Development and implementation of theoretical models to study the growth mechanisms of supermassive black holes in the high-redshift Universe and their co-evolution with their host galaxies.
Posted on: 28/01/2026
Deadline: 07/02/2026
Deadline: 07/02/2026
Scientific-Disciplinary Group
02/PHYS-05 - Astrophysics And Cosmology, Earth- Space- And Climate Physics
Description
The planned research activity falls within the framework of the FIS3 DAWN project: Charting the path to cosmic dawn through the footprints of the first stars and black holes. In particular, it involves the development and implementation of high-resolution numerical simulations to describe the early growth phase of seed black holes in primordial galaxies and the effects of black hole feedback on their host galaxies.
Compensation
39,224 Euro
Job posting website
Number of positions
1
Funding body
SAPIENZA UNIVERSITA' ROMA
How to apply
View the original posting on the MUR website: Go to MUR website