Kinematic Self-Similar Solutions and Their Properties

Details Kinematic Self-Similar Solutions and Their Properties Kinematic Self-Similar Solutions and Their Properties

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1950m&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

We derive some properties of spacetimes which contain an irrotational dust fluid and in which there is a kinematic self-similarity vector field of the second, zeroth or infinite kind. For the spherically symmetric case, in which a kinematic self-similarity vector is neither parallel nor orthogonal to the fluid flow, we obtain the explicit forms of the solutions, which belong to the marginally bound Lemaître-Tolman-Bondi solutions. The physical properties of the solutions are also discussed.

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