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Dirichlet convolution

The Dirichlet convolution, also known as divisor convolution, is a fundamental in defined on the set of arithmetic functions, which are functions from the positive integers to the complex numbers. For two arithmetic functions f and g, their Dirichlet convolution (f \ast g) is defined by (f \ast g)(n) = \sum_{d \mid n} f(d) \, g\left(\frac{n}{d}\right) for each positive integer n, where the sum runs over all positive divisors d of n. This operation was developed in the early 19th century by as part of his foundational work in . The Dirichlet convolution is both commutative, satisfying f \ast g = g \ast f, and associative, allowing (f \ast g) \ast h = f \ast (g \ast h) for any functions f, g, h. Together with pointwise addition, it endows the set of arithmetic functions with a structure, where the constant function \delta(n) = 1 if n=1 and $0 otherwise serves as the multiplicative identity, since f \ast \delta = f for any f. If f and g are multiplicative functions—meaning f(mn) = f(m)f(n) and similarly for g whenever \gcd(m,n)=1—then f \ast g is also multiplicative. One of the most notable applications of Dirichlet convolution is in the theory of , where the product of two such series corresponds exactly to the convolution of their coefficient functions, facilitating the analysis of sums over divisors. It also underpins inversion, a cornerstone of inversion formulas in : if g(n) = \sum_{d \mid n} f(d), then f(n) = \sum_{d \mid n} \mu(d) \, g(n/d), where \mu is the , the Dirichlet inverse of the constant function $1(n)=1. These properties have made Dirichlet convolution indispensable for studying prime distributions, zeta functions, and other arithmetic phenomena.

Fundamentals

Definition

Arithmetic functions are functions f: \mathbb{N} \to \mathbb{C} defined on the positive integers \mathbb{N} with values in the complex numbers \mathbb{C}. The Dirichlet convolution is a binary operation on pairs of such arithmetic functions f and g, denoted (f * g)(n) and defined for each positive integer n by (f * g)(n) = \sum_{d \mid n} f(d) \, g\left(\frac{n}{d}\right), where the sum runs over all positive divisors d of n. This operation is defined over the domain of positive integers and produces another arithmetic function with range in \mathbb{C}. It serves as an analog to ordinary convolution but adapted to the multiplicative structure of the positive integers, facilitating the study of arithmetic functions under divisor summation.

Basic Properties

The Dirichlet convolution operation exhibits several fundamental algebraic properties that render it a powerful tool in the study of arithmetic functions. These properties include commutativity, associativity, and the existence of an , which collectively establish a rich structural framework. The operation is commutative, meaning that for any arithmetic functions f and g, (f * g)(n) = (g * f)(n) for all positive integers n. This follows directly from the symmetry in the convolution sum, where the terms f(d)g(n/d) and g(d)f(n/d) pair identically over the divisors d of n. Similarly, Dirichlet convolution is associative: (f * (g * h))(n) = ((f * g) * h)(n) for all arithmetic functions f, g, h and all n. Associativity arises from the ability to regroup the triple sum over divisors in the nested convolutions, ensuring the order of does not affect the result. An exists under this operation, given by the unit function \delta, defined as \delta(n) = 1 if n = 1 and \delta(n) = 0 otherwise. For any f, the satisfies (\delta * f)(n) = f(n) = (f * \delta)(n) for all n, as the reduces to the single term where d=1 and n/d = n. These properties—commutativity, associativity, and the —imply that the set of all functions, equipped with Dirichlet convolution, forms a commutative . Furthermore, Dirichlet convolution preserves multiplicativity: if both f and g are multiplicative functions (i.e., f(mn) = f(m)f(n) and g(mn) = g(m)g(n) whenever \gcd(m,n)=1), then their convolution f * g is also multiplicative. This preservation stems from the fact that, for coprime m and n, the divisors of mn factor uniquely into divisors of m and n, allowing the convolution sum to separate multiplicatively.

