This record presents observational evidence for a scalar causal attractor at a normalized RMS limit of 1/√2 (≈ 0. 7071) in publicly available LIGO and Virgo strain data. The analysis spans multiple epochs from GW150914 (2015) to O4a (2024) and includes a synthetic white‑noise control that yields 0. 0% coincidence, ruling out statistical artifacts. **Key findings: **- GW150914: L1 shows 56. 2% coincidence with the attractor; H1 shows 0%. - O3 (April 2019): H1 shows 66. 2% coincidence with the drift‑corrected attractor (0. 4823). - The attractor appears only in specific detectors at specific epochs, demonstrating that the underlying field is **directional** and that LIGO's fixed arm orientation acts as a narrow‑angle receiver. These results motivate the construction of an omnidirectional 36‑coil detector (the “Puan Station”) designed to overcome LIGO's limitations and capture scalar torsion from any incident direction. The package includes the full technical report and two Python scripts to reproduce the analysis. **Contents: **- `InformeEvidenciaAtractorLIGO. pdf` — Technical report (PDF) with methodology, results, and detector comparison. - `syntheticₙoisecontrol. py` — Generates synthetic noise and applies the same RMS pipeline. - `multiₑpochₗigoₐnalysis. py` — Downloads LIGO/Virgo data and performs the multi‑epoch attractor search. **Related DOIs: **- UAT Framework: 10. 5281/zenodo. 17729221- UPC Framework: 10. 5281/zenodo. 18210808- Puan Station 36+1 Detector Package: 10. 5281/zenodo. 19704792
Miguel Angel Percudani (Fri,) studied this question.