Changes between Version 3 and Version 4 of DMsimp
- Timestamp:
- Jun 11, 2015, 10:56:10 PM (9 years ago)
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DMsimp
v3 v4 3 3 === Authors === 4 4 * s-channel 5 * Antony Martini (Université catholique de Louvain) 6 * Emails: antony.martini @ uclouvain.be 5 7 * Kentarou Mawatari (Vrije Universiteit Brussel) 6 8 * Emails: kentarou.mawatari @ vub.ac.be 7 * Antony Martini (Université catholique de Louvain)8 * Emails: antony.martini @ uclouvain.be9 * Electro-weak10 * 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) 11 13 * Emails: cenzhang @ bnl.gov 12 14 13 15 === Description of the model === 14 16 15 This is simplified dark matter models .17 This is simplified dark matter models for NLO. 16 18 Our effective lagrangian consists of different types of DM: 17 19 … … 36 38 37 39 * [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 39 41 40 42 === Version updates ===