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

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  • Saoussan Kallel-Jallouli

    (Faculté des Sciences de Tunis, Department of Mathematics, Université de Tunnis El Manar, LR03ES04, Tunis, 2092, Tunisia)

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.

Suggested Citation

  • Saoussan Kallel-Jallouli, 2024. "Keplerian Motion Inside an Isolated Dark Matter Halo and the Hubble’s Law," International Journal of Research and Scientific Innovation, International Journal of Research and Scientific Innovation (IJRSI), vol. 11(9), pages 1225-1235, September.
  • Handle: RePEc:bjc:journl:v:11:y:2024:i:9:p:1225-1235
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