Abstract
We study the scale-dependent bias of the halo power spectrum arising from primordial non-Gaussianity. We present an analytic result of the halo bias including up to the trispectrum contributions. We find that the scale-dependent bias opens a new possibility of probing the relation between the non-linearity parametersfNL and τNL.
| Original language | English |
|---|---|
| Pages (from-to) | L79-L82 |
| Journal | Monthly Notices of the Royal Astronomical Society: Letters |
| Volume | 417 |
| Issue number | 1 |
| DOIs | |
| State | Published - Oct 2011 |
Keywords
- Cosmology: theory
- Galaxies: haloes
- Large-scale structure of Universe