Changes between Version 3 and Version 4 of DMsimp


Ignore:
Timestamp:
06/11/15 22:56:10 (5 years ago)
Author:
mawatari
Comment:

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  • DMsimp

    v3 v4  
    33=== Authors ===
    44 * s-channel
     5   * Antony Martini (Université catholique de Louvain)
     6      * Emails: antony.martini @ uclouvain.be
    57   * Kentarou Mawatari (Vrije Universiteit Brussel)
    68      * Emails: kentarou.mawatari @ vub.ac.be
    7    * Antony Martini (Université catholique de Louvain)
    8       * Emails: antony.martini @ uclouvain.be
    9  * Electro-weak
    10    * Cen Zhang
     9 * electroweak
     10   * Jian Wang (Johnnas Gutenberg University of Mainz)
     11      * Emails: jian.wang @ uni-mainz.de
     12   * Cen Zhang (Brookhaven National Laboratory)
    1113      * Emails: cenzhang @ bnl.gov
    1214
    1315=== Description of the model ===
    1416
    15 This is simplified dark matter models.
     17This is simplified dark matter models for NLO.
    1618Our effective lagrangian consists of different types of DM:
    1719
     
    3638
    3739*  [http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/DMsimp/DMsimp_UFO.zip DMsimp_UFO.zip]: the s-channel model files in UFO format
    38 
     40* :  the s-channel+EW model files in UFO format
    3941
    4042=== Version updates ===