Changes between Version 22 and Version 23 of DMsimp
- Timestamp:
- Aug 11, 2015, 5:12:47 PM (9 years ago)
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DMsimp
v22 v23 1 = = Simplified dark matter models ==2 3 == = Authors ===1 = Simplified dark matter models = 2 3 == Authors == 4 4 * s-channel 5 5 * Antony Martini (Université catholique de Louvain) & Kentarou Mawatari (Vrije Universiteit Brussel) … … 9 9 * Emails: cenzhang @ bnl.gov 10 10 11 == = Description of the model ===11 == Description of the model == 12 12 13 13 This is simplified dark matter models for NLO. … … 32 32 One can find the model lagrangian in the [http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/DMsimp/note.pdf note]. 33 33 34 ---- 35 36 == '''Beta version'''== 37 38 === Model files === 39 * TBD : the s-channel model files in UFO format 40 * TO BE DONE: include the s-channel+EW model files in UFO format 41 42 === NLO process samples for s-channel mediators=== 43 Remember that "scalar" below means scalar/pseudoscalar and "vector" means vector/axial-vector. 44 45 * NLO vector mediator + jets [[BR]] 46 47 {{{ 48 import model DMsimp_s_spin1 49 generate p p > xd xd~ j [QCD] 50 generate p p > xd xd~ j j [QCD] 51 52 {{{ 53 54 * NLO ttbar associated production with a scalar mediator coupling only to tops[[BR]] 55 56 57 {{{ 58 import model DMsimp_s_spin0 59 generate p p > xd xd~ t t~ [QCD] 60 }}} 61 62 63 ---- 64 == '''Alpha version''' == 34 65 === Model files === 35 66