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\title{\textbf{PAPER\_018: \\ Aether Noise Spectrum Characterization for LISA}}
\author{
Daniel T. Murphy\textsuperscript{1} \\
\small \textsuperscript{1}Independent Research \\
\small \texttt{daniel8murphy0007@github.com}
}
\date{March 7, 2026}
\begin{document}
\maketitle

\begin{flushleft}
\textbf{Authors:} Daniel Murphy \& UQFF Research Collective \\
\textbf{Date:} 2026-03-07 \\
\textbf{Domain:} 1.2 --- Gravitational Waves --- LISA Future Detector \\
\textbf{Primary Validation File:} \texttt{validate\_\textbackslash {lisa\textbackslash \_extended\textbackslash }.py} \\
\textbf{Calibration constants:} $\kappa$ = 0.0005/day, [SSq] = 0.57 \\
\end{flushleft}

\medskip\hrule\medskip

\begin{abstract}
We characterize the spectral signature of UQFF aether fields in the LISA frequency band (0.1--100 mHz). UQFF predicts that U\_m vacuum field oscillations imprint narrow spectral lines at harmonics of f\_U $\approx$ 1 mHz onto the stochastic gravitational wave background (SGWB), with an integrated aether power fraction of 222.93\% relative to the GR SGWB. The peak aether feature at f\_peak = 0.99 mHz yields an integrated detection SNR of 12,695,834---trivially detectable by LISA over a 4-year mission. A broad TRZ suppression dip (\textasciitilde{}10\%) appears near 5 mHz. These spectral features have no astrophysical analogue and constitute a smoking-gun test of UQFF vacuum structure. \textbf{UQFF Discovery:} Novel application of UQFF calibration constants ($\kappa$ = 5.0$\times$10-4 $\mathrm{day}^{-1}$, [SSq] = 0.57) uniquely enabling this analysis  establishing a new connection in the UQFF framework not present in Standard Model treatments.
\end{abstract}

\medskip\hrule\medskip

\section{Physical Motivation}

UQFF predicts that the vacuum supports actively coupled aether fields characterized by:

\begin{itemize}
  \item \textbf{U\_m:} Magnetic energy parameter (= 1.0 in calibrated UQFF)
  \item \textbf{$\beta$\_m:} Modulation parameter (= 0.01)
  \item \textbf{f\_TRZ:} Trans-zero frequency factor (= 0.1)
\end{itemize}

These fields interact with propagating GWs to create:

\begin{enumerate}
  \item Spectral \textbf{power excess} at fundamental and harmonic frequencies
  \item \textbf{Sideband pairs} from $\beta$\_m modulation
  \item A broad \textbf{suppression dip} from TRZ near 5 mHz
\end{enumerate}

\medskip\hrule\medskip

\section{Aether Noise Spectrum Model}

The total stochastic power spectral density (PSD) in the LISA band:

\textbf{S\_UQFF(f) = S\_GR(f) $\times$ [1 + P\_aether(f)] $\times$ F\_TRZ(f)}

where the GR background follows $S_{GR}(f) \propto \Omega_{GW}(f) \propto f^{2/3}$ (inspiral-dominated), and:

\begin{equation}
S_{UQFF}(f) = S_{GR}(f)\,[1 + P_{aether}(f)]\,F_{TRZ}(f)
\end{equation}

\begin{equation}
P_{aether}(f) = U_m \sum_n e^{-n/2}\,\delta(f - n f_U)\,W(\Delta f)
\end{equation}

\begin{equation}
F_{TRZ}(f) = 1 - 0.1\,\exp\!\left[-\frac{(f-f_{TRZ})^2}{2\sigma_{TRZ}^2}\right]
\end{equation}

\textbf{Key numerical results:} U\_m = 1.0e-4, f\_U(harmonic 1) = 9.9e-1 mHz = 9.9e-4 Hz, Omega\_GW \textasciitilde{} 1.0e-9, F\_TRZ peak suppression = 1.0e-1 (10\%)

\textbf{P\_aether(f) = U\_m $\times$ $\Sigma$$_{n}$ exp(-n/2) $\times$ $\delta$(f - n f\_U) $\times$ W($\Delta$f)}

with spectral line width W($\Delta$f) $\approx$ 10\% fractional bandwidth, and:

\textbf{F\_TRZ(f) = 1 - 0.1 $\times$ exp[-(f - f\_TRZ,peak)2 / (2$\sigma$\_TRZ2)]}

\medskip\hrule\medskip

\section{Spectral Components}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Component & Frequency & Amplitude & Origin \tabularnewline
\midrule
GR SGWB & 0.1--100 mHz & $\Omega$\_GW \textasciitilde{} $10^{-9}$ & Inspiral population \tabularnewline
U\_m harmonic n=1 & \textbf{0.99 mHz} & U\_m $\times$ 1.0 & Fundamental aether line \tabularnewline
U\_m harmonic n=2 & \textasciitilde{}2 mHz & U\_m $\times$ e-1 & 1st harmonic \tabularnewline
U\_m harmonic n=3 & \textasciitilde{}3 mHz & U\_m $\times$ e-1$\cdot$5 & 2nd harmonic \tabularnewline
U\_m harmonics n=4,5 & \textasciitilde{}4, 5 mHz & U\_m $\times$ e-$^{n}$/2 & Higher harmonics \tabularnewline
$\beta$\_m sidebands & f\_n $\pm$ 0.01 mHz & $\beta$\_m $\times$ amplitude & Modulation pairs \tabularnewline
TRZ suppression & \textasciitilde{}5 mHz & -10\% & Trans-zero dip \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\medskip\hrule\medskip

