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Investigation of generalised uncertainty principle effects on FRW cosmology

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arxiv 2401.09477 v2 pith:SPTK32NL submitted 2024-01-15 gr-qc hep-th

classification gr-qchep-th
keywords apparenteffectshorizoncosmologygeneralisedmaximumminimumdensity
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abstract

Based on the entropy-area relation from Nouicer's generalised uncertainty principle (GUP), we derive the GUP modified Friedmann equations from the first law of thermodynamics at apparent horizon. We find a minimum apparent horizon due to the minimal length notion of GUP. We show that the energy density of universe has a maximum and finite value at the minimum apparent horizon. Both minimum apparent horizon and maximum energy density imply the absence of the Big Bang singularity. Moreover, we investigate the GUP effects on the deceleration parameter for flat case. Finally, we examine the validity of generalised second law (GSL) of thermodynamics. We show that GSL always holds in a region enclosed by apparent horizon for the GUP effects. We also investigate the GSL in $\Lambda CDM$ cosmology and find that the total entropy change of universe has a maximum value in the presence of GUP effects. To better grasp the effects of Nouicer's GUP on cosmology, we compare our results with those obtained from quadratic GUP (QGUP).

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Effective matter sectors from modified entropies

    gr-qc 2025-11 conditional novelty 4.0 of 10

    Choosing a modified entropy S(r) fixes a metric f(r)=1-4πM/S'(r), and the Einstein tensor of that metric acts as an anisotropic effective fluid.

  2. The new higher-order generalized uncertainty principle and primordial big bang nucleosynthesis

    gr-qc 2024-11 reject novelty 4.0 of 10

    A higher-order GUP is fitted to BBN abundances, but arithmetic errors invalidate the reported parameter bounds.

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