Gauge-Invariant Formalism of Cosmological Weak Lensing

TL;DR

This paper develops a gauge-invariant formalism for cosmological weak lensing that includes all relativistic effects from scalar, vector, and tensor perturbations, clarifying the physical observables and their invariance.

Contribution

It introduces a comprehensive, gauge-invariant framework for weak lensing that accounts for relativistic effects and clarifies the physical interpretation of lensing observables.

Findings

Gauge-invariance of lensing observables verified

Relativistic effects contribute to all lensing measurements

Physical rotation vanishes at linear order even with vector and tensor perturbations

Abstract

We present the gauge-invariant formalism of cosmological weak lensing, accounting for all the relativistic effects due to the scalar, vector, and tensor perturbations at the linear order. While the light propagation is fully described by the geodesic equation, the relation of the photon wavevector to the physical quantities requires the specification of the frames, where they are defined. By constructing the local tetrad bases at the observer and the source positions, we clarify the relation of the weak lensing observables such as the convergence, the shear, and the rotation to the physical size and shape defined in the source rest-frame and the observed angle and redshift measured in the observer rest-frame. Compared to the standard lensing formalism, additional relativistic effects contribute to all the lensing observables. We explicitly verify the gauge-invariance of the lensing observables and compare our results to previous work. In particular, we demonstrate that even in the presence of the vector and tensor perturbations, the physical rotation of the lensing observables vanishes at the linear order, while the tetrad basis rotates along the light propagation compared to a FRW coordinate. Though the latter is often used as a probe of primordial gravitational waves, the rotation of the tetrad basis is indeed not a physical observable. We further clarify its relation to the E-B decomposition in weak lensing. Our formalism provides a transparent and comprehensive perspective of cosmological weak lensing.