Kugelblitz (astrophysics)

In theoretical physics, a Schwarzschild kugelblitz is a concentration of heat, light or radiation so intense that its energy forms an event horizon and becomes self-trapped: according to general relativity and the equivalence of mass and energy, if enough radiation is aimed into a region, the concentration of energy can warp spacetime enough for the region to become a black hole, although this would be a black hole whose original mass–energy had been in the form of radiant energy rather than matter.^[1] In simpler terms, a kugelblitz is a black hole formed from radiation as opposed to matter. Such a black hole would nonetheless have properties identical to one of equivalent mass and angular momentum began more conventionally, following the no-hair theorem.

The best-known reference to the kugelblitz idea in English is probably John Archibald Wheeler's 1955 paper "Geons",^[2] which explored the idea of creating particles (or toy models of particles) from spacetime curvature, called geons. Wheeler's paper on geons also introduced the idea that lines of electric charge trapped in a wormhole throat might be used to model the properties of a charged particle-pair.

Kugelblitz drives have been considered possible future black hole starship engines.^[3][4]

A man-made kugelblitz would only be conceivable with a gamma-ray laser 1 billion times stronger than the current hypothesized ones, and it would have to produce a pulse that was one 100 billionth of the current duration of a modern laser's pulse. A single pulse would need to equate to the energy produced by the sun in 1/10 of a second.

A kugelblitz of this size would last five years, and a device similar to a Dyson sphere could be constructed around it to harness the energy produced by the Hawking radiation.

See also[]

• Bekenstein bound
• Ronald Mallett
• Micro black hole

References[]

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