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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 integer-valued functions. German mathematician Carl Friedrich Gauss (1777–1855) said, "Mathe ...
, an arithmetic, arithmetical, or number-theoretic function is for most authors any function ''f''(''n'') whose domain is the
positive integers 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 ...
and whose range is a
subset In mathematics, set ''A'' is a subset of a set ''B'' if all elements of ''A'' are also elements of ''B''; ''B'' is then a superset of ''A''. It is possible for ''A'' and ''B'' to be equal; if they are unequal, then ''A'' is a proper subset o ...
of the complex numbers. Hardy & Wright include in their definition the requirement that an arithmetical function "expresses some arithmetical property of ''n''". An example of an arithmetic function is the
divisor function In mathematics, and specifically in number theory, a divisor function is an arithmetic function related to the divisors of an integer. When referred to as ''the'' divisor function, it counts the ''number of divisors of an integer'' (includin ...
whose value at a positive integer ''n'' is equal to the number of divisors of ''n''. There is a larger class of number-theoretic functions that do not fit the above definition, for example, 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 i ...
s. This article provides links to functions of both classes. Arithmetic functions are often extremely irregular (see
table Table may refer to: * Table (furniture), a piece of furniture with a flat surface and one or more legs * Table (landform), a flat area of land * Table (information), a data arrangement with rows and columns * Table (database), how the table data ...
), but some of them have series expansions in terms of
Ramanujan's sum In number theory, Ramanujan's sum, usually denoted ''cq''(''n''), is a function of two positive integer variables ''q'' and ''n'' defined by the formula : c_q(n) = \sum_ e^, where (''a'', ''q'') = 1 means that ''a'' only takes on values coprime ...
.


Multiplicative and additive functions

An arithmetic function ''a'' is * completely additive if ''a''(''mn'') = ''a''(''m'') + ''a''(''n'') for all natural numbers ''m'' and ''n''; *
completely multiplicative In number theory, functions of positive integers which respect products are important and are called completely multiplicative functions or totally multiplicative functions. A weaker condition is also important, respecting only products of coprime ...
if ''a''(''mn'') = ''a''(''m'')''a''(''n'') for all natural numbers ''m'' and ''n''; Two whole numbers ''m'' and ''n'' are called coprime if their
greatest common divisor In mathematics, the greatest common divisor (GCD) of two or more integers, which are not all zero, is the largest positive integer that divides each of the integers. For two integers ''x'', ''y'', the greatest common divisor of ''x'' and ''y'' is ...
is 1, that is, if there is no
prime number 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 ...
that divides both of them. Then an arithmetic function ''a'' is *
additive Additive may refer to: Mathematics * Additive function, a function in number theory * Additive map, a function that preserves the addition operation * Additive set-functionn see Sigma additivity * Additive category, a preadditive category with fi ...
if ''a''(''mn'') = ''a''(''m'') + ''a''(''n'') for all coprime natural numbers ''m'' and ''n''; * multiplicative if ''a''(''mn'') = ''a''(''m'')''a''(''n'') for all coprime natural numbers ''m'' and ''n''.


Notation

In this article, \sum_p f(p) and \prod_p f(p) mean that the sum or product is over all
prime number 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 ...
s: \sum_p f(p) = f(2) + f(3) + f(5) + \cdots and \prod_p f(p)= f(2)f(3)f(5)\cdots. Similarly, \sum_ f(p^k) and \prod_ f(p^k) mean that the sum or product is over all
prime power In mathematics, a prime power is a positive integer which is a positive integer power of a single prime number. For example: , and are prime powers, while , and are not. The sequence of prime powers begins: 2, 3, 4, 5, 7, 8, 9, 11, 13, 16, 17 ...
s with strictly positive exponent (so is not included): \sum_ f(p^k) = \sum_p\sum_ f(p^k) = f(2) + f(3) + f(4) +f(5) +f(7)+f(8)+f(9)+\cdots. The notations \sum_ f(d) and \prod_ f(d) mean that the sum or product is over all positive divisors of ''n'', including 1 and ''n''. For example, if , then \prod_ f(d) = f(1)f(2) f(3) f(4) f(6) f(12). The notations can be combined: \sum_ f(p) and \prod_ f(p) mean that the sum or product is over all prime divisors of ''n''. For example, if ''n'' = 18, then \sum_ f(p) = f(2) + f(3), and similarly \sum_ f(p^k) and \prod_ f(p^k) mean that the sum or product is over all prime powers dividing ''n''. For example, if ''n'' = 24, then \prod_ f(p^k) = f(2) f(3) f(4) f(8).


