Black Hole Thermodynamics ✍️

Black hole thermodynamics reveals that black holes behave like thermodynamic systems, with properties such as temperature and entropy. According to quantum mechanics, black holes emit thermal radiation-known as Hawking radiation-due to quantum fluctuations near the event horizon. This radiation causes black holes to lose mass and slowly evaporate over time.

 The temperature of this radiation is inversely proportional to the black hole's mass, meaning smaller black holes emit more intensely. Ultimately, this suggests that black holes are not completely black, but can slowly vanish, raising deep questions about information loss and quantum gravity.