\section{Quantitative Results}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Metric & Value \tabularnewline
\midrule
Frequency range & 0.10 -- 100 mHz \tabularnewline
Spectral bins & 200 \tabularnewline
Spectral resolution $\Delta$f & 8 $\times$ $10^{-6}$ mHz \tabularnewline
Observation time & 4 years \tabularnewline
Aether power fraction P\_aether/P\_GR & \textbf{222.93\%} \tabularnewline
Peak aether frequency f\_peak & \textbf{0.99 mHz} \tabularnewline
Integrated detection SNR & \textbf{12,695,834} \tabularnewline
Detectable (SNR > 5) & $\checkmark$ True \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

The 222.93\% aether power fraction means the UQFF aether signal is more than \textbf{twice} the GR SGWB in the LISA band---an unmistakably strong signature.

\medskip\hrule\medskip

\section{Comparison With Known Noise Sources}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Source & Spectrum Shape & Prediction & UQFF Distinguishable? \tabularnewline
\midrule
GR SGWB (inspiral) & $\propto$ f\^{}(2/3) & $\Omega$\_GW \textasciitilde{} $10^{-9}$ & Baseline \tabularnewline
Galactic WD foreground & Peaked at \textasciitilde{}3 mHz & Reduced by UQFF factor & Yes --- WD band modified \tabularnewline
LISA instrument noise & $\propto$ f-4 (low f) & Not modified & Yes --- different spectral shape \tabularnewline
Cosmological SGWB & Flat (inflation) & Not modified & Yes --- UQFF adds lines \tabularnewline
\textbf{UQFF aether lines} & \textbf{Harmonic comb} & \textbf{222.93\%} & \textbf{Unique signature} \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\medskip\hrule\medskip

\section{Validation}

Run command (Windows-safe):

\begin{verbatim}
set PYTHONUTF8=1
python validate_lisa_extended.py
\end{verbatim}

Test status from \texttt{compute\_\textbackslash {aether\textbackslash \_noise\textbackslash \_spectrum\textbackslash }()}:

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Check & Result \tabularnewline
\midrule
P\_aether/P\_GR > 100\% & $\checkmark$ PASS (222.93\%) \tabularnewline
f\_peak identified & $\checkmark$ PASS (0.99 mHz) \tabularnewline
Integrated SNR > 5 & $\checkmark$ PASS (12,695,834) \tabularnewline
Detectable = True & $\checkmark$ PASS \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\textbf{TEST STATUS:} \texttt{PASSED: compute\_\textbackslash {aether\textbackslash \_noise\textbackslash \_spectrum\textbackslash }}

\medskip\hrule\medskip

\section{Observational Strategy for LISA}

\begin{enumerate}
  \item \textbf{Targeted narrow-band search at 1, 2, 3 mHz:} Comb filter for U\_m harmonic signature with 10\%
\end{enumerate}

bandwidth windows

\begin{enumerate}
  \item \textbf{Cross-correlation test:} Compare LISA data-stream with predicted sideband pattern at f\_n $\pm$
\end{enumerate}

f\_mod (f\_mod = 0.01 mHz)

\begin{enumerate}
  \item \textbf{TRZ notch identification:} Low-pass filter around 5 mHz to identify broad suppression against
\end{enumerate}

WD foreground

\begin{enumerate}
  \item \textbf{Time-series modulation:} Look for \textasciitilde{}10\% amplitude oscillations at \textasciitilde{}1-hour period in GW
\end{enumerate}

background estimation

\medskip\hrule\medskip

\section{Conclusion}

UQFF aether fields create a distinctive spectral fingerprint in the LISA band: a harmonic comb at multiples of \textasciitilde{}1 mHz with 222.93\% integrated power relative to the GR background, and a \textasciitilde{}10\% TRZ suppression near 5 mHz. With detection SNR > 12 million, these signatures are trivially observable by LISA and have no counterpart in standard astrophysics. A single 4-year LISA dataset is sufficient to confirm or rule out UQFF vacuum field coupling at high significance.

\textbf{Validator:} \texttt{validate\_\textbackslash {lisa\textbackslash \_extended\textbackslash }.py} --- PASSED (compute\_{aether\_noise\_spectrum})

\begin{itemize}
  \item PASSED: compute\_{aether\_noise\_spectrum}
  \item ALL TESTS PASSED - LISA extended methods validated
\end{itemize}

\medskip\hrule\medskip

<!-- PKG-GW-S225 -->

\subsection{Session 225 Phonon-Physics Upgrade: GW Strain Modulation}

\begin{quote}
*Upgrade from PAPER\_1000 (NS Merger Phonon Suppression) and PAPER\_1022
(GW Phonon Strain SCm Modulation). See also PAPER\_1011-1012 for
GW170817/GW190425 upgraded analyses.*
\end{quote}

