Hyper-accretion April 7-11, 2014
Hyper-accretion April 7-11, 2014
Kavli Institute for the Physics and Mathematics of the Universe
Images courtesy of Ken Nagamine
Contact: hyper-accretion2014@ipmu.jp
Accretion, at rates substantially in excess of
the Eddington limit, is implicated in tidal
disruption events, gamma-ray bursts, some
X-ray binaries and supermassive black hole
formation. Despite this ubiquity, the physical
principles that govern hyper-accretion remain
to be determined. Recent advances in
numerical radiation hydrodynamics, along
with observations of the time-dependence
of hyper-accreting flows following tidal disruptions, offer new opportunities to make progress. The workshop is intended to facilitate interaction between observers and theorists working on hyper-accretion in different astrophysical systems, and to identify new directions for future research.