← Physics in Binary Pulse Theory
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Black hole
In Binary Pulse Theory: Null Well
Same thing, new nameIn standard physics
A region where gravity is so strong that nothing, not even light, escapes from inside its event horizon.
In Binary Pulse Theory
BPT calls it a Null Well. It is where collapse ends, but its core is a null state rather than infinite curvature, and it is not an end: a Null Well is the crucible of a child universe.
The BPT terms behind it
A Null Well is what contemporary physics calls a black hole: the book's name for it, and the book's reading of what it is. A Null Well is the collapse destination for structures that fail to achieve recursive closure within their time constraint, τ(m) > ⥂⌂: the point at which such a structure returns to the…
The Null Well State (S∅) is the complete computational void, the physical state as seen from outside, that holds at a position once its collapse time has passed: S∅(x,τ,n) = ∅ for every time τ later than the collapse time τ⇃(x,n,ℨ). A Null Well is what contemporary physics calls a black hole.
The Null Well Formation Condition is the rule that when local recursion at a point approaches the critical recursion threshold, the region passes into substrate nullity: ℜ(x,t,ℨ) → ℜ⨶(ℨ) ⇒ ∅▱. A Null Well is what contemporary physics calls a black hole.
The Null Well Reactivation Condition is the threshold for a Null Well to restart: the data energy accumulated at a position must reach or exceed the genesis data energy for its harmonic level, ↁ⚕⫷(x,n,ℨ) ≥ ↁ⚕⟨(n,ℨ). A Null Well is what contemporary physics calls a black hole.
Also known as
black holes · stellar black hole · supermassive black hole
Related
The standard physics term is here to help you find your way in; the book itself writes in BPT's own terms. Read them in the lexicon, or start the book at Binary Pulse Theory.