Ω(''n''), ''ω''(''n''), ''ν''''p''(''n'') – prime power decomposition

The
fundamental theorem of arithmetic In mathematics, the fundamental theorem of arithmetic, also called the unique factorization theorem and prime factorization theorem, states that every integer greater than 1 can be represented uniquely as a product of prime numbers, up to the ord ...
states that any positive integer ''n'' can be represented uniquely as a product of powers of primes: n = p_1^\cdots p_k^ where ''p''1 < ''p''2 < ... < ''p''''k'' are primes and the ''aj'' are positive integers. (1 is given by the empty product.) It is often convenient to write this as an infinite product over all the primes, where all but a finite number have a zero exponent. Define the ''p''-adic valuation ν''p''(''n'') to be the exponent of the highest power of the prime ''p'' that divides ''n''. That is, if ''p'' is one of the ''p''''i'' then ''ν''''p''(''n'') = ''a''''i'', otherwise it is zero. Then n = \prod_p p^. In terms of the above the
prime omega function In number theory, the prime omega functions \omega(n) and \Omega(n) count the number of prime factors of a natural number n. Thereby \omega(n) (little omega) counts each ''distinct'' prime factor, whereas the related function \Omega(n) (big omega) ...
s ω and Ω are defined by To avoid repetition, whenever possible formulas for the functions listed in this article are given in terms of ''n'' and the corresponding ''p''''i'', ''a''''i'', ω, and Ω.


Multiplicative functions


σ''k''(''n''), τ(''n''), ''d''(''n'') – divisor sums

σ''k''(''n'') is the sum of the ''k''th powers of the positive divisors of ''n'', including 1 and ''n'', where ''k'' is a complex number. σ1(''n''), the sum of the (positive) divisors of ''n'', is usually denoted by σ(''n''). Since a positive number to the zero power is one, σ0(''n'') is therefore the number of (positive) divisors of ''n''; it is usually denoted by ''d''(''n'') or τ(''n'') (for the German ''Teiler'' = divisors). \sigma_k(n) = \prod_^ \frac= \prod_^ \left(1 + p_i^k + p_i^ + \cdots + p_i^\right). Setting ''k'' = 0 in the second product gives \tau(n) = d(n) = (1 + a_)(1+a_)\cdots(1+a_).


φ(''n'') – Euler totient function

φ(''n''), the Euler totient function, is the number of positive integers not greater than ''n'' that are coprime to ''n''. \varphi(n) = n \prod_ \left(1-\frac\right) = n \left(\frac\right)\left(\frac\right) \cdots \left(\frac\right) .


J''k''(''n'') – Jordan totient function

J''k''(''n''), the Jordan totient function, is the number of ''k''-tuples of positive integers all less than or equal to ''n'' that form a coprime (''k'' + 1)-tuple together with ''n''. It is a generalization of Euler's totient, . J_k(n) = n^k \prod_ \left(1-\frac\right) = n^k \left(\frac\right)\left(\frac\right) \cdots \left(\frac\right) .


μ(''n'') – Möbius function

μ(''n''), the Möbius function, is important because of the
Möbius inversion Moebius, Möbius or Mobius may refer to: People * August Ferdinand Möbius (1790–1868), German mathematician and astronomer * Theodor Möbius (1821–1890), German philologist * Karl Möbius (1825–1908), German zoologist and ecologist * Pa ...
formula. See
Dirichlet convolution In mathematics, the Dirichlet convolution is a binary operation defined for arithmetic functions; it is important in number theory. It was developed by Peter Gustav Lejeune Dirichlet. Definition If f , g : \mathbb\to\mathbb are two arithmetic fu ...
, below. \mu(n)=\begin (-1)^=(-1)^ &\text\; \omega(n) = \Omega(n)\\ 0&\text\;\omega(n) \ne \Omega(n). \end This implies that μ(1) = 1. (Because Ω(1) = ω(1) = 0.)


τ(''n'') – Ramanujan tau function

τ(''n''), the Ramanujan tau function, is defined by its
generating function In mathematics, a generating function is a way of encoding an infinite sequence of numbers () by treating them as the coefficients of a formal power series. This series is called the generating function of the sequence. Unlike an ordinary serie ...
identity: \sum_\tau(n)q^n=q\prod_(1-q^n)^. Although it is hard to say exactly what "arithmetical property of ''n''" it "expresses", (''τ''(''n'') is (2π)−12 times the ''n''th Fourier coefficient in the
q-expansion In mathematics, a modular form is a (complex) analytic function on the upper half-plane satisfying a certain kind of functional equation with respect to the group action of the modular group, and also satisfying a growth condition. The theory of ...
of the
modular discriminant In mathematics, the Weierstrass elliptic functions are elliptic functions that take a particularly simple form. They are named for Karl Weierstrass. This class of functions are also referred to as ℘-functions and they are usually denoted by the ...
function) it is included among the arithmetical functions because it is multiplicative and it occurs in identities involving certain σ''k''(''n'') and ''r''''k''(''n'') functions (because these are also coefficients in the expansion of
modular form In mathematics, a modular form is a (complex) analytic function on the upper half-plane satisfying a certain kind of functional equation with respect to the group action of the modular group, and also satisfying a growth condition. The theory ...
s).


