Odd Parity Preference

Analyses of COBE, WMAP, and Planck CMB temperature maps at low multipoles (roughly l?50) show an apparent excess of power in odd multipoles compared to even ones, corresponding to a preference for point-parity antisymmetry that is not expected in the statistically isotropic, parity-neutral ΛCDM model (Kim & Naselsky 2011; Zhao 2014). This “odd-parity preference” is closely related to the lack of large-angle correlation and appears direction-dependent, so within ΛCDM it typically demands either finely tuned primordial conditions, unusual cosmic topology, or subtle systematics/foreground explanations, none of which arise naturally in the simplest hot Big Bang plus inflation picture (Land & Magueijo 2005; Gruppuso et al. 2011).

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