arXiv:1301.2778·v2·Cosmology and Nongalactic Astrophysics
Scale-dependent bias due to primordial vector fields
Maresuke Shiraishi · Shuichiro Yokoyama · Kiyotomo Ichiki · Takahiko Matsubara
Abstract
Anisotropic stress perturbations induced by primordial Gaussian vector fields create non-Gaussianity in curvature perturbations. We found that such non-Gaussianity closely resembles the local-type non-Gaussianity parametrized by , and generates scale-dependent bias in large-scale structures. We also found a simple relationship between the scale-dependent bias and the power spectrum of the vector fields. When the vector fields are interpreted as primordial magnetic fields, the effective is shown to be always negative. The scale-dependent bias provides a new approach to probing primordial vector fields.
Comments: 9 pages, 5 figures. Accepted for publication in MNRAS Mon.Not.Roy.Astron.Soc. (2013)