Polypolar spherical harmonic decomposition of galaxy correlators in redshift space: Toward testing cosmic rotational symmetry
arXiv:1612.02645 · doi:10.1103/PhysRevD.95.063508
Abstract
We propose an efficient way to test rotational invariance in the cosmological perturbations by use of galaxy correlation functions. In symmetry-breaking cases, the galaxy power spectrum can have extra angular dependence in addition to the usual one due to the redshift-space distortion, . We confirm that, via the decomposition into not the usual Legendre basis but the bipolar spherical harmonic one , the symmetry-breaking signal can be completely distinguished from the usual isotropic one since the former yields nonvanishing modes but the latter is confined to the one. As a demonstration, we analyze the signatures due to primordial-origin symmetry breakings such as the well-known quadrupolar-type and dipolar-type power asymmetries and find nonzero and modes, respectively. Fisher matrix forecasts of their constraints indicate that the -level sensitivity could be achieved by the SDSS or BOSS-CMASS data, and an order-of-magnitude improvement is expected in a near future survey as PFS or Euclid by virtue of an increase in accessible Fourier mode. Our methodology is model-independent and hence applicable to the searches for various types of statistically anisotropic fluctuations.
arXiv comment13 pages, 2 figures, 3 tables; version matching publication in PRD
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