Video Lectures

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Turbulence in Planet Formation

Phil Armitage

A combination of sub-mm observations and numerical simulations have the potential to yield direct constraints on the environment of planet formation. After a review of recent observational surprises, I will discuss the implications of our first...

After a basic introduction on how asteroseismology works in practice, we illustrate its application to various kinds of stars of different mass and evolutionary stage. We show how detected oscillation modes allow us to understand details of the...

Extending the Prym map

Samuel Grushevsky
The Torelli map associates to a genus g curve its Jacobian - a $g$-dimensional principally polarized abelian variety. It turns out, by the works of Mumford and Namikawa in the 1970s (resp. Alexeev and Brunyate in 2010s), that the Torelli map extends...