General Relativity Challenged by New Tension Discovered in Dark Siren Cosmology
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HONOLULU - Txylo -- Study suggests "invisible wedge" in distance measurements could impact Hubble Tension resolution: 512 simulations fail to match observed propagation anomaly.

Independent researcher Aiden B. Smith has announced the release of a new study, "A calibrated dark-siren tension with General-Relativity propagation," which identifies a statistically significant anomaly in how gravitational waves appear to propagate through the universe. The study analyzes data from the GWTC-3 catalogue and suggests that "dark sirens"—gravitational-wave events without visible light counterparts—prefer a model where waves decay differently than General Relativity (GR) predicts.

For years, the "Hubble Tension"—a persistent mismatch between measurements of the universe's expansion rate from the early universe versus the late universe—has perplexed cosmologists. Standard siren cosmology typically assumes that gravitational waves are clean distance indicators that follow Einstein's General Relativity exactly. However, Smith's analysis asks a sharper question: does the observed data actually fit that assumption?

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The new research reports a "calibrated propagation anomaly" in 36 dark sirens. The analysis compares the standard GR baseline against a modified-propagation history where gravitational waves experience additional effective "friction" as they travel.

Key Findings of the Study:

• Strong Statistical Preference: The observed catalogue yields a predictive score shift of Delta LPD = +3.670 in favor of the modified-propagation model. In the study's scoring framework, this makes the modified model approximately 39 times more predictive than the standard GR baseline.
• Failed Null Tests: To test if this was a random fluctuation, the study ran 512 GR-consistent simulations (injections). None of these simulations approached the scale of the anomaly observed in the real data.
• The "Invisible Wedge": The study argues that if gravitational-wave luminosity distances differ from electromagnetic distances, any analysis assuming standard GR is biased by construction. This acts as an "invisible wedge" that distorts the mapping from observed amplitudes to cosmic expansion history.
• Robustness: The signal survived "stress testing," including sky-rotation controls (scrambling the sky positions) and systematics matrices, suggesting the issue lies deep within the distance-redshift data rather than simple coincidences.

"The immediate alternative to new physics is a subtle, unmodelled failure in our catalogues or selection functions," says Smith. "But whether this is a new physical 'friction' or a hidden systematic, the result is the same: GR-locked distance inference is currently acting as a hidden systematic in late-time cosmology. We must test the propagation of these waves as seriously as we test our instruments."

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The scientific value of the result is diagnostic: it quantifies how far current dark-siren analyses can be pushed before the assumption of perfect General Relativity propagation breaks down.

The full manuscript, analysis artifacts, and summary tables have been archived on Zenodo to ensure transparency and reproducibility. The work is also available on Smith's research hub, QuasarDipolePhenomenon.org, alongside his previous work on the CatWISE quasar dipole.

About the Researcher:

Aiden B. Smith is an independent researcher and Data Analyst focused on statistical methods, catalogue systematics, and large-scale structure in cosmology.

Data and Reproducibility:

Manuscript/Project Archive DOI: 10.5281/zenodo.18604204

Website: https://quasardipolephenomenon.org