The Type A/B minimal-depth spectrum is infinite and co-infinite

Theorem · hosted from the CENTL repository

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Theorem

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Status: proved synthesis theorem

Date: 2026-08-14

Project: Free Computation Foundation / CENTL

Claim boundary: this theorem concerns the minimal depth spectrum inside López Type A/B congruence solutions. It does not prove that every prime has finite C_AB, and it does not prove the Erdős-Straus conjecture. Literature priority for this spectrum formulation remains under review.

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1. Spectrum

Define the prime minimal-depth spectrum

\mathcal D_{\mathbb P} = \{k\ge1:\exists\text{ prime }p\text{ with }C_{AB}(p)=k\}.

Define also the hard-class infinite-realization spectrum

\mathcal D_H = \{k:\text{infinitely many primes }p\equiv h\pmod{840} \text{ for some }h\in H\text{ satisfy }C_{AB}(p)=k\}.

The prime-modulus backbone and the Mersenne shadow lattice give opposite infinite families.

2. Infinite realized side

Let

q=4k-1

be prime with q>7.

The prime-modulus backbone theorem gives a target Type A/B candidate at depth k whose target modulus is a new CRT coordinate relative to all previous layers. Finite congruence avoidance plus Dirichlet then gives infinitely many primes, even in the hard class

p\equiv1\pmod{840},

with

\boxed{C_{AB}(p)=k.}

There are infinitely many primes

q\equiv3\pmod4,

so there are infinitely many such depths

k=(q+1)/4.

Therefore

\boxed{\mathcal D_H\text{ is infinite}.}

In particular

\boxed{\mathcal D_{\mathbb P}\text{ is infinite}.}

3. Infinite impossible side

The Mersenne shadow theorem gives, for a,b>=1,

a+2\mid b+2, \quad a<b \Longrightarrow T_{2^b}\text{ is completely shadowed by }T_{2^a}.

Hence

\boxed{C_{AB}(n)\ne2^b}

for every integer n whenever such a proper divisor relation exists.

In particular, for every r>=2, take

b=3r-2.

Then

3\mid b+2,

so depth

\boxed{2^{3r-2}}

is completely shadowed by depth 2.

Thus there are infinitely many positive integers k that are not a minimal Type A/B depth for any integer, and therefore certainly not for any prime.

Hence

\boxed{\mathbb N\setminus\mathcal D_{\mathbb P}\text{ is infinite}.}

The same global gaps are absent from the hard-class spectrum, so

\boxed{\mathbb N\setminus\mathcal D_H\text{ is infinite}.}

4. Spectrum theorem

Combining the two sides:

Theorem

The Type A/B minimal-depth spectrum is infinite and co-infinite:

\boxed{

|\mathcal D_{\mathbb P}|=\infty, \qquad

|\mathbb N\setminus\mathcal D_{\mathbb P}|=\infty. }</div>

Moreover the hard-class infinite-realization spectrum is also infinite and co-infinite:

\boxed{

|\mathcal D_H|=\infty, \qquad

|\mathbb N\setminus\mathcal D_H|=\infty. }</div>

5. Stronger binary subsequence statement

Inside the subsequence of depths

k=2^b,

the Mersenne theorem proves that every b>=3 with composite b+2 is structurally impossible.

Only b+2 prime can escape that particular obstruction.

Therefore, if

E(B)=\#\{b\le B:2^b\text{ survives the Mersenne obstruction}\},

then

E(B)\le\pi(B+2)+O(1),

and hence

\boxed{E(B)/B\to0.}

So the complement of the spectrum occupies a density-one set of exponents inside this explicit sparse subsequence.

6. Conceptual meaning

The minimal Type A/B depth parameter is therefore not simply an unbounded complexity statistic whose every sufficiently large value eventually appears.

Its spectrum has two permanent arithmetic forces:

  1. arrival: independent prime-modulus coordinates create infinitely many realizable exact depths;
  2. deletion: modulus ancestry and exact trap containment create infinitely many structurally forbidden depths.

Thus the object is naturally a genuine arithmetic spectrum with both infinite support and infinite holes.

7. Paper-level consequence

The depth program can now state a clean unconditional theorem package:

\boxed{ \begin{array}{c} C_{AB}\text{ has unbounded finite values};\\ \text{infinitely many depths are infinitely prime-realizable};\\ \text{infinitely many depths are structurally impossible};\\ \text{therefore the minimal-depth spectrum is infinite and co-infinite.} \end{array} }

This is independent of whether López's universal Type A/B coverage conjecture is ultimately true.

Even if every prime has finite C_AB, the set of values taken by C_AB still has an infinite deterministic gap structure.

8. Next questions

  • What is the density of the spectrum among all positive depths?
  • Can additional infinite shadow lattices enlarge the known complement?
  • Can every non-shadowed depth be shown to lie in the spectrum under universal DSC-P?
  • What is the asymptotic counting function
D(X)=|\mathcal D_{\mathbb P}\cap[1,X]|?
  • How does the spectrum decompose into prime-modulus backbone values, composite-rescue values, and structural gaps?