''c''''q''(''n'') – Ramanujan's sum

''c''''q''(''n''), Ramanujan's sum, is the sum of the ''n''th powers of the primitive ''q''th
roots of unity In mathematics, a root of unity, occasionally called a de Moivre number, is any complex number that yields 1 when raised to some positive integer power . Roots of unity are used in many branches of mathematics, and are especially important i ...
: c_q(n) = \sum_ e^. Even though it is defined as a sum of complex numbers (irrational for most values of ''q''), it is an integer. For a fixed value of ''n'' it is multiplicative in ''q'': :If ''q'' and ''r'' are coprime, then c_q(n)c_r(n)=c_(n).


''ψ''(''n'') - Dedekind psi function

The
Dedekind psi function In number theory, the Dedekind psi function is the multiplicative function on the positive integers defined by : \psi(n) = n \prod_\left(1+\frac\right), where the product is taken over all primes p dividing n. (By convention, \psi(1), which is t ...
, used in the theory of
modular function In mathematics, a modular form is a (complex) analytic function on the upper half-plane satisfying a certain kind of functional equation with respect to the group action of the modular group, and also satisfying a growth condition. The theory of ...
s, is defined by the formula \psi(n) = n \prod_\left(1+\frac\right).


Completely multiplicative functions


λ(''n'') – Liouville function

''λ''(''n''), the Liouville function, is defined by \lambda (n) = (-1)^.


''χ''(''n'') – characters

All
Dirichlet character In analytic number theory and related branches of mathematics, a complex-valued arithmetic function \chi:\mathbb\rightarrow\mathbb is a Dirichlet character of modulus m (where m is a positive integer) if for all integers a and b: :1)   \ch ...
s ''χ''(''n'') are completely multiplicative. Two characters have special notations: The principal character (mod ''n'') is denoted by ''χ''0(''a'') (or ''χ''1(''a'')). It is defined as \chi_0(a) = \begin 1 & \text \gcd(a,n) = 1, \\ 0 & \text \gcd(a,n) \ne 1. \end The quadratic character (mod ''n'') is denoted by the
Jacobi symbol Jacobi symbol for various ''k'' (along top) and ''n'' (along left side). Only are shown, since due to rule (2) below any other ''k'' can be reduced modulo ''n''. Quadratic residues are highlighted in yellow — note that no entry with a J ...
for odd ''n'' (it is not defined for even ''n''): \left(\frac\right) = \left(\frac\right)^\left(\frac\right)^\cdots \left(\frac\right)^. In this formula (\tfrac) is the
Legendre symbol In number theory, the Legendre symbol is a multiplicative function with values 1, −1, 0 that is a quadratic character modulo an odd prime number ''p'': its value at a (nonzero) quadratic residue mod ''p'' is 1 and at a non-quadratic residue ...
, defined for all integers ''a'' and all odd primes ''p'' by \left(\frac\right) = \begin \;\;\,0 & \text a \equiv 0 \pmod p, \\+1 & \texta \not\equiv 0\pmod p \textx, \;a\equiv x^2\pmod p \\-1 & \text x. \end Following the normal convention for the empty product, \left(\frac\right) = 1.


Additive functions


''ω''(''n'') – distinct prime divisors

ω(''n''), defined above as the number of distinct primes dividing ''n'', is additive (see
Prime omega function In number theory, the prime omega functions \omega(n) and \Omega(n) count the number of prime factors of a natural number n. Thereby \omega(n) (little omega) counts each ''distinct'' prime factor, whereas the related function \Omega(n) (big omega) ...
).


Completely additive functions


Ω(''n'') – prime divisors

Ω(''n''), defined above as the number of prime factors of ''n'' counted with multiplicities, is completely additive (see
Prime omega function In number theory, the prime omega functions \omega(n) and \Omega(n) count the number of prime factors of a natural number n. Thereby \omega(n) (little omega) counts each ''distinct'' prime factor, whereas the related function \Omega(n) (big omega) ...
).


''ν''''p''(''n'') – ''p''-adic valuation of an integer ''n''

For a fixed prime ''p'', ''ν''''p''(''n''), defined above as the exponent of the largest power of ''p'' dividing ''n'', is completely additive.


Logarithmic derivative

\operatorname(n)=\frac = \sum_ \frac , where D(n) is the arithmetic derivative.


