PIRSA:14110069 Conference Strong Gravity

DOI10.48660/14110069

Conference/School: EHT 2014

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

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

@misc{ pirsa_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},
  year = {2014},
  month = {nov},
  note = {PIRSA:14110069 see, \url{https://pirsa.org}}
}

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*.

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