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Generalised Uncertainty Relations and the Problem of Dark Energy

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arxiv 2112.13938 v2 pith:EAMNKW5Q submitted 2021-12-27 gr-qc hep-phquant-ph

classification gr-qchep-phquant-ph
keywords uncertaintydarkenergygeneralisedquantumrelationsassociatedcanonical
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We outline a new model in which generalised uncertainty relations, that govern the behaviour of microscopic world, and dark energy, that determines the large-scale evolution of the Universe, are intrinsically linked via the quantum properties of space-time. In this approach the background is treated as a genuinely quantum object, with an associated state vector, and additional fluctuations of the geometry naturally give rise to the extended generalised uncertainty principle (EGUP). An effective dark energy density then emerges from the field that minimises the modified uncertainty relations. These results are obtained via modifications of the canonical quantum operators, but without modifications of the canonical Heisenberg algebra, allowing many well known problems associated with existing GUP models to be circumvented.

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  1. Stark Energy Shifts due to Quantum Gravity in RGUP Algebra

    gr-qc 2025-05 conditional novelty 4.0 of 10

    Applying the RGUP to the Stark effect yields beta-proportional energy shifts and an upper bound beta < 10^42 on the deformation parameter.

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