The activities of the theory group focus on the study of the fundamental interactions, encompassing a wide spectrum of interests which go from formal investigations, to theory and phenomenology of strings, fields and particles, to nuclear physics, to gravitation and cosmology, to statistical and quantum physics.
Why do neutrinos have mass? How do they oscillate? What is dark matter? Why is there so much more matter than antimatter in the Universe? What is the origin of masses and of the approximate fundamental symmetries? How did our Universe evolve to what we observe today? These are the key questions that motivate our research activity in the theory and phenomenology of astroparticle physics.
Understanding the origin and dynamics of the primordial universe when the energy was close to the Planck scale, as well as the dynamics of black holes, offer numerous challenges. These include quantum effects in gravitational interactions, the mechanism of cosmic inflation, the nature of dark matter and of dark matter.
The study of the fundamental interactions between the elementary constituents of matter at accelerators working at the energy and intensity frontiers, aims at providing an answer to some of the most enticing questions in physics: How comes that the Universe is matter dominated? What is the origin of the tiny neutrino masses? Is there new physics in reach beyond the electroweak scale? Do we fully understand the various regimes of strong interactions? What are the properties of nuclear systems at the stability limit and in extreme environments?
Quantum field theory is the primary theoretical tool to describe both fundamental interactions and condensed matter. Nevertheless, several issues still remain open. These include the study of non-perturbative effects also via exact methods like integrability, and the connection between fundamental physics at high scales and low-energy phenomenology.
String theory is a very promising candidate for a consistent theory of quantum gravity and the unification of all fundamental interactions. Typical ingredients of string theory include extra dimensions, supersymmetry and branes. The low-energy limit of string compactifications reproduces General Relativity and gauge theories similar to the Standard Model (SM). A complete understanding of the implications of string theory for particle physics and cosmology is currently an active area of research
The study of the quantum many body systems is the cornerstone of our understanding of different forms of matter, from its fundamental constituents to composite structures. As a result of important experimental advances that have allowed to synthesize new materials and to directly manipulate atomic structures, theory has developed new methods that integrate numerical simulations techniques with modern approaches to statistical field theory, importing also powerful tools from information theory and quantum computations, with a high impact in applications for data science.