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lm-003877 · 2026-09

CSM_RH Paper 19 — Zero-Density Exponent Law, Shrinking-Strip Barrier, and Closure Back to the Fixed-Zero-Strip Core

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CSM_RH Paper 19

Zero-Density Exponent Law, Shrinking-Strip Barrier, and Closure Back to the Fixed-Zero-Strip Core

Project: CSM_RH
Paper: 19
Version: v0.1
Date: 2026-09-05
Parent state: CSM_RH v1.9 / Paper 18
Campaign: 18 — PRINCIPAL_FEJER_ARC_POWER_ATTACK
Status: current large-value / zero-density closure audit; not a proof or disproof of RH


0. Trust boundary

This paper does not prove or disprove the Riemann Hypothesis.

Canonical root state:

RH_PROVED = FALSE
RH_DISPROVED = FALSE
GLOBAL_RH_CERTIFICATE = FALSE
CSM_RH_ROOT_STATUS = OPEN

Campaign 18 asks whether current large-value, zero-density, exceptional-set, and explicit-formula techniques can upgrade the principal Fejer arc from subpower precision to a fixed power.

The answer for the currently audited absolute zero-density schema is negative.

The main result is an exponent law which separates:

range threshold
from
precision threshold

and shows why improving zero density alone does not create a fixed power while the zero-free gap still shrinks with height.

No live GLM-5.3-Flash run is claimed.


1. Direct theorem candidate

Paper 17 introduced MLEPG.

Let

A(x)=ψ(x)x.A(x)=\psi(x)-x.

Let

H=Xα,0<α<1.H=X^\alpha, \qquad 0<\alpha<1.

Define

SΛ(X,H)=xA(x+H)A(x)2\mathcal S_\Lambda(X,H) = \sum_x |A(x+H)-A(x)|^2

with an appropriate finite or smoothed range around XX.

MLEPG asks for

SΛ(X,H)XH(logX)O(1)+XH2Xδ+o(1)\boxed{ \mathcal S_\Lambda(X,H) \ll XH(\log X)^{O(1)} + XH^2X^{-\delta+o(1)} }

for one fixed

δ>0.\delta>0.

Paper 18 proved that the principal Fejer arc is a necessary subproblem.


2. Guth–Maynard already prove the subpower L2L^2 analogue

In the proof of their almost-all short-interval prime theorem, Guth and Maynard use the explicit formula and reduce the problem to an L2L^2 estimate for a zero packet.

Their equation (13.4) has the form

X3Xρ<Txρ(1+Δ)ρ1ρ2dxΔ2X3exp(c(logX)1/4),\boxed{ \int_X^{3X} \left| \sum_{|\rho|<T} x^\rho \frac{ (1+\Delta)^\rho-1 }{ \rho } \right|^2 dx \ll \Delta^2X^3 \exp \left( -c(\log X)^{1/4} \right), }

at the scale used in their proof.

Since

HΔX,H\asymp \Delta X,

the natural normalization is

Δ2X3=XH2.\Delta^2X^3 = XH^2.

Thus the current large-value method already proves the structural analogue

XH2×Xo(1).\boxed{ XH^2 \times X^{-o(1)}. }

The missing MLEPG input is exactly the replacement

Xo(1)Xδ.X^{-o(1)} \longrightarrow X^{-\delta}.

3. Abstract zero-density input

Assume an upper bound

N(σ,T)TA0(1σ)+o(1)\boxed{ N(\sigma,T) \ll T^{A_0(1-\sigma)+o(1)} }

uniformly at the exponent level, where

A0>0A_0>0

is fixed.

For Guth–Maynard,

A0=3013.\boxed{ A_0=\frac{30}{13}. }

Take

H=XαH=X^\alpha

and the explicit-formula truncation height

T=X1α+o(1).\boxed{ T=X^{1-\alpha+o(1)}. }

This is the natural short-interval scale

TX/HT\asymp X/H

up to subpower factors.


4. Zero-density exponent law

A zero with real part σ\sigma contributes at squared L2L^2 exponent scale

H2X2σ1H^2X^{2\sigma-1}

relative to an XX -length integration range.

Equivalently, relative to the baseline

XH2,XH^2,

the single-zero exponent factor is

X2(1σ).X^{-2(1-\sigma)}.