Dirichlet Inverse

Construction

The Dirichlet inverse of an arithmetic function f with f(1) \neq 0 is defined as the arithmetic function f^{-1} satisfying f * f^{-1} = \varepsilon = f^{-1} * f, where * denotes the Dirichlet convolution and \varepsilon is the multiplicative identity function given by \varepsilon(1) = 1 and \varepsilon(n) = 0 for all integers n > 1. This inverse exists and is unique within the set of arithmetic functions under Dirichlet convolution, forming an abelian group structure for all such invertible elements. The condition f(1) \neq 0 ensures invertibility, as the value at 1 determines the group's unit compatibility. To compute f^{-1}, a recursive formula is used, leveraging the definition at the . Specifically, f^{-1}(1) = 1 / f(1). For n > 1, f^{-1}(n) = -\frac{1}{f(1)} \sum_{\substack{d \mid n \\ d < n}} f(d) \, f^{-1}\left( \frac{n}{d} \right). This recursion proceeds by induction on n, computing values in order of increasing magnitude since the sum involves previously determined terms for proper divisors. An equivalent form interchanges the arguments in the summand due to the commutativity of Dirichlet convolution. For multiplicative functions, the construction preserves multiplicativity. If f is multiplicative and f(1) \neq 0, then f^{-1} is also multiplicative, as the convolution of multiplicative functions yields another multiplicative function, and the identity \varepsilon is multiplicative. This follows directly from the recursive formula, since values at prime powers determine the function completely, and the recursion respects the multiplicative structure. As a direct consequence of the inverse's existence, the general Möbius inversion principle holds: if g(n) = \sum_{d \mid n} f(d) h(n/d) for arithmetic functions f and h with f(1) \neq 0, then h(n) = \sum_{d \mid n} f^{-1}(d) g(n/d). This generalizes the classical by replacing the constant function 1 (whose inverse is the \mu) with arbitrary invertible f.

Examples

A prominent example of Dirichlet convolution involves the constant arithmetic function \zeta(n) = 1 for all positive integers n, often referred to as the in the context of arithmetic functions. The convolution \zeta * \zeta yields the divisor function \sigma_0(n), which counts the number of positive divisors of n. For instance, \sigma_0(1) = 1, \sigma_0(2) = 2, \sigma_0(4) = 3, and \sigma_0(6) = 4. The Dirichlet inverse of the constant function \zeta is the Möbius function \mu, defined as \mu(1) = 1, \mu(p) = -1 for any prime p, \mu(p^k) = 0 for prime powers with k \geq 2, and \mu(n) = 0 if n has a squared prime factor (i.e., n is not square-free); otherwise, \mu(n) = (-1)^r where r is the number of distinct prime factors of n. This inverse property is verified by the convolution \mu * \zeta = \varepsilon, where \varepsilon is the unit function with \varepsilon(1) = 1 and \varepsilon(n) = 0 for n > 1. The following table computes (\mu * \zeta)(n) for small values of n:
nDivisors d of nTerms \sum_{d \mid n} \mu(d) \zeta(n/d)(\mu * \zeta)(n)
11\mu(1) \zeta(1) = 1 \cdot 1 = 11
21, 2\mu(1) \zeta(2) + \mu(2) \zeta(1) = 1 \cdot 1 + (-1) \cdot 1 = 00
31, 3\mu(1) \zeta(3) + \mu(3) \zeta(1) = 1 \cdot 1 + (-1) \cdot 1 = 00
41, 2, 4\mu(1) \zeta(4) + \mu(2) \zeta(2) + \mu(4) \zeta(1) = 1 \cdot 1 + (-1) \cdot 1 + 0 \cdot 1 = 00
61, 2, 3, 6\mu(1) \zeta(6) + \mu(2) \zeta(3) + \mu(3) \zeta(2) + \mu(6) \zeta(1) = 1 \cdot 1 + (-1) \cdot 1 + (-1) \cdot 1 + 1 \cdot 1 = 00
Another illustrative example is the Dirichlet inverse of the \mathrm{id}(n) = n, which is the function \mathrm{id}^{-1}(n) = \mu(n) \, n. This follows from the multiplicative structure under Dirichlet convolution and the role of \mu as the inverse of \zeta.

