A Yagel number of order and exponent pushes the sieve idea behind
Mersenne numbers ("exclude divisibility by 2") to its logical extreme:
where is the -th prime and the primorial of its predecessor. Both
constants are dictated by the prime sequence itself — the family has no free parameters and is
indexed purely by the lattice point . Two classical families appear as the boundary of
the grid: row consists of the Mersenne numbers, and column of the
primorial numbers . The companion face
(the second kind) carries the Euclid and Fermat forms on its edges.
Three structural properties drive everything: for every
prime — the maximal built-in small-prime sieve for the base; no exponent is ever
algebraically disqualified, so every lattice cell is a live candidate (unlike the Mersenne row);
and is fully factored by construction, so every prime in the family admits a fast
deterministic certificate.
A Lucas–Lehmer-type test for every row
Primality of is decided by a single -only Lucas ladder — an -fold
iteration of the degree- Chebyshev-type map . For
the map is and the criterion collapses to the classical Lucas–Lehmer test
verbatim. The cost is about two multiplications per bit, and the output is a proof, not
a probability. The observed prime density across the grid matches the sieve-adjusted expectation
exactly — no free parameters, in aggregate and row by row.
Running that machinery forward produced 1,079 certified Yagel
primes — including with 18,664
digits, a certified census of both faces for , a first certified prime in
every row through (milestones to ), and 22 twin pairs with both
members proven. Explore any cell of the grid on the datasets page —
it computes the exact value in your browser.