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| + | [[Radiative Processes in Astrophysics|Course Home]] |
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| ===Short Topical Videos=== | | ===Short Topical Videos=== |
| * [http://youtu.be/LXGBGNR5JxI Coulomb Focusing (Aaron Parsons)] | | * [http://youtu.be/LXGBGNR5JxI Coulomb Focusing (Aaron Parsons)] |
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| ===Reference Material=== | | ===Reference Material=== |
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| + | ===Need to Review?=== |
| + | * [[Collisional Excitations]] |
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| ===Related Topics=== | | ===Related Topics=== |
− | * Collisional Excitations | + | * [[Detailed Balance]] |
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| <latex> | | <latex> |
Latest revision as of 17:38, 5 December 2017
Course Home
Short Topical Videos[edit]
Reference Material[edit]
Need to Review?[edit]
Related Topics[edit]
Coulomb Focusing
Imagine an incident electron has kinetic energy
.
Coulomb focusing gives
cross-section.
We want to know how far away an electron with
can be aimed and still hit the
radius cloud around the ion. This is
, the impact parameter. Our collision cross-section
. Our angular momentum is conserved, so
We know that
, where
is the velocity
to the original electron velocity. This is a result of it falling toward the ion. Then:
Generally, the Coulomb focusing factor
because we want to excite, not ionize.
, so:
is the “collisional strength”, and generally is 0 below the
threshold, goes to 1 at the threshold, and decreases for increasing
, with some occasional spikes. Generally, it is of order 1, with some slight temperature dependency.
2000 K gas.
, so
. Then