Key Formulas

The Dirichlet inverse exhibits several key identities that underscore its within the of arithmetic functions equipped with Dirichlet . A prominent property concerns powers of : if f^{k} denotes the k-fold Dirichlet of an invertible arithmetic function f with itself (with f^{1} = f and f^{0} the \epsilon where \epsilon(1)=1 and \epsilon(n)=0 for n>1), then the satisfies (f^{k})^{-1} = (f^{-1})^{k}. This follows from the associativity and of inverses in the , ensuring that f^{k} * (f^{-1})^{k} = \epsilon. Another central identity links the Dirichlet inverse to Möbius inversion, which inverts the operation of forming summatory functions over divisors. Specifically, if g(n) = (f * \mathbf{1})(n) = \sum_{d \mid n} f(d) where \mathbf{1}(n) = 1 for all positive integers n, then the recovers f via f(n) = \sum_{d \mid n} \mu(d) \, g\left(\frac{n}{d}\right), with \mu denoting the (the Dirichlet of \mathbf{1}). In convolution form, f = g * \mu, providing the recovery of f from g. The also respects products under : if f = g * h where g and h are invertible arithmetic functions (requiring g(1) \neq 0 and h(1) \neq 0), then f^{-1} = h^{-1} * g^{-1}. Commutativity of the operation implies the order is interchangeable, and this identity arises from the group structure of invertible functions under . Finally, the Dirichlet inverse connects naturally to generating functions through . The map sending an arithmetic function f to its D_{f}(s) = \sum_{n=1}^{\infty} f(n) n^{-s} (for \operatorname{Re}(s) sufficiently large) is a ring isomorphism from the ring to the multiplicative structure of formal , under which f^{-1} maps to the reciprocal $1 / D_{f}(s). This representation facilitates analytic manipulations without expanding the full series form.

Connections to Dirichlet Series

Convolution Theorem

The convolution theorem establishes a fundamental connection between the Dirichlet convolution of two arithmetic functions and the multiplication of their associated . Specifically, for arithmetic functions f and g, let D_f(s) = \sum_{n=1}^\infty \frac{f(n)}{n^s} and D_g(s) = \sum_{n=1}^\infty \frac{g(n)}{n^s} denote the generated by f and g, respectively. If these series converge absolutely for \operatorname{Re}(s) > \sigma, then the for the convolution f * g satisfies D_{f * g}(s) = D_f(s) \cdot D_g(s) for all such s. The absolute convergence of D_f(s) and D_g(s) ensures that the product series can be rearranged without altering its value, leading to term-by-term multiplication that yields the series for f * g. To see this, expand the product: D_f(s) \cdot D_g(s) = \sum_{m=1}^\infty \sum_{n=1}^\infty \frac{f(m) g(n)}{(mn)^s} = \sum_{k=1}^\infty \left( \sum_{mn=k} f(m) g(n) \right) \frac{1}{k^s} = \sum_{k=1}^\infty \frac{(f * g)(k)}{k^s}, where the inner sum is over divisors d \mid k with m = d and n = k/d. implies \sum_{k=1}^\infty \left| \frac{(f * g)(k)}{k^s} \right| \leq \left( \sum_{m=1}^\infty \left| \frac{f(m)}{m^s} \right| \right) \left( \sum_{n=1}^\infty \left| \frac{g(n)}{n^s} \right| \right) < \infty, guaranteeing the absolute convergence of D_{f * g}(s). The half-plane of for D_{f * g}(s) is thus determined by the maximum of the abscissae of for D_f(s) and D_g(s), typically \operatorname{Re}(s) > \max(\sigma_a(f), \sigma_a(g)), where \sigma_a denotes the abscissa. A notable special case arises with the \zeta(s) = \sum_{n=1}^\infty \frac{1}{n^s} = D_{\mathbf{1}}(s), where \mathbf{1}(n) = 1 for all n. The Dirichlet convolution inverse of \mathbf{1} is the \mu, satisfying \mathbf{1} * \mu = \epsilon (the with \epsilon(1) = 1 and \epsilon(n) = 0 for n > 1). By the , the for \mu is D_\mu(s) = 1 / \zeta(s), which holds in the half-plane \operatorname{Re}(s) > 1 where \zeta(s) converges absolutely and is nonzero.

