Paper
Large-scale structure observables in general relativity
Published Jul 30, 2014 ·
Classical and Quantum Gravity
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Abstract
We review recent studies that rigorously define several key observables of the large-scale structure of the Universe in a general relativistic context. Specifically, we consider (i) redshift perturbation of cosmic clock events; (ii) distortion of cosmic rulers, including weak lensing shear and magnification; and (iii) observed number density of tracers of the large-scale structure. We provide covariant and gauge-invariant expressions of these observables. Our expressions are given for a linearly perturbed flat Friedmann–Robertson–Walker metric including scalar, vector, and tensor metric perturbations. While we restrict ourselves to linear order in perturbation theory, the approach can be straightforwardly generalized to higher order.
This paper reviews key observables of the large-scale structure of the Universe, including redshift perturbation, distortion of cosmic rulers, and observed number density of tracers, in a general relativistic context.
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