Article
Version 1
Preserved in Portico This version is not peer-reviewed
2D behavior of Gravity at Large Distance
Version 1
: Received: 10 August 2023 / Approved: 10 August 2023 / Online: 11 August 2023 (12:02:40 CEST)
Version 2 : Received: 11 August 2023 / Approved: 14 August 2023 / Online: 14 August 2023 (15:17:27 CEST)
Version 3 : Received: 10 November 2023 / Approved: 13 November 2023 / Online: 13 November 2023 (12:05:41 CET)
Version 4 : Received: 31 December 2023 / Approved: 3 January 2024 / Online: 4 January 2024 (03:31:45 CET)
Version 5 : Received: 12 May 2024 / Approved: 13 May 2024 / Online: 13 May 2024 (12:09:51 CEST)
Version 2 : Received: 11 August 2023 / Approved: 14 August 2023 / Online: 14 August 2023 (15:17:27 CEST)
Version 3 : Received: 10 November 2023 / Approved: 13 November 2023 / Online: 13 November 2023 (12:05:41 CET)
Version 4 : Received: 31 December 2023 / Approved: 3 January 2024 / Online: 4 January 2024 (03:31:45 CET)
Version 5 : Received: 12 May 2024 / Approved: 13 May 2024 / Online: 13 May 2024 (12:09:51 CEST)
How to cite: Kumar, N. 2D behavior of Gravity at Large Distance. Preprints 2023, 2023080891. https://doi.org/10.20944/preprints202308.0891.v1 Kumar, N. 2D behavior of Gravity at Large Distance. Preprints 2023, 2023080891. https://doi.org/10.20944/preprints202308.0891.v1
Abstract
In this paper, we show that the entropy or information flow of a gravitational system constrains the dependence of gravitational force on radial distance r which for very large r is equivalent to gravity in two dimensions. This proposal solves the problem of flat rotation curves of galaxies at very large distances.
Keywords
Dark Matter; Modified Gravity
Subject
Physical Sciences, Theoretical Physics
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.
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