@article{248d94d5f15c45e1bf9b4a6e8b1640ea,
title = "CMB B -mode non-Gaussianity: Optimal bispectrum estimator and Fisher forecasts",
abstract = "Upcoming cosmic microwave background (CMB) data can be used to explore harmonic 3-point functions that involve the B-mode component of the CMB polarization signal. We focus on bispectra describing the non-Gaussian correlation of the B-mode field and the CMB temperature anisotropies (T) and/or E-mode polarization, i.e.",
author = "Duivenvoorden, {Adriaan J.} and Meerburg, {P. Daniel} and Katherine Freese",
note = "Funding Information: The authors thank Joel Meyers, Alex van Engelen, William Coulton, Eiichiro Komatsu, and Sebastian Baum for useful discussions and thank an anonymous referee for helpful comments and suggestions. P. D. M. acknowledges support from Senior Kavli Institute Fellowships at the University of Cambridge and the Netherlands organization for scientific research (NWO) VIDI Grant (dossier 639.042.730). A. J. D. and K. F. acknowledge support by the Vetenskapsr{\aa}det (Swedish Research Council) through Contract No. 638-2013-8993 and the Oskar Klein Centre for Cosmoparticle Physics. K. F. acknowledges support from the Jeff and Gail Kodosky Endowed Chair in Physics, DOE Award No. DE-SC007859, and the LCTP at the University of Michigan. Some computations have been performed at the Owl Cluster funded by the University of Oslo and the Research Council of Norway through Grant No. 250672. Publisher Copyright: {\textcopyright} 2020 American Physical Society.",
year = "2020",
month = jul,
day = "15",
doi = "10.1103/PhysRevD.102.023521",
language = "English",
volume = "102",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "AMER PHYSICAL SOC",
number = "2",
}