activity
20162020
most citedIsocurvature bounds on axion-like particle dark matter in the post-inflationary scenario

23 citations · 23 across the 2 of their papers we have counts for

collaborators

15 papers

astro-ph.CO2020

Probing primordial non-Gaussianity with Fast Radio Bursts

Robert Reischke, Steffen Hagstotz, Robert Lilow

Fast radio bursts (FRBs) are astrophysical transients of currently unknown origin, and so far several events have been detected at extragalactic distances. The dispersion measure (…

astro-ph.CO2020

Information entropy in cosmological inference problems

Ana Marta Pinho, Robert Reischke, Marie Teich +1

The subject of this paper is a quantification of the information content of cosmological probes of the large-scale structures, specifically of temperature and polarisation anisotro…

gr-qc2020

Information geometry in cosmological inference problems

Eileen Giesel, Robert Reischke, Björn Malte Schäfer +1

Statistical inference more often than not involves models which are non-linear in the parameters thus leading to non-Gaussian posteriors. Many computational and analytical tools ex…

astro-ph.CO2020

Post-inflationary axion isocurvature perturbations facing CMB and large-scale structure

Martin Feix, Steffen Hagstotz, Andreas Pargner +3

Dark matter comprised of axion-like particles (ALPs) generated by the realignment mechanism in the post-inflationary scenario leads to primordial isocurvature fluctuations. The pow…

astro-ph.CO2019

Realistic systematic biases induced by residual intrinsic alignments in cosmic shear surveys

Robert Reischke, Björn Malte Schäfer

We study the parameter estimation bias induced by intrinsic alignments on a Euclid-like weak lensing survey. For the intrinsic alignment signal we assume a composite alignment mode…

astro-ph.CO2019

The Probability Distribution of Astrophysical Gravitational-Wave Background Fluctuations

Yonadav Barry Ginat, Vincent Desjacques, Robert Reischke +1

The coalescence of compact binary stars is expected to produce a stochastic background of gravitational waves (GW) observable with future GW detectors. Such backgrounds are usually…