Linked from

The 21 pages that link to Hawking radiation, each with the reason it gives.

• Black holeRelated: It gives black holes a temperature and predicts their eventual evaporation.

• Quantum gravityRelated: It links quantum field theory, gravity, and black-hole thermodynamics.

• Event horizonRelated: It gives black holes a temperature and links horizons to quantum effects.

• Black hole information paradoxRelated: Its apparently thermal character makes the radiation seem unable to encode the details of infalling matter.

• Black hole thermodynamicsRelated: Its temperature gives black holes a physical thermal interpretation.

• Primordial black holeRelated: It can evaporate low-mass primordial black holes over cosmic time.

• Planck scaleRelated: Its derivation combines quantum fields and classical gravity, foreshadowing the regime’s conceptual tensions.

• Classical limitRelated: Its derivation combines quantum fields with a classical spacetime background.

• Heat death of the universeRelated: Black-hole evaporation may be among the final processes in a heat-death scenario.

• Vacuum energyRelated: It illustrates how vacuum states near horizons can produce observable energy flux.

• Astronomical black holesRelated: It implies that black holes can lose mass even while trapping classical matter and light.

• Black hole astronomyRelated: Its direct detection is beyond current capability, leaving a major prediction observationally untested.

• Micro black holeRelated: It would make a sufficiently small black hole evaporate rapidly.

• Quantum vacuum stateRelated: Black-hole horizons make the choice of vacuum crucial to predicting outgoing particles.

• Timeline of the far futureRelated: It implies that black holes may evaporate over extraordinarily long timescales.

• White holeRelated: Black-hole evaporation gives a physical process that does not straightforwardly produce a white hole.