activity
20052026
most citedBeyond CDM: Problems, solutions, and the road ahead

530 citations · 2.1k across the 52 of their papers we have counts for

collaborators

52 papers

astro-ph.CO2026

Nonlinear velocity power spectrum: modeling the cosmological dependence on the Hubble constant and cold dark matter density

Francesca Lepori, Ruth Durrer, Martin Kunz +3

In this paper we present a semi-analytical model for the velocity power spectrum in $\La$CDM cosmology for wave numbers Mpc. We mainly concentrate on the dominant divergence…

astro-ph.CO2026

Signatures of kinetic gravity braiding in cosmological probes of the gravitational field

Ahmad Nouri-Zonoz, Farbod Hassani, Julian Adamek +2

We study the observational signatures of kinetic gravity braiding (KGB) models in relativistic cosmological probes constructed along the past light cone. Using the relativistic …

astro-ph.IM2026

gevolution 2.0: GPU-accelerated relativistic N-body simulations for cosmology

Julian Adamek, Øyvind Christiansen

High-performance computing is increasingly dominated by hardware acceleration using Graphics Processing Units (GPUs). To take advantage of this long-term trend, we implement a majo…

astro-ph.CO2026

Perturbative and numerical study of nonlinear relativistic effects in weak lensing

Matteo Magi, Francesca Lepori, Julian Adamek

The standard weak lensing formalism assumes that the lensing map relating the observed image of a source to its intrinsic shape depends only on the deflection angle. We show that t…

astro-ph.CO2025

Transverse Velocities in Real-Time Cosmology: Position Drift in Relativistic N-Body Simulations

Alexander Oestreicher, Chris Clarkson, Julian Adamek +1

The era of real-time cosmology has begun. It is now possible to directly measure the apparent drift of high-redshift astronomical sources across the sky . Th…

astro-ph.CO2025★ 2 cited

Redshift Drift in Relativistic N-Body Simulations

Alexander Oestreicher, Chris Clarkson, Julian Adamek +1

The cosmological redshift drift promises to be the first observable directly measuring the evolution of the cosmic expansion rate and should be detectable with upcoming surveys by…