Some considerations concerning newtonian charts
In Part I, spherically symmetric solutions of Rastall's 1971 gravitational field equations for empty space-time are examined. One static solution is found to be just a static spherically symmetric Newtonian metric; i.e., the metric of Rastall's 1968 scalar theory of gravity. However, there...
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Language: | English |
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University of British Columbia
2011
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Online Access: | http://hdl.handle.net/2429/34024 |