Structure formation in the quasi-steady state cosmology
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Date
2000-03-29
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Publisher
Springer
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.
Description
Keywords
Two point correlation function, Quasi-Steady State Cosmology (qssc), Basic theory of the qssc, Machian theory of gravity, Matter creation, cosmological solution, cosmological solution, Gravitational perturbations