Event ID: INT-24-90W
Note: This is an in-person workshop.
The opening of the gravitational wave sky is an historic time. LIGO has detected transient signals from merging black holes and neutron stars. This workshop aims to detect continuous gravitational wave signals from rotating neutron stars or new physics.
We invite experts from nuclear physics, particle physics, astrophysics, and gravitational physics communities to come to Seattle to tackle the many open questions. We hope to:
Sponsored by the InQubator for Quantum Simulation.
Sponsored by the InQubator for Quantum Simulation.
This workshop has been rescheduled to take place in Berkeley, CA from July 26, 2022 to July 29, 2022.
Event has been postponed.
Sponsored by the InQubator for Quantum Simulation.
The workshop addressed questions related to hadronization and its multiple manifestations in high-energy scattering processes. Hadronization is intrinsically connected to fundamental properties of QCD, such as confinement and the dynamical breaking of the chiral symmetry. Moreover, it plays an important role in the context of hadron and nuclear structure studies. In particular, a detailed understanding of hadronization is vital for the optimal preparation of the next generation of experiments, such as the Electron-Ion Collider.
Goal
The aim of this school is to introduce students to applications of lattice gauge theory in strongly interacting systems, using a modern teaching style to enhance student learning together with lectures describing the latest advances in the field.
School Topics
Tensor network methods are rapidly developing and evolving in many areas of quantum physics. They offer new ways of computing the properties of strongly interacting quantum matter. They provide new perspectives on theories with sign problems and/or significant entanglement. Tensor network ideas are also closely related to emerging efforts to design algorithms suitable for current and future quantum computing hardware or quantum simulation experiments. This program will bring together experts from a range of scientific fields with a common interest in these new methods.
A sound theoretical description of nuclear forces is pivotal for understanding many important physical observables over a wide range of energy scales and densities, from few-body physics to nuclear-structure observables to astrophysical phenomena. A systematic and precise theory for nuclear Hamiltonians is crucial to providing accurate predictions for these systems with controlled theoretical uncertainties, and to enable meaningful comparisons of theoretical calculations with experimental data and astrophysical observations.
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