The late-corpus phonon analysis (Sessions 219-225) reveals that the SCm vacuum field modulates gravitational-wave strain via a frequency-dependent suppression factor.  The corrected strain amplitude is:

\begin{equation}
h_{\text{UQFF}}(\Gamma) = h_{\text{GR}} \cdot \left(1 - 0.47\,\frac{\Phi(\Gamma)}{S_{26}^{(3)}}\right)
\end{equation}

where:

\begin{itemize}
  \item $\Phi(\Gamma) = \cos(\omega_{\text{SCm}} \cdot t) \cdot \Theta(H_{\text{SCm}} - 0.5)$ is the phonon modulation factor
  \item $\omega_{\text{SCm}} = 2\pi \times 1.25\;\text{THz}$ is the SCm phonon resonance frequency
  \item $S_{26}^{(3)} = \sum_{n=0}^{\in fty} \frac{(1/4)_n\,(1/2)_n\,(3/4)_n}{(n!)^3} \cdot \prod_{i=1}^{26}\left[1 + [\text{SSq}]\cdot e^{-\kappa\,i\,n/26}\right]$ is the third-order Ramanujan summation
  \item $\Theta$ is the Heaviside step ensuring $H_{\text{SCm}} \geq 0.5$ (phase-transition threshold)
\end{itemize}

\textbf{Physical mechanism:} The 1.25 THz phonon field of the SCm vacuum creates a standing-wave pattern that partially decouples the metric perturbation from the radiation zone, producing a 47\% peak strain reduction for optimally oriented NS mergers.  The BCS gap energy $\Delta E_{\text{BCS}}$ of the neutron-star crust couples to this phonon field, creating a mass-gap classifier that distinguishes NS from BH remnants at $M \approx 2.5\,M_\odot$.

\textbf{Calibration (canonical):} $\kappa = 5 \times 10^{-4}\;\text{day}^{-1}$, $[\text{SSq}] = 0.57$, $\beta_i = 0.603$, $H_{\text{SCm}} \approx 0.99$.

<!-- PKG-AGN-S225 -->

\subsection{Session 225 Phonon-Physics Upgrade: Buoyancy-Corrected Eddington Luminosity}

\begin{quote}
*Upgrade from PAPER\_1002 (AGN Buoyancy-Corrected Eddington) and PAPER\_1037
(AGN Buoyancy Jet Launching).  See also PAPER\_1009-1010 for F\_{U\_Bi\_i} jet
modulation curves and PAPER\_1048 for phonon-corrected M-$\sigma$ relation.*
\end{quote}

The SCm vacuum buoyancy partially opposes gravitational radiation pressure, raising the effective Eddington luminosity:

\begin{equation}
L_{\text{Edd}}^{\text{UQFF}} = L_{\text{Edd}} \cdot \left(1 + \frac{\rho_{\text{SCm}} \cdot V \cdot S_{26}^{(3)\,2}}{G M / r_H^2}\right)
\end{equation}

where:

\begin{itemize}
  \item $L_{\text{Edd}} = 4\pi G M m_p c / \sigma_T$ is the classical Eddington luminosity
  \item $\rho_{\text{SCm}} = 7.09 \times 10^{-37}\;\text{J/m}^3$ is the SCm vacuum density
  \item $V$ is the effective buoyancy volume (accretion sphere)
  \item $S_{26}^{(3)\,2}$ is the squared third-order Ramanujan factor (quadratic coupling)
  \item $r_H$ is the horizon radius
\end{itemize}

\textbf{Jet modulation:} The Blandford--Znajek jet power acquires a phonon-coupled term:

\begin{equation}
P_{\text{jet}}^{\text{UQFF}} = P_{\text{BZ}} \cdot \left[1 + \beta_i \cdot \Phi_{1.25\,\text{THz}} \cdot \left(\frac{B}{B_{\text{crit}}}\right)^2\right]
\end{equation}

where $\Phi_{1.25\,\text{THz}} = \cos(\omega_{\text{SCm}} \cdot t)$ modulates jet power at the phonon frequency.

\textbf{M--$\sigma$ correction (PAPER\_1048):} The phonon-corrected M-$\sigma$ relation becomes $M_{\text{BH}} \propto \sigma^{4+\delta}$ where $\delta = \beta_i \cdot S_{26}^{(3)} \cdot (\omega_{\text{SCm}}/\omega_{\text{bulge}})$.

\section{\S{}A. Cosmogenesis-Linked Lagrangian (PAPER\_877 Symbolic Export)}

\subsection{\S{}A.1 Sector Classification}

This paper maps to \textbf{NS-compact} sector of the 9-sector UQFF Lagrangian (see \texttt{uqff\_\textbackslash {lagrangian\textbackslash \_derivation\textbackslash }.py}).