The density bound permits approximately

TA0(1σ)+o(1)=XA0(1α)(1σ)+o(1)T^{A_0(1-\sigma)+o(1)} = X^{A_0(1-\alpha)(1-\sigma)+o(1)}

zeros at that real-part scale.

Therefore the absolute zero-density contribution has exponent ratio

XcA0(α)(1σ)+o(1),\boxed{ X^{-c_{A_0}(\alpha)(1-\sigma)+o(1)}, }

where

cA0(α)=2A0(1α).\boxed{ c_{A_0}(\alpha) = 2 - A_0(1-\alpha). }

This is the canonical density-to- L2L^2 exponent law for the present audit.


5. Range threshold

The density schema yields decay in the real-part variable only if

cA0(α)>0.c_{A_0}(\alpha)>0.

Thus:

Theorem 5.1 — Zero-Density Range Threshold

α>12A0.\boxed{ \alpha > 1-\frac2{A_0}. }

For

A0=3013,A_0=\frac{30}{13},

we obtain

12A0=12630=215.\begin{aligned} 1-\frac2{A_0} &= 1-\frac{26}{30} \\ &= \boxed{ \frac2{15}. } \end{aligned}

This recovers the Guth–Maynard almost-all short-interval threshold at exponent level.

The threshold is therefore a density-balance phenomenon.


6. Shrinking zero-free boundary

Let the available zero-free region have the form

ρ1η(T),\boxed{ \Re\rho \le 1-\eta(T), }

where

η(T)>0\eta(T)>0

and

η(T)0\eta(T)\to0

as

T.T\to\infty.

The Vinogradov–Korobov region is of this type.

The worst permitted real part in the density exponent law is then

σ=1η(T).\sigma = 1-\eta(T).

Substituting into Section 4 gives the best exponent ratio available from the absolute density schema:

XcA0(α)η(T)+o(1).\boxed{ X^{-c_{A_0}(\alpha)\eta(T)+o(1)}. }

Because

η(T)0,\eta(T)\to0,

this is

Xo(1).\boxed{ X^{-o(1)}. }

It is not a fixed power.


7. Shrinking-Strip Barrier Theorem

Theorem 7.1

Fix

A0<A_0<\infty

and

α>12A0.\alpha > 1-\frac2{A_0}.

Consider an explicit-formula L2L^2 proof schema which:

  1. bounds zero contributions by absolute values or positive moments at each real-part scale;
  2. uses only the density estimateN(σ,T)TA0(1σ)+o(1);N(\sigma,T) \ll T^{A_0(1-\sigma)+o(1)};
  3. uses a zero-free boundaryρ1η(T)\Re\rho \le 1-\eta(T) withη(T)0.\eta(T)\to0.

Then the zero-density exponent law supplies at best a subpower factor

Xo(1)\boxed{ X^{-o(1)} }

over the baseline XH2XH^2.

It cannot by itself produce

XδX^{-\delta}

for fixed

δ>0.\delta>0.

This theorem is about the specified proof schema.

It is not a universal impossibility theorem for all uses of zeros.


8. Improving zero density alone does not solve the precision problem

Suppose the density hypothesis were available in the ideal form

A0=2.A_0=2.

Then the range threshold becomes

α>0.\alpha>0.

Thus almost-all short-interval coverage could, at the density-balance level, extend to every fixed positive power scale.

But the precision factor would still be

X2αη(T)+o(1)=Xo(1)X^{-2\alpha\eta(T)+o(1)} = X^{-o(1)}

whenever

η(T)0.\eta(T)\to0.

Therefore:

Corollary 8.1

Even an optimal density exponent does not, by itself, give MLEPG fixed-power precision unless one also obtains:

a fixed zero-free gap,
or
new cancellation / coefficient isolation beyond the absolute density schema.

This cleanly separates the density problem from the fixed-strip problem.


9. Guth–Maynard proof location

Guth and Maynard prove

N(σ,T)T30(1σ)/13+o(1)N(\sigma,T) \le T^{30(1-\sigma)/13+o(1)}

and use the Vinogradov–Korobov zero-free region in their prime-distribution corollaries.

In their almost-all short-interval proof they choose a truncation scale corresponding to the interval length and reduce the problem to the zero-packet L2L^2 estimate described in Section 2.

The final saving is subpower.

The exponent law in this paper explains structurally why the new density exponent changes the admissible short-interval range to 2/152/15 but does not generate a fixed XX -power.


