Constraining Snyder and GUP models with low-mass stars
| dc.contributor.author | Pachol, Anna | |
| dc.contributor.author | Wojnar, Aneta | |
| dc.date.accessioned | 2024-08-13T12:34:25Z | |
| dc.date.available | 2024-08-13T12:34:25Z | |
| dc.date.created | 2023-12-18T14:44:28Z | |
| dc.date.issued | 2023 | |
| dc.identifier.citation | Pachoł, A., & Wojnar, A. (2023). Constraining Snyder and GUP models with low-mass stars. The European Physical Journal C, 83(12), Artikkel 1097. | en_US |
| dc.identifier.issn | 1434-6044 | |
| dc.identifier.uri | https://hdl.handle.net/11250/3146053 | |
| dc.description.abstract | We investigate the application of an equation of state that incorporates corrections derived from the Snyder model (and the Generalized Uncertainty Principle) to describe the behaviour of matter in a low-mass star. Remarkably, the resulting equations exhibit striking similarities to those arising from modified Einstein gravity theories. By modeling matter with realistic considerations, we are able to more effectively constrain the theory parameters, surpassing the limitations of existing astrophysical bounds. | en_US |
| dc.language.iso | eng | en_US |
| dc.rights | Navngivelse 4.0 Internasjonal | * |
| dc.rights.uri | http://creativecommons.org/licenses/by/4.0/deed.no | * |
| dc.title | Constraining Snyder and GUP models with low-mass stars | en_US |
| dc.type | Peer reviewed | en_US |
| dc.type | Journal article | en_US |
| dc.description.version | publishedVersion | en_US |
| dc.rights.holder | © The Author(s) 2023. | en_US |
| dc.source.volume | 83 | en_US |
| dc.source.journal | European Physical Journal C | en_US |
| dc.source.issue | 12 | en_US |
| dc.identifier.doi | https://doi.org/10.1140/epjc/s10052-023-12286-0 | |
| dc.identifier.cristin | 2215016 | |
| dc.source.articlenumber | 1097 | en_US |
| cristin.ispublished | true | |
| cristin.fulltext | postprint | |
| cristin.fulltext | original | |
| cristin.qualitycode | 2 |
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