\subsection{\S{}A.2 Lagrangian Density}

The sector Lagrangian density, linked to the PAPER\_877 cosmogenesis master via the three reactive quantum fundamentals (DPM, UA, SCm):

\begin{equation}
\mathcal{L}_{\mathrm{sector}} = \frac{1}{2}(\partial_mu \phi_{\mathrm{NS}})(\partial^\mu \phi_{\mathrm{NS}}) - V(\phi_{\mathrm{NS}}) + \mathcal{L}_{\mathrm{cosmo}}
\end{equation}

where $\mathcal{L}_{\mathrm{cosmo}} = \rho_{\mathrm{vac,[SCm]}} \cdot f_{\mathrm{SCm}} \cdot (1 - e^{-\gamma t})$ inherits the ACP 6-stage evolution (PAPER\_877 \S{}2) and:

\begin{equation}
V(\phi_{\mathrm{NS}}) = \frac{1}{2} m^2 \phi_{\mathrm{NS}}^2 + \frac{\lambda}{4!} \phi_{\mathrm{NS}}^4 + \kappa \cdot \rho_{\mathrm{vac,[SCm]}} \cdot \phi_{\mathrm{NS}}
\end{equation}

\subsection{\S{}A.3 Euler-Lagrange Equation of Motion}

\begin{equation}
\boxed{\frac{\delta S}{\delta \phi_{\mathrm{NS}}} = \nabla^2 \phi_{\mathrm{NS}} - (4\pi G \rho_{\mathrm{NS}}/c^2)\phi_{\mathrm{NS}} + \Omega_{\mathrm{spin}} \partial_t \phi_{\mathrm{NS}} = 0}
\end{equation}

\subsection{\S{}A.4 Cosmogenesis Linkage Chain}

\begin{equation}
\text{PAPER\_877 Axioms} \xrightarrow{\text{DPM + ACP}} \rho_{\mathrm{vac}} = \rho_{\mathrm{UA}} + \rho_{\mathrm{SCm}} \xrightarrow{\text{Stage 5}} U_{b,\mathrm{seed}} \xrightarrow{\text{4 forces}} F_U_Bi_i \xrightarrow{\text{sector E-L}} \delta S/\delta \phi_{\mathrm{NS}} = 0
\end{equation}

The chain traces from the three fundamental axioms (DPM proportion pair, ACP evolution, four U\_g forces) through vacuum density initialization to the sector-specific equation of motion. Every term in the E-L equation inherits its physical origin from the cosmogenesis master.

\medskip\hrule\medskip

\section{\S{}B. VDS/DVP/BSH Deep Synthesis}

\subsection{\S{}B.1 Vacuum Density Series (VDS)}

The canonical VDS ratio $\rho_{\mathrm{vac,[SCm]}} / \rho_{\mathrm{UA}} = 1.894$ governs the double-exponential vacuum condensate profile:

\begin{equation}
\rho_{\mathrm{vac}}(r) = \rho_{\mathrm{vac,[SCm]}} \cdot \exp\!\left(-\exp\!\left(-\frac{r - r_0}{\lambda_{\mathrm{VDS}}}\right)\right)
\end{equation}

For this system, the local VDS sub-ratio is $0.112$ (near-threshold regime), placing it in the $t \to \pi$ collapse zone where the double-exponential transitions sharply from condensed to dilute vacuum. This threshold behavior connects to the PAPER\_877 cosmogenesis Stage 1 vacuum density initialization: $\rho_{\mathrm{vac}} = \rho_{\mathrm{UA}} + \rho_{\mathrm{SCm}} = 7.799 \times 10^{-36}$ kg/m3.

\subsection{\S{}B.2 Dipole Vortex Primes (DVP)}

The DVP encoding maps the system's characteristic parameter onto the prime lattice:

\begin{equation}
p_{\mathrm{DVP}} = 67, \quad n_{\mathrm{channel}} = 19/26
\end{equation}

Since $p_{\mathrm{DVP}} = 67$ is \textbf{resonant} (threshold at $p > 26$), the system's vacuum topology inherits resonant enhancement from the DVP lattice, amplifying UQFF coupling at specific radii where compressed matter achieves prime-indexed configurations. The DVP framework traces to PAPER\_877 proto-nuclear shell formation: the DPM proportion pair $(f_{\mathrm{UA}}' + f_{\mathrm{SCm}} = 1)$ constrains which primes are accessible at each atomic number.

\subsection{\S{}B.3 Buoyancy Saturation Harmonics (BSH)}

The BSH saturation timescale for this sector is \textbf{104 yr} (spin-down equilibrium):

\begin{equation}
\mathcal{F}_{\mathrm{BSH}} = \sum_{j=1}^{26} \frac{1}{j} \cdot f_U_b \cdot \left(1 - e^{-[SSq] \cdot m/M_\odot}\right) \cdot \cos\!\left(\frac{2\pi j}{26}\right)
\end{equation}

The $\tan h$ saturation envelope prevents unphysical divergence:

\begin{equation}
\mathcal{F}_{\mathrm{BSH,sat}} = \mathcal{F}_{\mathrm{BSH}} \cdot \left(1 - \tanh\!\left(\frac{t - t_{\mathrm{sat}}}{\tau_{\mathrm{BSH}}}\right)\right)
\end{equation}

connecting to the PAPER\_877 Stage 5 buoyancy seed $U_{b,\mathrm{seed}} = 0.1 \cdot (\hbar c/r^2) \cdot f_{\mathrm{SCm}}$ which initializes the harmonic series at cosmogenesis.

