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 language | English |
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Journal | European Physical Journal C |
Volume | 71 |
Issue number | 7 |
Pages (from-to) | 1706 |
ISSN | 1434-6044 |
DOIs | |
Publication status | Published - Jul 2011 |