activity
20072018
most citedThe Effect of Thermal Neutrino Motion on the Non-linear Cosmological Matter Power Spectrum

152 citations · 682 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2018★ 45 cited

Fully relativistic treatment of light neutrinos in -body simulations

Thomas Tram, Jacob Brandbyge, Jeppe Dakin +1

Cosmological -body simulations are typically purely run with particles using Newtonian equations of motion. However, such simulations can be made fully consistent with general r…

astro-ph.CO2018★ 12 cited

Momentum space sampling of neutrinos in -body simulations

Jacob Brandbyge, Steen Hannestad, Thomas Tram

Including massive neutrinos in -body simulations is a challenging task due to the large thermal velocities of the neutrinos. In particle based codes this leads to problems of sh…

astro-ph.CO2017★ 11 cited

Cosmological N-body simulations with generic hot dark matter

Jacob Brandbyge, Steen Hannestad

We have calculated the non-linear effects of generic fermionic and bosonic hot dark matter components in cosmological N-body simulations. For sub-eV masses, the non-linear power sp…

astro-ph.CO2017★ 36 cited

The effect of early radiation in N-body simulations of cosmic structure formation

Julian Adamek, Jacob Brandbyge, Christian Fidler +3

Newtonian N-body simulations have been employed successfully over the past decades for the simulation of the cosmological large-scale structure. Such simulations usually ignore rad…

astro-ph.CO2017★ 4 cited

Fourier imaging of non-linear structure formation

Jacob Brandbyge, Steen Hannestad

We perform a Fourier space decomposition of the dynamics of non-linear cosmological structure formation in LCDM models. From N-body simulations involving only cold dark matter we c…

astro-ph.CO2017★ 23 cited

The variance of the locally measured Hubble parameter explained with different estimators

Io Odderskov, Steen Hannestad, Jacob Brandbyge

We study the expected variance of measurements of the Hubble constant, , as calculated in either linear perturbation theory or using non-linear velocity power spectra derived…