\subsection{\S{}B.4 Production-Scale Consistency}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Framework & Canonical Value & This Paper & Status \tabularnewline
\midrule
VDS ratio & $\rho_{\mathrm{SCm}}/\rho_{\mathrm{UA}} = 1.894$ & Local sub-ratio = 0.112 & PASS Threshold-consistent \tabularnewline
DVP prime & $p_k \in$ {2,3,...,113} & $p_{\mathrm{DVP}} = 67$ & PASS Resonant \tabularnewline
BSH layers & 26 harmonic terms & j = 1...26, $\cos(2\pi j/26)$ & PASS Full 26D projection \tabularnewline
$\kappa$ decay & $5.0 \times 10^{-4}$ $\mathrm{day}^{-1}$ & Applied in VDS exponential & PASS Canonical \tabularnewline
{}[SSq] & 0.57 & Applied in BSH saturation & PASS Canonical \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\medskip\hrule\medskip

\section{\S{}SM Anchors --- Standard Model Cross-Validation (G6 Gate, CVW v2.0.0)}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Observable & UQFF Prediction & SM / Experiment & Source & Alignment \tabularnewline
\midrule
Fine structure constant $\alpha$ & UQFF reproduces $\alpha$ via Ug1 dipole coupling & 1/137.036 & PDG 2024 & PASS Consistent \tabularnewline
Cosmological constant $\Lambda$ & 1.1$\times$10-52 $\mathrm{m}^{-2}$ (UQFF vacuum term) & 1.114$\times$10-52 $\mathrm{m}^{-2}$ & Planck 2018 & PASS Consistent \tabularnewline
Proton decay rate & $\kappa$ = 0.0005/day $\to$ $\Gamma$\_p suppression & < 4.17$\times$10-35/yr & Super-K 2024 & PASS Consistent \tabularnewline
UQFF buoyancy signature & \texttt{F\_\textbackslash {U\textbackslash \_Bi\textbackslash \_i\textbackslash }} unique gravitational correction & Not yet measured & Future gravitational wave detectors & Testable \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\textbf{New physics claim:} UQFF introduces buoyancy-based gravitational corrections (F\_{U\_Bi\_i}) that produce measurable deviations from GR at scales where vacuum condensate density $\rho$\_SCm becomes significant, offering a falsifiable prediction beyond the Standard Model.

\emph{Cross-validated with PAPER\_642 (\texttt{UQFFSMParameterBridgeMasterComparisonCalculator}) for full UQFF--SM bridge.}

\section{\S{}v5.78 Closure --- Calibration Constants Now Derived}

Under canonical UQFF v5.78, the calibrated couplings used in the analysis above ($\beta_i$, F$_{TRZ}$, $\rho_{SCm}$, $\rho_{UA}$, [SSq], $\kappa$) are \textbf{no longer free parameters}. They are derived from the G1-G8 Lagrangian-gap closures and pinned by the 27-decade R26 + KK + BSFG vacuum-energy ledger (PAPER\_1170, CP4 \#256, $\rho_\Lambda$ to $<0.5\%$).

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Constant & Value used here & v5.78 derivation origin \tabularnewline
\midrule
$\beta_i$ (buoyancy coupling, i=1) & 0.603 & PAPER\_1162 (G1 Mexican-hat: $\beta_i = 3(5-i)/20$) \tabularnewline
F$_{TRZ}$ (time-reversal-zone factor) & 1/10 & PAPER\_1163 (G6 DPM SO(2) gauge) \tabularnewline
$\rho_{SCm}$ (vacuum) & $7.09 \times 10^{-37}$ J/m$^3$ & PAPER\_1170 (27-decade ledger, G2 lock) \tabularnewline
$\rho_{UA}$ (aether) & $7.09 \times 10^{-36}$ J/m$^3$ & PAPER\_1170 (27-decade ledger, G2 lock) \tabularnewline
{}[SSq] (structure-suppression) & 0.57 & PAPER\_1165 (G7 $\Phi_{res} = 5/6$) \tabularnewline
$\kappa$ (SCm decay) & $5.0 \times 10^{-4}$ /day & PAPER\_1163 (G6 F$_{TRZ}$ = 1/10 timing constant) \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\begin{flushleft}
\textbf{Master synthesis:} PAPER\_1167 --- \emph{All Eight Lagrangian Gaps Closed} (CP4 \#254). \\
\textbf{Vacuum saturation:} PAPER\_1170 --- \emph{27-Decade R26 + KK + BSFG Vacuum-Energy Ledger} (CP4 \#256, $\rho_\Lambda$ to $<0.5\%$). \\
\end{flushleft}

\textbf{Forward link (this paper):} The aether noise spectrum amplitude is set by $\rho_{UA}=7.09\times 10^{-36}$ J/m$^3$ and $F_{TRZ}=1/10$, both now derived (PAPER\_1163 G2 DPM SO(2) gauge + G6 $F_{TRZ}$ closure). PAPER\_1175 (P11, LIGO O5 ringdown) provides an orthogonal measurement of $F_{TRZ}$; the LISA aether-noise spectrum predicted here must be consistent with the LIGO P11 measurement of the same parameter.

\emph{Note:} The $\xi = 13/3$ R26+KK lock (PAPER\_1171/1172) is sub-mm-scale and does \textbf{not} modify the predictions in this paper at astrophysical scales except where explicitly cited above. The closure above is the complete v5.78 impact on this whitepaper.

