Week 2 Lecture material, handouts, and HW posted to the website - - PowerPoint PPT Presentation

week 2
SMART_READER_LITE
LIVE PREVIEW

Week 2 Lecture material, handouts, and HW posted to the website - - PowerPoint PPT Presentation

Week 2 Lecture material, handouts, and HW posted to the website Chapter 5: Ionization losses by energetic ions plowing through a neutral medium Chapter 6: Radiation losses by energetic electrons getting deflected by ions in a plasma ASTR/PHYS


slide-1
SLIDE 1

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics

Week 2

1

Lecture material, handouts, and HW posted to the website Chapter 5: Ionization losses by energetic ions plowing through a neutral medium Chapter 6: Radiation losses by energetic electrons getting deflected by ions in a plasma

slide-2
SLIDE 2

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics

“Swordy Plot” particle flux of CRs at the Earth

2

  • Fig. 15.1
slide-3
SLIDE 3

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics 3

  • Fig. 5.1
  • Fig. 5.2
slide-4
SLIDE 4

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics

Relativistic Case: Ionization losses

4

  • Fig. 5.3
slide-5
SLIDE 5

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics 5

  • Fig. 5.4

Non-rel. Relativistic

slide-6
SLIDE 6

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics

Bethe-Bloch Formula

6

  • Fig. 5.5
slide-7
SLIDE 7

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics

Radiation of an accelerated charge

7

  • Fig. 6.1
slide-8
SLIDE 8

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics

Relativistic Case: electron radiation losses

8

  • Fig. 5.3
slide-9
SLIDE 9

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics 9

slide-10
SLIDE 10

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics

Bremsstrahlung of a single electron, for a single impact parameter b

10

  • Fig. 6.2
slide-11
SLIDE 11

Spring 2020: Week 02 ASTR/PHYS 5590: High Energy Astrophysics

Bremsstrahlung emissivity from a thermal distribution

  • f electrons

11