activity
20242026
collaborators

7 papers

gr-qc2026

Spinning charged test particle dynamics around a Schwarzschild black hole embedded in a homogeneous magnetic field

Misbah Shahzadi, Martin Kolos, Ondrej Zelenka +1

We study the dynamics of spinning charged test particles orbiting a Schwarzschild black hole immersed in a test uniform magnetic field. This setup provides a simple but physically…

gr-qc2026

Waveform Modelling for the Laser Interferometer Space Antenna

LISA Consortium Waveform Working Group, Niayesh Afshordi, Sarp Akçay +144

LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will exp…

gr-qc2025

Extreme mass ratio inspirals into black holes surrounded by matter: Resonance crossings

Michal Stratený, Georgios Lukes-Gerakopoulos, Ondřej Zelenka

The forthcoming space-based gravitational-wave observatory Laser Interferometer Space Antenna (LISA) should enable the detection of Extreme Mass Ratio Inspirals (EMRIs), in which a…

gr-qc2025

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

gr-qc2025

Circular equatorial orbits of extended bodies with spin-induced quadrupole around a Kerr black hole: Comparing spin-supplementary conditions

Misbah Shahzadi, Georgios Lukes-Gerakopoulos, Martin Kološ

The worldline of an extended body in curved spacetime can be described by the Mathisson-Papapetrou-Dixon equations when its centroid, i.e., its center of mass, is fixed by a spin s…

gr-qc2024

Combining Machine Learning with Recurrence Analysis for resonance detection

Ondřej Zelenka, Ondřej Kopáček, Georgios Lukes-Gerakopoulos

The width of a resonance in a nearly integrable system, i.e. in a non-integrable system where chaotic motion is still not prominent, can tell us how a perturbation parameter is dri…