Schematic illustration of the competing processes governing the evolution of an endoparasitic black hole (EBH) inside a compact star. The EBH simultaneously accretes baryonic matter from the stellar medium (black arrows) and captured dark-matter particles (blue arrows), while losing mass through Hawking radiation (red arrows). The three panels illustrate the possible regimes: (a) accretion dominates and the EBH grows, (b) accretion and Hawking evaporation balance and the EBH remains at approximately constant mass, and (c) Hawking evaporation dominates and the EBH shrinks and ultimately evaporates. The relative number of arrows schematically represents the balance between the corresponding mass-flow rates. In case (b), EBH can have a mass as small as 40 metric tons. Credit: H. A. Adarsha
...Read More
Astronomy/Space 
Recent Comments