supermassive black hole. These enigmatic entities, ranging from millions to billions of times the mass of our Sun, generate such intense gravitational pull that even light cannot escape their grasp. These black holes are so colossal that they influence the formation of the galaxies around them. They play a crucial role in star creation, galactic development, and even the dynamics of complete clusters. Our Milky Way galaxy is no different. At its core resides Sagittarius A*, a supermassive black hole weighing four million solar masses. While these black holes are essential for the existence of galaxies, we are still uncertain about the precise mechanisms that lead to the formation of these gigantic cosmic entities.
Nevertheless, a recent investigation focusing on the Pop III.1 framework, spearheaded by theoretical astrophysicist Jonathan Tan from the University of Virginia, tackles this issue with a renewed viewpoint. Tan, a distinguished professor well-known for his contributions to the fields of star and planet formation, utilizes decades of research to establish the foundation for an innovative theory that may elucidate how these colossal cosmic objects came into being. The findings suggest that the collapse of first-generation stars, often referred to as primordial stars, might have led to the emergence of supermassive black holes.
