In an intriguing development in astrophysics, the Max Planck Institute for Astrophysics has devised a model suggesting that primordial black holes, proposed by Stephen Hawking, could be caught within newly formed stars, known as Hawking Stars. These black holes, theorized to have formed immediately after the Big Bang, could vary in size from that of an atom to a mountain and are purportedly present in stars like the Sun, enhancing their brightness.
Unraveling the Mystery of Hawking Stars
The research, published in The Astrophysical Journal, argues that Hawking Stars could be a key to understanding stellar evolution and the existence of dark matter. It suggests that these stars could be detected through a technique known as astroseismology. This intriguing hypothesis provides a fresh perspective on the study of black holes, taking us a step closer to decoding the enigmas of the universe.
Linking Primordial Black Holes to Dark Matter
The Max Planck Institute's model offers a new explanation to the existence of dark matter. It postulates that primordial black holes ensnared by Hawking Stars might be a substantial constituent of dark matter. This confluence of black holes and dark matter paves the way for a more comprehensive understanding of the cosmic realm and its myriad mysteries.
The study also suggests that Hawking Stars could be more commonplace in globular clusters and ultra-faint dwarf galaxies. This could provide a fresh pathway to test the existence of primordial black holes and their relationship with dark matter.