activity
20152025
most citedWIMPs and stellar-mass primordial black holes are incompatible

137 citations · 370 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2025

Heating and scattering of stellar distributions by ultralight dark matter

Andrew Eberhardt, Mateja Gosenca, Lam Hui

Due to wave interference, an ultralight light dark matter halo has stochastic, granular substructures which can scatter stars, leading to the heating of stellar distributions. Stud…

astro-ph.CO2023

Aspherical ULDM Collapse: Variation in the Core-Halo Mass Relation

Emily Kendall, Mateja Gosenca, Richard Easther

Ultralight dark matter (ULDM) is an interesting alternative to the cold dark matter (CDM) paradigm. Due to the extremely low mass of the constituent particle ( eV),…

stat.AP2023

Commuter Count: Inferring Travel Patterns from Location Data

Nathan Musoke, Emily Kendall, Mateja Gosenca +4

In this Working Paper we analyse computational strategies for using aggregated spatio-temporal population data acquired from telecommunications networks to infer travel and movemen…

astro-ph.CO2023★ 35 cited

Multifield Ultralight Dark Matter

Mateja Gosenca, Andrew Eberhardt, Yourong Wang +4

Ultralight dark matter (ULDM) is usually taken to be a single scalar field. Here we explore the possibility that ULDM consists of light scalar fields with only gravitational in…

astro-ph.CO2020★ 91 cited

AxioNyx: Simulating Mixed Fuzzy and Cold Dark Matter

Bodo Schwabe, Mateja Gosenca, Christoph Behrens +2

The distinctive effects of fuzzy dark matter are most visible at non-linear galactic scales. We present the first simulations of mixed fuzzy and cold dark matter, obtained with an…

astro-ph.CO2019★ 137 cited

WIMPs and stellar-mass primordial black holes are incompatible

Julian Adamek, Christian T. Byrnes, Mateja Gosenca +1

We recently showed that postulated ultracompact minihalos with a steep density profile do not form in realistic simulations with enhanced initial perturbations. In this paper we as…

astro-ph.CO2018★ 28 cited

Semiclassical path to cosmic large-scale structure

Cora Uhlemann, Cornelius Rampf, Mateja Gosenca +1

We chart a path toward solving for the nonlinear gravitational dynamics of cold dark matter by relying on a semiclassical description using the propagator. The evolution of the pro…

astro-ph.CO2017★ 57 cited

3D simulations with boosted primordial power spectra and ultracompact minihalos

Mateja Gosenca, Julian Adamek, Christian T. Byrnes +1

We perform three-dimensional simulations of structure formation in the early Universe, when boosting the primordial power spectrum on approximately kpc scales. We demonstrate that…

astro-ph.CO2015★ 11 cited

Spherically Symmetric N-body Simulations with General Relativistic Dynamics

Julian Adamek, Mateja Gosenca, Shaun Hotchkiss

Within a cosmological context, we study the behaviour of collisionless particles in the weak field approximation to General Relativity, allowing for large gradients of the fields a…

gr-qc2015★ 11 cited

Dynamical Analysis of Scalar Field Cosmologies with Spatial Curvature

Mateja Gosenca, Peter Coles

We explore the dynamical behaviour of cosmological models involving a scalar field (with an exponential potential and a canonical kinetic term) and a matter fluid with spatial curv…