Narlikar, J. V.2012-03-232012-03-232000-03-29http://hdl.handle.net/11007/1563In this paper we introduce a toy model for understanding the growth of structures and the two point correlation functions in the cotext of the Quasi-Steady State Cosmology (qssc). The paper first describes the essential features of the qssc and then addresses the problem of structure formation.enTwo point correlation functionQuasi-Steady State Cosmology (qssc)Basic theory of the qsscMachian theory of gravityMatter creationcosmological solutioncosmological solutionGravitational perturbationsStructure formation in the quasi-steady state cosmologyArticle