Nuclear Theory for New Physics
Aula Leonardi
ECT* - Villa Tambosi

The combined “standard models" of fundamental interactions and cosmology leave a number of questions about the observed universe without answer. Outstanding puzzles include the origin and nature of neutrino mass, the origin of the matter-antimatter asymmetry in the universe, and the nature of dark matter. Low-energy processes involving neutrinos, hadrons, and nuclei have the potential to shed light directly or indirectly on some of these great mysteries. Given the potentially very high impact of the experimental program of electroweak and Beyond the Standard Model (BSM) physics with nuclei and the crucial need for the corresponding theory, we propose a DTP focused on ‘nuclear theory for new physics’. Through lectures and problem-solving sessions this DTP will provide nuclear theory students the motivation and context for electroweak and BSM studies with nuclei as well as the basic theoretical and computational tools needed in these studies. This DTP aims to establish a common ground for nuclear theory students in different sub-communities interfacing in the study of electroweak and BSM physics with nuclei: phenomenology and Effective Field Theory, lattice QCD, and nuclear structure. The concepts and tools presented at this DTP will prepare the students to apply cutting edge methodologies to challenging problems in the field and to identify new directions.
Lecturers
Francesca Bonaiti, Oak Ridge National Laboratory
Mattia Bruno, Università Milano-Bicocca
Wouter Dekens, University of Washington
Bhupal Dev, Washington University in St. Louis
Alex Gnech, Old Dominion University
Yuval Grossman, Cornell University
Heiko Hergert, Michigan State University
Garrett King, Los Alamos National Laboratory
Sebastian Koenig, North Carolina State University
Dimitra Pefkou, CERN
Chien Yeah Seng, University of Tennessee
Ubirajara van Kolck, ECT*
Supporting projects and institutions