10. Gafni–Tao exceptional-set framework

Gafni and Tao define, for fixed relative-error tolerance

δ>0,\delta>0,

an exceptional set of intervals where the short-interval PNT fails at that tolerance.

They then define exceptional-set exponents and derive explicit bounds from zero-density information.

This is strong quantitative information about the number of bad intervals.

However the parameter δ\delta in the theorem framework is fixed while XX tends to infinity.

By diagonalizing over fixed values

δ=1,12,13,,\delta=1,\frac12,\frac13,\ldots,

one obtains an o(H)o(H) error outside a density-zero set.

One does not obtain a polynomially shrinking threshold

HXη.HX^{-\eta}.

11. Fixed-threshold versus shrinking-threshold mismatch

Suppose for each fixed

ε>0\varepsilon>0

one proves

ΔHA(x)εH|\Delta_HA(x)| \le \varepsilon H

outside an exceptional set of power-saving size.

Then the good-set contribution to the lag energy is still

ε2XH2.\boxed{ \varepsilon^2XH^2. }

For fixed ε\varepsilon, this has no fixed XX -power saving.

Taking ε\varepsilon arbitrarily small after the theorem is proved does not create a bound

Xδ.X^{-\delta}.

To obtain MLEPG through a good/bad decomposition, one needs a threshold which shrinks quantitatively with XX, for example

ΔHA(x)HXη1\boxed{ |\Delta_HA(x)| \le HX^{-\eta_1} }

on the good set.

Create:

O-RH-043
FIXED_THRESHOLD_EXCEPTIONAL_SET_MISMATCH
status:
  CERTIFIED

12. Guth–Maynard and Gafni–Tao combined

The two technologies address different axes.

Guth–Maynard

Improves:

zero-density exponent;
large-value estimates;
range of short intervals;
subpower quantitative error.

Gafni–Tao

Improves:

quantification of exceptional-set size;
translation from zero-density / zero additive energy to bad-interval counts.

Neither currently supplies:

fixed-power shrinking error threshold in L2.\boxed{ \text{fixed-power shrinking error threshold in }L^2. }

Thus their combination does not currently prove MLEPG.


13. Density blindness to a fixed off-axis zero

For every fixed

β<1,\beta<1,

a density bound of the form

N(σ,T)TA0(1σ)+o(1)N(\sigma,T) \ll T^{A_0(1-\sigma)+o(1)}

permits finitely many zeros with real part β\beta.

A single such zero is negligible for the asymptotic count N(σ,T)N(\sigma,T).

Therefore density information alone cannot exclude a fixed off-axis zero.

But a fixed zero with real part

β\beta

has short-interval explicit-formula amplitude at the natural scale

HXβ1H X^{\beta-1}

and squared integrated scale

H2X2β1.H^2X^{2\beta-1}.

Thus fixed-power principal-arc / lag-energy control must ultimately be sensitive to individual persistent off-axis zero modes.

Create:

O-RH-044
ZERO_DENSITY_SINGLE_ZERO_BLINDNESS
status:
  CERTIFIED AS STRENGTH AUDIT

This is not a claim that one zero automatically gives a rigorous lower bound without a coefficient-recovery argument.

It records the information deficit of density estimates.


14. Closure back to the fixed-zero-strip core

Paper 17 gives the deterministic chain

MLEPG(α,δ)n2Nψ(n)n2N3κ+o(1)\operatorname{MLEPG}(\alpha,\delta) \Longrightarrow \sum_{n\le2N} |\psi(n)-n|^2 \ll N^{3-\kappa+o(1)}

for some

κ>0.\kappa>0.

At exponent level, a fixed zero

ρ=β+iγ\rho = \beta+i\gamma

contributes the scale

N2β+1N^{2\beta+1}

to the PNT mean-square explicit formula.

Thus the bound

N3κ+o(1)N^{3-\kappa+o(1)}

has the fixed-strip strength

β1κ2.\boxed{ \beta \le 1-\frac{\kappa}{2}. }

This is the same exponent law already encountered in the earlier ZPPF / principal zeta-packet campaigns.

Therefore the direct PESC branch has closed a loop:

PESC
  ->
MLEPG candidate
  ->
principal Fejer arc
  ->
explicit formula / zero density
  ->
fixed-zero-strip strength

The loop is not circular as a proof.

It is a closure-space strength identification.


