The QGSKY project focuses on theoretical and phenomenological aspects of QFT, RG, and theories beyond RG, considering observations derived from so-called precision cosmology. Our nodes collaboratively engage in various projects, and while our main interests lie in theoretical and phenomenological aspects, our IS's expertise spans from the phenomenology of particle physics to cosmology and relativistic astrophysics. Common threads of the IS include:
- Extended gravity theories
- Non-local QFT and non-local gravity theories
- Dark matter and dark energy
- QFT in curved spacetime
- Exact solutions of black holes
- Theoretical cosmology
Structured staff:
- Paolo Salucci (coordinator) (SISSA)
- Andrea Lapi (SISSA)
- Riccardo Valdarnini (SISSA)