Gap Diagonal Identity
For the lattice $\{(r,M) : 1 \le r \le M \le G\}$, the fraction of pairs on the diagonal $|M-r|=g$ that are coprime equals $\varphi(g)/g$ — a direct consequence of Euler's totient function. The identity is classical; reading the lattice as a family of diagonal strips, each carrying its own density, gives a geometric way to decompose and visualize C(n).
At $n=0$, diagonal strip $g$ has coprime density exactly $\varphi(g)/g$ — a classical fact.
As $n$ grows, the block-coprime condition imposes additional constraints: a pair $(r, r+g)$ must
now satisfy $\gcd(r, r+g+j) = 1$ for $j = 0, \ldots, n$. This modifies the local density
on each strip by eliminating extra residue classes at each prime dividing $g, g+1, \ldots, g+n$.
The formula below gives the block-coprime density restricted to diagonal strip $g$ at depth $n$:
This per-strip formula describes how each diagonal behaves individually. The global C(n) is not exactly a weighted average of these per-strip densities, since that would require the strips to be independent — they aren't, as they share prime factors. The diagonal decomposition is a visualization and a close approximation rather than an exact identity once n>0.
- Geometric decomposition: reading the lattice as diagonal strips, each with its own density φ(g)/g, gives a visual explanation for why C(n)'s Euler product looks the way it does — each prime p contributes most strongly through the diagonals it divides.
- Classical foundation: the density φ(g)/g on diagonal g is a direct consequence of Euler's totient formula and periodicity.
- Hardy–Littlewood parallel: the per-strip block-coprime density is structurally similar to the local factors in Hardy–Littlewood's singular series for prime constellations. The Hardy–Littlewood conjecture itself remains unproven, and the parallel here is suggestive rather than a formal connection.
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