Two- and Three-Dimensional Probes of Parity in Primordial Gravity Waves

Kiyoshi Wesley Masui, Ue-Li Pen, and Neil Turok
Phys. Rev. Lett. 118, 221301 – Published 1 June 2017
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Abstract

We show that three-dimensional information is critical to discerning the effects of parity violation in the primordial gravity-wave background. If present, helical gravity waves induce parity-violating correlations in the cosmic microwave background (CMB) between parity-odd polarization B modes and parity-even temperature anisotropies (T) or polarization E modes. Unfortunately, EB correlations are much weaker than would be naively expected, which we show is due to an approximate symmetry resulting from the two-dimensional nature of the CMB. The detectability of parity-violating correlations is exacerbated by the fact that the handedness of individual modes cannot be discerned in the two-dimensional CMB, leading to a noise contribution from scalar matter perturbations. In contrast, the tidal imprints of primordial gravity waves fossilized into the large-scale structure of the Universe are a three-dimensional probe of parity violation. Using such fossils the handedness of gravity waves may be determined on a mode-by-mode basis, permitting future surveys to probe helicity at the percent level if the amplitude of primordial gravity waves is near current observational upper limits.

  • Figure
  • Received 23 February 2017

DOI:https://doi.org/10.1103/PhysRevLett.118.221301

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Kiyoshi Wesley Masui*

  • Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Rd, Vancouver, British Columbia V6T 1Z1, Canada

Ue-Li Pen

  • Canadian Institute for Theoretical Astrophysics, 60 St. George Street, Toronto, Ontario M5S 3H8, Canada
  • Canadian Institute for Advanced Research, CIFAR Program in Cosmology and Gravity, Toronto, Ontario, M5G 1Z8, Canada
  • Dunlap Institute for Astronomy & Astrophysics, University of Toronto, 50 St. George Street, Toronto, Ontario, M5S 3H4, Canada
  • Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada

Neil Turok

  • Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada

  • *kiyo@physics.ubc.ca

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Issue

Vol. 118, Iss. 22 — 2 June 2017

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