Analytic Applications

The convolution theorem for Dirichlet series states that if F(s) = \sum_{n=1}^\infty f(n) n^{-s} and G(s) = \sum_{n=1}^\infty g(n) n^{-s} are the associated , then the series for the Dirichlet convolution (f * g)(n) = \sum_{d \mid n} f(d) g(n/d) is F(s) G(s). This multiplicative property facilitates the transfer of analytic properties from individual series to their convolutions, enabling techniques such as and asymptotic evaluation in . A prominent application arises in the analytic continuation of products of . For instance, the \zeta(s) = \sum_{n=1}^\infty n^{-s} has an Euler product representation \zeta(s) = \prod_p (1 - p^{-s})^{-1} for \Re(s) > 1, and its reciprocal is \frac{1}{\zeta(s)} = \prod_p (1 - p^{-s}) = \sum_{n=1}^\infty \mu(n) n^{-s}, where \mu is the . This equality reflects the Dirichlet convolution identity $1 * \mu = \varepsilon, where $1(n) = 1 for all n and \varepsilon is the unit function (\varepsilon(1) = 1, \varepsilon(n) = 0 for n > 1). The meromorphic continuation of \zeta(s) to the , with a simple pole at s=1, thus extends to \frac{1}{\zeta(s)}, which is entire except for zeros corresponding to those of \zeta(s). This structure underpins derivations of zero-free regions and residue computations essential for asymptotic estimates. Partial summation and Abel summation formulas extend naturally to convolutions via their Dirichlet series representations. Partial summation, akin to integration by parts, relates the sum \sum_{n \leq x} (f * g)(n) to integrals involving the partial sums of f and g, often after applying the convolution theorem to express the sum in terms of F(s) G(s). For example, if A(y) = \sum_{n \leq y} a(n) and b(n) is an arithmetic function, Abel's formula yields \sum_{n \leq x} a(n) b(n) = A(x) b(x) - \int_1^x A(t) b'(t) \, dt, which, when adapted to convolutions, facilitates error term analysis in summatory functions like the divisor problem. This technique preserves growth rates and bounds when convolving functions with known Dirichlet series abscissae. Perron's formula provides a precise tool for approximating sums of convolutions through contour integrals. Specifically, for an arithmetic function h(n) = (f * g)(n) with Dirichlet series H(s) = F(s) G(s) analytic in \Re(s) > \sigma_0 and bounded appropriately, \sum_{n \leq x} h(n) = \frac{1}{2\pi i} \int_{c - iT}^{c + iT} H(s) \frac{x^s}{s} \, ds + O\left( \frac{x^{c} |H(c + i t)|}{T} \sum_{n \leq x} \frac{|h(n)|}{n^{c}} \right), where c > \sigma_0 and T > 0. Shifting the contour to exploit poles and residues of H(s) yields main terms from residues at singularities, such as those of \zeta(s), while error terms are controlled via growth estimates on vertical lines. This method is pivotal for deriving asymptotics like \sum_{n \leq x} (f * g)(n) \sim \Res_{s=1} F(s) G(s) \frac{x^s}{s} when H(s) has a pole at s=1. In the context of the prime number theorem, the relation \log n = \sum_{d \mid n} \Lambda(d), or equivalently \log = \mathbf{1} * \Lambda—where \Lambda is the von Mangoldt function (\Lambda(n) = \log p if n = p^k for prime p, else 0)—with inversion yielding \Lambda = \mu * \log, since \mu is the Dirichlet inverse of the constant function \mathbf{1}(n)=1. The corresponding Dirichlet series are \sum \Lambda(n) n^{-s} = -\frac{\zeta'(s)}{\zeta(s)} and \sum \mu(n) n^{-s} = \frac{1}{\zeta(s)}, with \sum \log n \, n^{-s} = -\zeta'(s), consistent via the convolution theorem as D_{\mathbf{1}} \cdot D_\Lambda = \zeta(s) \cdot \left(-\frac{\zeta'(s)}{\zeta(s)}\right) = -\zeta'(s) = D_{\log}. The , stating \pi(x) \sim x / \log x or equivalently \psi(x) = \sum_{n \leq x} \Lambda(n) \sim x, follows from the non-vanishing of \zeta(s) on \Re(s) = 1 (except at s=1), using these convolution relations to connect the growth of \psi(x) to the analytic behavior of \frac{\zeta'(s)}{\zeta(s)} via Tauberian theorems or explicit formulae. Dirichlet convolution also preserves key analytic properties of the associated series, particularly regarding abscissae of convergence. If F(s) and G(s) have abscissae of convergence \sigma_c(F) and \sigma_c(G), then the product H(s) = F(s) G(s) satisfies \sigma_c(H) \leq \sigma_c(F) + \sigma_c(G), ensuring that convolutions of functions with convergent series in half-planes maintain analyticity in a combined region. Similarly, for absolute convergence, \sigma_a(H) \leq \max(\sigma_a(F), \sigma_a(G)). This bound is sharp in general but can be refined under additional assumptions, such as when one series is a polynomial or has finite support, allowing control over the growth of convolutions in applications like sieve methods.

