Null Well Class Effects on Pulse Diameter

Null Well Class Effects on Pulse Diameter is the book's classification of how a Null Well, by its geometry and spin, sets the base Pulse Diameter PD₀ and the harmonic signature of the universe that emerges from it. A Null Well is what contemporary physics calls a black hole. The book lists four classes. Schwarzschild (non-rotating): baseline PD₀, isotropic signature. Kerr (rotating): PD₀ shortened, mild anisotropy. Extreme Kerr (near-maximal spin): PD₀ near its minimal bound, strong anisotropy. Binary merger (two Kerr-type holes): PD₀ compressed through mass-energy summation and spin injection, with multi-harmonic offsets and anisotropic early expansion. A binary Kerr–Kerr merger gives a PD₀ shorter than either progenitor could alone: the summed mass deepens the potential well, spin injection adds frame-dragging that tightens harmonic closure, and gravitational-wave interference embeds a permanent anisotropic bias in the closure geometry. The Pulse Diameter is the spatial width of the pulse; the time to cross it is the Pulse Rhythm, so a shorter diameter means a faster rhythm and a shorter Local Pulse Tempo, ①⥂⧗'⌂ = 2·①⊕'⌂/𝒞→'⌂. The book reads this as time being an inherited quantity: every tick of a universe's clock carries the imprint of the Null Well that spawned it, preserved through Pulse Diameter inheritance. It connects to Pulse Diameter Definition, Pulse Rhythm Definition, Null Well Collision Channel Classification, Binary Kerr–Kerr Merger Origin and Multi-Harmonic Offsets.