Limits on anisotropic inflation from the Planck data

Jaiseung Kim, Eiichiro Komatsu

101 Citationer (Scopus)

Abstract

Temperature anisotropy of the cosmic microwave background offers a test of the fundamental symmetry of spacetime during cosmic inflation. Violation of rotational symmetry yields a distinct signature in the power spectrum of primordial fluctuations as P(k)=P0(k)[1+g *(k^·E^cl)2], where E^cl is a preferred direction in space and g* is an amplitude. Using the Planck 2013 temperature maps, we find no evidence for violation of rotational symmetry, g*=0.002±0.016 (68% C.L.), once the known effects of asymmetry of the Planck beams and Galactic foreground emission are removed. (Based on observations obtained with the Planck Collaboration, a ESA science mission with instruments and contributions directly funded by ESA Member States, NASA, and Canada.)

OriginalsprogEngelsk
Artikelnummer101301
TidsskriftPhysical Review D (Particles, Fields, Gravitation and Cosmology)
Vol/bind88
Udgave nummer10
ISSN1550-7998
DOI
StatusUdgivet - 14 nov. 2013

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