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Classical relativity theory

In Jeremy Butterfield & John Earman (eds.), Philosophy of Physics. Amsterdam and Boston: Elsevier (2006)

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  1. The cosmological constant, the fate of the universe, unimodular gravity, and all that.John Earman - 2003 - Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics 34 (4):559-577.
    The cosmological constant is back. Several lines of evidence point to the conclusion that either there is a positive cosmological constant or else the universe is filled with a strange form of matter (“quintessence”) that mimics some of the effects of a positive lambda. This paper investigates the implications of the former possibility. Two senses in which the cosmological constant can be a constant are distinguished: the capital Λ sense in which lambda is a universal constant on a par with (...)
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  • On relativity theory and openness of the future.Howard Stein - 1991 - Philosophy of Science 58 (2):147-167.
    It has been repeatedly argued, most recently by Nicholas Maxwell, that the special theory of relativity is incompatible with the view that the future is in some degree undetermined; and Maxwell contends that this is a reason to reject that theory. In the present paper, an analysis is offered of the notion of indeterminateness (or "becoming") that is uniquely appropriate to the special theory of relativity, in the light of a set of natural conditions upon such a notion; and reasons (...)
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  • .Jeremy Butterfield & John Earman - 1977
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  • The force of Newtonian cosmology: Acceleration is relative.John D. Norton - 1995 - Philosophy of Science 62 (4):511-522.
    1. Introduction. David Malament has described a natural and satisfying resolution of the traditional problems of Newtonian cosmology—natural in the sense that it effects the escape by altering Newtonian gravitation theory in a way that leaves its observational predictions completely unaffected. I am in full agreement with his approach. There is one part of his account, however, over which Malament has been excessively modest. The resolution requires a modification to Newtonian gravitation theory. Malament presents the modification as so straightforward as (...)
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  • The Cosmological Woes of Newtonian Gravitation Theory.John D. Norton - 1982 - In John Norton (ed.).
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  • Theories of Newtonian gravity and empirical indistinguishability.Jonathan Bain - 2004 - Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics 35 (3):345-376.
    In this essay, I examine the curved spacetime formulation of Newtonian gravity known as Newton–Cartan gravity and compare it with flat spacetime formulations. Two versions of Newton–Cartan gravity can be identified in the physics literature—a ‘‘weak’’ version and a ‘‘strong’’ version. The strong version has a constrained Hamiltonian formulation and consequently a well-defined gauge structure, whereas the weak version does not (with some qualifications). Moreover, the strong version is best compared with the structure of what Earman (World enough and spacetime. (...)
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  • Conventionalism and the Philosophy of Henri Poincare.Peter Laurence Spirtes - 1981 - Dissertation, University of Pittsburgh
    The thesis of the conventionality of simultaneity in the special theory of relativity has been the subject of controversy for over fifty years Unfortunately, debates about this thesis have sometimes been marred by a failure to clearly distinguish different conventionalist theories. In my dissertation I evaluate, clarify, and carefully distinguish a number of different conventionalist theories, and thus clear up some of the confusion surrounding the thesis of the conventionality of simultaneity . In particular, I examine the following conventionalist theories. (...)
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  • Foundations and current problems of general relativity (notes by graham dixon, petros florides and gerald lemmer).Andrzej Trautman - 1965 - In A. Trautman (ed.), Lectures on general relativity. Englewood Cliffs, N.J.,: Prentice-Hall. pp. 1--1.
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  • The analysis of singular spacetimes.Erik Curiel - 1999 - Philosophy of Science 66 (3):145.
    Much controversy surrounds the question of what ought to be the proper definition of 'singularity' in general relativity, and the question of whether the prediction of such entities leads to a crisis for the theory. I argue that a definition in terms of curve incompleteness is adequate, and in particular that the idea that singularities correspond to 'missing points' has insurmountable problems. I conclude that singularities per se pose no serious problem for the theory, but their analysis does bring into (...)
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