In this paper, we show an analogue of Kural et al.'s result on Alladi's formula for global function fields. Explicitly, we show that for a global function field K, if a set S of prime divisors has a natural density δ(S) within prime divisors, thenwhere µ(D) is the Möbius function on divisors and D(K, S) is the set of all effective distinguishable divisors whose smallest prime factors are in S. As applications, we get the analogue of Dawsey's and Sweeting and Woo's results to the Chebotarev Density Theorem for function fields, and the analogue of Alladi's result to the Prime Polynomial Theorem for arithmetic progressions. We also display a connection between the Möbius function and the Fourier coefficients of modular form associated to elliptic curves. The proof of our main theorem is similar to the approach in Kural et al.'s article.where ϕ is Euler's totient function.Alladi's formula (3) shows a relationship between the Möbius function µ(n) and the density of primes in arithmetic progressions. In 2017, Dawsey [6] first generalized (3) to the setting of Chebotarev densities for finite Galois extensions of Q. Then Sweeting and Woo [17] generalized Dawsey's result to number fields. Recently, Kural et al. [12] generalized all these results to natural densities of sets of primes. The second author of this article showed the analogues of these results over Q for some arithmetic functions other than µ in [19,21,20]. In this paper, we will show the analogue of Kural et al.'s result over global function fields.Let p be a prime and let q be a power of prime p. Let F q be a finite field of q elements. Take K/F p (x) to be a finite extension with constant field F q , which is called a global function field (or simply a function field). A prime divisor (or simply a prime) in K is defined to be a discrete valuation ring R P with maximal ideal P such that F q ⊂ R P and the quotient field of R P is K. The norm of P , denote by |P |, is defined to be the size of the residue field κ P of R P , i.e. |P | = #(R P /P ) = #κ P , which is a power q deg P of the cardinality of the ground field F q . Here the exponent deg P is called the degree of P .