A Role for the Fauxrizon in the Semiclassical Limit of a Fuzzball.

Recent work on the status of astrophysical modeling in the wake of quantum gravity indicates that a "fauxrizon" (a portmanteau of faux horizon), such as is relevant to understanding astrophysical black holes according to the fuzzball proposal within string theory, might ultimately solve the familiar...

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Publicado en:Philosophy of Science Vol. 91; no. 1; pp. 225 - 243
Autor principal: Schneider, Mike D.
Formato: Artículo
Publicado: Cambridge University Press Jan2024
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Acceso en línea:Ver este registro en EBSCOhost
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        atl: A Role for the Fauxrizon in the Semiclassical Limit of a Fuzzball.
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        au: Schneider, Mike D.
        affil: Department of Philosophy, University of Missouri, Columbia, MO, USA
      su:
        String theory
        Black holes
        Semiclassical limits
        Quantum gravity
      sug:
        subj:
          String theory
          Black holes
          Semiclassical limits
          Quantum gravity
      ab: Recent work on the status of astrophysical modeling in the wake of quantum gravity indicates that a "fauxrizon" (a portmanteau of faux horizon), such as is relevant to understanding astrophysical black holes according to the fuzzball proposal within string theory, might ultimately solve the familiar black hole evaporation paradox. I clarify, with general upshots for the foundations of quantum gravity research, some of what this suggestion would amount to: identification of intertheoretic constraints on global spacetime structure in (observer-relative) semiclassical models of fuzzballs.
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