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A <!--Schwarzschild -->'''kugelblitz''' is a [[theoretical physics|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 equivalence|mass–energy]] was in the form of [[radiant energy]] rather than matter
|last=Senovilla|first=J.M.M.
|year=2014
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|volume=32 |issue=1 |pages=017001
|arxiv=1408.2778|bibcode=2015CQGra..32a7001S|s2cid=119266727
}}</ref> , however as soon as it forms, it is indistinguishable from an ordinary Black Hole, meaning there is currently no way to trace the origins of a Black Hole.
[[John Archibald Wheeler]]'s 1955 ''[[Physical Review]]'' paper entitled "[[Geon (physics)|geons]]" refers to the kugelblitz phenomena and explores the idea of creating such particles (or [[toy model]]s of particles) from [[spacetime]] curvature.<ref name = Wheeler1955PhysRev>{{cite journal |last=Wheeler |first=J. A. |authorlink=John Archibald Wheeler |year=1955 |title=Geons |journal=[[Physical Review]] |doi=10.1103/PhysRev.97.511 |bibcode = 1955PhRv...97..511W |volume=97 |issue=2 |pages=511–536
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