Neither multiplicative nor additive


(''x''), Π(''x''), ''θ''(''x''), ''ψ''(''x'') – prime-counting functions

These important functions (which are not arithmetic functions) are defined for non-negative real arguments, and are used in the various statements and proofs of the
prime number theorem In mathematics, the prime number theorem (PNT) describes the asymptotic distribution of the prime numbers among the positive integers. It formalizes the intuitive idea that primes become less common as they become larger by precisely quantifying ...
. They are summation functions (see the main section just below) of arithmetic functions which are neither multiplicative nor additive. (''x''), the prime-counting function, is the number of primes not exceeding ''x''. It is the summation function of the characteristic function of the prime numbers. \pi(x) = \sum_ 1 A related function counts prime powers with weight 1 for primes, 1/2 for their squares, 1/3 for cubes, ... It is the summation function of the arithmetic function which takes the value 1/''k'' on integers which are the k-th power of some prime number, and the value 0 on other integers. \Pi(x) = \sum_\frac. ''θ''(''x'') and ''ψ''(''x''), the Chebyshev functions, are defined as sums of the natural logarithms of the primes not exceeding ''x''. \vartheta(x)=\sum_ \log p, \psi(x) = \sum_ \log p. The Chebyshev function ''ψ''(''x'') is the summation function of the von Mangoldt function just below.


Λ(''n'') – von Mangoldt function

Λ(''n''), the von Mangoldt function, is 0 unless the argument ''n'' is a prime power , in which case it is the natural log of the prime ''p'': \Lambda(n) = \begin \log p &\text n = 2,3,4,5,7,8,9,11,13,16,\ldots=p^k \text\\ 0&\text n=1,6,10,12,14,15,18,20,21,\dots \;\;\;\;\text. \end


''p''(''n'') – partition function

''p''(''n''), the partition function, is the number of ways of representing ''n'' as a sum of positive integers, where two representations with the same summands in a different order are not counted as being different: p(n) = \left, \left\\.


λ(''n'') – Carmichael function

''λ''(''n''), the Carmichael function, is the smallest positive number such that a^\equiv 1 \pmod   for all ''a'' coprime to ''n''. Equivalently, it is the
least common multiple In arithmetic and number theory, the least common multiple, lowest common multiple, or smallest common multiple of two integers ''a'' and ''b'', usually denoted by lcm(''a'', ''b''), is the smallest positive integer that is divisible by bo ...
of the orders of the elements of the multiplicative group of integers modulo ''n''. For powers of odd primes and for 2 and 4, ''λ''(''n'') is equal to the Euler totient function of ''n''; for powers of 2 greater than 4 it is equal to one half of the Euler totient function of ''n'': \lambda(n) = \begin \;\;\phi(n) &\textn = 2,3,4,5,7,9,11,13,17,19,23,25,27,\dots\\ \tfrac 1 2 \phi(n)&\textn=8,16,32,64,\dots \end and for general ''n'' it is the least common multiple of λ of each of the prime power factors of ''n'': \lambda(p_1^p_2^ \dots p_^) = \operatorname lambda(p_1^),\;\lambda(p_2^),\dots,\lambda(p_^)


''h''(''n'') – Class number

''h''(''n''), the class number function, is the order of the
ideal class group In number theory, the ideal class group (or class group) of an algebraic number field is the quotient group where is the group of fractional ideals of the ring of integers of , and is its subgroup of principal ideals. The class group is a mea ...
of an algebraic extension of the rationals with
discriminant In mathematics, the discriminant of a polynomial is a quantity that depends on the coefficients and allows deducing some properties of the roots without computing them. More precisely, it is a polynomial function of the coefficients of the origi ...
''n''. The notation is ambiguous, as there are in general many extensions with the same discriminant. See
quadratic field In algebraic number theory, a quadratic field is an algebraic number field of degree two over \mathbf, the rational numbers. Every such quadratic field is some \mathbf(\sqrt) where d is a (uniquely defined) square-free integer different from 0 ...
and cyclotomic field for classical examples.


''r''''k''(''n'') – Sum of ''k'' squares

''r''''k''(''n'') is the number of ways ''n'' can be represented as the sum of ''k'' squares, where representations that differ only in the order of the summands or in the signs of the square roots are counted as different. r_k(n) = \left, \left\\


''D''(''n'') – Arithmetic derivative

Using the Heaviside notation for the derivative, the
arithmetic derivative In number theory, the Lagarias arithmetic derivative or number derivative is a function defined for integers, based on prime factorization, by analogy with the product rule for the derivative of a function that is used in mathematical analysis. ...
''D''(''n'') is a function such that * D(n) = 1 if ''n'' prime, and * D(mn) = m D(n) + D(m) n (the
product rule In calculus, the product rule (or Leibniz rule or Leibniz product rule) is a formula used to find the derivatives of products of two or more functions. For two functions, it may be stated in Lagrange's notation as (u \cdot v)' = u ' \cdot v + ...
)


