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Role of acceleration in the expansion of the universe and its influence on an early-universe modified version of the Heisenberg uncertainty principle
Author(s) -
Andrew Beckwith
Publication year - 2017
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/880/1/012057
Subject(s) - acceleration , scale factor (cosmology) , uncertainty principle , metric expansion of space , physics , universe , theoretical physics , scale (ratio) , work (physics) , cosmology , classical mechanics , mathematical physics , dark energy , astrophysics , quantum mechanics , quantum
From first principles, we examine what adding acceleration does, and does not do, as to an early-universe modified version of the Heisenberg uncertainty principle. In doing so, we examine a Friedmann equation for the evolution of the scale factor, using two cases explicitly—when the acceleration of the expansion of the scale factor is kept in and when it is out—and the intermediate case of when the acceleration and scale factors are important but not dominant. In doing so we tie this discussion into earlier work done on the HUP.

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