Studying Active Galactic Nuclei through GRMHD and Radiation Transport Models

Studying Active Galactic Nuclei through GRMHD and Radiation Transport Models

College of Science and Engineering via YouTube Direct link

Introduction

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1 of 30

Introduction

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Classroom Contents

Studying Active Galactic Nuclei through GRMHD and Radiation Transport Models

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  1. 1 Introduction
  2. 2 Active galactic nuclei
  3. 3 GRMHD
  4. 4 Density Plot
  5. 5 Harm Output
  6. 6 Extinction Map
  7. 7 Monte Carlo Code
  8. 8 Thermal Distribution
  9. 9 Emission Profile
  10. 10 Sagittarius A Star
  11. 11 Compton Bumps
  12. 12 Second Bump
  13. 13 Problems
  14. 14 Modifications
  15. 15 Monte Carlo Test
  16. 16 Velocity Modifications
  17. 17 Photon Boosting
  18. 18 relativistic aberration of life
  19. 19 single zone trial
  20. 20 scattering frequency adjustment
  21. 21 velocity adjustment
  22. 22 jet modeling
  23. 23 magnetic turbulence
  24. 24 shearing box approximation
  25. 25 shearing box limitations
  26. 26 Athena MHD code
  27. 27 Shearing factor
  28. 28 Shearing box
  29. 29 Turbulence plot
  30. 30 Harm data

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