| _version_ | 1866901376922025984 |
|---|---|
| author | ÇAKIR, Olcay Kaan |
| author_facet | ÇAKIR, Olcay Kaan |
| contents | <p>This work presents a singularity-free interpretation of black holes based on the Vacuum Elasticity Model (VEM). In this framework, black holes are not geometric singularities but elastic rupture surfaces formed when vacuum stress reaches its critical limit. The event horizon corresponds to the collapse of wave-carrying capacity, and the interior becomes an amorphous vacuum phase with finite density and stress. Mathematical derivations are provided to demonstrate why singularities cannot form within VEM.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_17761901 |
| institution | Zenodo |
| language | |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Black Holes as Elastic Rupture Surfaces in the Vacuum Elasticity Model (VEM) ÇAKIR, Olcay Kaan <p>This work presents a singularity-free interpretation of black holes based on the Vacuum Elasticity Model (VEM). In this framework, black holes are not geometric singularities but elastic rupture surfaces formed when vacuum stress reaches its critical limit. The event horizon corresponds to the collapse of wave-carrying capacity, and the interior becomes an amorphous vacuum phase with finite density and stress. Mathematical derivations are provided to demonstrate why singularities cannot form within VEM.</p> |
| title | Black Holes as Elastic Rupture Surfaces in the Vacuum Elasticity Model (VEM) |
| url | https://doi.org/10.5281/zenodo.17761901 |