We propose a Lorentz-covariant theory of gravity, and explain its theoretical origins in the problem of time in Newtonian physics. In this retarded gravitation theory (RGT), the gravitational force depends upon both retarded position and velocity, and the equations of motion are time-asymmetric retarded functional differential equations. We explicitly solve these equations, under simplifying assumptions, for various NASA spacecraft. This shows that the differences from Newtonian gravity, though tiny within the solar system, are just appropriate to explain the flyby anomaly as a effect due to earth’s rotation. The differences can, however, be large in the case of a spiral galaxy, and we show that the combined velocity drag from a large number of co-rotating stars enormously speeds up a test particle. Thus, the non-Newtonian behaviour of rotation curves in a spiral galaxy may be explained as being due to velocity drag rather than dark matter. RGT can also be tested in the laboratory. It necessitates a reappraisal of current laboratory methods of determining the Newtonian gravitational constant G. Since RGT makes no speculative assumptions, its refutation would have serious implications across physics.
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1 October 2012
THE SIXTH INTERNATIONAL SCHOOL ON FIELD THEORY AND GRAVITATION-2012
23–27 April 2012
Petrópolis - RJ, Brazil
Research Article|
October 01 2012
Retarded gravitation theory Available to Purchase
C. K. Raju
C. K. Raju
School of Mathematical Sciences, Universiti Sains Malaysia, 11800 Penang, Malaysia and Current address: Albukhary International University, 05200 Alor Setar,
Malaysia
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C. K. Raju
School of Mathematical Sciences, Universiti Sains Malaysia, 11800 Penang, Malaysia and Current address: Albukhary International University, 05200 Alor Setar,
Malaysia
AIP Conf. Proc. 1483, 260–276 (2012)
Citation
C. K. Raju; Retarded gravitation theory. AIP Conf. Proc. 1 October 2012; 1483 (1): 260–276. https://doi.org/10.1063/1.4756973
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