PhD Student in Astrophysics · ITA/ZAH, Heidelberg University
I am a computational astrophysicist modelling how black holes grow from stellar to intermediate and supermassive masses, and what their gravitational-wave mergers reveal about the early Universe. I showed that AGN disks can grow black holes through the pair-instability gap into the intermediate-mass range, but only in low-viscosity disks with efficient gas hardening, and that the resulting populations match systems like GW190521 and GW231123.
Intermediate-mass black holes · AGN disk dynamics · star cluster dynamics · gravitational-wave sources · stellar collisions · Einstein Telescope science
I wrote about the multiple formation channels of binary black hole mergers, with a focus on AGN disks and hierarchical assembly, for the Heidelberg STRUCTURES Excellence Cluster blog. Read the article →
Co-organizer of the annual workshop A dance of stars and black holes for school-aged students as part of the national Girls' Day programme in Germany (2024, 2025, 2026).
My paper on the formation of binary black holes in AGN disks was featured on Gist.Science, a platform making research accessible to a broad audience. Read the summary →
Member of the organizing committee of Scholé, a nonprofit that brings physics, philosophy, and history to the general public through weekly seminars and an annual Summer School in Calabria, Italy.