Simplified dark matter models

Authors

• s-channel
  • Antony Martini (Université catholique de Louvain)
    • Emails: antony.martini @ uclouvain.be
  • Kentarou Mawatari (Vrije Universiteit Brussel)
    • Emails: kentarou.mawatari @ vub.ac.be
• electroweak
  • Jian Wang (Johnnas Gutenberg University of Mainz)
    • Emails: jian.wang @ uni-mainz.de
  • Cen Zhang (Brookhaven National Laboratory)
    • Emails: cenzhang @ bnl.gov

Description of the model

This is simplified dark matter models for NLO. Our lagrangian consists of different types of DM:

• Xr (real scalar DM)
• Xc (complex scalar DM)
• Xd (Dirac spinor DM)
• Xm (Majorana spinor DM) (to be done.)
• ...

and different types of mediators:

• s-channel
  • Y0 (spin-0)
  • Y1 (spin-1)
  • Y2 (spin-2) (to be done.)
  • ...

• t-channel (to be done.)

Model files

• DMsimp_UFO.zip: the s-channel model files in UFO format
• : the s-channel+EW model files in UFO format

Version updates

*2015.06.11 - v0.1_alpha: alpha version.