The empirical process approach for detection of non-Gaussianity in the CMB

Details The empirical process approach for detection of non-Gaussianity in the CMB The empirical process approach for detection of non-Gaussianity in the CMB

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003newar..47..811h&link_type=abstract

New Astronomy Reviews, Volume 47, Issue 8-10, p. 811-814.

Astronomy and Astrophysics

Astronomy

Scientific paper

In three recent papers [Phys. Rev. D 66 (2002) 063006; Phys. Rev. D, 2003, in press; Annals of Statistics, 2003, under revision], we presented a new approach for measuring non-Gaussianity of the cosmic microwave background (CMB) anisotropy pattern, based on the multivariate empirical distribution function of the spherical harmonics alm of a CMB map. Here, we review briefly these results and their applications to non-Gaussian maps generated by non-standard models of inflation [Phys. Rev. D 65 (2002) 103505].

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