Torsion in the Classical Spacetime Context.

Teleparallel gravity, an empirically equivalent counterpart to general relativity, represents the influence of gravity using torsional forces. It raises questions about theory interpretation and underdetermination. To better understand the torsional forces of teleparallel gravity, we consider a cont...

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Published in:Philosophy of Science Vol. 91; no. 5; pp. 1262 - 1274
Main Authors: Meskhidze, Helen, Weatherall, James Owen
Format: Article
Published: Cambridge University Press Dec2024
Subjects:
Online Access:View this record in EBSCOhost
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          Meskhidze, Helen
          Weatherall, James Owen
        affil:
          Black Hole Initiative, Harvard University, Cambridge, MA, USA
          Department of Logic and Philosophy of Science, University of California, Irvine, Irvine, CA, USA
      su:
        General relativity (Physics)
        Model theory
        Torsion
        Spacetime
        Gravity
      sug:
        subj:
          General relativity (Physics)
          Model theory
          Torsion
          Spacetime
          Gravity
      ab: Teleparallel gravity, an empirically equivalent counterpart to general relativity, represents the influence of gravity using torsional forces. It raises questions about theory interpretation and underdetermination. To better understand the torsional forces of teleparallel gravity, we consider a context in which forces are better understood: classical spacetimes. We propose a method of incorporating torsion into the classical spacetime context that yields a classical theory of gravity with a closed temporal metric and spacetime torsion. We then prove a result analogous to the Trautman degeometrization theorem: that every model of Newton–Cartan theory gives rise, non-uniquely, to a model of this theory.
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    language: English
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