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20102026
most citedNonlinear Evolution of Cosmological Structures in Warm Dark Matter Models

283 citations · 4k across the 56 of their papers we have counts for

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Showing 2014Show all

6 papers · 1 filter

astro-ph.CO2014

Structure formation with suppressed small-scale perturbations

Aurel Schneider

All commonly considered dark matter scenarios are based on hypothetical particles with small but non-zero thermal velocities and tiny interaction cross-sections. A generic conseque…

astro-ph.GA2014★ 36 cited

Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model

Jaehyun Lee, Sukyoung K. Yi, Pascal J. Elahi +13

A halo merger tree forms the essential backbone of a semi-analytic model for galaxy formation and evolution. Recent studies have pointed out that extracting merger trees from numer…

astro-ph.CO2014★ 1 cited

The same with less: The cosmic web of warm versus cold dark matter dwarf galaxies

Darren S. Reed, Aurel Schneider, Robert E. Smith +3

We explore fundamental properties of the distribution of low mass dark matter halos within the cosmic web using warm dark matter (WDM) and cold dark matter (CDM) cosmological simul…

hep-ph2014★ 64 cited

Production of Sterile Neutrino Dark Matter and the 3.5 keV line

Alexander Merle, Aurel Schneider

The recent observation of an X-ray line at an energy of 3.5 keV mainly from galaxy clusters has initiated a discussion about whether we may have seen a possible dark matter signal.…

astro-ph.CO2014★ 42 cited

The life and death of cosmic voids

P. M. Sutter, Pascal Elahi, Bridget Falck +5

We investigate the formation, growth, merger history, movement, and destruction of cosmic voids detected via the watershed transform code VIDE in a cosmological N-body dark matter…

astro-ph.CO2014★ 48 cited

Sussing Merger Trees: the influence of the halo finder

Santiago Avila, Alexander Knebe, Frazer R. Pearce +9

Merger tree codes are routinely used to follow the growth and merger of dark matter haloes in simulations of cosmic structure formation. Whereas in Srisawat et. al. we compared the…