While most detected binaries to date are consistent with circular inspirals, there is mounting evidence that eccentricity may already be present in current events, with claims ranging from high-mass and low-mass black hole binaries to neutron star–black hole systems. Understanding, modeling, and interpreting eccentric sources is both timely and urgent.
The workshop will bring together experts in theory, numerical relativity, data analysis, and astrophysics, as well as younger researchers entering these fields. We aim to create a collaborative environment where participants can share results, exchange ideas, and identify the next key steps.
The application deadline is June 1st, 2026. Depending on the number of people applying, participants might need to be selected. We will be in touch soon after the deadline, so please do not make travel plans until you hear back from us.
Register here