Semi-analytical Study on the Generic Degeneracy for Galaxy Clustering Measurements

Abstract

From the galaxy power spectrum in redshift space, we derive semi-analytical results on the generic degeneracy of galaxy clustering measurements. Defining the observables $\bar{A}=Gb{\sigma }_8$ and $\bar{R}=Gf{\sigma }_8$, (being $G$ the growth function, $b$ the bias, $f$ the growth rate, and ${\sigma }_8$ the amplitude of the power spectrum), we perform a Fisher matrix formalism to forecast the expected precision of these quantities for a Euclid-like survey. Among the results we found that galaxy surveys have generically a slightly negative correlation between $\bar{A}$ and $\bar{R}$, and they can always measure $\bar{R}$ about 3.7 to 4.7 times better than $\bar{A}$.

4 pages, typos corrected, to appear in the proceedings of the IAU Symposium 306 "Statistical Challenges in 21st Century Cosmology", May 25-29, 2014, Lisbon, Portugal

References in corpus (3)

• Testing cosmological structure formation using redshift-space distortions
• Observables and unobservables in dark energy cosmologies
• Model-independent constraints on the cosmological anisotropic stress