In 1962, Sambhunath Srivastava found an explicit solution when n = 5 . His solution is given by θ θ = sin ⁡ ⁡ ( ln ⁡ ⁡ ξ ξ ) ξ ξ [ 3 − − 2 sin 2 ⁡ ⁡ ( ln ⁡ ⁡ ξ ξ ) ] , and from this solution, a family of solutions θ θ ( ξ ξ ) → → A θ θ ( A ξ ξ ) can be obtained using homology transformation. Since this solution does not satisfy the conditions at the origin (in fact, it is oscillatory with amplitudes growing indefinitely as the origin is approached), this solution can be used in composite stellar models.