Hawking radiation is the theoretical process by which black holes emit radiation due to quantum effects, potentially leading to their gradual evaporation over time.
Overview
Experimental Evidence
Theoretical Foundations
History Of Hawking Radiation
Mathematics Of Hawking Radiation
Related Concepts In Astrophysics
Implications For Black Hole Physics
Current Research And Future Directions
Hawking Radiation And Quantum Mechanics
Quantum Mechanics
Stephen Hawking
Black Holes
Temperature
Dark Matter
Information
Discovery
Universe
Building
โ ๏ธ Hawking radiation is a theoretical prediction by physicist Stephen Hawking in 1974.
๐ It suggests that black holes can emit radiation due to quantum effects near their event horizons.
โ๏ธ The radiation arises from virtual particle-antiparticle pairs that are spontaneously created in empty space.
๐ก Hawking radiation implies that black holes can lose mass and eventually evaporate over time.
๐ It challenges the classical view that nothing can escape a black hole's gravitational pull.
๐ The temperature of Hawking radiation is inversely proportional to the mass of the black hole.
๐ณ๏ธ Smaller black holes emit more Hawking radiation than larger ones, leading to faster evaporation.
๐ญ Finding Hawking radiation directly has yet to be achieved but remains an ongoing area of research.
๐ As a black hole loses mass through Hawking radiation, it becomes hotter and emits more radiation.
๐ The study of Hawking radiation connects quantum mechanics, thermodynamics, and general relativity.
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