Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-06-10
Phys.Rev.D66:063008,2002
Astronomy and Astrophysics
Astrophysics
16 pages, 4 figures; typographical errors corrected
Scientific paper
10.1103/PhysRevD.66.063008
We develop the formalism necessary to study four-point functions of the cosmic microwave background (CMB) temperature and polarization fields. We determine the general form of CMB trispectra, with the constraints imposed by the assumption of statistical isotropy of the CMB fields, and derive expressions for their estimators, as well as their Gaussian noise properties. We apply these techniques to initial non-Gaussianity of a form motivated by inflationary models. Due to the large number of four-point configurations, the sensitivity of the trispectra to initial non-Gaussianity approaches that of the temperature bispectrum at high multipole moment. These trispectra techniques will also be useful in the study of secondary anisotropies induced for example by the gravitational lensing of the CMB by the large scale structure of the universe.
Hu Wayne
Okamoto Takemi
No associations
LandOfFree
The Angular Trispectra of CMB Temperature and Polarization does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Angular Trispectra of CMB Temperature and Polarization, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Angular Trispectra of CMB Temperature and Polarization will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-518289