Black-Hole Stars as Resonant Informational Collapse- A Falsifiability Roadmap for TGIU
Recent JWST observations of compact “little red dots,” including the object nicknamed The Cliff (z≈3.5), show an extreme Balmer break and line properties difficult to reconcile with standard stellar-population models. A leading explanation invokes a young black hole embedded in a dense, reprocessing gas cocoon—popularly termed a “black-hole star.” Within the Universal Gravito–Informational Theory (TGIU), such systems are reinterpreted as resonant informational–entropic collapse nodes, regulated by TEF and capable of leaving memory (GDM-like) imprints in radiation and gas microphysics. This note condenses a test program with concrete, falsifiable signatures that distinguish a TGIU overlay from conventional dense-gas/AGN models, using current facilities (JWST, ALMA) and forthcoming surveys (LSST/Euclid, ELTs, LISA).
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2025-09-25
- DOI
- https://doi.org/10.5281/zenodo.17202896
- Primary Topic
- Plant Molecular Biology Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00