Note. This is an old backup copy of the darksusy web page. Please go to the current darksusy webpage.
DarkSUSY is a flexible and modular Fortran package to calculate observables for a variety of dark matter candidates. It is written by Joakim Edsjö, Torsten Bringmann, Paolo Gondolo, Piero Ullio, Lars Bergström, Mia Schelke, Ted Baltz, and Gintaras Duda. On these pages you will find information about DarkSUSY and you can also download the package.
Finally, DarkSUSY 6 has arrived with a completely new structure and the possibility to add new particle physics modules!
If you use DarkSUSY, please refer to the following publication describing DarkSUSY:
T. Bringmann, J. Edsjö, P. Gondolo, P. Ullio and L. Bergström,
Please also cite (for code up to release version 4.1 contained in later versions)
P. Gondolo, J. Edsjö, P. Ullio, L. Bergström, M. Schelke and E.A. Baltz,
JCAP 07 (2004) 008 [astro-ph/0406204]
as well as this web page as
J. Edsjö, T. Bringmann, P. Gondolo, P. Ullio, L. Bergström, M. Schelke, E.A. Baltz and G. Duda, http://www.darksusy.org.
Note. You should also refer to the original physics work on which DarkSUSY is based and which DarkSUSY uses. Most notably, DarkSUSY is interfaced (and uses) the following codes (for the MSSM module):
A new version, 6.1.0, is available as of 2018-06-13. Click on the download button at the left to get to the download page.
If you have questions, please send an e-mail to one of the DarkSUSY authors.
If you have questions about some specific part of DarkSUSY you will find whom
to contact in the header of each routine.