Production of Topological Defects at the End of Inflation
作者： Mairi Sakellariadou
DOI: 10.1007/978-3-540-74353-8_10
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摘要: Cosmological inflation and topological defects have been considered for a long time, either in disagreement or competition. On the one hand an inflationary era is required to solve shortcomings of hot big bang model, while on other cosmic strings string-like objects are predicted be formed early universe. Thus, has find ways so that both can coexist. I discuss how reconcile cosmological with strings.
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