We aim at strengthening the communication and collaboration between the European groups involved in theoretical and phenomenological studies in small-x physics. Understanding the dynamics of the strong interaction at high energies is one of the central topics in nuclear and particle physics. From a fundamental point of view, Quantum Chromodynamics (QCD) is today the only quantum field theory that may be studied experimentally in all regimes from strong to weak coupling and from confined to deconfined matter. From an applied point of view, QCD processes constitute the main background and source of uncertainties for the precise determination of parameters in the Standard Model and for searches of new physics. Increasing our understanding of the dynamics of QCD at high energies is of extreme importance for several reasons:
- A genuinely new, non-linear regime of QCD is expected to occur at high energies. Here the Color Glass Condensate (CGC) effective theory provides a controlled weak coupling description applicable in spite of the nonperturbatively large gluonic field strengths. Hints of the breaking of fixed-order perturbation theory have been found at HERA and RHIC, but only data from the LHC and future DIS experiments can unambiguously establish the existence of the nonlinear regime.
- The behavior of gluons carrying only a small fraction x of the proton and nuclear momentum determines the bulk of particle production in relativistic heavy ion collisions. These gluons provide the initial conditions for the subsequent evolution towards a quark-gluon plasma in nuclear collisions at the LHC. A good control of these initial conditions is paramount for understanding the emergence of collectivity at the macroscopic level from the microscopic QCD dynamics.
- New developments in high energy QCD also have implications for rarer observables in the hard domain, where parton densities are not large but linear small-x physics, beyond fixed-order perturbation theory, may nevertheless play a crucial role.
- The nuclear wave function at small x determines the cross sections for interactions of high-energy cosmic rays in the atmosphere, thus the determination of their energy and composition.
Lead beneficiary: USC - Spain
Co-leadership: JYU - Finland
Spokespersons: This email address is being protected from spambots. You need JavaScript enabled to view it., This email address is being protected from spambots. You need JavaScript enabled to view it.
Partners: CNRS - This email address is being protected from spambots. You need JavaScript enabled to view it., IFJ PAN - This email address is being protected from spambots. You need JavaScript enabled to view it.