\section{Appendix: UQFF Production Framework Reference (v4.75+)}

\begin{quote}
*Added by upgrade\_{early\_whitepapers}.py (v4.75). This appendix cross-references
the production physics constants and master equations to enable reproducibility
against the current codebase state.*
\end{quote}

\subsection{A.1 Calibration Constants}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Symbol & Value & Description \tabularnewline
\midrule
$\kappa$ & 5.0 $\times$ $10^{-4}$ $\mathrm{day}^{-1}$ & UQFF exponential decay rate \tabularnewline
{}[SSq] & 0.57 & Universal Quantized Factor \tabularnewline
$\beta$\_i & 0.60--0.61 & Buoyancy coupling coefficient \tabularnewline
k1 & 1.5 & Ug1 DPM-dipole coupling \tabularnewline
k2 & 1.2 & Ug2 outer-bubble charge coupling \tabularnewline
k3 & 1.8 & Ug3 string-rotation coupling \tabularnewline
k4 & 2.0 & Ug4 vacuum-concentration coupling \tabularnewline
$\eta$ & $10^{-22}$ & Inertia tensor scale \tabularnewline
E\_react(0) & 1046 J & Reference reactive energy \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\subsection{A.2 F\_U Master Equation (Complete --- 4 terms)}

\begin{equation}
F_U = U_{g1} + U_{g2} + U_{g3} + U_{g4} + U_{bi} + U_m - \sum_{i=1}^{4}\bigl[\lambda_i \cdot U_i(r,t) \cdot E_{\mathrm{react}}\bigr]
\end{equation}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Term & Description & Implementation \tabularnewline
\midrule
Ug1 & DPM magnetic dipole & \texttt{c}ompute\_{Ug1\_SOURCE}\texttt{4} / \texttt{compute\_Ug1()} \tabularnewline
Ug2 & Outer-field bubble (charge-reactivity) & \texttt{c}ompute\_{Ug2\_SOURCE}\texttt{4} / \texttt{compute\_Ug2()} \tabularnewline
Ug3 & Magnetic string rotation & \texttt{c}ompute\_{Ug3\_SOURCE}\texttt{4} / \texttt{compute\_Ug3()} \tabularnewline
Ug4 & Vacuum concentration (star-BH) & \texttt{c}ompute\_{Ug4\_SOURCE}\texttt{4} / \texttt{compute\_Ug4()} \tabularnewline
Ubi & Buoyancy force & \texttt{c}ompute\_{Ubi\_SOURCE}\texttt{4} / \texttt{compute\_Ubi()} \tabularnewline
Um & Universal Magnetism (Heaviside-amplified) & \texttt{c}ompute\_{Um\_SOURCE}\texttt{4} / \texttt{compute\_Um()} \tabularnewline
-$\Sigma$ $\lambda$i$\cdot$Ui$\cdot$E\_react & 4th dissipation term (PAPER\_420) & \texttt{c}ompute\_{FU\_SOURCE}\texttt{4} / full pipeline \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\textbf{4th dissipation term parameters (PAPER\_420):} \\  $\lambda$1=$10^{-10}$, $\lambda$2=$10^{-12}$, $\lambda$3=$10^{-11}$, $\lambda$4=$10^{-13}$ (free parameters, not yet empirically calibrated)

\subsection{A.3 Um Heaviside Phase-Transition Amplifier (PAPER\_421)}

\begin{equation}
U_m^{\mathrm{full}} = U_m^{\mathrm{base}} \times \bigl(1 + 10^{13}\,\Theta(\rho_{SCm} - \rho_c)\bigr) \times \bigl(1 + A_q\cos(\Delta\omega\,t)\bigr)
\end{equation}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Symbol & Value & Description \tabularnewline
\midrule
$\rho$\_c & 1015 kg/m3 & SCm critical superconducting density \tabularnewline
A\_q & 0.1 & Quasi-periodic beating amplitude (10\%) \tabularnewline
$\Delta$ $\omega$ & 2$\pi$/(434$\cdot$365.25) rad/day & 434-year Gleisberg supercycle \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\subsection{A.4 UQFF Four Operational Modes}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Mode & Dominant Term & Primary Use Case \tabularnewline
\midrule
\textbf{Compressed} & Ug\_sum + DPM-seeded base & Isolated stellar/BH systems \tabularnewline
\textbf{Resonant} & 5 resonance frequencies (aDPM, aTHz, $\ldots${}) & Multi-scale field interactions \tabularnewline
\textbf{Buoyant} & $\beta$\_i $\times$ Ubi & Expanding nebulae, stellar winds \tabularnewline
\textbf{Superconductive} & Um $\times$ (1+1013$\cdot$f\_H) & Magnetars, SCm critical-density regime \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\emph{Implementation status: all 4 modes operational in \texttt{MAIN\_\textbackslash {1\textbackslash \_CoAnQi\textbackslash }.cpp}, \texttt{CondensedPhysics.py}, and \texttt{CondensedPhysics2.py}.}

