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Is the anisotropic interaction of luminous matter responsible for the extrinsic gravitation usually attributed to exotic dark matter?

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  • Halayka, S.

Abstract

It is considered that the extrinsic gravitational attraction related to the spiral galaxy flat rotation curve problem is an emergent property of any non-spherically symmetric gravitationally bound distribution of luminous matter. Also discussed briefly within the context of this model are the hierarchy problem, the fractal nature of interaction, as well as rigid body rotation and asymptotic freedom.

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  • Halayka, S., 2009. "Is the anisotropic interaction of luminous matter responsible for the extrinsic gravitation usually attributed to exotic dark matter?," Chaos, Solitons & Fractals, Elsevier, vol. 42(1), pages 113-118.
    • Handle: RePEc:eee:chsofr:v:42:y:2009:i:1:p:113-118
    DOI: 10.1016/j.chaos.2008.10.036
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    1. El Naschie, M.S., 2008. "Using Witten’s five Brane theory and the holographic principle to derive the value of the electromagnetic fine structure constant α¯0=1/137," Chaos, Solitons & Fractals, Elsevier, vol. 38(4), pages 1051-1053.
    2. Iovane, G., 2006. "Cantorian space–time, Fantappie’s final group, accelerated universe and other consequences," Chaos, Solitons & Fractals, Elsevier, vol. 27(3), pages 618-629.
    3. El Naschie, M.S., 2008. "The internal dynamics of the exceptional Lie symmetry groups hierarchy and the coupling constants of unification," Chaos, Solitons & Fractals, Elsevier, vol. 38(4), pages 1031-1038.
    4. Iovane, G., 2007. "Hypersingular integral equations, Kähler manifolds and Thurston mirroring effect in ϵ(∞) Cantorian spacetime," Chaos, Solitons & Fractals, Elsevier, vol. 31(5), pages 1041-1053.
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