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Billy Meier
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Rosunwell 'o5

Billy Meier Beamship, showing energy displacement

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Black Hole
Infalling matter
Sharp event horizon
point of no return
Point-like singularity
Hawking radiation consists of random energy
Potential wormholes to other universes
Multiverses

Fuzzball
Infalling matter
No sharp event horizon
Messy surface stores information
in vibrating strings
Hawking radiation carries
information back out
Wormholes may exist
but are unreachable

Evolution theory of black holes
1915
Albert Einstein's general theory of relativity describes how matter and energy bend space-time.
1916
Karl Schwarzschild solves Einstein's equations for the case f a very dense point mass.
1965
Roger Penrose develops the idea of a singularity, a point wheere space becomes infinitely dense.
1967
John Wheeler coins the term "black hole" to describe a star that collapses to a singularity.
1969
Penrose suggests that singularities are hidden behind an event horizon.
1973
Stephen Hawking and Jacob Bekenstein calculate the entropy - a measure of the amount of information - in a black hole and get a very large answer.
1975
Hawking shows quantum mechanics predicts that energy escapes from black holes. he and colleague Kip Thorne bet John Preskill that this Hawking radiation cannot carry information.
1996
Andrew Strominger and Cumrun Vafa use string theory to calculate the entropy of a black hole, geting the same answer as Hawking and Bekenstein.
2004
Calculations in quantum mechanics and string theory suggest that information can escape from black hles. Hawking concedes the bet. Models of black holes from string theory cast doubt on the idea of singularity.

New Scientist 22 January 2005 P.30-33

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