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Similar

M. Costanzi, F. Villaescusa-Navarro, M. Viel, J.-Q. Xia, S. Borgani, E. Castorina et al., Cosmology with massive neutrinos III: the halo mass function andan application to galaxy clusters , JCAP 1312
Original
2013
Cited alongside, same era.
Euclid Theory Working Group
Original
2013
Cited alongside, same era.
B. Audren, J. Lesgourgues, K. Benabed and S. Prunet, Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code , JCAP 1302
Original
2013
Cited alongside, same era.
F. Villaescusa-Navarro, F. Marulli, M. Viel, E. Branchini, E. Castorina, E. Sefusatti et al., Cosmology with massive neutrinos I: towards a realistic modeling of the relation between matter, haloes and galaxies , JCAP 1403
Original
2014
Cited alongside, same era.

Then

M. Gerbino, M. Lattanzi, O. Mena and K. Freese, A novel approach to quantifying the sensitivity of current and future cosmological datasets to the neutrino mass ordering through Bayesian hierarchical modeling , Phys. Lett. B775
Original
2017
Later among the works it cites.
F. Simpson, R. Jimenez, C. Pena-Garay and L. Verde, Strong Bayesian Evidence for the Normal Neutrino Hierarchy , JCAP 1706
Original
2017
Later among the works it cites.
W. Yang, R. C. Nunes, S. Pan and D. F. Mota, Effects of neutrino mass hierarchies on dynamical dark energy models , Phys. Rev. D95
Original
2017
Later among the works it cites.
C. S. Lorenz, E. Calabrese and D. Alonso, Distinguishing between Neutrinos and time-varying Dark Energy through Cosmic Time , Phys. Rev. D96
Original
2017
Later among the works it cites.

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2018

Bias due to neutrinos must not uncorrect'd go

Vagnozzi, Sunny, Brinckmann, Thejs, Archidiacono, Maria et al.

Understand

In cosmologies with massive neutrinos, the galaxy bias defined with respect to the total matter field (cold dark matter, baryons, and non-relativistic neutrinos) depends on the sum of the neutrino masses $M_{\nu}$, and becomes scale-dependent even on large scales.

This effect has been usually neglected given the sensitivity of current surveys, but becomes a severe systematic for future surveys aiming to provide the first detection of non-zero $M_{\nu}$.
The effect can be corrected for by defining the bias with respect to the density field of cold dark matter and baryons instead of the total matter field.
In this work, we provide a simple prescription for correctly mitigating the neutrino-induced scale-dependent bias effect in a practical way.