction to the result of Bays and Hudson. found a smaller interval for a crossing, which was slightly improved by . The same source shows that there exists a number x violating \pi(x) < \operatorname(x), below e^< 1.39718 \times 10^. This can be reduced to e^< 1.39717 \times 10^ assuming the Riemann hypothesis. gave 1.39716 \times 10^. Rigorously, proved that there are no crossover points below x = 10^8, improved by to 8\times 10^, by to 10^, by to 1.39\times 10^, and by to 10^. There is no explicit value x known for certain to have the property \pi(x) > \operatorname(x), though computer calculations suggest some explicit numbers that are quite likely to satisfy this. Even though the
natural density In number theory, natural density (also referred to as asymptotic density or arithmetic density) is one method to measure how "large" a subset of the set of natural numbers is. It relies chiefly on the probability of encountering members of the de ...
of the positive integers for which \pi(x) > \operatorname(x) does not exist, showed that the
logarithmic density In number theory, natural density (also referred to as asymptotic density or arithmetic density) is one method to measure how "large" a subset of the set of natural numbers is. It relies chiefly on the probability of encountering members of the de ...
of these positive integers does exist and is positive. showed that this proportion is about 0.00000026, which is surprisingly large given how far one has to go to find the first example.


Riemann's formula

Riemann gave an explicit formula for \pi(x), whose leading terms are (ignoring some subtle convergence questions) :\pi(x) = \operatorname(x) - \tfrac\operatorname(\sqrt) - \sum_ \operatorname(x^\rho) + \text where the sum is over all \rho in the set of non-trivial zeros of the Riemann zeta function. The largest error term in the approximation \pi(x) \approx \operatorname(x) (if the
Riemann hypothesis In mathematics, the Riemann hypothesis is the conjecture that the Riemann zeta function has its zeros only at the negative even integers and complex numbers with real part . Many consider it to be the most important unsolved problem in ...
is true) is negative \tfrac\operatorname(\sqrt), showing that \operatorname(x) is usually larger than \pi(x). The other terms above are somewhat smaller, and moreover tend to have different, seemingly random complex arguments, so mostly cancel out. Occasionally however, several of the larger ones might happen to have roughly the same complex argument, in which case they will reinforce each other instead of cancelling and will overwhelm the term \tfrac\operatorname(\sqrt). The reason why the Skewes number is so large is that these smaller terms are quite a ''lot'' smaller than the leading error term, mainly because the first complex zero of the zeta function has quite a large imaginary part, so a large number (several hundred) of them need to have roughly the same argument in order to overwhelm the dominant term. The chance of N random complex numbers having roughly the same argument is about 1 in 2^N. This explains why \pi(x) is sometimes larger than \operatorname(x), and also why it is rare for this to happen. It also shows why finding places where this happens depends on large scale calculations of millions of high precision zeros of the Riemann zeta function. The argument above is not a proof, as it assumes the zeros of the Riemann zeta function are random, which is not true. Roughly speaking, Littlewood's proof consists of Dirichlet's approximation theorem to show that sometimes many terms have about the same argument. In the event that the Riemann hypothesis is false, the argument is much simpler, essentially because the terms \operatorname(x^) for zeros violating the Riemann hypothesis (with real part greater than ) are eventually larger than \operatorname(x^). The reason for the term \tfrac\mathrm(x^) is that, roughly speaking, \mathrm(x) actually counts powers of
primes A prime number (or a prime) is a natural number greater than 1 that is not a product of two smaller natural numbers. A natural number greater than 1 that is not prime is called a composite number. For example, 5 is prime because the only ways ...
, rather than the primes themselves, with p^n weighted by \frac. The term \tfrac\mathrm(x^) is roughly analogous to a second-order correction accounting for
squares In Euclidean geometry, a square is a regular quadrilateral, which means that it has four equal sides and four equal angles (90-degree angles, π/2 radian angles, or right angles). It can also be defined as a rectangle with two equal-length adj ...
of primes.


Equivalent for prime ''k''-tuples

An equivalent definition of Skewes' number exists for prime ''k''-tuples (). Let P = (p, p+i_1, p+i_2, ..., p+i_k) denote a prime (''k'' + 1)-tuple, \pi_P(x) the number of primes p below x such that p, p+i_1, p+i_2, ..., p+i_k are all prime, let \operatorname(x) = \int_2^x \frac and let C_P denote its Hardy-Littlewood constant (see
First Hardy-Littlewood conjecture A twin prime is a prime number that is either 2 less or 2 more than another prime number—for example, either member of the twin prime pair (41, 43). In other words, a twin prime is a prime that has a prime gap of two. Sometimes the term ''twin pr ...
). Then the first prime p that violates the Hardy-Littlewood inequality for the (''k'' + 1)-tuple P, i.e., the first prime p such that : \pi_P(p) > C_P \operatorname_P(p), (if such a prime exists) is the ''Skewes number for P.'' The table below shows the currently known Skewes numbers for prime ''k''-tuples: The Skewes number (if it exists) for
sexy prime In number theory, sexy primes are prime numbers that differ from each other by 6. For example, the numbers 5 and 11 are both sexy primes, because both are prime and . The term "sexy prime" is a pun stemming from the Latin word for six: . If o ...
s (p, p+6) is still unknown. It is also unknown whether all admissible ''k''-tuples have a corresponding Skewes number.


References

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External links

* * {{Large numbers Large numbers Number theory Large integers