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Quasi-steady state cosmology (QSS) is a nonstandard cosmology proposed in 1993 by Fred Hoyle, Geoffrey Burbidge, and Jayant V. Narlikar as an alternative to the big bang. The idea suggests there may have been expansions and pockets of creation other than the big bang occurring over time within the universe, sometimes referred to as minibangs, mini-creation events, or little bangs. After the observation of an accelerating universe, further modifications of the model were done. Mainstream cosmologists who have reviewed QSS have pointed out flaws and some discrepancies with observations left unexplained by proponents. [1]<br /><br />Contents [hide]<br />1 Description <br />2 Goals and targets <br />3 See also <br />4 External articles and references <br /> <br /><br /><br />[edit]<br />Description<br />The issues of observational and astronomical concerns over the universe's origins, history, structure, and dynamics from the Quasi-steady state were discussed in two papers, Astrophysical deductions from the quasi-steady state (1994) [2] and Astronomy Further astrophysical quantities expected in a quasi-steady state [3]. The basic theoretical framework was expounded upon in Quasi-Steady State Cosmology: Analytical Solutions of Field Equations and Their Relations to Observations [4]. R Sachs, J V Narlikar and F Hoyle researched and arrived at the exact solutions of the basic equations that gave simple homogeneous and isotropic models (such as in The Quasi-Steady State Cosmology: Analytical Solutions of Field Equations and Their Relations to Observations [5]). The production of light nuclei have been researched by F Hoyle, G Burbidge and J V Narlikar [6] and by Burbidge and Hoyle [7]. The process of structure formation was achievable through a "toy model" (by Ali Nayeri, Sunu Engineer, J. V. Narlikar, and F. Hoyle) and may offer a viable choice to the "standard" hot big bang cosmology. [8] With recent evidence indicating that the universe is accelerating, the quasi-steady state had pr