Differences

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

--- pegasus:overview [02/02/2020 16:49] – lipatov
+++ pegasus:overview [16/06/2020 13:56] – lipatov
@@ Line 59: / Line 59: @@
   * From the list of available processes one can select the necessary process and then (optionally) correct the default kinematical restrictions, flux definition, list of requested observables and corresponding binnings etc. This can be done by double clicking on the requested process or via main menu (using //Edit -> Task// option).
-  * For each of the observables one can manually edit the default binning according to own wishes. As another option, the binning can be uploaded immediately from the data file. Several commonly used formats (such as ''.yoda'', ''.yaml'', ''.csv'' or plain data format, compatible with [[http://www.gnuplot.info|Gnuplot]] tool) as provided by [[https://www.hepdata.net|HepData]] repository are supported.
+  * For each of the observables one can manually edit the default binning according to own wishes. As another option, the binning can be uploaded immediately from the data file. Several commonly used formats (such as ''.yoda'', ''.yaml'', ''.csv'' or plain data format, compatible with [[http://www.gnuplot.info|Gnuplot]] tool) as provided by [[https://www.hepdata.net|HEPData]] repository are supported.
   * The user-defined setup for any process (total center-of-mass energy, selected parton densities, kinematical restrictions, binnings etc) can be saved to a configuration file in some internal format (''*.pegasus''). This can be done via the main menu (using //File -> Save// or //File -> Save As// options) or via the popup menu available on right mouse button click or via appropriate button in the button panel. Of course, the configuration file can be loaded and a user-defined setup can be used in further applications. This can be done via main menu (with //File -> Open// option) or via popup menu or via //Open// button on the button panel.
   * Weighted or unweighted events can be generated. This option is available via main menu //Edit -> Settings -> Generated events// or via popup menu.
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   * Conventional (collinear) parton densities in a proton are numbered according to the [[https://lhapdf.hepforge.org|LHAPDF]] scheme, while TMD parton distributions are numbered according to the [[https://tmdlib.hepforge.org|TMDLib]] package.
-The produced ''*.lhe'' file can then be processed with an external program to introduce some peculiar event selection, to include parton showers, to hadronize the final particles, etc. It is found
+The produced ''*.lhe'' file can then be processed with an external program to introduce some peculiar event selection, [[pegasus:showering| to include parton showers, to hadronize the final particles]], etc. It is found
 to be compatible with such Monte Carlo generators as [[http://home.thep.lu.se/Pythia|PYTHIA 8.2]] and [[https://cascade.hepforge.org|CASCADE]].
@@ Line 120: / Line 120: @@
 ===== References =====
-  * A.V. Lipatov, M.A. Malyshev, S.P. Baranov, [[https://arxiv.org/abs/1912.04204|arXiv:1912.04204 [hep-ph] ]]
+  * A.V. Lipatov, M.A. Malyshev, S.P. Baranov, [[https://doi.org/10.1140/epjc/s10052-020-7898-6|Eur. Phys. J. C 80, 330 (2020) ]]
 ===== Acknowledgements ======
@@ Line 130: / Line 130: @@
 We are also grateful to Maria Mikova, Natalia Ovechkina and Anastasia Zotova for their support and help for the design of the program.
-We thank Vladimir Lyubushkin (JINR, Dubna), who contributed to the functionality and stability of PEGASUS.
+Contributions to the physics in PEGASUS were provided by Anatoly Kotikov (JINR, Dubna) and
+Nizami Abdulov (MSU, Moscow). We thank Vladimir Lyubushkin (JINR, Dubna),
+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,
 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.