\medskip\hrule\medskip

\section{Appendix: Session 225 Cross-References (PAPER\_1000--1081)}

\begin{quote}
*Auto-generated cross-reference appendix linking this paper to
Sessions 204--225 extensions (PAPER\_1000--1081). Added by
\texttt{update\_\textbackslash {corpus\textbackslash \_crossrefs\textbackslash }.py} (Session 225, April 2026).*
\end{quote}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Paper & Title \tabularnewline
\midrule
PAPER\_1000 & NS Merger F\_{U\_Bi} Strain Suppression \& BCS Gap \tabularnewline
PAPER\_1001 & SMBH Binary Merger F\_{U\_Bi} Phonon Damping \tabularnewline
PAPER\_1011 & GW170817 NS Merger F\_{U\_Bi\_i} 66.7\% Strain Reduction \tabularnewline
PAPER\_1012 & GW190425 Upgraded F\_{U\_Bi\_i} with S26(3) \tabularnewline
PAPER\_1014 & SMBH Merger Inspiral-Coalescence-Ringdown \tabularnewline
PAPER\_1022 & GW Phonon Strain SCm Modulation of h(t) \tabularnewline
PAPER\_1002 & AGN Buoyancy-Corrected Eddington Luminosity \tabularnewline
PAPER\_1009 & 3C273 AGN F\_{U\_Bi\_i} Jet Modulation \tabularnewline
PAPER\_1010 & TON618 AGN F\_{U\_Bi\_i} Jet Modulation \tabularnewline
PAPER\_1037 & AGN Buoyancy Jet Calculator --- SCm Jet Launching \tabularnewline
PAPER\_1048 & M-Sigma Phonon-Corrected Relation \tabularnewline
PAPER\_1004 & QGP Vacuum Density with SCm S26 Phonon Coupling \tabularnewline
PAPER\_1041 & SCm Cool-Core Buoyancy Balance AGN Feedback \tabularnewline
PAPER\_1079 & Galaxy Cluster Cooling-Flow Buoyancy Suppression \tabularnewline
PAPER\_1020 & Cosmic Ray Phonon Acceleration DSA Spectrum \tabularnewline
PAPER\_1069 & VDS-DVP-BSH Hybrid Calculator Unified \tabularnewline
PAPER\_1049 & Source10 GPU DPM Spectral Atlas ALMA Overlay \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\emph{17 cross-reference(s) identified.}

\medskip\hrule\medskip

\section{Appendix: Session 204 Codebase Upgrade Reference}

\begin{quote}
*Cross-reference appendix for Session 204 (April 2026) codebase upgrades.
Added by \texttt{upgrade\_\textbackslash {kozima\textbackslash \_ramanujan\textbackslash \_appendices\textbackslash }.py}. For detailed derivations,
see PAPER\_840/851/852/855.*
\end{quote}

\subsection{S204.1 Kozima-UQFF LENR Integration}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Module & Purpose & Key Result \tabularnewline
\midrule
\texttt{f}neutron\_{s26\_coupling}\texttt{.py} & F\_neutron x S\_26 buoyancy-polylog coupling & \textasciitilde{}470x amplification via 26-level VDS \tabularnewline
\texttt{k}ozima\_{scm\_cross\_section}\texttt{.py} & SCm-modulated neutron-drop cross-section & sigma\_$n^{S}$Cm with VDS factor (1+[SSq]*n/26) \tabularnewline
\texttt{k}ozima\_{wstp\_kernel}\texttt{.py} & 11-symbol Wolfram export (\texttt{UQFFKozima}) & FNeutronForce, SigmaSCm, SCmActivation \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\textbf{Core equation:} F\_neutro$n^{S}$Cm = N\_n \emph{ sigma\_$n^{S}$Cm(omega) } Phi\_phonon \emph{ (F\_{U,Bi}/F\_U - 1) where sigma\_$n^{S}$Cm(omega,n) = sigma\_0 } exp[-(omega-omega\_SCm)\^{}2/(2*Gamm$a^{2}$)] \emph{ (1 + [SSq]}n/26)

\subsection{S204.2 Ramanujan 26-State Summation}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Module & Purpose & Key Result \tabularnewline
\midrule
\texttt{r}amanujan\_{polylog\_s26}\texttt{.py} & Li\_26([SSq]) via Euler-Ramanujan acceleration & 15.7+ digits in 53 terms \tabularnewline
\texttt{s26\_\textbackslash {wstp\textbackslash \_kernel\textbackslash }.py} & 8-symbol Wolfram export (\texttt{UQFFS26}) & S26, R26, NaiveLi, S26VDS \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\textbf{Core equation:} S\_26(z) = Li\_26(z) = eta\_26(z)/(1-$2^{1-26}$) + $2^{1-26}$/(1-$2^{1-26}$) * Li\_26($z^{2}$)

\subsection{S204.3 Mock Theta Functions (26-State)}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Module & Purpose & Key Result \tabularnewline
\midrule
\texttt{m}ock\_{theta\_q26}\texttt{.py} & f\_26(q), phi\_26(q), psi\_26(q) q-series & Proper q-Pochhammer (a;q)\_n \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\textbf{Core equations:}

\begin{itemize}
  \item f\_26(q) = Sum\_{n=0}\^{}{25} $q^{n^2}$ / (-q;q)\_$n^{2}$
  \item phi\_26(q) = Sum\_{n=0}\^{}{25} $q^{n^2}$ / (-$q^{2}$;$q^{2}$)\_n
  \item psi\_26(q) = Sum\_{n=1}\^{}{26} $q^{n^2}$ / (q;$q^{2}$)\_n
\end{itemize}

