Kugelblitz (astrophysics)

id: kugelblitz-astrophysics-178-18778406
title: Kugelblitz (astrophysics)
text: A kugelblitz is a theoretical astrophysical object predicted by general relativity. It is a concentration of heat, light or radiation so intense that its energy forms an event horizon and becomes self-trapped. In other words, if enough radiation is aimed into a region of space, the concentration of energy can warp spacetime so much that it creates a black hole. This would be a black hole whose original mass–energy was in the form of radiant energy rather than matter; however, there is currently
brand slug: wiki
category slug: encyclopedia
description: Black hole created from the concentration of energy
original url: https://en.wikipedia.org/wiki/Kugelblitz_(astrophysics)
date created: 2006-11-08T20:15:38Z
date modified: 2024-09-04T17:58:08Z
main entity: {"identifier":"Q3003861","url":"https://www.wikidata.org/entity/Q3003861"}
image:
fields total: 13
integrity: 15

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