Changes between Version 2 and Version 3 of pNG


Ignore:
Timestamp:
Dec 2, 2019, 2:22:18 AM (5 years ago)
Author:
Ankit Beniwal
Comment:

Added summary of the model files.

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  • pNG

    v2 v3  
    1 == pNG dark matter model ==
    2 === Author ===
     1== pseudo-Nambu-Goldstone (pNG) Dark Matter ==
    32
    4 Céline Degrande
     3pseudo-Nambu-Goldstone (pNG) dark matter in a complex scalar singlet model with a softly broken global U(1) symmetry.
    54
    6    * IPPP,Durham University
    7    * celine.degrande@durham.ac.uk
    8 
    9 Gauthier Durieux
    10 
    11    * UCL
    12    * ‎gauthier.durieux@uclouvain.be]
    13 
    14 Fabio Maltoni
    15 
    16    * UCL
    17    * fabio.maltoni@uclouvain.be
    18 
    19 Cen Zhang
    20 
    21    * BNL
    22    * cenzhang@bnl.gov
    23 
    24 
    25 
    26 === Description of the model & reference ===
    27 
    28 The top effective theory model contains the dimension-six operators affecting top flavor changing processes. The UFO model can be used for computation at the NLO in QCD.
    29 
    30 [http://inspirehep.net/record/1334937&FORMAT=WWW&SEQUENCE= Phys.Rev. D91 (2015) 034024]: C. Degrande, F. Maltoni, J. Wang, C. Zhang, ''Automatic computations at next-to-leading order in QCD for top-quark flavor-changing neutral processes''
    31 
    32 [http://inspirehep.net/record/1335409&FORMAT=WWW&SEQUENCE= Phys.Rev. D91 (2015) 074017]: G. Durieux, F. Maltoni, C. Zhang, ''Global approach to top-quark flavor-changing interactions''
     5Reference: C. Arina, A. Beniwal, C. Degrande, J. Heisig and A. Scaffidi, ''Global fit of pseudo-Nambu-Goldstone Dark Matter'', 2019.
    336
    347=== Model files ===
    358
    36 The UFO ([/attachment/wiki/TopFCNC/TopFCNC.tar.gz TopFCNC.tar.gz]) and the FeynRules model ([/attachment/wiki/TopFCNC/TopEFTFCNC.fr TopEFTFCNC.fr]) are available
     9Author: A. Beniwal (CP3, UCLouvain)
     10
     11Model Lagrangian is based on: C. Gross, O. Lebedev and T. Toma, ''Cancellation Mechanism for Dark-Matter–Nucleon Interaction'', Phys. Rev. Lett. 119 (2017) no. 19, 191801, [arXiv:1708.02253]
     12
     13Model files are available here:
     14
     15 * [/attachment/wiki/pNG/SM_with_pNG.fr FeynRules] model file and [/attachment/wiki/pNG/SM_with_pNG.nb Mathematica] notebook
     16 * [/attachment/wiki/pNG/CalcHEP_files.zip CalcHEP files]
     17 * [/attachment/wiki/pNG/UFO_files.zip UFO files]
     18 * [/attachment/wiki/pNG/FeynArts_files.zip FeynArts files]
     19
     20=== Contact details ===
     21
     22For reporting issues/bugs, please contact: A. Beniwal (ankit.beniwal@uclouvain.be).
     23
     24=== Updates ===
     25
     2602/12/2019 : Uploaded model files for the pNG DM.
    3727
    3828
    39 === Update ===
    40 
    41 12/02/2016 : UFO at NLO updated after a fix of the color algebra in NLOCT
    42 
    43