Difference between revisions of "Simulating Particle Trajectories"
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(New page: This article discusses numerical simulations of particle trajectories in the "silver" permanent magnet. '''Description of Code''' '''Results of parameter space scans''' '''"Ideal" o...) |
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'''Description of Code''' | '''Description of Code''' | ||
+ | The general problem of modeling relativistic particle trajectories in electromagnetic fields boils down to solving the following system of six differential equations: | ||
+ | <math>\frac{d\vec{x}}{dt}=\vec{v}=\frac{1}{\gamma m_0}\vec{p}</math> | ||
+ | <math>\frac{d\vec{p}}{dt}=q\left(\vec{E}+\frac{1}{\gamma m_0}\vec{p}\times\vec{B}\right)</math> | ||
+ | where <math>\vec{x}<\math> is the position of the particle, <math>\vec{p}</math> is the momentum of the particle, <math>m_0</math> is the rest energy of the particle, and <math>\gamma</math> is the usual relativistic factor. | ||
+ | subject to the appropriate boundary conditions. | ||
'''Results of parameter space scans''' | '''Results of parameter space scans''' |
Revision as of 19:21, 10 June 2009
This article discusses numerical simulations of particle trajectories in the "silver" permanent magnet.
Description of Code
The general problem of modeling relativistic particle trajectories in electromagnetic fields boils down to solving the following system of six differential equations:
where is the momentum of the particle, is the rest energy of the particle, and is the usual relativistic factor.subject to the appropriate boundary conditions.
Results of parameter space scans
"Ideal" orientation of magnet for 5 MeV photons
Pairs produced elsewhere on the beam