2019
DOI: 10.1016/j.shpsb.2018.10.001
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Background independence: Lessons for further decades of dispute

Abstract: Background independence begins life as an informal property that a physical theory might have, often glossed as 'doesn't posit a fixed spacetime background'. Interest in trying to offer a precise account of background independence has been sparked by the pronouncements of several theorists working on quantum gravity that background independence embodies in some sense an essential discovery of the General Theory of Relativity, and a feature we should strive to carry forward to future physical theories. This pap… Show more

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Cited by 4 publications
(6 citation statements)
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“…where M is a differentiable (3+1)-manifold, η ab , is a fixed Lorentzian metric field 9 , and φ : M → R is a dynamical real scalar field. By contrast, a theory's dynamically possible models (DPMs), are the subset of the KPMs which obey the theory's dynamical equations.…”
Section: A Klein Gordon Equationmentioning
confidence: 99%
See 4 more Smart Citations
“…where M is a differentiable (3+1)-manifold, η ab , is a fixed Lorentzian metric field 9 , and φ : M → R is a dynamical real scalar field. By contrast, a theory's dynamically possible models (DPMs), are the subset of the KPMs which obey the theory's dynamical equations.…”
Section: A Klein Gordon Equationmentioning
confidence: 99%
“…It is important to distinguish two kinds of symmetry [5] (spacetime 8 The name SR1 is picked to follow the notation set in [1]. 9 It's important to note the difference between ηµν and η ab . Any tensor object with greek indices (e.g., ηµν ) is to be understood as the components of a certain tensor in a particular coordinate system.…”
Section: Klein Gordon -Symmetriesmentioning
confidence: 99%
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