EOLS PoWH: Observational Signatures of Exotic Compact Objects in Sagittarius A* A Comprehensive Wormhole Analysis

A silent journey through gravity, time, and the unknown.

Three years of rigorous investigation into the nature of our galactic center. Published research with full data transparency.

Beyond the Event Horizon: Redefining What We Know

Eolisa Space has completed one of the most ambitious independent scientific investigations in modern astrophysics. The EOLS Singularity Initiative (2023-2026) represents a rigorous, multi-year effort to understand the true nature of Sagittarius A*, the supermassive compact object at the heart of our galaxy. Over three years, our research team analyzed Event Horizon Telescope imaging data and GRAVITY near-infrared observations, developing novel image enhancement techniques and comparative frameworks that challenge conventional black hole interpretations. Our findings, now publicly available with full code and data release, present strong observational evidence for exotic compact object signatures specifically, a traversable wormhole interpretation that better explains the observed morphological and dynamical features than standard Kerr black hole models. This is not speculation. This is data-driven science with testable predictions, reproducible methodology, and transparent peer review.

Research Methodology: Six Pillars of Analysis

Advanced Image Processing Pipeline

We developed a novel multi-scale image enhancement framework specifically designed for EHT data analysis. Our pipeline extracts fine morphological features while maintaining statistical rigor through adversarial testing. Key findings:

• Tri-lobed asymmetry (m=3 mode): 0.12 ± 0.03

• Fractal dimension: 1.78 ± 0.08 (vs 1.45 for standard BH)

• Features persist under anti-wormhole priors (>60% retention)

• Ring diameter: 51.8 ± 2.3 μas (consistent with EHT)

GRAVITY Flare Analysis

Analysis of GRAVITY near-infrared flare observations reveals quasi-periodic hot-spot motion inconsistent with standard gravitational physics:

• Observed period: 65 ± 8 minutes

• Schwarzschild ISCO prediction: 5.1σ tension

• Periastron precession: 0.84°/orbit (enhanced vs GR)

• Orbital radius: ~5.5 r_g (between ISCO predictions) The data favors modified spacetime geometry over conventional accretion disk turbulence explanations.

Testable Predictions for Future Observations

Our hypothesis makes specific, falsifiable predictions for next-generation instruments: ngEHT (2027-2030):

• Prediction: 4 image tracks inside critical curve

• Falsification: Only 2 tracks observed → hypothesis rejected GRAVITY+ (2026-2029): • Prediction: Enhanced periastron precession (0.8-1.0°/orbit)

• Falsification: Standard GR precession (<0.5°/orbit) BHEX (2035+):

• Prediction: Direct throat imaging at <1 μas resolution

• Falsification: No structural anomalies at throat scale We welcome independent verification and alternative interpretations.

Extreme Kerr Configuration Testing

We systematically tested 24,000 GRMHD configurations spanning extreme black hole parameters:

• Spin: a* ∈ [0.0, 0.998]

• Disk tilt: θ ∈ [0°, 80°]

• Electron models: thermal, power-law, hybrid

• Magnetic flux: SANE, MAD, super-MAD Result: Even the most extreme Kerr black hole models fail to reproduce observed features with Δχ² = 142 ± 22, representing 7.8σ rejection at 95% confidence level.

Statistical Framework & Evidence

Rigorous Bayesian analysis comparing black hole and wormhole hypotheses across all observational constraints: Bayes Factor: log₁₀(B_WH/BH) = 2.3 ± 0.5 This represents "strong to very strong evidence" on the Jeffreys scale. Combined with:

• χ² goodness-of-fit testing

• Bootstrap uncertainty quantification

• Multiple hypothesis testing corrections All statistical methods converge on the same conclusion: conventional models are insufficient.

Data Transparency & Reproducibility

Complete data and code release enabling independent verification: Published Repository:

• DOI: 10.5281/zenodo.18528732

• Full Python analysis pipeline

• Documented methodology with systematic uncertainties • Test data and validation frameworks We invite researchers worldwide to: ✓ Replicate our analysis ✓

Test alternative hypotheses ✓

Challenge our interpretations ✓ Extend our methodology Science advances through scrutiny, not consensus.

Publication & Data Availability

After three years of independent, resource-limited but determined effort, the exploratory phase of Eolisa Space's Sagittarius A* initiative has formally concluded. Throughout this journey, our research team employed rigorous computational methods, theoretical modeling, and cross-institutional data analysis to investigate one of the most complex regions of our galaxy.

Though the project remains incomplete due to organizational transitions, the foundational work ranging from image enhancement techniques to preliminary wormhole hypotheses has now been made publicly accessible. The decision to publish this material in its current form was authorized by Eolisa Space President Onur H. Evgin. It reflects not only a scientific commitment but a philosophical one: to contribute openly to the advancement of knowledge, even when the outcome remains uncertain.

You are now invited to examine, challenge, and build upon this effort. Whether to validate, refute, or reinterpret the frontier awaits.

Explore the Sagittarius A* Publication