THEORY

User Tools

Site Tools

Trace:
pegasus:overview

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revisionPrevious revision
Next revision		Previous revision
Next revisionBoth sides next revision
pegasus:overview [02/09/2023 13:10] – lipatovpegasus:overview [02/09/2023 13:39] – lipatov
Line 70: Line 70:
  
 ^ Set      ^  Order of a<sub>s</sub>      ^  N<sub>f</sub>  ^  QCD scale [MeV]  ^  Reference  ^ ^ Set      ^  Order of a<sub>s</sub>      ^  N<sub>f</sub>  ^  QCD scale [MeV]  ^  Reference  ^
 +| LLM'2022 (CCFM)  |  2  |  4  |  200  |  [[https://arxiv.org/abs/2211.03727|A.V. Lipatov, G.I. Lykasov, M.A. Malyshev]]  |
 | A0 (CCFM)  |  1  |  4  |  250  |  [[https://arxiv.org/abs/hep-ph/0411287|H. Jung]]  | | A0 (CCFM)  |  1  |  4  |  250  |  [[https://arxiv.org/abs/hep-ph/0411287|H. Jung]]  |
 | B0 (CCFM)  |  1  |  4  |  250  |  [[https://arxiv.org/abs/hep-ph/0411287|H. Jung]]  | | B0 (CCFM)  |  1  |  4  |  250  |  [[https://arxiv.org/abs/hep-ph/0411287|H. Jung]]  |
 | JH'2013 set 1 (CCFM)  |  2  |  4  |  200  |  [[https://arxiv.org/abs/1312.7875|F. Hautmann, H. Jung]]  | | JH'2013 set 1 (CCFM)  |  2  |  4  |  200  |  [[https://arxiv.org/abs/1312.7875|F. Hautmann, H. Jung]]  |
 | JH'2013 set 2 (CCFM)  |  2  |  4  |  200  |  [[https://arxiv.org/abs/1312.7875|F. Hautmann, H. Jung]]  | | JH'2013 set 2 (CCFM)  |  2  |  4  |  200  |  [[https://arxiv.org/abs/1312.7875|F. Hautmann, H. Jung]]  |
-| KMR (MMHT'2014)  |  1  |  5  |  211  |  [[https://arxiv.org/abs/hep-ph/9911379|M.A. Kimber, A.D. Martin, M.G. Ryskin]] \\ [[https://arxiv.org/abs/hep-ph/0306169|G. Watt, A.D. Martin, M.G. Ryskin]]   | +| KLSZ'2020 (KMR)  |  1  |  4  |  143  |  [[https://arxiv.org/abs/1911.01445|A.V. Kotikov, A.V. Lipatov, B.G. Shaikhatdenov, P. Zhang]]   |
-| KMR (NNPDF3.1)  |  1  |  5  |  167  |  [[https://arxiv.org/abs/hep-ph/9911379|M.A. Kimber, A.D. Martin, M.G. Ryskin]] \\ [[https://arxiv.org/abs/hep-ph/0306169|G. Watt, A.D. Martin, M.G. Ryskin]]   | +
-| KMR (DAS set 1)  |  1  |  4  |  143  |  [[https://arxiv.org/abs/1911.01445|A.V. Kotikov, A.V. Lipatov, B.G. Shaikhatdenov, P. Zhang]]   | +
-| KMR (DAS set 2)  |  1  |  4  |  143  |  [[https://arxiv.org/abs/1911.01445|A.V. Kotikov, A.V. Lipatov, B.G. Shaikhatdenov, P. Zhang]]   |+
 | PB NLO set 1  |  2  |  4  |  118  |  [[https://arxiv.org/abs/1704.01757|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]   | | PB NLO set 1  |  2  |  4  |  118  |  [[https://arxiv.org/abs/1704.01757|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]   |
 | PB NLO set 2  |  2  |  4  |  118  |  [[https://arxiv.org/abs/1704.01757|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]   | | PB NLO set 2  |  2  |  4  |  118  |  [[https://arxiv.org/abs/1704.01757|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]   |
Line 83: Line 81:
 The A0+, A0-, B0+, B0-, JH'2013 set 1(2)+ and JH'2013 set 1(2)- distributions, needed The A0+, A0-, B0+, B0-, JH'2013 set 1(2)+ and JH'2013 set 1(2)- distributions, needed
 to estimate the scale uncertainties of the CCFM-based calculations, are not shown in the Table. to estimate the scale uncertainties of the CCFM-based calculations, are not shown in the Table.
 +
 +Additionally, any other TMD gluon density in a proton could be used: 
 +one just have to upload it from the separate data file (prepared in the standard uPDFEvolve format).
  
 ===== Strong coupling and masses of particles ===== ===== Strong coupling and masses of particles =====
pegasus/overview.txt · Last modified: 15/04/2024 10:14 by lipatov