| dc.contributor.author | Brevik, Iver Håkon | |
| dc.contributor.author | Timoshkin, A. V. | |
| dc.date.accessioned | 2021-11-03T08:59:49Z | |
| dc.date.available | 2021-11-03T08:59:49Z | |
| dc.date.created | 2020-12-02T11:41:20Z | |
| dc.date.issued | 2021 | |
| dc.identifier.citation | International Journal of Modern Physics D. 2021, 30 (2), . | en_US |
| dc.identifier.issn | 0218-2718 | |
| dc.identifier.uri | https://hdl.handle.net/11250/2827477 | |
| dc.description.abstract | We describe the evolution of the early and late universe from thermodynamic considerations, using the generalized nonextensive Tsallis entropy with a variable exponent. A new element in our analysis is the inclusion of a bulk viscosity in the description of the cosmic fluid. Using the generalized Friedmann equation, a description of the early and the late universe is obtained. | en_US |
| dc.language.iso | eng | en_US |
| dc.publisher | World Scientific Publishing | en_US |
| dc.relation.uri | arXiv:2011.09207 [gr-qc] | |
| dc.title | Thermodynamic aspects of of entropic cosmology with viscosity | en_US |
| dc.type | Peer reviewed | en_US |
| dc.type | Journal article | en_US |
| dc.description.version | acceptedVersion | en_US |
| dc.rights.holder | Locked until 11.12.2021 due to copyright restrictions. This is the authors' accepted manuscript to an article published by World Scientific Publishing Company. | en_US |
| dc.source.pagenumber | 9 | en_US |
| dc.source.volume | 30 | en_US |
| dc.source.journal | International Journal of Modern Physics D | en_US |
| dc.source.issue | 2 | en_US |
| dc.identifier.doi | 10.1142/S0218271821500085 | |
| dc.identifier.cristin | 1855257 | |
| cristin.ispublished | true | |
| cristin.fulltext | postprint | |
| cristin.qualitycode | 1 | |
