This workshop is motivated by the broad similarities surrounding the theory of disc mediated migration on scales ranging from protoplanetary discs to galactic nuclei. Migration theory thus underpins our understanding of some of the most topical problems in contemporary astrophysics, i.e. the establishment of planetary system `architecture' and the processes driving the merging of black holes.
We invite participants from both the protoplanetary disc and gravitational wave communities to attend this three day meeting which will address theory and numerical simulations of migration as well as its broader implications. We will also discuss new opportunities in both fields for observational calibration of the migration process (e.g. by observations using ALMA, SPHERE, GPI, LIGO, LISA, PTA, ....).
Local Organising Committee can be emailed at firstname.lastname@example.org
The abstract submission is now closed. Successful applicants will be informed by the end of March.