Spherically symmetric static bulk viscous fluid in rosen's modified bimetric theory of relativity

In this paper we have studied the static spherically symmetric metric ds² = g²(r)dt² - dr² -R²(r)(dθ² + sin² θdφ²) with energy momentum tensor for the bulk viscous fluid distribution and we have adopted the procedure of Khadekar and Kondawar (2006) for bulk viscous fluid and obtained the results on the line of Khadekar and Kondawar (2006) which represents the Schwarzschild interior solution.