Fuzzball (string theory) (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Fuzzball (string theory)" in English language version.

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aps.org

physics.aps.org

archive.today

arxiv.org

  • The primary paper was a 2002 publication (#3, below) titled "A proposal to resolve the black hole information paradox". The list:
    1) "AdS/CFT duality and the black hole information paradox", Oleg Lunin and Samir D. Mathur, arXiv:hep-th/0109154, (September 20, 2001). This is a paper about the AdS/CFT correspondence, which examines the relationships between two different theories: Anti-de Sitter space (AdS), and Conformal field theory (CFT), wherein the former deals with quantum gravity and the latter deals with quantum field theory. The AdS/CFT correspondence is central to resolving the black hole information paradox.
    2) "Statistical interpretation of Bekenstein entropy for systems with a stretched horizon", Oleg Lunin and Samir D. Mathur, ArXiv:hep-th/0202072, (February 12, 2002)
    3) "A proposal to resolve the black hole information paradox", Samir D. Mathur, ArXiv:hep-th/0205192, (May 19, 2002)
    4) "The fuzzball proposal for black holes: an elementary review", Samir D. Mathur, ArXiv:hep-th/0502050, (February 3, 2005)
    5) "What Exactly is the Information Paradox?", Samir D. Mathur, ArXiv:0803.2030, (March 13, 2008)
    6) "Fuzzballs and the information paradox: a summary and conjectures", Samir D. Mathur, ArXiv:0909.1038, (October 24, 2008)
    7) "The information paradox: A pedagogical introduction", Samir D. Mathur, ArXiv:0909.1038, (January 25, 2011)
    8) "Black Holes and Beyond", Samir D. Mathur, ArXiv:1205.0776, (May 14, 2012)
  • Samir D. Mathur. "A proposal to resolve the black hole information paradox", ArXiv:hep-th/0205192, (May 19, 2002).

atlas.cern

brainmaster.com

  • In his paper, "Particle Creation by Black Holes" (PDF), Hawking wrote, in §2 on p. 204, as follows:
    However there is a classical phenomenon called superradiance [14-17] in which waves incident in certain modes on a rotating or charged black hole are scattered with increased amplitude [see Section (3)].

    In §3, 'Angular Momentum and Charge,' which is 2½ pages starting on p. 213, Hawking began the formula-rich section with the following:

    If the collapsing body was rotating or electrically charged, the resulting black hole would settle down to a stationary state which was described, not by the Schwarzchild solution, but by a charged Kerr solution characterised by the mass M, the angular momentum J, and the charge Q.

    Superradiance was proposed theoretically by Robert H. Dicke in 1954, and in 1973 was experimentally observed in hydrogen fluoride atoms by N. Skribanowitz et al. However, superradiance is yet to be detected at black holes, per "Black hole 'superradiance' phenomenon may aid quest for dark matter", Paul Sutter, Space.com, (August 16, 2022).

caltech.edu

ned.ipac.caltech.edu

doi.org

fnal.gov

news.fnal.gov

home.cern

nytimes.com

ohio-state.edu

asc.ohio-state.edu

  • Samir D. Mathur. "The fuzzball paradigm for black holes: FAQ", (January 22, 2009) (395 KB).

osu.edu

news.osu.edu

quantamagazine.org

  • Jennifer Ouellette. "The Fuzzball Fix for a Black Hole Paradox", Quanta Magazine, (June 23, 2015).
  • Nadis, Steve (2 December 2019). "Black Hole Singularities Are as Inescapable as Expected". quantamagazine.org. Quanta Magazine. Archived from the original on 14 April 2020. Retrieved 22 April 2020.

sciencefocus.com

scientificamerican.com

space.com

  • In his paper, "Particle Creation by Black Holes" (PDF), Hawking wrote, in §2 on p. 204, as follows:
    However there is a classical phenomenon called superradiance [14-17] in which waves incident in certain modes on a rotating or charged black hole are scattered with increased amplitude [see Section (3)].

    In §3, 'Angular Momentum and Charge,' which is 2½ pages starting on p. 213, Hawking began the formula-rich section with the following:

    If the collapsing body was rotating or electrically charged, the resulting black hole would settle down to a stationary state which was described, not by the Schwarzchild solution, but by a charged Kerr solution characterised by the mass M, the angular momentum J, and the charge Q.

    Superradiance was proposed theoretically by Robert H. Dicke in 1954, and in 1973 was experimentally observed in hydrogen fluoride atoms by N. Skribanowitz et al. However, superradiance is yet to be detected at black holes, per "Black hole 'superradiance' phenomenon may aid quest for dark matter", Paul Sutter, Space.com, (August 16, 2022).

uniroma1.it

phys.uniroma1.it

vttoth.com

web.archive.org

  • Nadis, Steve (2 December 2019). "Black Hole Singularities Are as Inescapable as Expected". quantamagazine.org. Quanta Magazine. Archived from the original on 14 April 2020. Retrieved 22 April 2020.