Similarity, Topology, and Physical Significance in Relativity Theory

British Journal for the Philosophy of Science 67 (2):365-389 (2016)
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Abstract

Stephen Hawking, among others, has proposed that the topological stability of a property of space-time is a necessary condition for it to be physically significant. What counts as stable, however, depends crucially on the choice of topology. Some physicists have thus suggested that one should find a canonical topology, a single ‘right’ topology for every inquiry. While certain such choices might be initially motivated, some little-discussed examples of Robert Geroch and some propositions of my own show that the main candidates—and each possible choice, to some extent—faces the horns of a no-go result. I suggest that instead of trying to decide what the ‘right’ topology is for all problems, one should let the details of particular types of problems guide the choice of an appropriate topology.

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Samuel C. Fletcher
University of Minnesota

Citations of this work

Categories and the Foundations of Classical Field Theories.James Owen Weatherall - forthcoming - In Elaine Landry (ed.), Categories for the Working Philosopher. Oxford, UK: Oxford University Press.
The Implementation, Interpretation, and Justification of Likelihoods in Cosmology.C. D. McCoy - 2018 - Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics 62:19-35.
Toward an Understanding of Parochial Observables.Benjamin Feintzeig - 2016 - British Journal for the Philosophy of Science:axw010.

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Philosophical papers.David Kellogg Lewis - 1983 - New York: Oxford University Press.
Counterfactuals.David Lewis - 1973 - Foundations of Language 13 (1):145-151.
Counterfactuals.David Lewis - 1973 - Tijdschrift Voor Filosofie 36 (3):602-605.

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