15. New obstruction: density / strip decoupling

Create:

O-RH-042
ZERO_DENSITY_SHRINKING_STRIP_EXPONENT_BARRIER
status:
  CERTIFIED FOR ABSOLUTE EXPLICIT-FORMULA SCHEMA

Statement:

A finite zero-density exponent determines the short-interval range threshold through 2A0(1α)2-A_0(1-\alpha), but a shrinking zero-free boundary forces the resulting power gain to shrink to zero. Density improvement alone therefore cannot supply MLEPG fixed-power precision within the audited absolute explicit-formula schema.


16. Status of Campaign 18 tracks

P1 — Guth–Maynard large-value upgrade

status:
  CURRENT METHOD ALREADY PRODUCES L2 SUBPOWER

fixed power:
  NO

barrier:
  shrinking zero-free boundary in absolute density summation

P2 — Gafni–Tao exceptional-set optimization

status:
  STRONG EXCEPTIONAL-SET COUNTING

shrinking polynomial good-error threshold:
  NOT PROVIDED BY CURRENT FRAMEWORK

fixed-power L2:
  NO

P3 — principal Dirichlet-polynomial mean square

status:
  CURRENT LARGE-VALUE INPUT IMPROVES DENSITY/RANGE

single-zero-sensitive fixed power:
  NOT IDENTIFIED

P4 — smooth explicit-formula zero packet

status:
  STRENGTH AUDIT CONFIRMS FIXED-STRIP SCALE

new coefficient-isolation theorem:
  NOT PROVED

17. What a genuinely new input must do

Any successful next mechanism must be sensitive to a single persistent near- 11 zero.

Density-only information is insufficient.

The new input must do at least one of:

S1 — fixed zero-free gap

Directly prove

ρ1η0\Re\rho \le 1-\eta_0

for some fixed

η0>0.\eta_0>0.

S2 — coefficient recovery / isolation

Show that a persistent off-axis zero contributes a noncancellable amount to the principal Fejer / lag-energy observable.

Then MLEPG would exclude it.

S3 — phase-sensitive zero-packet coercivity

Use the structure of the zero packet beyond absolute counting to obtain a fixed-power lower/upper incompatibility.

S4 — new prime-side theorem independent of zero density

Prove MLEPG directly by arithmetic methods whose fixed power is not obtained by summing a density estimate.


18. New survivor

Create:

S-RH-027
SINGLE_ZERO_SENSITIVE_PRINCIPAL_ARC_MECHANISM
status:
  OPEN

Definition:

a theorem mechanism which can detect or exclude the contribution of one persistent off-axis zero in the principal Fejer / short-interval L2L^2 observable, rather than merely bound how many such zeros may exist.

This is a mechanism requirement.

It is not a new target.


19. Campaign 18 verdict

GUTH-MAYNARD ZERO DENSITY
  RANGE BREAKTHROUGH

GUTH-MAYNARD PRINCIPAL L2
  SUBPOWER

GAFNI-TAO EXCEPTIONAL SET
  POWER-SIZED BAD-SET INFORMATION POSSIBLE

GAFNI-TAO GOOD ERROR THRESHOLD
  FIXED / o(1), NOT POLYNOMIALLY SHRINKING

ABSOLUTE ZERO-DENSITY SCHEMA
  CANNOT CREATE FIXED POWER WITH SHRINKING ZERO-FREE GAP

DENSITY HYPOTHESIS ALONE
  STILL NOT ENOUGH FOR FIXED POWER

MLEPG
  OPEN

PESC
  OPEN

No fixed-power theorem is proved.


20. Campaign 19

The next campaign is:

CSM_RH Campaign 19
SINGLE_ZERO_SENSITIVE_THEOREM_GENERATION

The root target remains PESC.

The working theorem candidate remains MLEPG.

The new design constraint is:

every candidate mechanism must be capable of distinguishing
"no near-1 zero"
from
"one persistent near-1 zero".

Density-only candidates are rejected automatically.


21. Campaign 19 tracks

Z1 — multiscale coefficient recovery

Use principal Fejer energies over a family of scales HH to recover a fixed zero mode.

A valid proof must quantify the inverse map and control all other zeros.

Z2 — smooth Mellin packet coercivity

Replace the hard interval kernel by a smooth positive packet and test whether Mellin coefficients of individual zeros can be isolated with a fixed exponent.

