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Similar

F. Marulli, C. Carbone, M. Viel, L. Moscardini and A. Cimatti, Effects of massive neutrinos on the large-scale structure of the Universe , Mon. Not. Roy. Astron. Soc. 418
Original
2011
Cited alongside, same era.
P. M. Sutter, G. Lavaux, B. D. Wandelt and D. H. Weinberg, A First Application of the Alcock-Paczynski Test to Stacked Cosmic Voids , Astrophys. J. 761
Original
2012
Cited alongside, same era.
J. Lesgourgues and S. Pastor, Neutrino mass from Cosmology , ArXiv e-prints (2012) [ 1212.6154 ]
Original
2012
Cited alongside, same era.
M. A. Aragon-Calvo and A. S. Szalay, The hierarchical structure and dynamics of voids , Mon. Not. Roy. Astron. Soc. 428
Original
2013
Cited alongside, same era.
T. Baldauf, U. Seljak, R. E. Smith, N. Hamaus and V. Desjacques, Halo stochasticity from exclusion and nonlinear clustering , Phys. Rev. D 88

Then

A. Banerjee and N. Dalal, Simulating nonlinear cosmological structure formation with massive neutrinos , JCAP 11
Original
2016
Later among the works it cites.
G. Pollina, M. Baldi, F. Marulli and L. Moscardini, Cosmic voids in coupled dark energy cosmologies: the impact of halo bias , Mon. Not. Roy. Astron. Soc. 455
Original
2016
Later among the works it cites.
C. Carbone, M. Petkova and K. Dolag, DEMNUni: ISW, Rees-Sciama, and weak-lensing in the presence of massive neutrinos , JCAP 7
Original
2016
Later among the works it cites.
J. Clampitt, B. Jain and C. Sánchez, Clustering and bias measurements of SDSS voids , Mon. Not. Roy. Astron. Soc. 456
Original
2016
Later among the works it cites.
S. Alam, M. Ata, S. Bailey, F. Beutler, D. Bizyaev, J. A. Blazek et al., The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample , Mon. Not. Roy. Astron. Soc. 470

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2019

The bias of cosmic voids in the presence of massive neutrinos

Schuster, Nico, Hamaus, Nico, Pisani, Alice et al.

Understand

Cosmic voids offer an extraordinary opportunity to study the effects of massive neutrinos on cosmological scales.

Because they are freely streaming, neutrinos can penetrate the interior of voids more easily than cold dark matter or baryons, which makes their relative contribution to the mass budget in voids much higher than elsewhere in the Universe.
In simulations it has recently been shown how various characteristics of voids in the matter distribution are affected by neutrinos, such as their abundance, density profiles, dynamics, and clustering properties.
However, the tracers used to identify voids in observations (e.g., galaxies or halos) are affected by neutrinos as well, and isolating the unique neutrino signatures inherent to voids becomes more difficult.