Changes between Version 55 and Version 56 of HeavyN
- Timestamp:
- May 26, 2021, 9:41:24 AM (3 years ago)
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HeavyN
v55 v56 9 9 D. Alva and T. Han [ [#Alva 1] ]; C. Degrande, O. Mattelear, and J. Turner [ [#Degrande 2] ]; S. Pascoli and C. Weiland [ [#Pascoli 3], [#Pascoli2 4] ]; and V. Cirigliano, W. Dekens, J. de Vries, K. Fuyuto, E. Mereghetti [ [#Cirigliano 5] ]. 10 10 11 For detailed instructions and examples on using the HeavyN UFO libraries, see C. Degrande, et al, arXiv:1602.06957 and S. Pascoli, et al, arXiv:1812.08750 . For heavy neutrinos in vSMEFT, see V. Cirigliano, et al, arXiv:2105.11462. 11 12 ==== Usage resources ==== 13 14 * For detailed instructions and examples on using the HeavyN UFO libraries, see C. Degrande, et al, arXiv:1602.06957 and S. Pascoli, et al, arXiv:1812.08750 . 15 * For heavy neutrinos in vSMEFT, see V. Cirigliano, et al, arXiv:2105.11462. 16 * See '''Validation''' section below for additional information 17 18 ==== Citation requests ==== 12 19 13 20 * For studies of heavy Majorana neutrinos, please consider citing [ [#Atre 6] ] for the Lagrangian and [ [#Alva 1], [#Degrande 2] ] for the Majorana FR/UFO files. 14 21 * For studies of heavy Dirac neutrinos, please also consider citing [ [#Pascoli2 4] ]. 15 * For studies of heavy neutrinos in vSMEFT, please consider citing [ [#Cirigliano 5] ].22 * [[span(style=color: #FF0000, '''*New*''' )]] For studies of heavy neutrinos in vSMEFT, please consider citing [ [#Cirigliano 5] ]. 16 23 17 24 == Model Description == 18 === Majorana ===25 === Majorana N === 19 26 This effective/simplified model extends the Standard Model (SM) field content by introducing three right-handed (RH) neutrinos, which are singlets under the SM gauge symmetry (no color, weak isospin, or weak hypercharge charges). Each RH neutrino possesses one RH Majorana mass. After electroweak symmetry breaking, the Lagrangian with three heavy Majorana neutrinos ''N''i (for i=1,2,3) is given by [ [#Atre 6] ] 20 27 {{{ … … 50 57 The lepton number- and flavor-violating interactions of the Lagrangian allow for modeling of the Type I, Inverse, and Linear seesaw mechanisms at both lepton, hadron, and lepto-hadron colliders. 51 58 52 === Dirac ===59 === Dirac N === 53 60 The Dirac variant of the HeavyN model file contains the same interaction Lagrangian as the Majorana case. The heavy Dirac neutrinos' kinetic and mass terms are [ [#Pascoli2 4] ] 54 61 {{{ … … 59 66 }}} 60 67 61 === vSMEFT===68 === [[span(style=color: #FF0000, '''*New*''' )]] vSMEFT at dimension six === 62 69 In the {{{HeavyN_vSMEFTdim6}}} UFO [ [#Cirigliano 5] ], the {{{HeavyN}}} (Majorana) Lagrangian is extended by the dimension-six EFT operator 63 70 {{{ … … 119 126 * [https://feynrules.irmp.ucl.ac.be/attachment/wiki/HeavyN/heavyN_Dirac.fr heavyN_Dirac.fr]: Main model file. Relies on sm.fr (default FR model file) being declared elsewhere. 120 127 121 ==== vSMEFT ====128 ==== [[span(style=color: #FF0000, '''*New*''' )]] vSMEFT ==== 122 129 * [https://feynrules.irmp.ucl.ac.be/raw-attachment/wiki/HeavyN/SM_HeavyN_vSMEFTdim6_NLO.tgz SM_HeavyN_vSMEFTdim6_NLO.tgz]: Standalone NLO UFO folder. Assumes massless bottom quark and tau lepton, diagonal CKM. 123 130