Galaxy rotation curves in the \(\mu\)-deformation based approach to dark matter

We elaborate further the \(\mu\)-deformation-based approach to modeling dark matter, in addition to the earlier proposed use of \(\mu\)-deformed thermodynamics. Herein, we construct \(\mu\)-deformed analogs of the Lane-Emden equation (for density profiles), and find their solutions. Using these, we...

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Veröffentlicht in:	arXiv.org 2019-11
Hauptverfasser:	Gavrilik, A M, Kachurik, I I, Khelashvili, M V
Format:	Artikel
Sprache:	eng
Schlagworte:	Bose-Einstein condensates Dark matter Deformation Galactic rotation Galaxies Mathematical models Parameters
Online-Zugang:	Volltext
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