Title: Mass ejection, compact objects, and electromagnetic transients
Abstract:
Mass ejection is involved in the generation of many types of electromagnetic transient, often in the presence of at least one compact stellar object. A variety of processes can cause mass to become unbound from a gravitational field, including neutrino emission or absorption, magnetic stresses, angular momentum transport, or nuclear processes. In this talk I will discuss astrophysical situations in which non-trivial mass ejection from the vicinity of a compact object should occur, including the accretion disk formed in a neutron star merger, failed supernovae, and accretion disks from white dwarf - neutron star mergers.
TSI Seminars take place weekly during the Fall and Winter terms. TSI seminars are intended to be accessible to scientists from the entire breadth of backgrounds at TSI, including, Physics, Planetary Science, Geology, Atmospheric Science, and Astrobiology. Our seminar series is partially funded by the Centre de recherche en astrophysique du Québec (CRAQ).