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Standard and generalized Newtonian gravities as `gauge' theories of the extended Galilei group: II. Dynamical 3-space theories

R De Pietri et al 1995 Class. Quantum Grav. 12 255-272   doi: 10.1088/0264-9381/12/1/020  Help

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R De Pietri-+++, L Lusanna§ and M Pauri++||
-+ Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA
++ INFN, Sezione di Milano, Gruppo collegato di Parma, Italy
§ INFN, Sezione di Firenze, Largo E Fermi 2, 50127 Arcetri (FI), Italy
|| Centre for Philosophy of Science, University of Pittsburgh, 817D Cathedral of Learning, Pittsburgh, PA 15260, USA

Abstract. In the preceding paper we developed a reformulation of Newtonian gravitation as a gauge theory of the extended Galilei group. In the present one we derive two generalizations of Newton's theory (a 10-fields and an 11-fields theory) in terms of an explicit Lagrangian realization of the absolute time dynamics of a Riemannian 3-space. They turn out to be gauge-invariant theories of the extended Galilei group in the same sense in which general relativity is said to be a gauge theory of the Poincaré group. The 10-fields theory provides a dynamical realization of some of the so-called `Newtonian spacetime structures' which have been classified geometrically by Künzle and Kuchar. The 11-fields theory involves a dilaton-like scalar potential in addition to a generalized Newtonian potential and, like general relativity, has a 3-metric with two dynamical degrees of freedom. It is interesting to find that, within the linear approximation, such degrees of freedom show graviton-like features: they satisfy a wave equation and propagate with a velocity related to the generalized scalar Newtonian potential.

PACS numbers: 0450, 0490, 0350

Print publication: Issue 1 (January 1995)
Received 6 May 1994, in final form 30 August 1994

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