2018
DOI: 10.1038/s41598-018-19181-9
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A new bound on polymer quantization via an opto-mechanical setup

Abstract: The existence of a minimal measurable length as a characteristic length in the Planck scale is one of the main features of quantum gravity and has been widely explored in the context. Various different deformations of spacetime have been employed successfully for the purpose. However, polymer quantization approach is a relatively new and dynamic field towards the quantum gravity phenomenology, which emerges from the symmetric sector of the loop quantum gravity. In this article, we extend the standard ideas of … Show more

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Cited by 45 publications
(34 citation statements)
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“…where we have considered the condition p u = 0. This expression results exactly the uncertainty relation obtained by [32], which is completely analogous to the ones appearing within the context of generalized uncertainty principle (GUP) scenarios analyzed within String Theory and Loop Quantum Gravity [16], [31], [33]. Nevertheless, in the case of the polymer representation there is a key difference with respect to the GUP's.…”
Section: The Uncertainty Principlesupporting
confidence: 80%
“…where we have considered the condition p u = 0. This expression results exactly the uncertainty relation obtained by [32], which is completely analogous to the ones appearing within the context of generalized uncertainty principle (GUP) scenarios analyzed within String Theory and Loop Quantum Gravity [16], [31], [33]. Nevertheless, in the case of the polymer representation there is a key difference with respect to the GUP's.…”
Section: The Uncertainty Principlesupporting
confidence: 80%
“…However, many studies have appeared in literature, with the aim to set bounds on (see, for instance, Refs. [ 20 24 ]).…”
Section: Introductionmentioning
confidence: 99%
“…However, we do not identify a mechanism for the reduction of the Cosmological Constant value to the actual one. A qualitative implementation of the upper limits for a Polymer cut-off on the physical space [20] provides a vacuum energy density many orders of magnitude greater than the one requested by the Universe acceleration. We can only stress that the calculated ground state of the scalar field Hamiltonian function is not a state for the quantum dynamics of the system and, therefore, we dynamically have to deal with a time dependent expectation value on the vacuum state of the scalar field.…”
Section: Introductionmentioning
confidence: 99%