Difference between revisions of "RDYNLAB"

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(New page: This is a library for modeling '''R'''elativistic '''DYN'''amics in the '''LAB'' frame. It uses an eigth order Runge-Kutta algorithm to solve the relativistic dynamical equations for parti...)
 
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This is a library for modeling '''R'''elativistic '''DYN'''amics in the '''LAB'' frame. It uses an eigth order Runge-Kutta algorithm to solve the relativistic dynamical equations for particle motion, including radiative power losses for charged particles, as described in [[Simulating Particle Trajectories|this page]].
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This is a library for modeling Relativistic DYNamics in the LAB frame. It uses an eigth order Runge-Kutta algorithm to solve the relativistic dynamical equations for particle motion, including radiative power losses for charged particles, as described in [[Simulating Particle Trajectories|this page]].
  
 
I am unable to post code to the wiki, so I have copied and pasted it all here. You will need all of these files in order to compile the code. GSL must be installed before you can compile this library.
 
I am unable to post code to the wiki, so I have copied and pasted it all here. You will need all of these files in order to compile the code. GSL must be installed before you can compile this library.

Revision as of 22:35, 17 June 2009

This is a library for modeling Relativistic DYNamics in the LAB frame. It uses an eigth order Runge-Kutta algorithm to solve the relativistic dynamical equations for particle motion, including radiative power losses for charged particles, as described in this page.

I am unable to post code to the wiki, so I have copied and pasted it all here. You will need all of these files in order to compile the code. GSL must be installed before you can compile this library.

The code can be compiled into a shared object library using the autoconf, automake, and libtool tools. Optionally, you could just compile these source files into other programs.

Return to Simulating Particle Trajectories