The relativity and equivalence principles for self-gravitating systems

In Dennis Lehmkuhl, Gregor Schiemann & Erhard Scholz (eds.), Towards a Theory of Spacetime Theories. New York, NY: Birkhauser (2016)
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Abstract

I criticise the view that the relativity and equivalence principles are consequences of the small-scale structure of the metric in general relativity, by arguing that these principles also apply to systems with non-trivial self-gravitation and hence non-trivial spacetime curvature (such as black holes). I provide an alternative account, incorporating aspects of the criticised view, which allows both principles to apply to systems with self-gravity.

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2009-03-27

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David Wallace
University of Pittsburgh

Citations of this work

Fundamental and Emergent Geometry in Newtonian Physics.David Wallace - 2020 - British Journal for the Philosophy of Science 71 (1):1-32.
Empirical Consequences of Symmetries.David Wallace & Hilary Greaves - 2014 - British Journal for the Philosophy of Science 65 (1):59-89.
The case for black hole thermodynamics part I: Phenomenological thermodynamics.David Wallace - 2018 - Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics 64:52-67.
The case for black hole thermodynamics part II: Statistical mechanics.David Wallace - 2018 - Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics 66 (C):103-117.
A Primer on Energy Conditions.Erik Curiel - 2016 - In Dennis Lehmkuhl, Gregor Schiemann & Erhard Scholz (eds.), Towards a Theory of Spacetime Theories. New York, NY: Birkhauser. pp. 43-104.

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