Theoretical Foundations, Observational Constraints, and Empirical Refutation
This repository contains the research paper "Are We Really in a Black Hole?", which investigates the hypothesis that our observable universe exists inside a black hole.
The study evaluates this idea using general relativity, cosmological observations, and statistical analysis, and compares it against the standard ΛCDM cosmological model.
- Analyze mathematical similarities between black hole interiors and cosmological models
- Test predictions against observational data
- Perform Bayesian model comparison
- Evaluate the physical validity of black hole cosmology
- Metric comparisons (Schwarzschild vs FLRW)
- Holographic entropy calculations
- Bayesian inference using cosmological datasets
- Cross-validation with observational evidence
- Planck (CMB data)
- JWST (high-redshift galaxies)
- DESI (cosmic structure)
- LIGO/Virgo/KAGRA (gravitational waves)
- Event Horizon Telescope
- Strong statistical preference for ΛCDM over black hole cosmology
- No evidence of predicted black hole interior effects
- Observations contradict key assumptions of the hypothesis
Although the idea that the universe exists inside a black hole provides interesting theoretical parallels, it fails to match observational reality.
Key issues include:
- The universe’s accelerating expansion contradicts expected collapse behavior
- The isotropy of the cosmic microwave background does not support radial structure
- No observational evidence for predicted quantum or gravitational signatures
Bayesian analysis strongly favors the ΛCDM model, with extremely low probability for the black hole hypothesis.
Conclusion: The universe is not inside a black hole. The concept remains a theoretical analogy rather than a physical model.
├── Are We Really in a Black Hole.pdf ├── README.md
If you use this work, please cite:
Samuelson G,
"Are We Really in a Black Hole? Theoretical Foundations, Observational Constraints, and Empirical Refutation"
Contributions, suggestions, and discussions are welcome. Please open an issue or submit a pull request.
This work is licensed under a Creative Commons Attribution 4.0 International License.
This work is theoretical and based on currently available cosmological data and models.