How does the energy source distribution in a Dark Star differ from a standard star?
Dark Stars utilize a diffuse energy source throughout their volume
A standard, main-sequence star like the Sun derives almost all of its energy from a localized, intense region—the core—where thermonuclear fusion occurs, creating a sharp gradient of energy release. In contrast, the physics suggesting the support of a Dark Star relies on dark matter annihilation occurring throughout a substantial portion of the star's interior, rather than being confined to a tiny fusion zone. This means the energy generation mechanism is spread out, resulting in a different internal structure. This fundamental difference in energy distribution affects the star's overall structure, gravity profile, and effective temperature, leading to observational signatures that deviate significantly from established stellar models.
