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Phase Shift of the Keplerian Orbits inside Dark Matter Halos

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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

A new theory proposed the existence of a new kind of unseen staff named “Zaman†, responsible for the flow of time by its spin. Zaman solves the Dark Matter enigma. Moreover, for an isolated Zaman spherical halo U with differential rotation, if the relation between the radius of each shell R and the length T of its day is Keplerian; that is T2/R3 is constant, then, we proved the known linear Hubble relation is satisfied. In this work, we shall see how some distances can be elongated. We shall prove the Keplerian trajectories are discontinuous. More precisely, after each period, any test particle inside U will receive an instantaneous kick-off to be shifted from its initial orbital phase.

Suggested Citation

  • Saoussan Kallel-Jallouli, 2024. "Phase Shift of the Keplerian Orbits inside Dark Matter Halos," International Journal of Research and Scientific Innovation, International Journal of Research and Scientific Innovation (IJRSI), vol. 11(11), pages 500-517, November.
    • Handle: RePEc:bjc:journl:v:11:y:2024:i:11:p:500-517
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    References listed on IDEAS

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    1. H. Spruit & E. S. Phinney, 1998. "Birth kicks as the origin of pulsar rotation," Nature, Nature, vol. 393(6681), pages 139-141, May.
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