Particle Acceleration and Non-thermal Emission in Radiatively Inefficient Accretion Flows
APA
Quataert, E. (2014). Particle Acceleration and Non-thermal Emission in Radiatively Inefficient Accretion Flows. Perimeter Institute. https://pirsa.org/14110069
MLA
Quataert, Eliot. Particle Acceleration and Non-thermal Emission in Radiatively Inefficient Accretion Flows. Perimeter Institute, Nov. 10, 2014, https://pirsa.org/14110069
BibTex
@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}} }
University of California, Berkeley
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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*.