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Presentation on
Collision Phenomena
&
Excitation and Ionization
By Bijaya Basnet
Contents
1. Collision phenomena
- Collision phenomena
- Velocity distribution
- Elastic and Inelastic collision
- Reaction cross-section
2. Ionization and Excitation
- Excitation and ionization by electron collision
- Excitation and ionization by energetic particles or neutral particles
- Thermal ionization
- Penning ionization
- Photo ionization and Photo excitation
- Ion – Ion recombination
- Ion-electron recombination
Collision phenomena
From http://kayjayr-akshay.blogspot.com/2016/04/plasma-
fourth-state-of-matter.html
From
http://noyesharrigan.cmswiki.wikispaces.net/Maxwell-
Boltzmann+Distribution
temperature-of-electrons-and-heavy-
particles-in-the-plasma-as-a-function-of
pressure
From
https://www.researchgate.net/publication/257139583_Reducti
on_of_Oxide_Minerals_by_Hydrogen_Plasma_An_Overview
Comparison of Maxwellian and
Druyvesteyn Distributions
FromNicholasJamesBehlman
Thesisonplasma
Elastic and Inelastic collision
u1
u2
v1
v2
u1
u2
v1
v
v2
u1
u2
v1
u2
h𝑣
Mean free path and collision
frequency
+
+
+
+
+
+
+
+
+
+
+
+
Reaction cross-section
𝑑𝑛
𝑑𝑡
=−∝ 𝑛+ 𝑛− ∝ 6 × 3 ∝ 16 × 3
Excitation and Ionization
• Ionization and Excitation of atoms and
molecules by electron collision
Ionization Excitation
Ionization by electron impact
Cumulative (multistage)
ionization
Single (direct) ionization
• Ionization and Excitation of atoms and
molecules by energetic ions or neutral
particles
Ionization Excitation
Thermal ionization
From http://article.sapub.org/10.5923.j.instrument.20120105.02.html
Penning ionization
• 𝐴 + 𝐵∗
→ 𝐴+
+ 𝑒 + 𝐵
• Condition
Ionization potential of A is less than Excitation
potential of metastable particle𝐵∗
Photo-ionization
• 𝐴 + ℎ𝑣 = 𝐴+
+ 𝑒−
, ℎ𝑣 > 𝑉𝐼
Photo-excitation
• 𝐴 + ℎ𝑣 = 𝐴∗
, 𝑉𝐼> ℎ𝑣 > 𝑉𝐸
Ion-Ion recombination
• Radiative recombination
𝐴+
+ 𝐵−
→ 𝐴𝐵 + ℎ𝑣
• Mutual neutralization
𝐴+
+ 𝐵−
→ 𝐴∗
+ 𝐵∗
• Three body recombination
𝐴+
+ 𝐵−
+ 𝑀 → 𝐴𝐵 + 𝑀
Ion-electron recombination
• Radiative recombination
𝐴+ + 𝑒− → 𝐴∗ + ℎ𝑣
• Dielectronic recombination
𝐴+ + 𝑒− → 𝐴∗∗
𝐴∗∗ → 𝐴∗ + ℎ𝑣
𝐴∗∗ + 𝐵 → 𝐴∗ + 𝐵∗
• Dissociative recombination
𝐴𝐵+
+ 𝑒−
→ 𝐴∗
+ 𝐵∗
• Three body recombination
𝐴+
+ 𝑒−
+ 𝑒−
→ 𝐴 + 𝑒−
𝐴+ + 𝑒− + 𝐵 → 𝐴 + 𝐵
Any question?

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Ch 1,2 collision phenomenon bijay basnet (Devid Peter)

Editor's Notes

  1. The most signicant difference between the Maxwellian energy distribution and the Druyvesteyn distribution is the different power of in the exponential argument. Physically, the Druyvesteyn distribution is specific to electrons interacting with neutrals of comparatively low energy. Figure is a graphical comparison between the Maxwellian and Druyvesteyn distributions.
  2. The nuclear cross section of a nucleus is used to characterize the probability that a nuclear reaction will occur. The concept of a nuclear cross section can be quantified physically in terms of "characteristic area" where a larger area means a larger probability of interaction.
  3. Recombination coefficient: 10^(-14) cm^3/s , 10^(-8) to 10^(-7), Te^(1/2), 10^(-7) to 10^(-6)
  4. 10^(-10)-10^(-13), 10^(-12), , ne(kTe/e)^-(9/2) p(kTe/e)^-(5/2)