Accelerator physics codes

A charged particle accelerator is a complex machine that takes elementary charged particles and accelerates them to very high energies. Accelerator physics is a field of physics encompassing all the aspects required to design and operate the equipment and to understand the resulting dynamics of the charged particles. There are software packages associated with each such domain. There are a large number of such codes. The 1990 edition of the Los Alamos Accelerator Code Group's compendium [1] provides summaries of more than 200 codes. Certain of those codes are still in use today although many are obsolete. Another index of existing and historical accelerator simulation codes is located at [2]

Single particle dynamics codes

For many applications it is sufficient to track a single particle through the relevant electric and magnetic fields. Some such codes include:

Single Particle DynamicsSpin TrackingTaylor MapsCollective EffectsSynchrotron Radiation TrackingExtensibleNotes
Accelerator Toolbox (AT),[3] YesYes[4]NoYesNoYes
ASTRA[5] YesNoNoYesNoYes For space-charge effects evaluation
BDSIM[6] YesNoNoNoNoYes For particle-matter interaction studies.
Beta [7] YesNoNoNoNoNo No longer maintained.
Bmad (contains PTC) [8] YesYesYesYesYesYes Reproduces PTC's unique beam line structures
COSY INFINITY [9] YesYesYesNoNoYes
Elegant [10] YesNoNoYesNoNo
MAD and MAD-X (includes PTC) [11] YesNoNoNoNoNo
OCELOT [12] YesNoNoYesYesYes
OPA [13] YesNoNoNoNoNo
Propaga[14] YesNoNoNoNoYes
PTC[15] YesYesYesNoNoYes
SAD [16] YesNoNoNoNoNo
SAMM [17] YesYesNoNoNoNo
SixTrack [18] YesNoNoNoNoNo Can run on BOINC
TRACY and variants[19] YesNoNoNoNoNo
Zgoubi [20] YesYesNoNoNoNo

Columns

Spin Tracking
Tracking of a particle's spin.
Taylor Maps
Construction of Taylor series maps that can be used for simulating particle motion and also can be used for such things as extracting single particle resonance strengths.
Collective effects
The interactions between the particles in the beam can have important effects on the behavior, control and dynamics. Collective effects take different forms from Intrabeam Scattering (IBS) which is a direct particle-particle interaction to wakefields which are mediated by the vacuum chamber wall of the machine the particles are traveling in. In general, the effect of direct particle-particle interactions is less with higher energy particle beams. At very low energies, space charge has a large effect on a particle beam and thus becomes hard to calculate. The above simulation codes do not handle low energy space charge effects. See below for a list of programs that can handle low energy space charge forces.
Synchrotron radiation tracking
Ability to track the synchrotron radiation (mainly X-rays) produced by the acceleration of charged particles.
Extensible
Object oriented coding to make it relatively easy to extend the capabilities.

Space Charge Codes

The self interaction (e.g. space charge) of the charged particle beam can cause growth of the beam, such as with bunch lengthening, or intrabeam scattering. Additionally, space charge effects may cause instabilities and associated beam loss. Typically the Poisson equation is solved at intervals during the tracking using Particle-in-cell algorithms. Space charge effects lessen at higher energies so at higher energies the space charge effects may be modeled using simpler algorithms that are computationally much faster than the algorithms used at lower energies. Codes that handle low energy space charge effects, including computation of growth values and instability thresholds, include:

At higher energies, space charge effects include Touschek scattering and coherent synchrotron radiation (CSR). Codes that handle higher energy space charge include:

  • Bmad
  • ELEGANT
  • MaryLie
  • SAD

Impedance computation codes

An important class of collective effects may be summarized in terms of the beams response to an "impedance". An important job is thus the computation of this impedance for the machine. Codes for this computation include

Magnet and other hardware-modeling codes

To control the charged particle beam, appropriate electric and magnetic fields must be created. There are software packages to help in the design and understanding of the magnets, RF cavities, and other elements that create these fields. Codes include

Lattice file format and data interchange issues

Given the variety of modelling tasks, there is not one common data format that has developed. For describing the layout of an accelerator and the corresponding elements, one uses a so-called "lattice file". There have been numerous attempts at unifying the lattice file formats used in different codes. One unification attempt is the Accelerator Markup Language, and the Universal Accelerator Parser.[44] Another attempt at a unified approach to accelerator codes is the UAL or Universal Accelerator Library.[45]

The file formats used in MAD may be the most common, with translation routines available to convert to an input form needed for a different code. Associated with the Elegant code is a data format called SDDS, with an associated suite of tools. If one uses a Matlab-based code, such as Accelerator Toolbox, one has available all the tools within Matlab.