Summation functions

Given an arithmetic function ''a''(''n''), its summation function ''A''(''x'') is defined by A(x) := \sum_ a(n) . ''A'' can be regarded as a function of a real variable. Given a positive integer ''m'', ''A'' is constant along
open interval In mathematics, a (real) interval is a set of real numbers that contains all real numbers lying between any two numbers of the set. For example, the set of numbers satisfying is an interval which contains , , and all numbers in between. Othe ...
s ''m'' < ''x'' < ''m'' + 1, and has a
jump discontinuity Continuous functions are of utmost importance in mathematics, functions and applications. However, not all functions are continuous. If a function is not continuous at a point in its domain, one says that it has a discontinuity there. The set of ...
at each integer for which ''a''(''m'') ≠ 0. Since such functions are often represented by series and integrals, to achieve pointwise convergence it is usual to define the value at the discontinuities as the average of the values to the left and right: A_0(m) := \frac 1 2 \left(\sum_ a(n) +\sum_ a(n)\right) = A(m) - \frac 1 2 a(m) . Individual values of arithmetic functions may fluctuate wildly – as in most of the above examples. Summation functions "smooth out" these fluctuations. In some cases it may be possible to find asymptotic behaviour for the summation function for large ''x''. A classical example of this phenomenon is given by the
divisor summatory function In mathematics, a divisor of an integer n, also called a factor of n, is an integer m that may be multiplied by some integer to produce n. In this case, one also says that n is a multiple of m. An integer n is divisible or evenly divisible by ...
, the summation function of ''d''(''n''), the number of divisors of ''n'': \liminf_ d(n) = 2 \limsup_\frac = \log 2 \lim_\frac = 1. An average order of an arithmetic function is some simpler or better-understood function which has the same summation function asymptotically, and hence takes the same values "on average". We say that ''g'' is an ''average order'' of ''f'' if \sum_ f(n) \sim \sum_ g(n) as ''x'' tends to infinity. The example above shows that ''d''(''n'') has the average order log(''n'').


Dirichlet convolution

Given an arithmetic function ''a''(''n''), let ''F''''a''(''s''), for complex ''s'', be the function defined by the corresponding
Dirichlet series In mathematics, a Dirichlet series is any series of the form \sum_^\infty \frac, where ''s'' is complex, and a_n is a complex sequence. It is a special case of general Dirichlet series. Dirichlet series play a variety of important roles in ana ...
(where it converges): F_a(s) := \sum_^\infty \frac . ''F''''a''(''s'') is called a
generating function In mathematics, a generating function is a way of encoding an infinite sequence of numbers () by treating them as the coefficients of a formal power series. This series is called the generating function of the sequence. Unlike an ordinary serie ...
of ''a''(''n''). The simplest such series, corresponding to the constant function ''a''(''n'') = 1 for all ''n'', is ''ς''(''s'') 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 generating function of the Möbius function is the inverse of the zeta function: \zeta(s)\,\sum_^\infty\frac=1, \;\;\Re s >0. Consider two arithmetic functions ''a'' and ''b'' and their respective generating functions ''F''''a''(''s'') and ''F''''b''(''s''). The product ''F''''a''(''s'')''F''''b''(''s'') can be computed as follows: F_a(s)F_b(s) = \left( \sum_^\frac \right)\left( \sum_^\frac \right) . It is a straightforward exercise to show that if ''c''(''n'') is defined by c(n) := \sum_ a(i)b(j) = \sum_a(i)b\left(\frac\right) , then F_c(s) = F_a(s) F_b(s). This function ''c'' is called the
Dirichlet convolution In mathematics, the Dirichlet convolution is a binary operation defined for arithmetic functions; it is important in number theory. It was developed by Peter Gustav Lejeune Dirichlet. Definition If f , g : \mathbb\to\mathbb are two arithmetic fu ...
of ''a'' and ''b'', and is denoted by a*b. A particularly important case is convolution with the constant function ''a''(''n'') = 1 for all ''n'', corresponding to multiplying the generating function by the zeta function: g(n) = \sum_f(d). Multiplying by the inverse of the zeta function gives the
Möbius inversion Moebius, Möbius or Mobius may refer to: People * August Ferdinand Möbius (1790–1868), German mathematician and astronomer * Theodor Möbius (1821–1890), German philologist * Karl Möbius (1825–1908), German zoologist and ecologist * Pa ...
formula: f(n) = \sum_\mu\left(\frac\right)g(d). If ''f'' is multiplicative, then so is ''g''. If ''f'' is completely multiplicative, then ''g'' is multiplicative, but may or may not be completely multiplicative.


