In mathematics, the classic Möbius inversion formula was introduced into number theory during the 19th century by August Ferdinand Möbius.
Other Möbius inversion formulas are obtained when different local finite partially ordered sets replace the classic case of the natural numbers ordered by divisibility; for an account of those, see incidence algebra.
Statement of the formula
The classic version states that if g(n) and f(n) are arithmetic functions satisfying
where μ is the Möbius function and the sums extend over all positive divisors d of n. In effect, the original f(n) can be determined given g(n) by using the inversion formula. The two sequences are said to be Möbius transforms of each other.
The formula is also correct if f and g are functions from the positive integers into some abelian group (viewed as a Z-module).
In the language of Dirichlet convolutions , the first formula may be written as
where * denotes the Dirichlet convolution, and 1 is the constant function 1(n) = 1. The second formula is then written as
Many specific examples are given in the article on multiplicative functions.
Given an arithmetic function, one can generate a bi-infinite sequence of other arithmetic functions by repeatedly applying the first summation.
For example, if one starts with Euler's totient function φ, and repeatedly applies the transformation process, one obtains:
If the starting function is the Möbius function itself, the list of functions is:
Both of these lists of functions extend infinitely in both directions. The Möbius inversion formula enables these lists to be traversed backwards. The generated sequences can perhaps be more easily understood by considering the corresponding Dirichlet series: each repeated application of the transform corresponds to multiplication by the Riemann zeta function.
An equivalent formulation of the inversion formula more useful in combinatorics is as follows: suppose F(x) and G(x) are complex-valued functions defined on the interval [1,∞) such that
Here the sums extend over all positive integers n which are less than or equal to x.
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