Z3 — zero-pair Gram positivity with gauge control

Build a canonical zero-mode Gram form whose diagonal from one off-axis orbit cannot be removed by representation changes or uncontrolled cross terms.

Paper 07's Gram-gauge obstruction must be respected.

Z4 — prime-side multiscale contraction

Avoid zeros entirely and prove a fixed-power recurrence for lag energies across scales.

The recurrence must have linear cumulative contraction mass.


22. Campaign 19 rejection filters

Reject a candidate if:

R1. It uses only a zero-density count.

R2. It uses a shrinking zero-free region and calls the resulting subpower a fixed power.

R3. It controls exceptional-set size without a polynomially shrinking good-error threshold.

R4. It assumes a fixed zero-free strip.

R5. It ignores cancellation among zero modes in a coefficient-recovery claim.

R6. It creates a gauge-dependent Gram gap.

R7. It merely restates PESC / MLEPG.


23. External calibration

The present audit uses the following current results.

  1. Guth–Maynard, New large value estimates for Dirichlet polynomials, Annals of Mathematics 203 (2026), prove

    N(σ,T)T30(1σ)/13+o(1)N(\sigma,T) \le T^{30(1-\sigma)/13+o(1)}

    and obtain almost-all prime asymptotics for short intervals beginning at exponent 2/15+ε2/15+\varepsilon. Their proof reduces the almost-all result to an explicit-formula L2L^2 zero-packet estimate and obtains subpower exponential decay.

  2. Gafni–Tao, On the number of exceptional intervals to the prime number theorem in short intervals, Essential Number Theory 5 (2026), develop explicit bounds on exceptional-set exponents from zero-density and zero-additive-energy estimates. Their exceptional-set definitions use fixed relative-error tolerances.

  3. Matomäki–Radziwiłł–Shao–Tao–Teräväinen, Higher uniformity of arithmetic functions in short intervals II. Almost all intervals, Inventiones Mathematicae 244 (2026), record the current almost-all short-interval PNT range and arbitrary logarithmic quantitative accuracy.

None supplies a fixed XX -power principal-arc estimate.


24. State transition

The canonical transition is:

CSM_RH v1.9
  ->
CSM_RH v1.10

with:

Campaign 18
  CLOSED_AS_ZERO_DENSITY_AND_EXCEPTIONAL_SET_PRECISION_AUDIT

O-RH-042
  ZERO_DENSITY_SHRINKING_STRIP_EXPONENT_BARRIER
  CREATED / CERTIFIED FOR ABSOLUTE EXPLICIT-FORMULA SCHEMA

O-RH-043
  FIXED_THRESHOLD_EXCEPTIONAL_SET_MISMATCH
  CREATED / CERTIFIED

O-RH-044
  ZERO_DENSITY_SINGLE_ZERO_BLINDNESS
  CREATED / CERTIFIED AS STRENGTH AUDIT

S-RH-027
  SINGLE_ZERO_SENSITIVE_PRINCIPAL_ARC_MECHANISM
  CREATED / OPEN

F-RH-016
  MLEPG
  REMAINS OPEN

F-RH-010
  PESC
  REMAINS OPEN / ROOT TARGET

Campaign 19
  SINGLE_ZERO_SENSITIVE_THEOREM_GENERATION
  READY

25. Final status

RH = OPEN

PESC = OPEN

MLEPG = OPEN

CURRENT ZERO-DENSITY RANGE = STRONG

CURRENT ZERO-DENSITY PRECISION = SUBPOWER

2/15 = RANGE THRESHOLD, NOT FIXED-POWER THRESHOLD

GAFNI-TAO = EXCEPTIONAL-SET TOOL, NOT SHRINKING-THRESHOLD POWER L2

DENSITY-ONLY SCHEMA = SINGLE-ZERO BLIND

NEXT REQUIREMENT = SINGLE-ZERO-SENSITIVE MECHANISM

NEXT CAMPAIGN = 19

The key exponent identity is

cA0(α)=2A0(1α).\boxed{ c_{A_0}(\alpha) = 2 - A_0(1-\alpha). }

It controls whether zero-density information can gain anything at a short-interval scale.

But the actual fixed-power exponent available from a shrinking zero-free boundary is only

cA0(α)η(T),\boxed{ c_{A_0}(\alpha)\eta(T), }

which tends to zero.

The next theorem-generation round must therefore add information which is qualitatively stronger than density.