On Quasinormal Modes for Scalar Perturbations of Static Spherically   Symmetric Black Holes in Nash Embedding Framework
  In this paper we investigate scalar perturbations of black holes embedded in a five dimensional bulk space. It is calculated the quasinormal frequencies of a such black holes using the third order of Wentzel, Kramers, Brillouin (WKB) approximation for scalar perturbations. The results are presented in tables along the text. 
S.C. Ulhoa, R.G.G. Amorim, Abra\~ao J. S. Capistrano
gr-qc