Keplerian Motion Inside an Isolated Dark Matter Halo and the Hubble’s Law

Saoussan Kallel-Jallouli
Additional contact information
Saoussan Kallel-Jallouli: Faculté des Sciences de Tunis, Department of Mathematics, Université de Tunnis El Manar, LR03ES04, Tunis, 2092, Tunisia

International Journal of Research and Scientific Innovation, 2024, vol. 11, issue 9, 1225-1235

Abstract: : Recently, the existence of a new kind of staff, named “Zaman†, responsible for time variation by its spin, was established. The proposed model offered a suitable solution for the Dark Matter enigma. In this work, we generalize the previously solid body rotating spherical halo U to a differential rotation, where each spherical shell of radius R has a length of the day T(R) related to R with the Kepler’s relation: . We prove that the linear Hubble’s relation, , is just a consequence of our new “time†-model, and does not need any special hypothesis nor any special non Euclidean topology on U.

Date: 2024
References: View complete reference list from CitEc
Citations:

Downloads: (external link)
https://www.rsisinternational.org/journals/ijrsi/d ... ssue-9/1225-1235.pdf (application/pdf)
https://rsisinternational.org/journals/ijrsi/artic ... and-the-hubbles-law/ (text/html)

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:bjc:journl:v:11:y:2024:i:9:p:1225-1235

Access Statistics for this article

International Journal of Research and Scientific Innovation is currently edited by Dr. Renu Malsaria

More articles in International Journal of Research and Scientific Innovation from International Journal of Research and Scientific Innovation (IJRSI)
Bibliographic data for series maintained by Dr. Renu Malsaria ().