The Fractal Star Hypothesis: Heavy Elements as Pre-Folded Spacetime within an Infinite Fractal Descent Framework
Abstract
In the conventional paradigm of theoretical astrophysics, the lifecycle of a massive star () invariably concludes with a catastrophic core collapse, a process governed by the delicate equilibrium between thermonuclear radiation pressure and gravitational contraction. Throughout its main-sequence lifespan, a star relies on the continuous fusion of increasingly heavier elements to sustain the outward pressure required to counteract its own immense mass. However, as nuclear nucleosynthesis progresses through the alpha ladder—fusing carbon, oxygen, neon, and silicon—the stellar core eventually synthesizes iron-56. Iron possesses the highest binding energy per nucleon of any naturally occurring isotope. Consequently, it cannot undergo further exothermic fusion; any attempt to fuse iron consumes more thermal energy than it releases.
Fields of Study & Subjects
Stellar
planetary
and galactic studies
Gamma-ray bursts and supernovae
Cosmology and Gravitation Theories
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 5 March 2026
- Language
- EN