For thresholds , write and similarly for the other truncations. Vaughan's identity isIt decomposes a sum weighted by into short, Type I, and Type II bilinear sums.
For reduced with and , the displayed bound follows by splitting Vaughan identity with parameters . Type I sums use short geometric-sum bounds; type II sums use the Cauchy-Schwarz inequality and rational spacing to control bilinear cancellation. A badly approximable number has a Dirichlet approximant with , yielding and hence .
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The Von Mangoldt function is nonnegative and satisfies . Therefore the middle short-divisor coefficient in the Vaughan identity has the displayed pointwise bound. Grouping its long-divisor term as , with , gives . This grouping permits bounded-coefficient Type II sums after division by .
The displayed identity is exact for all positive integers and all positive cutoffs. Expand and use . The two truncated terms are short sums; the negative term is a type I sum over divisors at most ; the last term is a type II sum with both factor variables larger than a cutoff. This form of the Vaughan identity is specific to Möbius weights.
For , if and , the Vaughan identity for the Möbius function gives a type I sum or a type II sum of modulus at least . The first is , with . The second is , with . Both coefficient sequences are bounded by the divisor function. Thus correlation forces either detection by small-modulus periodic indicators or a large multiplicatively organized bilinear sum, without claiming that itself is literally periodic or multiplicative.
For Dirichlet convolution, let and . Prime factorization gives and . With subscripts denoting truncation at ,Rearranging proves the Vaughan identity.
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Vaughan's identity is an important result in analytic number theory, particularly in the context of additive number theory and the study of sums of arithmetic functions. The identity provides a way to express the sum of a function over a set of integers in terms of more manageable sums and is often used in the context of problems involving the distribution of prime numbers.