Imprint of inflation on galaxy shape correlations
  We show that intrinsic (not lensing-induced) correlations between galaxy
shapes offer a new probe of primordial non-Gaussianity and inflationary physics
which is complementary to galaxy number counts. Specifically, intrinsic
alignment correlations are sensitive to an anisotropic squeezed limit
bispectrum of the primordial perturbations. Such a feature arises in solid
inflation, as well as more broadly in the presence of light higher spin fields
during inflation (as pointed out recently by Arkani-Hamed and Maldacena). We
present a derivation of the all-sky two-point correlations of intrinsic shapes
and number counts in the presence of non-Gaussianity with general angular
dependence, and show that a quadrupolar (spin-2) anisotropy leads to the analog
in galaxy shapes of the well-known scale-dependent bias induced in number
counts by isotropic (spin-0) non-Gaussianity. Moreover, in presence of non-zero
anisotropic non-Gaussianity, the quadrupole of galaxy shapes becomes sensitive
to far superhorizon modes. These effects come about because long-wavelength
modes induce a local anisotropy in the initial power spectrum, with which
galaxies will correlate. We forecast that future imaging surveys could provide
constraints on the amplitude of anisotropic non-Gaussianity that are comparable
to those from the Cosmic Microwave Background (CMB). These are complementary as
they probe different physical scales. The constraints, however, depend on the
sensitivity of galaxy shapes to the initial conditions which we only roughly
estimate from observed tidal alignments.
