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- W3103185596 abstract "A large-scale temperature perturbation has a non-zero correlation with the power spectrum of B-modes of cosmological origin on short scales while the corresponding correlation is expected to be zero for B-modes sourced by galactic foregrounds. We thus compute the squeezed limit of a three-point function in which one correlates the temperature fluctuations at large scales with two polarization modes at small scales. In the particular case of the B-mode polarization we obtain a relation that connects the squeezed limit of the TBB three-point function with the cosmological B-mode power spectrum, which can be used as a consistency relation. This could in principle help to distinguish a primordial signal from that induced by inter-stellar dust." @default.
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- W3103185596 date "2014-10-07" @default.
- W3103185596 modified "2023-09-23" @default.
- W3103185596 title "A consistency relation for the CMB B-mode polarization in the squeezed limit" @default.
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- W3103185596 doi "https://doi.org/10.1088/1475-7516/2014/10/011" @default.
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