Relations among the functions

There are a great many formulas connecting arithmetical functions with each other and with the functions of analysis, especially powers, roots, and the exponential and log functions. The page divisor sum identities contains many more generalized and related examples of identities involving arithmetic functions. Here are a few examples:


Dirichlet convolutions

: \sum_\mu(\delta)= \sum_\lambda\left(\frac\right), \mu(\delta), = \begin 1 & \text n=1\\ 0 & \text n\ne1 \end     where ''λ'' is the Liouville function. :\sum_\varphi(\delta) = n.       ::\varphi(n) =\sum_\mu\left(\frac\right)\delta =n\sum_\frac.       Möbius inversion :\sum_ J_k(d) = n^k.       :: J_k(n) =\sum_\mu\left(\frac\right)\delta^k =n^k\sum_\frac.       Möbius inversion :\sum_\delta^sJ_r(\delta)J_s\left(\frac\right) = J_(n)       :\sum_\varphi(\delta)d\left(\frac\right) = \sigma(n).       :\sum_, \mu(\delta), = 2^.       ::, \mu(n), =\sum_\mu\left(\frac\right)2^.       Möbius inversion :\sum_2^=d(n^2).       ::2^=\sum_\mu\left(\frac\right)d(\delta^2).       Möbius inversion :\sum_d(\delta^2)=d^2(n).       ::d(n^2)=\sum_\mu\left(\frac\right)d^2(\delta).       Möbius inversion :\sum_d\left(\frac\right)2^=d^2(n).       :\sum_\lambda(\delta)=\begin &1\text n \text\\ &0\text n \text \end     where λ is the
Liouville function The Liouville Lambda function, denoted by λ(''n'') and named after Joseph Liouville, is an important arithmetic function. Its value is +1 if ''n'' is the product of an even number of prime numbers, and −1 if it is the product of an odd number o ...
. :\sum_\Lambda(\delta) = \log n.       ::\Lambda(n)=\sum_\mu\left(\frac\right)\log(\delta).       Möbius inversion


Sums of squares

For all k \ge 4,\;\;\; r_k(n) > 0.     (
Lagrange's four-square theorem Lagrange's four-square theorem, also known as Bachet's conjecture, states that every natural number can be represented as the sum of four integer squares. That is, the squares form an additive basis of order four. p = a_0^2 + a_1^2 + a_2^2 + a_ ...
). : r_2(n) = 4\sum_\left(\frac\right), where the
Kronecker symbol In number theory, the Kronecker symbol, written as \left(\frac an\right) or (a, n), is a generalization of the Jacobi symbol to all integers n. It was introduced by . Definition Let n be a non-zero integer, with prime factorization :n=u \cdo ...
has the values : \left(\frac\right) = \begin +1&\textn\equiv 1 \pmod 4 \\ -1&\textn\equiv 3 \pmod 4\\ \;\;\;0&\textn\text.\\ \end There is a formula for r3 in the section on class numbers below. r_4(n) = 8 \sum_d = 8 (2+(-1)^n)\sum_d = \begin 8\sigma(n)&\text n \text\\ 24\sigma\left(\frac\right)&\text n \text \end, where .     r_6(n) = 16 \sum_ \chi\left(\frac\right)d^2 - 4\sum_ \chi(d)d^2, where \chi(n) = \left(\frac\right).Hardy & Wright, § 20.13 Define the function as \sigma_k^*(n) = (-1)^\sum_(-1)^d d^k= \begin \sum_ d^k=\sigma_k(n)&\text n \text\\ \sum_d^k -\sum_d^k&\text n \text. \end That is, if ''n'' is odd, is the sum of the ''k''th powers of the divisors of ''n'', that is, and if ''n'' is even it is the sum of the ''k''th powers of the even divisors of ''n'' minus the sum of the ''k''th powers of the odd divisors of ''n''. :r_8(n) = 16\sigma_3^*(n).     Adopt the convention that Ramanujan's if ''x'' is not an integer. : r_(n) = \frac\sigma_^*(n) + \frac\left\    


