Abstract
In 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.
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Narlikar, J.V. Structure Formation in the Quasi-Steady State Cosmology. General Relativity and Gravitation 32, 1091–1106 (2000). https://doi.org/10.1023/A:1001925811980
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DOI: https://doi.org/10.1023/A:1001925811980