Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

MOND, MONG and the Oort cloud

Version 1 : Received: 10 January 2024 / Approved: 15 January 2024 / Online: 15 January 2024 (11:51:42 CET)

How to cite: Sivaram, C.; Kiren, O.; Rebecca, L.; Kenath, A. MOND, MONG and the Oort cloud. Preprints 2024, 2024011126. https://doi.org/10.20944/preprints202401.1126.v1 Sivaram, C.; Kiren, O.; Rebecca, L.; Kenath, A. MOND, MONG and the Oort cloud. Preprints 2024, 2024011126. https://doi.org/10.20944/preprints202401.1126.v1

Abstract

The definitive negative results of various direct searches for dark matter particles and non-observation of them has increasingly indicated that we should consider alternate models like the Modification of Newtonian Dynamics (MOND) and Modification of Newtonian Gravity (MONG). It is puzzling how the Oort cloud, despite its great distance from the Sun, is gravitationally bound to the Sun’s gravity. In this work, we suggest that this could be explained by the modifications to Newtonian dynamics (MOND) and to gravity (MONG).

Keywords

Oort cloud; Modified Newtonian Dynamics; Modified Newtonian Gravity

Subject

Physical Sciences, Astronomy and Astrophysics

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