The Institute for Nuclear Theory, a national resource funded by the US Department of Energy and the University of Washington, provides an environment for scientists to advance the frontiers of subatomic physics. Scientific meetings at the INT attract hundreds of visitors annually from around the world to hasten breakthrough discoveries through collaborations.
Welcome to the Institute for Nuclear Theory (INT)
Dark Matter in Compact Objects, Stars, and Low-Energy Experiments (22-2b)
This program aims to advance efforts to identify and characterize the observable signatures of dark matter and new physics beyond the standard model (BSM) in compact objects and stars and the complementarity of these signatures with those of terrestrial experiments and cosmological probes.
Parton Distributions and Nucleon Structure (22-83W)
In this workshop, we will bring together leading experts in hadron physics from the theoretical, phenomenological, and lattice communities. This workshop will promote cross-collaborations on extracting distribution functions and will have profound impact on both theory and experiment.
Heavy Flavor Production in Heavy‐Ion and Elementary Collisions (22-3)
Heavy flavor probes of the Quark-Gluon Plasma are required to realize the heavy-ion physics programs of the LHC and the new and final RHIC experimental program, sPHENIX.
Dense Nuclear Matter Equation of State from Heavy-Ion Collisions (22-84W)
Constraining the dependence of the dense nuclear matter equation of state (EOS) on baryon density is a long-standing problem of nuclear physics.