Cosmic Rays in Astrochemical Models - Understanding Interstellar Chemistry

Cosmic Rays in Astrochemical Models - Understanding Interstellar Chemistry

AVS Knights via YouTube Direct link

A general method for the inclusion of radiation chemistry in astrochemical models

22 of 31

22 of 31

A general method for the inclusion of radiation chemistry in astrochemical models

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Cosmic Rays in Astrochemical Models - Understanding Interstellar Chemistry

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  1. 1 Intro
  2. 2 Extraterrestrial Radiation The First Hint
  3. 3 Confirmation of Extraterrestrial Origin
  4. 4 Evidence of Extraterrestrial Origin
  5. 5 The Origin of the name "Cosmic Ray"
  6. 6 The Nature of Cosmic Rays
  7. 7 Composition of Cosmic Rays
  8. 8 Where Do Cosmic Rays Come From?
  9. 9 Cosmic Ray Energy Distribution
  10. 10 Cosmic Rays in the Interstellar Medium
  11. 11 Rock
  12. 12 Murchison Meteorite
  13. 13 How does irradiation change the ice composition?
  14. 14 Ionizing Radiation "Tracks"
  15. 15 Monte Carlo Models
  16. 16 Part IV
  17. 17 A new model of the chemistry of ionizing radiation in solids: CIRIS
  18. 18 CIRIS Algorithm
  19. 19 Experimental Physical Conditions
  20. 20 An Initial Attempt at Simulating Particle Tracks
  21. 21 CIRIS Data
  22. 22 A general method for the inclusion of radiation chemistry in astrochemical models
  23. 23 Back Cover Design
  24. 24 The Importance of Excited Species at Low Temperatures
  25. 25 Step 1: Elementary Processes
  26. 26 Step 2
  27. 27 Rate Coefficients
  28. 28 Bulk Chemistry Like the surface, but slower?
  29. 29 Radicals In Ices An Extreme Scenario
  30. 30 Bulk Chemistry: Unlike the surface and faster?
  31. 31 Shingledecker et al. (2019)

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