Abstract

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept to measure the gravitational-wave signature of primordial inflation through its distinctive imprint on the linear polarization of thecosmic microwave background (CMB). Its optical system couples a polarizing Fourier transform spectrometerto the sky to measure the differential signal between orthogonal linear polarization states from two co-pointedbeams on the sky. The double differential nature of the four-port measurement mitigates beam-related systematic errors common to the two-port systems used in most CMB measurements. Systematic errors coupling unpolarized temperature gradients to a false polarized signal cancel to first order for any individual detector. Thiscommon-mode cancellation is performed optically, prior to detection, and does not depend on the instrumentcalibration. Systematic errors coupling temperature to polarization cancel to second order when comparing signals from independent detectors. We describe the polarized beam patterns for PIXIE and assess the systematicerror for measurements of CMB polarization.

Highlights

  • Polarization of the cosmic microwave background (CMB) provides a powerful test of the physics of the early universe

  • Scalar sources such as temperature or density perturbations can only generate even-parity E-modes, while gravitational waves created during an inflationary epoch in the early universe can generate either parity

  • We describe the polarized beam patterns for PIXIE and assess the systematic error for measurements of CMB polarization

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Summary

Introduction

Polarization of the cosmic microwave background (CMB) provides a powerful test of the physics of the early universe. Where r is the power ratio of gravitational waves to density fluctuations.[9] In most large-field models, r is predicted to be of order 0.01, corresponding to polarized amplitude 30 nK or energy near the grand unified theory scale, 1016 GeV. Signals at this amplitude could be detected by a dedicated polarimeter, providing a critical test of a central component of modern cosmology. We describe the polarized beam patterns for PIXIE and assess the systematic error for measurements of CMB polarization

PIXIE Optical System
Single-Detector Response
Additional Symmetries
Combined Detector Response
Tolerance
Findings
Discussion
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