Analytical r-mode solution with gravitational radiation reaction force
arXiv:astro-ph/0512097 · doi:10.1142/9789812774439_0014
Abstract
We present and discuss the analytical r-mode solution to the linearized hydrodynamic equations of a slowly rotating, Newtonian, barotropic, non-magnetized, perfect-fluid star in which the gravitational radiation reaction force is present.
3 pages, in Proceedings of the 5th International Workshop "New Worlds in Astroparticle Physics", Faro, Portugal, 8-10 January 2005