Sharif Digital Repository

Black holes are theoretically significant because they are (ideal) entities fully described by just three properties: mass, charge, and spin. Their importance also stems from their unique status as spacetime entities with universal properties, including the event horizon and—when including the singularity—representing the boundary of space and time. Beyond their spacetime properties, black holes are also thermodynamic systems. Their behavior requires a theory that integrates both spacetime and thermodynamics. A black hole is something that requires both a theory of spacetime and a theory of thermodynamics to describe and explain its behavior. A consistent description of time, spacetime, and...