Codes in applications of particle accelerators

There are many applications of particle accelerators. For example, two important applications are elementary particle physics and synchrotron radiation production. When performing a modeling task for any accelerator operation, the results of charged particle beam dynamics simulations must feed into the associated application. Thus, for a full simulation, one must include the codes in associated applications. For particle physics, the simulation may be continued in a detector with a code such as Geant4.

For a synchrotron radiation facility, for example, the electron beam produces an x-ray beam that then travels down a beamline before reaching the experiment. Thus, the electron beam modeling software must interface with the x-ray optics modelling software such as SRW,[46] Shadow,[47] McXTrace,[48] or Spectra.[49] Bmad[8] can model both X-rays and charged particle beams. The x-rays are used in an experiment which may be modeled and analyzed with various software, such as the DAWN science platform.[50] OCELOT [51] also includes both synchrotron radiation calculation and x-ray propagation models.

See also

References

  1. Computer Codes for Particle Accelerator Design and Analysis: A Compendium, Second Edition, Helen Stokes Deaven and Kwok Chi Dominic Chen, Los Alamos National Laboratory report number LA-UR-90-1766, 290 pages (1990).
  2. the CERN CARE/HHH website Archived December 13, 2012, at the Wayback Machine.
  3. ATcollab website
  4. See https://github.com/carmignani/festa
  5. ASTRA Homepage
  6. user's guide
  7. 1 2 Bmad home page at cornell.edu
  8. ELEGANT,a Flexible SDDS Compliant Code for Accelerator Simulation software
  9. MAD/MAD-X homepage at cern.ch
  10. OPA website
  11. Propaga GitHub repository
  12. SAD home page at kek.jp
  13. SAMM, another Matlab based tracking code, at liv.ac.uk
  14. SixTrack home page at cern.ch
  15. libtracy at sourceforge.net
  16. Zgoubi home page at sourceforge.net
  17. ASTRA Homepage
  18. TRANFT user's manual, BNL--77074-2006-IR http://www.osti.gov/scitech/biblio/896444
  19. THE MULTIPARTICLE TRACKING CODES SBTRACK AND MBTRACK. R. Nagaoka, PAC '09 paper here
  20. ORBIT home page at ornl.gov
  21. PyORBIT repository
  22. Synergia home page at fnal.gov
  23. "IMPACT homepage at Berkeley Lab". Archived from the original on 2015-04-16. Retrieved 2015-04-09.
  24. OPAL homepage
  25. GPT, General Particle Tracer, at pulsar.nl Archived October 28, 2013, at the Wayback Machine.
  26. VSim at Tech-X
  27. TraceWin at CEA Saclay
  28. PIC solver at cst.com
  29. ABCI home page at kek.jp
  30. 1 2 ACE3P at slac.stanford.gov
  31. CST, Computer Simulation Technology at cst.com
  32. GdfidL, Gitter drueber, fertig ist die Laube at gdfidl.de
  33. T. Weiland, DESY
  34. VSim at Tech-X
  35. COMSOL home page at comsol.com
  36. CST Electromagnetic Studio at cst.com
  37. OPERA at magnet-design-software.com
  38. VSim at Tech-X
  39. Description of AML and UAP at cornell.edu
  40. See references by N. Malitsky and Talman such as this manual from 2002.
  41. SRW home page at esrf.eu
  42. Shadow home page at esrf.eu
  43. McXTrace home page at mcxtrace.org
  44. Spectra home page at riken.go.jp
  45. DAWN science platform website
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.