A Classification of spherically symmetric kinematic selfsimilar perfect fluid solutions

Jul, 2002
33 pages
Published in:
  • Prog.Theor.Phys. 108 (2002) 819-851
e-Print:
Report number:
  • WU-AP-150-02

Citations per year

20032006200920122015012345
Abstract: (arXiv)
We classify all spherically symmetric spacetimes admitting a kinematic self-similar vector of the second, zeroth or infinite kind. We assume that the perfect fluid obeys either a polytropic equation of state or an equation of state of the form p=Kμp=K\mu, where pp and μ\mu are the pressure and the energy density, respectively, and KK is a constant. We study the cases in which the kinematic self-similar vector is not only ``tilted'' but also parallel or orthogonal to the fluid flow. We find that, in contrast to Newtonian gravity, the polytropic perfect-fluid solutions compatible with the kinematic self-similarity are the Friedmann-Robertson-Walker solution and general static solutions. We find three new exact solutions which we call the dynamical solutions (A) and (B) and Λ\Lambda-cylinder solution, respectively.