「ファイアウォール (物理学)」の版間の差分

<!---A '''black hole firewall''' is a hypothetical phenomenon where an observer that falls into an old [[black hole]] encounters high-energy [[quantum|quanta]] at (or near) the [[event horizon]]. The "firewall" phenomenon was proposed in 2012 by Almheiri, [[Donald Marolf|Marolf]], [[Joseph Polchinski|Polchinski]], and Sully<ref>A. Almheiri, D. Marolf, J. Polchinski, and J. Sully (2012). "Black Holes: Complementarity or Firewalls?," arXiv:1207.3123 [http://arxiv.org/abs/1207.3123]</ref> as a possible solution to an apparent inconsistency in [[black hole complementarity]]. The proposal is often referred to as the "AMPS" firewall, an acronym for the names of the authors of the 2012 paper. The occurrence of a firewall at the event horizon of a black hole was proposed by [[Friedwardt Winterberg]] 11 years earlier.<ref>{{cite journal|last=Winterberg|first=Friedwardt|title=Gamma-Ray Bursters and Lorentzian Relativity|journal=Z. Naturforsch|date=2001 Aug 29|volume=56a|pages=889–892}}</ref> The use of a firewall to resolve this inconsistency remains controversial as of 2013, with high-energy physicists divided as to the solution to the paradox.<ref name="nature/Fire in the hole">Astrophysics: Fire in the hole! http://www.nature.com/news/astrophysics-fire-in-the-hole-1.12726</ref>-->

 

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