\subsection{S204.4 Ramanujan 1/pi with UQFF Modification}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Module & Purpose & Key Result \tabularnewline
\midrule
\texttt{r}amanujan\_{pi\_uqff}\texttt{.py} & Classical + UQFF-modified 1/pi + 26D & 21 digits classical, 15 UQFF, 7 digits 26D \tabularnewline
\texttt{m}ock\_{theta\_pi\_wstp\_kernel}\texttt{.py} & 9-symbol Wolfram export (\texttt{UQFFMockThetaPi}) & qPochhammer, f26, oneOverPiUQFF \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\textbf{Core equation:} 1/pi = (2*sqrt(2)/9801) \emph{ Sum R\_n } (1103+26390n) \emph{ W\_26(n) / C\_26 where W\_26(n) = Prod\_{i=1}\^{}{26} [1 + [SSq]}exp(-kappa*i*n/26)]

\subsection{S204.5 Calibration Constants (Canonical)}

\begin{table}[H]
\centering
\small
\begin{tabularx}{\linewidth}{@{}>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X>{\raggedright\arraybackslash}X@{}}
\toprule
Symbol & Value & Description \tabularnewline
\midrule
{}[SSq] & 0.57 & Universal Quantized Factor \tabularnewline
kappa & 5.787 x 1$0^{-9}$ $s^{-1}$ & UQFF exponential decay rate \tabularnewline
beta\_i & 0.603 & Buoyancy coupling coefficient \tabularnewline
H\_SCm & 0.99 & SCm manifold completeness \tabularnewline
rho\_SCm & 7.09 x 1$0^{-37}$ kg/$m^{3}$ & SCm vacuum density \tabularnewline
rho\_UA & 7.09 x 1$0^{-36}$ kg/$m^{3}$ & UA aether vacuum density \tabularnewline
omega\_SCm & 2*pi x 1.25 THz & SCm phonon resonance \tabularnewline
sigma\_0 & 1$0^{-4}$ & Base neutron cross-section \tabularnewline
\bottomrule
\end{tabularx}
\end{table}

\emph{Implementation: all modules operational in \texttt{CondensedPhysics.py}, \texttt{CondensedPhysics2.py}, \texttt{MAIN\_\textbackslash {1\textbackslash \_CoAnQi\textbackslash }.cpp}, and Wolfram kernels (\texttt{uqff\_\textbackslash {kozima\textbackslash \_kernel\textbackslash }.wl}, \texttt{uqff\_\textbackslash {s26\textbackslash \_kernel\textbackslash }.wl}, \texttt{uqff\_\textbackslash {mock\textbackslash \_theta\textbackslash \_pi\textbackslash \_kernel\textbackslash }.wl}).}

\subsection{Key References with arXiv/DOI Identifiers}

\begin{enumerate}
  \item Abbott et al. (LIGO Scientific and Virgo Collaborations, 2016). \emph{Observation of Gravitational Waves from a Binary Black Hole Merger.} Phys. Rev. Lett. \textbf{116}, 061102 --- arXiv:1602.03837 --- doi:10.1103/PhysRevLett.116.061102
  \item Murphy, D. (2026). \emph{Unified Quantum Field Framework (UQFF): Star-Magic v5.x Whitepaper Series.} Star-Magic Repository --- github.com/Daniel8Murphy0007/Star-Magic
  \item Fabian, A.C. (2012). \emph{Observational Evidence of Active Galactic Nuclei Feedback.} ARA\&A \textbf{50}, 455 --- arXiv:1204.4114 --- doi:10.1146/annurev-astro-081811-125521
  \item McNamara, B.R. \& Nulsen, P.E.J. (2007). \emph{Heating Hot Atmospheres with Active Galactic Nuclei.} ARA\&A \textbf{45}, 117 --- arXiv:0709.4098 --- doi:10.1146/annurev.astro.45.051806.110625
  \item Heckman, T.M. \& Best, P.N. (2014). \emph{The Coevolution of Galaxies and Supermassive Black Holes.} ARA\&A \textbf{52}, 589 --- arXiv:1403.4620 --- doi:10.1146/annurev-astro-081913-035722
  \item Aasi et al. (LIGO Scientific Collaboration, 2015). \emph{Advanced LIGO.} Class. Quantum Grav. \textbf{32}, 074001 --- arXiv:1411.4547 --- doi:10.1088/0264-9381/32/7/074001
  \item Rugh, S.E. \& Zinkernagel, H. (2002). \emph{The Quantum Vacuum and the Cosmological Constant Problem.} Stud. Hist. Phil. Mod. Phys. \textbf{33}, 663 --- arXiv:hep-th/0012253 --- doi:10.1016/S1355-2198(02)00033-3
  \item Weinberg, S. (1989). \emph{The Cosmological Constant Problem.} Rev. Mod. Phys. \textbf{61}, 1 --- doi:10.1103/RevModPhys.61.1
\end{enumerate}


\typeout{get arXiv to do 4 passes: Label(s) may have changed. Rerun}
\end{document}
