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Signature of Gravity Waves in the Polarization of the Microwave Background

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Seljak, Uros̆, Zaldarriaga, Matias·1997·Physical Review Letters

Abstract

Using spin-weighted decomposition of polarization in the cosmic microwave background (CMB) we show that a particular combination of Stokes $Q$ and $U$ parameters vanishes for primordial fluctuations generated by scalar modes, but does not for those generated by primordial gravity waves. Because of this gravity wave detection is not limited by cosmic variance as in the case of temperature fluctuations. We present the exact expressions for various polarization power spectra, which are valid on any scale. Numerical evaluation in inflation-based models shows that the expected signal is of the order of 0.5 $\ensuremath{\mu}$K, which could be directly tested in future CMB experiments.

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Metadata

Authors
Seljak, U., & Zaldarriaga, M.
Venue
Physical Review Letters
Published
1997-03-17
Volume
78
Issue
11
Pages
2054-2057
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2016888141
Cited by
978
References
0
FWCI
15.46
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Signature of Gravity Waves in the Polarization of the Microwave Background. https://app.cochat.ai/papers/10.1103/physrevlett.78.2054
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Seljak, U., & Zaldarriaga, M. (1997). Signature of Gravity Waves in the Polarization of the Microwave Background. Physical Review Letters. https://doi.org/10.1103/physrevlett.78.2054

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