Dark radiation and dark matter in large volume compactifications

Tetsutaro Higaki, Fuminobu Takahashi

Research output: Contribution to journalArticle

79 Citations (Scopus)

Abstract

We argue that dark radiation is naturally generated from the decay of the overall volume modulus in the LARGE volume scenario. We consider both sequestered and non-sequestered cases, and find that the axionic superpartner of the modulus is produced by the modulus decay and it can account for the dark radiation suggested by observations, while the modulus decay through the Giudice-Masiero term gives the dominant contribution to the total decay rate. In the sequestered case, the lightest supersymmetric particles produced by the modulus decay can naturally account for the observed dark matter density. In the non-sequestered case, on the other hand, the supersymmetric particles are not produced by the modulus decay, since the soft masses are of order the heavy gravitino mass. The QCD axion will then be a plausible dark matter candidate.

Original languageEnglish
Article number125
JournalJournal of High Energy Physics
Volume2012
Issue number11
DOIs
Publication statusPublished - 2012
Externally publishedYes

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dark matter
decay
radiation
gravitinos
decay rates
quantum chromodynamics

Keywords

  • Strings and branes phenomenology
  • Supersymmetry Phenomenology

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Dark radiation and dark matter in large volume compactifications. / Higaki, Tetsutaro; Takahashi, Fuminobu.

In: Journal of High Energy Physics, Vol. 2012, No. 11, 125, 2012.

Research output: Contribution to journalArticle

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