Cosmic variance in inflation with two light scalars

Béatrice Bonga, Suddhasattwa Brahma, Anne Sylvie Deutsch, Sarah Shandera

Research output: Contribution to journalArticle

16 Citations (Scopus)

Abstract

We examine the squeezed limit of the bispectrum when a light scalar with arbitrary non-derivative self-interactions is coupled to the inflaton. We find that when the hidden sector scalar is sufficiently light (m ≲ 0.1 H), the coupling between long and short wavelength modes from the series of higher order correlation functions (from arbitrary order contact diagrams) causes the statistics of the fluctuations to vary in sub-volumes. This means that observations of primordial non-Gaussianity cannot be used to uniquely reconstruct the potential of the hidden field. However, the local bispectrum induced by mode-coupling from these diagrams always has the same squeezed limit, so the field's locally determined mass is not affected by this cosmic variance.

Original languageEnglish (US)
Article number018
JournalJournal of Cosmology and Astroparticle Physics
Volume2016
Issue number5
DOIs
StatePublished - May 6 2016

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diagrams
scalars
coupled modes
sectors
statistics
causes
wavelengths
interactions

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics

Cite this

Bonga, Béatrice ; Brahma, Suddhasattwa ; Deutsch, Anne Sylvie ; Shandera, Sarah. / Cosmic variance in inflation with two light scalars. In: Journal of Cosmology and Astroparticle Physics. 2016 ; Vol. 2016, No. 5.
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Cosmic variance in inflation with two light scalars. / Bonga, Béatrice; Brahma, Suddhasattwa; Deutsch, Anne Sylvie; Shandera, Sarah.

In: Journal of Cosmology and Astroparticle Physics, Vol. 2016, No. 5, 018, 06.05.2016.

Research output: Contribution to journalArticle

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