Changes between Version 102 and Version 103 of SMEFT
- Timestamp:
- Jan 1, 2021, 6:18:59 PM (4 years ago)
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SMEFT
v102 v103 11 11 ''NBIA and Discovery Center, Niels Bohr Institute, University of Copenhagen'' 12 12 13 14 == References == 15 16 * I. Brivio, Y. Jiang and M. Trott, ''The SMEFTsim package, theory and tools'', JHEP **1712** (2017) 070 [https://arxiv.org/abs/1709.06492/ arXiv:1709.06492] 17 18 * I. Brivio, "SMEFTsim 3.0 -- a practical guide". [https://arxiv.org/abs/2012.11343 arXiv:2012.11343] 19 13 20 ---- 14 21 … … 21 28 22 29 23 The SMEFTsim package provides implementations for 3different flavor symmetry assumptions and 2 input scheme choices.30 The SMEFTsim package provides implementations for 5 different flavor symmetry assumptions and 2 input scheme choices. 24 31 25 The flavor symmetry assumptions adopted are (see [https://arxiv.org/abs/ 1709.06492/ arXiv:1709.06492] for a detailed description)32 The flavor symmetry assumptions adopted are (see [https://arxiv.org/abs/2012.11343 arxiv:2012.11343] for a detailed description) 26 33 * The flavour general case 27 34 * The U(3)^5^ flavor symmetric case, with non-SM CP-violating phases 28 35 * A linear Minimal flavor violation (MFV) ansatz [https://arxiv.org/abs/hep-ph/0207036/ arXiv:0207036], in which non-SM CP-violating effects are neglected, but linear flavor-violating spurion insertions are allowed in quark currents 36 * A case with a U(2)^3^ symmetry in the quark sector and U(1)^3^ symmetry in the lepton sector, following the baseline recommendations of [http://arxiv.org/abs/1802.07237 arXiv:1802.07237] for top quark physics 37 * A case with a U(2)^3^ symmetry in the quark sector and a U(3)^2^ symmetry in the lepton sector. 29 38 30 39 For each model it is free to choose between two input parameters sets for the electroweak sector, namely: … … 32 41 * m,,W,, scheme: {m,,W,,, m,,Z,, , G,,f,,} 33 42 34 Importantly, field rotations required to have canonically normalized kinetic terms and parameter redefinitions following from the choice of an input parameters set are automatically applied in the Lagrangian. 43 Field rotations required to have canonically normalized kinetic terms and parameter redefinitions following from the choice of an input parameters set are automatically applied in the Lagrangian. 44 Pre-exported UFO files to be interfaced with MadGraph5_aMC@NLO can be downloaded from this page. 35 45 36 Two independent models sets (A and B) are supplied. Each set contains a main file, a number of subroutines and restriction files.37 The two sets differ in the structure and in the technical implementation of L^(6)^, but they produce consistent results. The use of both sets is recommended for debugging and validation of the numerical results.[[BR]]38 Pre-exported UFO files to be interfaced with MadGraph5_aMC@NLO can also be downloaded from this page (see Table below).39 40 41 We would appreciate if you could report to us any inconsistency or bugs.42 46 43 47 … … 52 56 53 57 58 Numerical files in the WCxf format ([https://arxiv.org/abs/1712.05298 arXiv:1712.05298], https://wcxf.github.io) can be translated into a param_card for SMEFTsim using the dedicated command-line script now available in the WCxf package. 54 59 55 Numerical files in the WCxf format (https://wcxf.github.io) can be translated into a param_card for SMEFTsim using the dedicated command-line script now available in the WCxf package. 60 61 62 == Latest release == 63 64 SMEFTsim version 3 has been released in December 2020. 65 The source code and UFO models are currently hosted on https://github.com/SMEFTsim/SMEFTsim. 66 The complete documentation and release notes can be found on the website https://smeftsim.github.io/ 67 68 A copy of the latest version of the UFO models is made available on this page, as part of the FeynRules database. 69 70 For questions, bug reports and feature requests, please submit a GitHub issue at https://github.com/SMEFTsim/SMEFTsim/issues 71 72 73 74 A detailed list of changes made in v3.0 is provided in the associated scientific publication. The main updates are: 75 76 - two new flavor assumptions have been added, called top and topU3l, that follow the recommendations for the study of top quark processes. 77 - a new feature has been implemented, that allows the inclusion of linearized SMEFT corrections in the propagators of the W,Z,h bosons and of the top quark. 78 - the description of the SM Higgs-gluon vertices in the heavy-top EFT has been substantially improved with a full matching up to d=7. 79 - the parameterization of Wilson coefficients has been moved from Abs/Ph to Re/Im. 80 - all interaction vertices are included in the UFO models. 81 - more interaction orders have been added to the UFO models, in order to provide more control on each class of EFT contributions. 82 83 84 85 ---- 86 87 == Older releases == 88 89 Up to version v2.1, two independent models sets (A and B) were supplied. 90 91 Each set contains a main file, a number of subroutines and restriction files. 92 The two sets differ in the structure and in the technical implementation of L^(6)^, but they produce consistent results. The use of both sets was recommended for debugging and validation of the numerical results.[[BR]] 93 94 Starting from version v3.0 only one set of models is provided, based on the older set A. 95 56 96 57 97 58 98 '''Related bugs and threads''' 59 99 60 The most recent version ofSMEFTsim requires MadGraph5_aMC@NLO v2.6.1. [[BR]]100 SMEFTsim requires MadGraph5_aMC@NLO v2.6.1. [[BR]] 61 101 If still experiencing errors, please refer to the following threads or contact us. 62 102 … … 66 106 67 107 108 '''Change log''' 68 109 69 == Change log ==70 110 71 111 '' Note that the version number adopted in two model Sets is independent.'' 72 112 73 113 ''' 74 NEW v3.0''' (22.12.2020) download from https://github.com/SMEFTsim75 114 76 115 set A - v2.1 (14.12.2018) … … 110 149 111 150 112 == References ==113 114 * I. Brivio, Y. Jiang and M. Trott, ''The SMEFTsim package, theory and tools'', JHEP **1712** (2017) 070 [https://arxiv.org/abs/1709.06492/ arXiv:1709.06492]115 116 * J. Aebischer, I. Brivio, A. Celis, J. Evans, Y. Jiang, J. Kumar, X. Pan, W. Porod, J. Rosiek, D. Shih, F. Staub, D. Straub, D. Dyk, A. Vicente, ''WCxf: an exchange format for Wilson coefficients beyond the Standard Model'', arXiv:1712.05298117 118 151 ---- 119 152 120 '''Model Set A''' 153 ''' FeynRules source code''' 154 155 ''Model Set A'' 121 156 122 157 * [attachment:"SMEFTsim-setA-v2.1.tar.gz"] This archive contains all the FeynRules files. 123 158 * [attachment:"SMEFTsim-setA.nb"] Example of a Mathematica® notebook loading the model 124 159 125 '' 'Model Set B''160 ''Model Set B'' 126 161 127 162 In the master code two flags are established: __Scheme__ and __Flavor__, which are used to identify the input scheme and flavor assumption being adopted in loading the model. … … 132 167 ---- 133 168 134 == Pre-exported UFO files (include restriction cards) == 169 '''Pre-exported UFO files (include restriction cards)''' 135 170 136 171 || || Set A || || Set B (v 1.3)|| ||