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2018

Cubic Halo Bias in Eulerian and Lagrangian Space

Abidi, Muntazir Mehdi, Baldauf, Tobias

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Predictions of the next-to-leading order, i.e.

one-loop, halo power spectra depend on local and non-local bias parameters up to cubic order.
The linear bias parameter can be estimated from the large scale limit of the halo-matter power spectrum, and the second order bias parameters from the large scale, tree-level, bispectrum.
Cubic operators would naturally be quantified using the tree-level trispectrum.

Cubic Halo Bias in Eulerian and Lagrangian Space · Around

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