Detecting relic gravitational waves in the CMB: a statistical bias

Wen Zhao

Abstract

Analyzing the imprint of relic gravitational waves (RGWs) on the cosmic microwave background (CMB) power spectra provides a way to determine the signal of RGWs. In this Letter, we discuss a statistical bias, which could exist in the data analysis and has the tendency to overlook the RGWs. We also explain why this bias exists, and how to avoid it.

Original languageEnglish
JournalEuropean Physical Journal C
Volume71
Issue number7
Pages (from-to)1706
ISSN1434-6044
DOIs
Publication statusPublished - Jul 2011

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