Changes between Version 55 and Version 56 of HeavyN


Ignore:
Timestamp:
May 26, 2021, 9:41:24 AM (3 years ago)
Author:
Richard Ruiz
Comment:

Updated entry information

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  • HeavyN

    v55 v56  
    99D. 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] ].
    1010
    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 ====
    1219
    1320* 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.
    1421* 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] ].
    1623
    1724== Model Description ==
    18 === Majorana ===
     25=== Majorana N ===
    1926This 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] ]
    2027{{{
     
    5057The 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.
    5158
    52 === Dirac ===
     59=== Dirac N ===
    5360The 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] ]
    5461{{{
     
    5966}}}
    6067
    61 === vSMEFT ===
     68=== [[span(style=color: #FF0000, '''*New*''' )]] vSMEFT at dimension six ===
    6269In the {{{HeavyN_vSMEFTdim6}}} UFO [ [#Cirigliano 5] ], the {{{HeavyN}}} (Majorana) Lagrangian is extended by the dimension-six EFT operator
    6370{{{
     
    119126 * [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.
    120127
    121 ==== vSMEFT ====
     128==== [[span(style=color: #FF0000, '''*New*''' )]] vSMEFT ====
    122129* [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.
    123130