Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Pair production
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
=== Basic kinematics === These properties can be derived through the kinematics of the interaction. Using [[four vector]] notation, the conservation of energy–momentum before and after the interaction gives:<ref> {{cite web |last=Kuncic |first=Zdenka, Dr. |date=12 March 2013 |title=PRadiation Physics and Dosimetry |series=PHYS 5012 |website=Index of Dr. Kuncic's Lectures |publisher=The University of Sydney |place=Sydney, Australia |url=http://www.physics.usyd.edu.au/~kuncic/lectures/RP3_slides.pdf |access-date=2015-04-14 |url-status=dead |archive-url=https://web.archive.org/web/20160311042609/http://www.physics.usyd.edu.au/~kuncic/lectures/RP3_slides.pdf |archive-date=11 March 2016 }} </ref> : <math>p_\gamma = p_{\text{e}^-} + p_{\text{e}^+} + p_{\text{ʀ}}</math> where <math>p_\text{ʀ}</math> is the recoil of the nucleus. Note the modulus of the four vector : <math>A \equiv (A^0,\mathbf{A}) </math> is : <math>A^2 = A^{\mu} A_{\mu} = - (A^0)^2 + \mathbf{A} \cdot \mathbf{A} </math> which implies that <math>(p_\gamma)^2 = 0 </math> for all cases and <math>(p_{\text{e}^-})^2 = -m_\text{e}^2 c^2 </math>. We can square the conservation equation : <math>(p_\gamma)^2 = (p_{\text{e}^-} + p_{\text{e}^+} + p_\text{ʀ})^2 </math> However, in most cases the recoil of the nucleus is small compared to the energy of the photon and can be neglected. Taking this approximation of <math>p_{R} \approx 0</math> and expanding the remaining relation : <math>(p_\gamma)^2 \approx (p_{\text{e}^-})^2 + 2 p_{\text{e}^-} p_{\text{e}^+} + (p_{\text{e}^+})^2 </math> : <math>-2\, m_\text{e}^2 c^2 + 2 \left( -\frac{E^2}{c^2} + \mathbf{p}_{\text{e}^-} \cdot \mathbf{p}_{\text{e}^+} \right) \approx 0 </math> : <math>2\,(\gamma^2 - 1)\,m_\text{e}^2\,c^2\,(\cos \theta_\text{e} - 1) \approx 0 </math> Therefore, this approximation can only be satisfied if the electron and positron are emitted in very nearly the same direction, that is, <math>\theta_\text{e} \approx 0 </math>. This derivation is a semi-classical approximation. An exact derivation of the kinematics can be done taking into account the full [[quantum mechanical scattering of photon and nucleus]].
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Pair production
(section)
Add topic