Changes between Version 22 and Version 23 of DMsimp


Ignore:
Timestamp:
08/11/15 17:12:47 (5 years ago)
Author:
amartini
Comment:

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  • DMsimp

    v22 v23  
    1 == Simplified dark matter models ==
    2 
    3 === Authors ===
     1= Simplified dark matter models =
     2
     3== Authors ==
    44 * s-channel
    55   * Antony Martini (Université catholique de Louvain) & Kentarou Mawatari (Vrije Universiteit Brussel)
     
    99      * Emails: cenzhang @ bnl.gov
    1010
    11 === Description of the model ===
     11== Description of the model ==
    1212
    1313This is simplified dark matter models for NLO.
     
    3232One can find the model lagrangian in the [http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/DMsimp/note.pdf note].
    3333
     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===
     43Remember that "scalar" below means scalar/pseudoscalar and "vector" means vector/axial-vector.
     44
     45* NLO vector mediator + jets [[BR]]
     46
     47{{{
     48import model DMsimp_s_spin1
     49generate p p > xd xd~ j [QCD]
     50generate 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{{{
     58import model DMsimp_s_spin0
     59generate p p > xd xd~ t t~ [QCD]
     60}}}
     61
     62
     63----
     64== '''Alpha version''' ==
    3465=== Model files ===
    3566