Constraining Snyder and GUP models with low-mass stars

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 a...

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Main Authors: Anna Pachoł, Aneta Wojnar
Format: Article
Language:English
Published: SpringerOpen 2023-12-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-023-12286-0
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author Anna Pachoł
Aneta Wojnar
author_facet Anna Pachoł
Aneta Wojnar
author_sort Anna Pachoł
collection DOAJ
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. The bound we obtain is $$\beta _0 \le 4.5 \times 10^{47}$$ β 0 ≤ 4.5 × 10 47 . We underline the significance of realistic matter modeling in order to enhance our understanding of effects arising in quantum gravity phenomenology and implications of quantum gravitational corrections in astrophysical systems.
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spelling doaj.art-5d8c05e2efa0451c89a9b198a71d04802024-03-31T11:31:29ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522023-12-01831211010.1140/epjc/s10052-023-12286-0Constraining Snyder and GUP models with low-mass starsAnna Pachoł0Aneta Wojnar1Department of Microsystems, University of South-Eastern Norway, Campus VestfoldDepartamento de Física Teórica & IPARCOS, Universidad Complutense de MadridAbstract 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. The bound we obtain is $$\beta _0 \le 4.5 \times 10^{47}$$ β 0 ≤ 4.5 × 10 47 . We underline the significance of realistic matter modeling in order to enhance our understanding of effects arising in quantum gravity phenomenology and implications of quantum gravitational corrections in astrophysical systems.https://doi.org/10.1140/epjc/s10052-023-12286-0
spellingShingle Anna Pachoł
Aneta Wojnar
Constraining Snyder and GUP models with low-mass stars
European Physical Journal C: Particles and Fields
title Constraining Snyder and GUP models with low-mass stars
title_full Constraining Snyder and GUP models with low-mass stars
title_fullStr Constraining Snyder and GUP models with low-mass stars
title_full_unstemmed Constraining Snyder and GUP models with low-mass stars
title_short Constraining Snyder and GUP models with low-mass stars
title_sort constraining snyder and gup models with low mass stars
url https://doi.org/10.1140/epjc/s10052-023-12286-0
work_keys_str_mv AT annapachoł constrainingsnyderandgupmodelswithlowmassstars
AT anetawojnar constrainingsnyderandgupmodelswithlowmassstars