Changes between Version 1 and Version 2 of pNG


Ignore:
Timestamp:
11/29/19 15:11:00 (7 months ago)
Author:
degrande
Comment:

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  • pNG

    v1 v2  
    1 pNG dark matter model
     1== pNG dark matter model ==
     2=== Author ===
     3
     4Céline Degrande
     5
     6   * IPPP,Durham University
     7   * celine.degrande@durham.ac.uk
     8
     9Gauthier Durieux
     10
     11   * UCL
     12   * ‎gauthier.durieux@uclouvain.be]
     13
     14Fabio Maltoni
     15
     16   * UCL
     17   * fabio.maltoni@uclouvain.be
     18
     19Cen Zhang
     20
     21   * BNL
     22   * cenzhang@bnl.gov
     23
     24
     25
     26=== Description of the model & reference ===
     27
     28The 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''
     33
     34=== Model files ===
     35
     36The UFO ([/attachment/wiki/TopFCNC/TopFCNC.tar.gz TopFCNC.tar.gz]) and the FeynRules model ([/attachment/wiki/TopFCNC/TopEFTFCNC.fr TopEFTFCNC.fr]) are available
     37
     38
     39=== Update ===
     40
     4112/02/2016 : UFO at NLO updated after a fix of the color algebra in NLOCT
     42
     43