Video URL

https://pirsa.org/14110069

Particle Acceleration and Non-thermal Emission in Radiatively Inefficient Accretion Flows

Quataert, E. (2014). Particle Acceleration and Non-thermal Emission in Radiatively Inefficient Accretion Flows. Perimeter Institute for Theoretical Physics. https://pirsa.org/14110069

Quataert, Eliot. Particle Acceleration and Non-thermal Emission in Radiatively Inefficient Accretion Flows. Perimeter Institute for Theoretical Physics, Nov. 10, 2014, https://pirsa.org/14110069 

          @misc{ scivideos_PIRSA:14110069,
            doi = {10.48660/14110069},
            url = {https://pirsa.org/14110069},
            author = {Quataert, Eliot},
            keywords = {Strong Gravity},
            language = {en},
            title = {Particle Acceleration and Non-thermal Emission in Radiatively Inefficient Accretion Flows},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {nov},
            note = {PIRSA:14110069 see, \url{https://scivideos.org/pirsa/14110069}}
          }

Eliot Quataert University of California, Berkeley

DOI 10.48660/14110069
Source Repository PIRSA
Collection
Talk Type Conference
Subject

Abstract

I summarize several physical processes that can produce efficient particle acceleration in radiatively inefficient accretion flows. I then describe the implications for non-thermal emission and EHT observations of Sgr A*.