activity
19992026
most citedA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulence

301 citations · 6.3k across the 162 of their papers we have counts for

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7 papers · 1 filter

astro-ph2008

The prospects of finding the first quasars in the universe

Dominik R. G. Schleicher, Marco Spaans, Ralf S. Klessen

We study the prospects of finding the first quasars in the universe with ALMA and JWST. For this purpose, we derive a model for the high-redshift black hole population based on obs…

astro-ph2008★ 8 cited

Cosmic constraints rule out s-wave annihilation of light dark matter

Dominik R. G. Schleicher, Simon C. O. Glover, Robi Banerjee +1

Light dark matter annihilating into electron-positron pairs emits a significant amount of internal bremsstrahlung that may contribute to the cosmic gamma-ray background. The amount…

astro-ph2008★ 38 cited

Dark stars: Implications and constraints from cosmic reionization and extragalactic background radiation

Dominik R. G. Schleicher, Robi Banerjee, Ralf S. Klessen

Dark stars powered by dark matter annihilation have been proposed as the first luminous sources in the universe. These stars are believed to form in the central dark matter cusp of…

astro-ph2008★ 7 cited

The formation of the first galaxies and the transition to low-mass star formation

Thomas H. Greif, Dominik R. G. Schleicher, Jarrett L. Johnson +6

The formation of the first galaxies at redshifts z ~ 10-15 signaled the transition from the simple initial state of the universe to one of ever increasing complexity. We here revie…

astro-ph2008★ 51 cited

Influence of primordial magnetic fields on 21 cm emission

Dominik R. G. Schleicher, Robi Banerjee, Ralf S. Klessen

Magnetic fields in the early universe can significantly alter the thermal evolution and the ionization history during the dark ages. This is reflected in the 21 cm line of atomic h…

astro-ph2008★ 74 cited

Effects of primordial chemistry on the cosmic microwave background

D. R. G. Schleicher, D. Galli, F. Palla +4

Previous works have demonstrated that the generation of secondary CMB anisotropies due to the molecular optical depth is likely too small to be observed. In this paper, we examine…