Divisor sum convolutions

Here "convolution" does not mean "Dirichlet convolution" but instead refers to the formula for the coefficients of the product of two power series: : \left(\sum_^\infty a_n x^n\right)\left(\sum_^\infty b_n x^n\right) = \sum_^\infty \sum_^\infty a_i b_j x^ = \sum_^\infty \left(\sum_^n a_i b_\right) x^n = \sum_^\infty c_n x^n . The sequence c_n = \sum_^n a_i b_ is called the
convolution In mathematics (in particular, functional analysis), convolution is a mathematical operation on two functions ( and ) that produces a third function (f*g) that expresses how the shape of one is modified by the other. The term ''convolution'' ...
or the
Cauchy product In mathematics, more specifically in mathematical analysis, the Cauchy product is the discrete convolution of two infinite series. It is named after the French mathematician Augustin-Louis Cauchy. Definitions The Cauchy product may apply to infini ...
of the sequences ''a''''n'' and ''b''''n''.
These formulas may be proved analytically (see
Eisenstein series Eisenstein series, named after German mathematician Gotthold Eisenstein, are particular modular forms with infinite series expansions that may be written down directly. Originally defined for the modular group, Eisenstein series can be generaliz ...
) or by elementary methods. : \sigma_3(n) = \frac\left\.    Ramanujan, ''On Certain Arithmetical Functions'', Table IV; ''Papers'', p. 146 : \sigma_5(n) = \frac\left\.    Koblitz, ex. III.2.8 : \begin \sigma_7(n) &=\frac\left\\\ &=\sigma_3(n) + 120\sum_\sigma_3(k)\sigma_3(n-k). \end     : \begin \sigma_9(n) &= \frac\left\\\ &= \frac\left\. \end     : \tau(n) = \frac\sigma_(n) + \frac\sigma_(n) - \frac\sum_\sigma_5(k)\sigma_5(n-k),     where ''τ''(''n'') is Ramanujan's function.     Since ''σ''''k''(''n'') (for natural number ''k'') and ''τ''(''n'') are integers, the above formulas can be used to prove congruences for the functions. See
Ramanujan tau function The Ramanujan tau function, studied by , is the function \tau : \mathbb \rarr\mathbb defined by the following identity: :\sum_\tau(n)q^n=q\prod_\left(1-q^n\right)^ = q\phi(q)^ = \eta(z)^=\Delta(z), where with , \phi is the Euler function, is the ...
for some examples. Extend the domain of the partition function by setting : p(n)=\frac\sum_\sigma(k)p(n-k).       This recurrence can be used to compute ''p''(''n'').


Class number related

Peter Gustav Lejeune Dirichlet Johann Peter Gustav Lejeune Dirichlet (; 13 February 1805 – 5 May 1859) was a German mathematician who made deep contributions to number theory (including creating the field of analytic number theory), and to the theory of Fourier series and ...
discovered formulas that relate the class number ''h'' of
quadratic number field In algebraic number theory, a quadratic field is an algebraic number field of degree two over \mathbf, the rational numbers. Every such quadratic field is some \mathbf(\sqrt) where d is a (uniquely defined) square-free integer different from 0 a ...
s to the Jacobi symbol. An integer ''D'' is called a fundamental discriminant if it is the
discriminant In mathematics, the discriminant of a polynomial is a quantity that depends on the coefficients and allows deducing some properties of the roots without computing them. More precisely, it is a polynomial function of the coefficients of the origi ...
of a quadratic number field. This is equivalent to ''D'' ≠ 1 and either a) ''D'' is squarefree and ''D'' ≡ 1 (mod 4) or b) ''D'' ≡ 0 (mod 4), ''D''/4 is squarefree, and ''D''/4 ≡ 2 or 3 (mod 4). Extend the Jacobi symbol to accept even numbers in the "denominator" by defining the
Kronecker symbol In number theory, the Kronecker symbol, written as \left(\frac an\right) or (a, n), is a generalization of the Jacobi symbol to all integers n. It was introduced by . Definition Let n be a non-zero integer, with prime factorization :n=u \cdo ...
: \left(\frac\right) = \begin \;\;\,0&\text a \text \\(-1)^&\texta \text \end Then if ''D'' < −4 is a fundamental discriminant \begin h(D) & = \frac \sum_^r\left(\frac\right)\\ & = \frac \sum_^\left(\frac\right). \end There is also a formula relating ''r''3 and ''h''. Again, let ''D'' be a fundamental discriminant, ''D'' < −4. Then r_3(, D, ) = 12\left(1-\left(\frac\right)\right)h(D).


Prime-count related

Let H_n = 1 + \frac 1 2 + \frac 1 3 + \cdots +\frac   be the ''n''th
harmonic number In mathematics, the -th harmonic number is the sum of the reciprocals of the first natural numbers: H_n= 1+\frac+\frac+\cdots+\frac =\sum_^n \frac. Starting from , the sequence of harmonic numbers begins: 1, \frac, \frac, \frac, \frac, \dot ...
. Then : \sigma(n) \le H_n + e^\log H_n   is true for every natural number ''n'' if and only if the Riemann hypothesis is true.     The Riemann hypothesis is also equivalent to the statement that, for all ''n'' > 5040, \sigma(n) < e^\gamma n \log \log n (where γ is the
Euler–Mascheroni constant Euler's constant (sometimes also called the Euler–Mascheroni constant) is a mathematical constant usually denoted by the lowercase Greek letter gamma (). It is defined as the limiting difference between the harmonic series and the natural lo ...
). This is Robin's theorem. :\sum_\nu_p(n) = \Omega(n). :\psi(x)=\sum_\Lambda(n).     :\Pi(x)= \sum_\frac.     :e^=\prod_p.     :e^= \operatorname ,2,\dots,\lfloor x\rfloor    


