Appendix U — Derivation 21: CMB Interference Structure from Modal Origins

Appendix U — CMB Harmonics as Coherence-Shell Interference

(concept sketch • simulation notebook to follow)

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This note outlines how Phase-Biased Geometry could reproduce the CMB
acoustic-peak spectrum without plasma sound waves.
No numerical fit is claimed; a dedicated notebook
cmb-coherence-shell.ipynb will generate a full C curve once the
spherical-harmonic mode sum is implemented.


1 The CMB in PBG


2 Boundary harmonics

Each marginal mode on the sphere is approximated by

ψm(θ,ϕ)=AmeimϕP(cosθ),

with the angular quantum number and m=.
Interference between many such modes gives an angular power

C=|mam|2,am=ψ(θ,ϕ)Ym(θ,ϕ)dΩ.

3 Peak positions from geometry

Phase alignment enforces

peakλcRs,

so the first peak appears at the largest wavelength
(Rs/λc).
Higher peaks correspond to harmonic numbers 2peak,
3peak, etc., with damping as constructive interference
falters at small scales.


4 No photon–baryon plasma required

Standard ΛCDM PBG coherence shell
Standing sound waves Boundary-anchored phase modes
Sound horizon sets Rs/λc sets
Damping from Silk viscosity Damping from phase-decoherence
Peaks need baryon loading Peaks need only mode geometry

Both pictures can yield similar C spectra; the difference lies in
underlying physics, not mathematics.


5 Next-step simulation (notebook plan)

  1. Choose λc from the locked constants
    k=β/α (Appendix AA).
  2. Populate random phase coefficients Am with a
    blue-tilted spectrum (saturation bias).
  3. Compute C up to =2500.
  4. Compare with Planck likelihood (plot only; no parameter fit).

Notebook stub: notebooks/cmb-coherence-shell.ipynb.


Take-away

In PBG, the microwave background is interpreted as
harmonic interference on a coherence boundary, not as fossil sound
waves. Quantitative agreement with the observed peak pattern will be
tested once the harmonic-sum notebook is complete.

Appendix T | [Index](./Appendix Master) | Appendix V - Maxwell Equations