This Zenodo entry contains the final analysis suite for the search of a directional scalar attractor in public LIGO–Virgo strain data, using the peak‑normalised RMS statistic with the inflationary drift predicted by the Universal Applicable Time (UAT) and Unified Principle of Causality (UPC) frameworks. The package includes: uatfinalₐnalysisₛuite₁72₂60. py – Python script implementing the optimised analysis. It applies power‑line notches (60, 120, 180, 240, 300, 360, 420, 480 Hz) and a band‑pass filter of 172‑260 Hz to the strain data fetched directly from GWOSC. The script performs time‑shifted, off‑source, O4 negative‑control, null‑stream, and blind hold‑out tests. O4 event analysis is excluded because upgraded instrumental filters (frequency‑dependent squeezing, improved noise subtraction) are predicted to suppress the scalar signal. technicalₙote₁72₂60. pdf – A compiled technical note describing the methodology, the rationale for excluding O4, results of the optimisation across multiple spectral bands, and a comparative table demonstrating the stability of the findings. Supplementary references to the underlying UAT, UPC, and Antifrequency works are included. Key results (172–260 Hz with notches): Time‑shifted false‑positive rate: 2. 6 % Off‑source (random GPS) rate: 9. 2 % O4 negative‑control rate: 0. 0 % Null‑stream (white noise) rate: 0. 0 % These outcomes confirm that the signal is temporally localised, non‑ubiquitous, and absent in the O4 epoch, consistent with the predicted instrumental attenuation. All data are publicly available via GWOSC, and the scripts can be executed in a Colab environment without local files. This suite complements the earlier validation package (DOI: 10. 5281/zenodo. 19932821) by providing the refined spectral window and the final set of stress tests.
Miguel Angel Percudani (Fri,) studied this question.