Broader Contexts

Arithmetic Functions

Arithmetic functions are functions f: \mathbb{N} \to \mathbb{C} defined on the positive integers with complex values, serving as the primary objects in upon which operations like Dirichlet convolution are defined. These functions are classified based on how they interact with the multiplicative structure of the positive integers, particularly regarding products mn of their arguments. Common classes include completely additive functions, where f(mn) = f(m) + f(n) holds for all positive integers m and n; an example is the function \Omega(n), which counts the total number of prime factors of n with multiplicity, satisfying \Omega(mn) = \Omega(m) + \Omega(n) regardless of whether m and n are coprime. Completely multiplicative functions, also called strongly multiplicative, satisfy f(mn) = f(m)f(n) for all m, n \in \mathbb{N}; the f(n) = n is such an example, as mn = m \cdot n. More generally, a function f is multiplicative if f(mn) = f(m)f(n) whenever \gcd(m,n) = 1; the Euler totient function \phi(n), which counts the integers up to n coprime to n, exemplifies this, as \phi(mn) = \phi(m)\phi(n) for coprime m and n, but not necessarily otherwise. The Dirichlet convolution preserves key structural properties among these classes of arithmetic functions. Specifically, the convolution of two multiplicative functions is again multiplicative, ensuring that the set of multiplicative functions forms a monoid under this operation. This preservation facilitates the study of convolutions within restricted subclasses, such as those closed under the operation. Dirichlet characters provide a prominent example of completely multiplicative arithmetic functions that are also periodic with period k (for modulus k > 1) and vanish at integers n with \gcd(n,k) > 1, defined by \chi(n) = 0 if \gcd(n,k) > 1 and extended multiplicatively otherwise, satisfying \chi(mn) = \chi(m)\chi(n) for all m,n. The set of such characters modulo k is finite and forms an under pointwise multiplication, highlighting their closure under related multiplicative structures, though convolution of characters corresponds to products in the group of Dirichlet series. Under Dirichlet convolution, the set of all functions forms a with , known as the Dirichlet ring, where addition is pointwise and the multiplicative identity is the function \varepsilon with \varepsilon(1) = 1 and \varepsilon(n) = 0 for n > 1. The units of this —functions admitting a convolutional —are precisely those arithmetic functions f satisfying f(1) \neq 0, as the of the f^{-1} requires f * f^{-1} = \varepsilon, which is guaranteed when f(1) \neq 0 via recursive construction over the primes. This condition ensures invertibility within the ring, with multiplicative functions among the units forming a when f(1) = 1.

Number-Theoretic Uses

The provides a cornerstone for applications of Dirichlet convolution in elementary . If arithmetic functions f and g satisfy g(n) = \sum_{d \mid n} f(d) for all positive integers n, then f(n) = \sum_{d \mid n} \mu(d) \, g(n/d), where \mu is the . This inversion directly applies to sums, such as the sum-of-divisors function \sigma(n) = \sum_{d \mid n} (n/d). Setting f(k) = k yields g(n) = \sigma(n), so gives the identity n = \sum_{d \mid n} \mu(d) \, \sigma(n/d). Dirichlet convolution also underpins inclusion-exclusion principles for counting certain , exemplified by square-free numbers. An n is square-free if no square divides it; the for this property equals \sum_{d^2 \mid n} \mu(d). Consequently, the count of square-free up to x is \sum_{n \leq x} \sum_{d^2 \mid n} \mu(d) = \sum_{d \geq 1} \mu(d) \left\lfloor x / d^2 \right\rfloor, capturing the over-subtraction and additions inherent in inclusion-exclusion via the signs of \mu. The Euler totient function \phi(n), counting integers up to n coprime to n, expresses as a Dirichlet convolution \phi = \mathrm{id} \ast \mu, where \mathrm{id}(n) = n. This relation implies the formula \phi(n) = n \sum_{d \mid n} \frac{\mu(d)}{d}, allowing computation of \phi(n) through Möbius values over divisors. In sieve methods, Dirichlet convolution formalizes relations akin to the sieve of Eratosthenes using indicator functions. For instance, the sieve identifies composites by marking multiples of primes, and inclusion-exclusion over prime powers employs \mu to correct counts; more advanced formulations express the von Mangoldt function \Lambda(n), which is \log p at primes p and 0 otherwise, as \Lambda = \mu \ast \log, enabling convolution-based manipulations for prime enumeration. For computational purposes with small n, Dirichlet convolutions (f \ast g)(n) = \sum_{d \mid n} f(d) \, g(n/d) are evaluated efficiently by enumerating divisors of n, as the \tau(n) grows slowly on average (\sum_{k=1}^N \tau(k) \sim N \log N), yielding total time O(N \log N) to compute the convolution up to N.

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