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.
2 More- Received 15 April 2013
DOI:https://doi.org/10.1103/PhysRevD.87.103505
© 2013 American Physical Society