Minimum length uncertainty relations in the presence of dark energy

We introduce a dark energy-modified minimum length uncertainty relation (DE-MLUR) or dark energy uncertainty principle (DE-UP) for short. The new relation is structurally similar to the MLUR introduced by Károlyházy (1968), and reproduced by Ng and van Dam (1994) using alternative arguments, but wit...

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Main Author: Lake, Matthew James
Other Authors: School of Physical and Mathematical Sciences
Format: Article
Language:English
Published: 2019
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Online Access:https://hdl.handle.net/10356/107053
http://hdl.handle.net/10220/49035
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Institution: Nanyang Technological University
Language: English
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spelling sg-ntu-dr.10356-1070532023-02-28T19:43:39Z Minimum length uncertainty relations in the presence of dark energy Lake, Matthew James School of Physical and Mathematical Sciences Dark Energy Minimum Length Uncertainty Relations DRNTU::Science::Physics We introduce a dark energy-modified minimum length uncertainty relation (DE-MLUR) or dark energy uncertainty principle (DE-UP) for short. The new relation is structurally similar to the MLUR introduced by Károlyházy (1968), and reproduced by Ng and van Dam (1994) using alternative arguments, but with a number of important differences. These include a dependence on the de Sitter horizon, which may be expressed in terms of the cosmological constant as ldS∼1/Λ−−√ . Applying the DE-UP to both charged and neutral particles, we obtain estimates of two limiting mass scales, expressed in terms of the fundamental constants {G,c,ℏ,Λ,e} . Evaluated numerically, the charged particle limit corresponds to the order of magnitude value of the electron mass ( me ), while the neutral particle limit is consistent with current experimental bounds on the mass of the electron neutrino ( mνe ). Possible cosmological consequences of the DE-UP are considered and we note that these lead naturally to a holographic relation between the bulk and the boundary of the Universe. Low and high energy regimes in which dark energy effects may dominate canonical quantum behaviour are identified and the possibility of testing the model using near-future experiments is briefly discussed. MOE (Min. of Education, S’pore) Published version 2019-07-01T03:48:36Z 2019-12-06T22:23:54Z 2019-07-01T03:48:36Z 2019-12-06T22:23:54Z 2019 Journal Article Lake, M. J. (2019). Minimum length uncertainty relations in the presence of dark energy. Galaxies, 7(1), 11-. doi:10.3390/galaxies7010011 2075-4434 https://hdl.handle.net/10356/107053 http://hdl.handle.net/10220/49035 10.3390/galaxies7010011 en Galaxies © 2019 The Author. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/). 42 p. application/pdf
institution Nanyang Technological University
building NTU Library
continent Asia
country Singapore
Singapore
content_provider NTU Library
collection DR-NTU
language English
topic Dark Energy
Minimum Length Uncertainty Relations
DRNTU::Science::Physics
spellingShingle Dark Energy
Minimum Length Uncertainty Relations
DRNTU::Science::Physics
Lake, Matthew James
Minimum length uncertainty relations in the presence of dark energy
description We introduce a dark energy-modified minimum length uncertainty relation (DE-MLUR) or dark energy uncertainty principle (DE-UP) for short. The new relation is structurally similar to the MLUR introduced by Károlyházy (1968), and reproduced by Ng and van Dam (1994) using alternative arguments, but with a number of important differences. These include a dependence on the de Sitter horizon, which may be expressed in terms of the cosmological constant as ldS∼1/Λ−−√ . Applying the DE-UP to both charged and neutral particles, we obtain estimates of two limiting mass scales, expressed in terms of the fundamental constants {G,c,ℏ,Λ,e} . Evaluated numerically, the charged particle limit corresponds to the order of magnitude value of the electron mass ( me ), while the neutral particle limit is consistent with current experimental bounds on the mass of the electron neutrino ( mνe ). Possible cosmological consequences of the DE-UP are considered and we note that these lead naturally to a holographic relation between the bulk and the boundary of the Universe. Low and high energy regimes in which dark energy effects may dominate canonical quantum behaviour are identified and the possibility of testing the model using near-future experiments is briefly discussed.
author2 School of Physical and Mathematical Sciences
author_facet School of Physical and Mathematical Sciences
Lake, Matthew James
format Article
author Lake, Matthew James
author_sort Lake, Matthew James
title Minimum length uncertainty relations in the presence of dark energy
title_short Minimum length uncertainty relations in the presence of dark energy
title_full Minimum length uncertainty relations in the presence of dark energy
title_fullStr Minimum length uncertainty relations in the presence of dark energy
title_full_unstemmed Minimum length uncertainty relations in the presence of dark energy
title_sort minimum length uncertainty relations in the presence of dark energy
publishDate 2019
url https://hdl.handle.net/10356/107053
http://hdl.handle.net/10220/49035
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