Bianchi V Brane-world Cosmology with a Generalized Chaplygin Gas
  In the context of brane cosmology, we investigate exact solution of the gravitational field equations in the Randall-Sundrum model for an anisotropic brane with Bianchi V geometry, with a generalized Chaplygin gas, which plays the role of dark energy and interacts with dark matter particles. Also, the behavior of the observationally important parameters like expansion and anisotropy is examined. 
\"Ozg\"ur Sevinc, G\"ul\c{c}in (Berkoz) Uluyazi
gr-qc