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- A theoretical idea for enabling interstellar travel is to propel a starship by creating an artificial black hole and using a parabolic reflector to reflect its Hawking radiation.
- In contrast, if it is a net emitter of energy, through Hawking radiation, it will become hotter and hotter until it boils away.
- Hawking radiation is required by the Unruh effect and the equivalence principle applied to black-hole horizons.
- Pair production is invoked in the heuristic explanation of hypothetical Hawking radiation.
- However, the escape of energy from black holes might be possible due to quantum activity (see Hawking radiation).
- However, quantum mechanical effects are believed to potentially allow the emission of Hawking radiation at this distance.
- Tiny black holes are theorized to emit Hawking radiation.
- A similar analysis can be used to explain Hawking radiation that causes the slow "evaporation" of black holes (although this is generally visualized as the escape of one particle from a virtual particle–antiparticle pair, the other particle having been captured by the black hole).
- With the Stefan–Boltzmann law, astronomers can easily infer the radii of stars. The law is also met in the thermodynamics of black holes in so-called Hawking radiation.
- Stellar-mass or larger black holes receive more mass from the cosmic microwave background than they emit through Hawking radiation and thus will grow instead of shrinking.
- The conservation of baryon number is not consistent with the physics of black hole evaporation via Hawking radiation.
- After being introduced to model the theoretical electrical characteristics of the horizon, the membrane approach was then pressed into service to model the Hawking radiation effect predicted by quantum mechanics.
- A 2009 article by Carlos Barceló, Stefano Finazzi, and Stefano Liberati uses quantum theory to argue that the Alcubierre drive at faster-than-light velocities is impossible mostly because extremely high temperatures caused by Hawking radiation would destroy anything inside the bubble at superluminal velocities and destabilize the bubble itself; the article also argues that these problems are absent if the bubble velocity is subluminal, although the drive still requires exotic matter.
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Contains translations by TU Chemnitz and Mr Honey's Business Dictionary (German-English only).
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