Cosmology at Ruđer
Simulation of cosmic structures, on the light cone from the Big Bang until today (left), and at the present time (right). ©
arXiv:2409.19049
Welcome!
Cosmology at Ruđer was newly formed in 2021. We are interested in addressing the
big questions in physics: what is dark matter and dark energy? What is the neutrino
mass scale? Are there new long-range forces in the dark sector? New light degrees
of freedom such as ultralight axions? What can we learn about the epoch of
primordial inflation? How can we relate theoretical predictions to observations?
Below you find:
- some details about our current research interests
- a list of affiliated members
Interested in a master/PhD/seminar/internship on cosmology? We can provide
guidance and (co-)supervision, also if you are not based in Zagreb, so get in contact
with us!
Giovanni Cabass works at the intersection between theory and data analysis. For
this, he mostly employs and advances methods from effective field theory. His main
interests are:
- understanding how much information lies in the perturbative
forward modelling of the galaxy density field as opposed to its
summary statistics
- using galaxy clustering observations to constrain the physics of
inflation, looking for new degrees of freedom during this epoch
and their properties
- recently, Giovanni is interested in learning how to apply AI and
Machine Learning tools in cosmological data analysis
Cornelius Rampf focuses on fluid dynamical aspects of cosmological structure
formation, with a particular emphasis on combining analytical methods and
numerical approaches (like N-body simulations). Some recent
branches of interest:
- Perturbation theory and asymptotic methods, primarily applied
within cosmology but recently extending to general fluid
dynamics;
- developing fast and/or accurate N-body simulation
techniques for cosmic structures by incorporating analytical
insights;
- general relativity and large-scale structure, in particular how massive neutrinos
can be efficiently modelled to sufficient accuracy.
Zvonimir Vlah works in the field of large-scale structure formation, developing novel
analytical and numerical methods for analysing data from galaxy surveys. Topics of
interest
- perturbation theory/effective field theory methods in
cosmological structure formation
- understanding correlators on the sky in light of new galaxy
surveys
- development of nonperturbative approaches in large-scale
structure formation
Affiliated members of the cosmology section:
- Nov 2024 - Mar 2025 Dennis Linde visiting PhD student (Parma, 2022-2025)
- Nov 2024 - Apr 2025 Szymon Juszczak, master student (Vienna, co-supervision)
- Nov 2024 - Apr 2025 Michelle Anderson, master student (Vienna, co-supervision)