Menon's identity

In 1965 P Kesava Menon proved \sum_ \gcd(k-1,n)=\varphi(n)d(n). This has been generalized by a number of mathematicians. For example, * B. Sury \sum_ \gcd(k_1-1,k_2,\dots,k_s,n) = \varphi(n)\sigma_(n). * N. Rao \sum_ \gcd(k_1-a_1,k_2-a_2,\dots,k_s-a_s,n)^s =J_s(n)d(n), where ''a''1, ''a''2, ..., ''a''''s'' are integers, gcd(''a''1, ''a''2, ..., ''a''''s'', ''n'') = 1. * László Fejes Tóth \sum_ \gcd(k^2-1,m_1)\gcd(k^2-1,m_2) =\varphi(n)\sum_ \varphi(\gcd(d_1, d_2))2^, where ''m''1 and ''m''2 are odd, ''m'' = lcm(''m''1, ''m''2). In fact, if ''f'' is any arithmetical function \sum_ f(\gcd(k-1,n)) =\varphi(n)\sum_\frac, where * stands for Dirichlet convolution.


Miscellaneous

Let ''m'' and ''n'' be distinct, odd, and positive. Then the Jacobi symbol satisfies the law of
quadratic reciprocity In number theory, the law of quadratic reciprocity is a theorem about modular arithmetic that gives conditions for the solvability of quadratic equations modulo prime numbers. Due to its subtlety, it has many formulations, but the most standard st ...
: \left(\frac\right) \left(\frac\right) = (-1)^. Let ''D''(''n'') be the arithmetic derivative. Then the logarithmic derivative \frac = \sum_ \frac . See
Arithmetic derivative In number theory, the Lagarias arithmetic derivative or number derivative is a function defined for integers, based on prime factorization, by analogy with the product rule for the derivative of a function that is used in mathematical analysis. ...
for details. Let ''λ''(''n'') be Liouville's function. Then :, \lambda(n), \mu(n) =\lambda(n), \mu(n), = \mu(n),     and :\lambda(n)\mu(n) = , \mu(n), =\mu^2(n).     Let ''λ''(''n'') be Carmichael's function. Then :\lambda(n)\mid \phi(n).     Further, :\lambda(n)= \phi(n) \textn=\begin 1,2, 4;\\ 3,5,7,9,11, \ldots \text p^k \textp\text;\\ 6,10,14,18,\ldots \text 2p^k\textp\text. \end See
Multiplicative group of integers modulo n In modular arithmetic, the integers coprime (relatively prime) to ''n'' from the set \ of ''n'' non-negative integers form a group under multiplication modulo ''n'', called the multiplicative group of integers modulo ''n''. Equivalently, the el ...
and
Primitive root modulo n In modular arithmetic, a number is a primitive root modulo  if every number coprime to is congruent to a power of modulo . That is, is a ''primitive root modulo''  if for every integer coprime to , there is some integer for which ...
.   :2^ \le d(n) \le 2^.     :\frac<\frac < 1.     :\begin c_q(n) &=\frac\phi(q)\\ &=\sum_\mu\left(\frac\right)\delta. \end         Note that  \phi(q) = \sum_\mu\left(\frac\right)\delta.     :c_q(1) = \mu(q). :c_q(q) = \phi(q). :\sum_d^(\delta) = \left(\sum_d(\delta)\right)^2.       Compare this with :d(uv) = \sum_\mu(\delta)d\left(\frac\right)d\left(\frac\right).     :\sigma_k(u)\sigma_k(v) = \sum_\delta^k\sigma_k\left(\frac\right).     :\tau(u)\tau(v) = \sum_\delta^\tau\left(\frac\right),     where ''τ''(''n'') is Ramanujan's function.    Apostol, ''Modular Functions ...'', ch. 6 eq. 3


First 100 values of some arithmetic functions


Notes


References

* * * * * * * * * * * * * * * * * *


Further reading

*


External links

* * Matthew Holden, Michael Orrison, Michael Varbl
Yet another Generalization of Euler's Totient Function
* Huard, Ou, Spearman, and Williams
Elementary Evaluation of Certain Convolution Sums Involving Divisor Functions
* Dineva, Rosica
The Euler Totient, the Möbius, and the Divisor Functions
* László Tóth
Menon's Identity and arithmetical sums representing functions of several variables
{{Authority control Functions and mappings