Changes between Version 35 and Version 36 of DMsimp


Ignore:
Timestamp:
08/24/15 16:53:39 (5 years ago)
Author:
mawatari
Comment:

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  • DMsimp

    v35 v36  
    11= Simplified dark matter models =
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    34== Authors ==
     
    89   * Jian Wang (Johnnas Gutenberg University of Mainz) & Cen Zhang (Brookhaven National Laboratory)
    910      * Emails: cenzhang @ bnl.gov
     11
    1012
    1113== Description of the model ==
     
    3638* [arXiv:1508.05327] : M. Backovic, M. Kramer, F. Maltoni, A. Martini, K. Mawatari, M. Pellen, "Higher-order QCD predictions for dark matter production at the LHC in simplified models with s-channel mediators".
    3739* [arXiv:1508.xxxxx] : M. Neubert, J. Wang, C. Zhang, "".
     40
    3841
    3942== Model files ==
     
    124127
    125128*2015.08.24 - v1.0: release version. [[BR]]
     129
     130
     131-----------------------
     132
     133== Model files for tools for DM relic abundance and DM (in)direct detections ==
     134
     135* [http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/DMsimp/DMsimp_s_spin1_LO_UFO.zip DMsimp_s_spin1_LO_UFO.zip] : The model files in UFO format (for MadDM).
     136* [http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/DMsimp/DMsimp_s_spin0__LO_UFO.zip DMsimp_s_spin0_LO_UFO.zip] : The model files in UFO format (for MadDM).
     137* [http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/DMsimp/DMsimp_s_spin1_LO_CH.zip DMsimp_s_spin1_LO_CH.zip] : The model files in CH format (for MicrOMEGAs).
     138* [http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/DMsimp/DMsimp_s_spin0__LO_CH.zip DMsimp_s_spin0_LO_CH.zip] : The model files in CH format (for MicrOMEGAs).
     139
     140(The model keeps all the quark masses finite, and apply only to tree-level processes.)