Dark radiation in LARGE volume models

Michele Cicoli, Joseph P. Conlon, Fernando Quevedo

Research output: Contribution to journalArticlepeer-review

Abstract

We consider reheating driven by volume modulus decays in the LARGE volume scenario. Such reheating always generates nonzero dark radiation through the decays to the axion partner, while the only competitive visible sector decays are Higgs pairs via the Giudice-Masiero term. In the framework of sequestered models where the cosmological moduli problem is absent, the simplest model with a shift-symmetric Higgs sector generates 1.56≤ΔNeff≤1.74. For more general cases, the known experimental bounds on ΔNeff strongly constrain the parameters and matter content of the models.

Original languageEnglish (US)
Article number043520
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume87
Issue number4
DOIs
StatePublished - Feb 12 2013

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Fingerprint

Dive into the research topics of 'Dark radiation in LARGE volume models'. Together they form a unique fingerprint.

Cite this