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2012

Cosmic Tides

Pen, Ue-Li, Sheth, Ravi, Harnois-Deraps, J. et al.

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We apply CMB lensing techniques to large scale structure and solve for the 3-D cosmic tidal field.

We use small scale filamentary structures to solve for the large scale tidal shear and gravitational potential.
By comparing this to the redshift space density field, one can measure the gravitational growth factor on large scales without cosmic variance.
This potentially enables accurate measurements of neutrino masses and reconstruction of radial modes lost in 21 cm intensity mapping, which are essential for CMB and other cross correlations.

Cosmic Tides · Around

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Then

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