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2008

Cosmic Shear from Scalar-Induced Gravitational Waves

Sarkar, Devdeep, Serra, Paolo, Cooray, Asantha et al.

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Weak gravitational lensing by foreground density perturbations generates a gradient mode in the shear of background images.

In contrast, cosmological tensor perturbations induce a non-zero curl mode associated with image rotations.
In this note, we study the lensing signatures of both primordial gravitational waves from inflation and second-order gravitational waves generated from the observed spectrum of primordial density fluctuations.
We derive the curl mode for galaxy lensing surveys at redshifts of 1 to 3 and for lensing of the cosmic microwave background (CMB) at a redshift of 1100.

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