Thorne–Hawking–Ross Formalism

The Thorne–Hawking–Ross Formalism is a theoretical framework used to understand black holes and the processes governing their behavior. Developed by physicists Kip Thorne, Stephen Hawking, and James Ross, it describes the interaction of matter and energy around black holes, particularly focusing on how they emit radiation, known as Hawking radiation. This formalism helps explain how black holes can lose mass and potentially evaporate over time, bridging concepts from general relativity and quantum mechanics. It provides insights into the fundamental nature of black holes and their role in the universe.