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We introduce the real space correlation function of $B$-mode polarization of the cosmic microwave background (CMB) as a probe of superhorizon tensor perturbations created by inflation.
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B. Allen, R. R. Caldwell, S. Dodelson, L. Knox, E. P. S. Shellard and A. Stebbins, “CMB Anisotropy Induced by Cosmic Strings on Angular Scales
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U. L. Pen, U. Seljak and N. Turok, “Power Spectra in Global Defect Theories of Cosmic Structure Formation,” Phys. Rev. Lett
1997
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D. N. Spergel and M. Zaldarriaga, “CMB Polarization as a Direct Test of Inflation,” Phys. Rev. Lett
1997
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M. Kamionkowski, A. Kosowsky and A. Stebbins, “Statistics of Cosmic Microwave Background Polarization,” Phys. Rev. D
1997
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M. Zaldarriaga and U. Seljak, “An All-Sky Analysis of Polarization in the Microwave Background,” Phys. Rev. D
1997
Cited alongside, same era.
H. V. Peiris
2003
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Y. T. Lin and B. D. Wandelt, “A Beginner’s Guide to the Theory of CMB Temperature and Polarization Power Spectra in the Line-of-Sight Formalism,” Astropart. Phys
2004
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U. Seljak and C. M. Hirata, “Gravitational Lensing as a Contaminant of the Gravity Wave Signal in the CMB,” Phys. Rev. D
2004
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J. R. Pritchard and M. Kamionkowski, “Cosmic Microwave Background Fluctuations from Gravitational Waves: An Analytic Approach,” Annals Phys
2005
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2008
Later among the works it cites.
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U. Seljak, U. L. Pen and N. Turok, “Polarization of the Microwave Background in Defect Models,” Phys. Rev. Lett
1997
Cited alongside, same era.
S. Dodelson, “Coherent Phase Argument for Inflation,” AIP Conf. Proc
2003
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2008
Later among the works it cites.