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- W4300889713 abstract "The accelerated expansion of the Universe is one of the greatest challenges of modern physics. One candidate to explain this phenomenon is a new field called dark energy. In this work we have used the Tsallis nonextensive statistical formulation of the Friedmann equation to explore the Barboza-Alcaniz and Chevalier-Polarski-Linder parametric dark energy models and the Wang-Meng and Dalal vacuum decay models. After that, we have discussed the observational tests and the constraints concerning the Tsallis nonextensive parameter." @default.
- W4300889713 created "2022-10-04" @default.
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- W4300889713 date "2014-03-22" @default.
- W4300889713 modified "2023-10-03" @default.
- W4300889713 title "Dark energy models through nonextensive Tsallis' statistics" @default.
- W4300889713 doi "https://doi.org/10.48550/arxiv.1403.5706" @default.
- W4300889713 hasPublicationYear "2014" @default.
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