The intrinsic bispectrum of the CMB from isocurvature initial conditions
Pedro Carrilho, Karim A. Malik

TL;DR
This paper calculates the contributions of isocurvature modes to the CMB bispectrum, assessing their detectability with current and future experiments, and constrains their amplitudes based on Planck data.
Contribution
It provides the first detailed computation of isocurvature mode contributions to the CMB bispectrum using a second-order Boltzmann solver and forecasts their detectability.
Findings
Single isocurvature modes have negligible effects within current constraints.
Large compensated isocurvature modes can produce detectable bispectra.
Future experiments could detect or constrain these modes significantly.
Abstract
Non-linear effects in the early Universe generate non-zero bispectra of the cosmic microwave background (CMB) temperature and polarization, even in the absence of primordial non-Gaussianity. In this paper, we compute the contributions from isocurvature modes to the CMB bispectra using a modified version of the second-order Boltzmann solver SONG. We investigate the ability of current and future CMB experiments to constrain these modes with observations of the bispectrum. Our results show that the enhancement due to single isocurvature modes mixed with the adiabatic mode is negligible for the parameter ranges currently allowed by the most recent Planck results. However, we find that a large compensated isocurvature mode can produce a detectable bispectrum when its correlation with the adiabatic mode is appreciable. The non-observation of this contribution in searches for the lensing…
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