Galactic dark matter and Bertrand space-times

Dipanjan Dey, Kaushik Bhattacharya, and Tapobrata Sarkar
Phys. Rev. D 87, 103505 – Published 10 May 2013

Abstract

Bertrand space-times (BSTs) are static, spherically symmetric solutions of Einstein’s equations, that admit stable, closed orbits. Starting from the fact that to a good approximation, stars in the disc or halo regions of typical galaxies move in such orbits, we propose that, under certain physical assumptions, the dark matter distribution of some low surface brightness galaxies can seed a particular class of BSTs. In the Newtonian limit, it is shown that for flat rotation curves, our proposal leads to an analytic prediction of the Navarro-Frenk-White dark matter profile of Navarro et al. [Astrophys. J. 462, 563 (1996)]. We further show that the dark matter distribution that seeds the BST is described by a two-fluid anisotropic model, and present its analytic solution. A new solution of the Einstein’s equations, with an internal BST and an external Schwarzschild metric, is also constructed.

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  • Received 15 April 2013

DOI:https://doi.org/10.1103/PhysRevD.87.103505

© 2013 American Physical Society

Authors & Affiliations

Dipanjan Dey*, Kaushik Bhattacharya, and Tapobrata Sarkar

  • Department of Physics, Indian Institute of Technology, Kanpur 208016, India

  • *deydip@iitk.ac.in
  • kaushikb@iitk.ac.in
  • tapo@iitk.ac.in

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Vol. 87, Iss. 10 — 15 May 2013

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