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Aether, dark energy and string compactifications
The nineteenth-century aether died with special relativity but was resurrected by general relativity in the form of dark energy; a tensile material with tension equal to its energy density. Such a material is provided by the D-branes of string-theory; these can support the fields of supersymmetric p...
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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The Royal Society
2022
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Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9251484/ https://www.ncbi.nlm.nih.gov/pubmed/35785979 http://dx.doi.org/10.1098/rsta.2021.0185 |
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author | Townsend, Paul K. |
author_facet | Townsend, Paul K. |
author_sort | Townsend, Paul K. |
collection | PubMed |
description | The nineteenth-century aether died with special relativity but was resurrected by general relativity in the form of dark energy; a tensile material with tension equal to its energy density. Such a material is provided by the D-branes of string-theory; these can support the fields of supersymmetric particle-physics, although their energy density is cancelled by orientifold singularities upon compactification. Dark energy can still arise from supersymmetry-breaking anti-D-branes but it is probably time-dependent. Recent results on time-dependent compactifications to an FLRW universe with late-time accelerated expansion are reviewed. This article is part of the theme issue ‘The future of mathematical cosmology, Volume 2’. |
format | Online Article Text |
id | pubmed-9251484 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2022 |
publisher | The Royal Society |
record_format | MEDLINE/PubMed |
spelling | pubmed-92514842022-07-09 Aether, dark energy and string compactifications Townsend, Paul K. Philos Trans A Math Phys Eng Sci Articles The nineteenth-century aether died with special relativity but was resurrected by general relativity in the form of dark energy; a tensile material with tension equal to its energy density. Such a material is provided by the D-branes of string-theory; these can support the fields of supersymmetric particle-physics, although their energy density is cancelled by orientifold singularities upon compactification. Dark energy can still arise from supersymmetry-breaking anti-D-branes but it is probably time-dependent. Recent results on time-dependent compactifications to an FLRW universe with late-time accelerated expansion are reviewed. This article is part of the theme issue ‘The future of mathematical cosmology, Volume 2’. The Royal Society 2022-08-22 2022-07-04 /pmc/articles/PMC9251484/ /pubmed/35785979 http://dx.doi.org/10.1098/rsta.2021.0185 Text en © 2022 The Authors. https://creativecommons.org/licenses/by/4.0/Published by the Royal Society under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) , which permits unrestricted use, provided the original author and source are credited. |
spellingShingle | Articles Townsend, Paul K. Aether, dark energy and string compactifications |
title | Aether, dark energy and string compactifications |
title_full | Aether, dark energy and string compactifications |
title_fullStr | Aether, dark energy and string compactifications |
title_full_unstemmed | Aether, dark energy and string compactifications |
title_short | Aether, dark energy and string compactifications |
title_sort | aether, dark energy and string compactifications |
topic | Articles |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9251484/ https://www.ncbi.nlm.nih.gov/pubmed/35785979 http://dx.doi.org/10.1098/rsta.2021.0185 |
work_keys_str_mv | AT townsendpaulk aetherdarkenergyandstringcompactifications |