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. Preprints2024, 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
Sivaram, C.; Kiren, O.; Rebecca, L.; Kenath, A. MOND, MONG and the Oort cloud. Preprints2024, 2024011126. https://doi.org/10.20944/preprints202401.1126.v1
APA Style
Sivaram, C., Kiren, O., Rebecca, L., & Kenath, A. (2024). MOND, MONG and the Oort cloud. Preprints. https://doi.org/10.20944/preprints202401.1126.v1
Chicago/Turabian Style
Sivaram, C., Louise Rebecca and Arun Kenath. 2024 "MOND, MONG and the Oort cloud" Preprints. 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).
Copyright:
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.