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pegasus:overview [25/02/2025 18:59] – [Implemented TMD gluon densities in a proton] lipatovpegasus:overview [25/02/2025 19:11] (current) – [Implemented TMD gluon densities in a proton] lipatov
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 ^ 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'2024 (CCFM)       |  2                       |  4              |  200              |  [[https://arxiv.org/abs/2404.09550|A.V. Lipatov, G.I. Lykasov, M.A. Malyshev]]                 |+| LLM'2024 (CCFM)¹       |  2                       |  4              |  200              |  [[https://arxiv.org/abs/2404.09550|A.V. Lipatov, G.I. Lykasov, M.A. Malyshev]]                 |
 | LLM'2022 (CCFM)       |  2                       |  4              |  200              |  [[https://arxiv.org/abs/2211.03727|A.V. Lipatov, G.I. Lykasov, M.A. Malyshev]]                 | | 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]]                                               |
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 | 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]]                                       |
-| KLSZ'2020 (KMR)       |  1                       |  4              |  143              |  [[https://arxiv.org/abs/1911.01445|A.V. Kotikov, A.V. Lipatov, B.G. Shaikhatdenov, P. Zhang]]  |+| KLSZ'2020 (KMR)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/1804.11152|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]    | | PB NLO set 1          |  2                       |  4              |  118              |  [[https://arxiv.org/abs/1804.11152|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]    |
 | PB NLO set 2          |  2                       |  4              |  118              |  [[https://arxiv.org/abs/1804.11152|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]    | | PB NLO set 2          |  2                       |  4              |  118              |  [[https://arxiv.org/abs/1804.11152|F. Hautmann, H. Jung, A. Lelek, V. Radescu, R. Zlebcik]]    |
  
-*Calculated using the fixed-flavor-number scheme (FFNS)+¹There is no quarks in the CCFM evolution\\ 
 +²Calculated in the Fixed-Flavor-Number Scheme (FFNS)
  
 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
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 [[http://pdg.lbl.gov/|Particle Data Group]]. [[http://pdg.lbl.gov/|Particle Data Group]].
 Any of these parameters can be easily changed using the convenient  Any of these parameters can be easily changed using the convenient 
-built-in Particle Data tool, which is available via main menu (// Edit -> Settings -> Particle data//)+built-in Particle Data tool, which is available via main menu (// Edit -> Particle data//)
 or popup menu or appropriate button on the button panel. or popup menu or appropriate button on the button panel.
  
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 PEGASUS is supplied with a tool to construct event files in the [[https://arxiv.org/abs/hep-ph/0609017|Les Houches Event format]]. This is a widely accepted format to present events, which is compatible with the majority of modern general purpose Monte-Carlo generators. PEGASUS is supplied with a tool to construct event files in the [[https://arxiv.org/abs/hep-ph/0609017|Les Houches Event format]]. This is a widely accepted format to present events, which is compatible with the majority of modern general purpose Monte-Carlo generators.
  
-The Les Houche Event ''*.lhe'' file, generated by the PEGASUS, consists of two main blocks: the first one contains the information about the number of the recorded events, the PDFs used, the colliding hadrons and their energies. Also the total cross section is shown. The second block represents a list of events, including the data on the interacting partons, their 4-momenta and color structure of the event. +The Les Houche Event ''*.lhe'' file, generated by the PEGASUS, consists of two main blocks: the first one contains the information about the number of the recorded events, the TMDs and/or PDFs used, the colliding hadrons and their energies. Also the total cross section is shown. The second block represents a list of events, including the data on the interacting partons, their 4-momenta and color structure of the event. 
 We mention the basic features of the ''*.lhe'' file, generated by PEGASUS: We mention the basic features of the ''*.lhe'' file, generated by PEGASUS:
  
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 We are also grateful to Maria Mikova, Natalia Ovechkina and Anastasia Zotova for their support and help for the design of the program. We are also grateful to Maria Mikova, Natalia Ovechkina and Anastasia Zotova for their support and help for the design of the program.
  
-Contributions to the physics in PEGASUS were provided by Anatoly Kotikov (JINR, Dubna),   +Contributions to the physics in PEGASUS were provided by Anatoly Kotikov (JINR, Dubna) and   
-Gennady Lykasov (JINR, Dubna) and Nizami Abdulov. We thank Vladimir Lyubushkin (JINR, Dubna) and Alsu Bagdatova (LPI, Moscow), who contributed significantly to the functionality and stability of PEGASUS.+Gennady Lykasov (JINR, Dubna). We thank Vladimir Lyubushkin (JINR, Dubna), Andrei Prokhorov (JINR, Dubna) and Alsu Bagdatova (LPI, Moscow), who contributed significantly to the functionality and stability of PEGASUS.
  
 We are especially grateful to Nikolai Zotov, who guided and supervised our first steps in High Energy Physics,  We are especially grateful to Nikolai Zotov, who guided and supervised our first steps in High Energy Physics, 
 who encouraged our progress in k<sub>t</sub>-factorization and whose enthusiasm consolidated our group. Nikolai Zotov passed away on January 2016. Our work is dedicated to his memory. who encouraged our progress in k<sub>t</sub>-factorization and whose enthusiasm consolidated our group. Nikolai Zotov passed away on January 2016. Our work is dedicated to his memory.
  
pegasus/overview.1740509971.txt.gz · Last modified: by lipatov