The Amplification Effect of Parallel Counter-streaming Gravitons

Authors: Kurt L. Becker

Amplification effect of counter-streaming gravitons may give a physical foundation to MOND. Abstract: Modified Newtonian Dynamics can explain the flat rotation curves of stars in very weak gravitational fields in the outlying regions of our galaxy, but it needs a physical basis to form a complete theory. In the MOND paradigm, acceleration decreases slower, by 1/r, than in Newtonian dynamics, 1/r2. This paper explores a physical process with amplifies the stream of gravitons between distant stars, thereby keeping gravity stronger at longer distances, yet allowing the acceleration to decrease as 1/r. The streams of gravitons between distant stars is parallel, allowing time for counter-streaming gravitons to interact with each other. This interaction will compress the beam and, most importantly, will pull adjacent streams into the main gravitation stream. This results in an amplification of gravity between the two stars. The frequency of gravitational interaction with the mass of the stars will decrease as 1/r, due to the longer travel time of the gravitons between the stars.

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[v1] 2019-11-03 10:26:31

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