= Simplified dark matter models = == Authors == * s-channel * Antony Martini (Université catholique de Louvain) & Kentarou Mawatari (Vrije Universiteit Brussel) * Emails: kentarou.mawatari @ vub.ac.be * electroweak * Jian Wang (Johnnas Gutenberg University of Mainz) & Cen Zhang (Brookhaven National Laboratory) * Emails: cenzhang @ bnl.gov == Description of the model == This is simplified dark matter models for NLO. Our lagrangian consists of different types of DM: * Xr (real scalar DM) * Xc (complex scalar DM) * Xd (Dirac spinor DM) * Xm (Majorana spinor DM) (to be done.) * ... and different types of mediators: * s-channel * Y0 (spin-0) * Y1 (spin-1) * Y2 (spin-2) (to be done.) * ... * t-channel (to be done.) One can find the model lagrangian in the [http://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/DMsimp/note.pdf note]. == '''Alpha version''' == [https://feynrules.irmp.ucl.ac.be/wiki/DMsimp_alpha] == '''Beta version'''== === Model files === * TBD : the s-channel model files in UFO format * TO BE DONE: include the s-channel+EW model files in UFO format === NLO QCD process samples for s-channel mediators=== Remember that "scalar" below means scalar/pseudoscalar and "vector" means vector/axial-vector. * NLO vector mediator + jets [[BR]] {{{ import model DMsimp_s_spin1 generate p p > xd xd~ j [QCD] generate p p > xd xd~ j j [QCD] }}} * NLO ttbar associated production with a scalar mediator coupling only to tops[[BR]] {{{ import model DMsimp_s_spin0 generate p p > xd xd~ t t~ [QCD] }}} === NLO EW process samples for s-channel mediators=== Remember that "scalar" below means scalar/pseudoscalar and "vector" means vector/axial-vector. * NLO scalar mediator + a,z,w+ [[BR]] {{{ DMsimp_ew_scalar_5f_UFO generate p p > xd xd~ z [QCD] generate p p > xd xd~ a [QCD] generate p p > xd xd~ w+ [QCD] }}} * NLO vector mediator + h[[BR]] {{{ For DMsimp_ew_vector_5f_UFO import model DMsimp_s_spin0 generate p p > xd xd~ h [QCD] }}} === Version updates === *2015.08.20 - v0.1_beta: beta version. [[BR]]