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  <identifier identifierType="URL">https://service.tib.eu/vdataset/openaire_12e2ba7a-baca-418a-aefb-ef4815eb158f</identifier>
  <creators>
    <creator>
      <creatorName> Paul K. Townsend</creatorName>
    </creator>
  </creators>
  <titles>
    <title>Supplementary material from "Aether, dark energy and string compactifications"</title>
  </titles>
  <publisher>Not defined</publisher>
  <publicationYear>2025</publicationYear>
  <contributors>
    <contributor>
      <contributorName> Paul K. Townsend</contributorName>
    </contributor>
  </contributors>
  <dates>
    <date dateType="Created">17/11/2025</date>
    <date dateType="Updated">17/11/2025</date>
  </dates>
  <resourceType resourceTypeGeneral="Dataset">Dataset</resourceType>
  <sizes>
    <size>0 kb</size>
  </sizes>
  <formats>
    <format></format>
  </formats>
  <descriptions>
    <description descriptionType="Other">{"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’."}</description>
  </descriptions>
</resource>
