Astrophysical Jets from accreting Black Holes

More documents

Recommendations

Info

II.1 Fermi Acceleration ● relativistic particle is reflected by a moving gas cloud ● transformations lead to energy gain E E ≈2 u c u2 2 c
II.2 Diffusive shock acceleration ● In a uniform magnetic field a freely moving charged particle follows a helical trajectory. The particles pitch is defined as: = p⋅ B pB so its momenta are p para =p p perp =1− 2 0.5 p
Page 1 and 2: Astrophysical Jets from accreting B
Page 3 and 4: I.Description of astrophysical jets
Page 5 and 6: I.1 Sources of Jets Active Galaxy N
Page 7 and 8: I.1 Sources of Jets Gamma Ray Burst
Page 9 and 10: I.3 Formation Mechanism ● not kno
Page 11: II. Acceleration in Jets
Page 15 and 16: II.2 Diffusive shock acceleration
Page 35 and 36: III.1 Synchrotron Emission ● part
Page 37 and 38: III.2 Inverse Compton Scattering
Page 39 and 40: III.3 Other Processes ● 1. proton
Page 41: II.2 Diffusive shock acceleration

Astrophysical Jets from accreting Black Holes

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?