LHC SUSY Cross Section Working Group
- Contributors: Christoph Borschensky, Zoltan Gecse, Michael Kraemer, Robin van der Leeuw, Anna Kulesza, Michelangelo Mangano, Sanjay Padhi, Tilman Plehn, Xavier Portell, Sezen Sekmen
- Mailing list: lhc-susy-cross-section-wg@cernNOSPAMch
, archive
.
- The cross-section values from these TWiki pages are available in JSON format in this public git repository on github
. (So far it only contains the 13 TeV cross sections.)
SUSY Cross Sections for 13, 14, 33 and 100 TeV pp Collisions
Abstract
We summarise the status of the cross section predictions for various supersymmetric processes in pp
collisions at sqrt(s)=13, 14, 33 and 100 TeV. This document is based on the agreement between the ATLAS and CMS
collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever
available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These
cross sections and their uncertainties are provided for various scale and PDF choices.
Documentation
Colored Sector
- NLO + NLL Tool for 13
, 14
, 33
and 100
TeV cross sections.
- Squark and gluino production cross sections in pp collisions at \sqrt(s) = 13, 14, 33 and 100 TeV
, C. Borschensky, M. Kramer, A. Kulesza, M. Mangano, S. Padhi, T. Plehn, X. Portell, arXiv:1407.5066
, published in Eur.Phys.J. C74 (2014) 12.
Electroweak Sector
NLO+NLL threshold resummed results from Resummino.
For slepton production:
- G. Bozzi, B. Fuks, and M. Klasen, Nucl. Phys. B 777, 157 (2007)
- B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, Eur. Phys. J. C 73, 2480 (2013)
- B. Fuks, M. Klasen, D. R. Lamprea and M. Rothering, JHEP 01 (2014) 168
- J. Fiaschi and M. Klasen, JHEP 03 (2018) 094
- W. Beenakker et al., Phys. Rev. Lett. 83 (1999) 3780, Erratum: Phys. Rev. Lett. 100 (2008) 029901
For gaugino production:
- J. Debove, B. Fuks, and M. Klasen, Nucl. Phys. B 842, 51 (2011)
- B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, JHEP 10 (2012) 081
- B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, Eur. Phys. J. C 73, 2480 (2013)
- J. Fiaschi and M. Klasen, Phys. Rev. D 98 (2018) 055014
- W. Beenakker et al., Phys. Rev. Lett. 83 (1999) 3780, Erratum: Phys. Rev. Lett. 100 (2008) 029901
(The last reference to the paper by W. Beenakker et al. is the reference for the original NLO results.)
Cross sections for various subprocesses - 13 TeV
Colored Sector
Electroweak Sector
Cross-section plots
The following plots show the cross-section values from the TWiki pages above:
The code to make these plots can be found on
github
.
Cross sections for various subprocesses - 14 TeV
Cross sections for various subprocesses - 33 TeV
Cross sections for various subprocesses - 100 TeV
Overview (Strong Production Only)
Reference: Squark and gluino production cross sections in pp collisions at \sqrt(s) = 13, 14, 33 and 100 TeV
, C. Borschensky, M. Kramer, A. Kulesza, M. Mangano, S. Padhi, T. Plehn, X. Portell, arXiv:1407.5066, Published in Eur.Phys.J. C74 (2014) 12
SUSY Cross Sections for 7 TeV pp Collisions
Abstract
We summarise the status of the cross section predictions for various supersymmetric processes in pp
collisions at sqrt(s)=7 TeV. This document is based on the agreement between the ATLAS and CMS
collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever
available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These
cross sections and their uncertainties are provided for various scale and PDF choices.
Cross sections for various subprocesses
Important notice: ATLAS and CMS used the same CMSSM tanbeta grid but the program performing the Renormalisation Group Equations is different (ATLAS is using ISAJET whereas CMS is using SOFTSUSY). These different programs lead to differences in mass at the 7 TeV scale. In particular, for the same starting m0 and m1/2 combination, the sparticle masses used in ATLAS are usually slightly higher than the ones used in CMS case. This effect has two effects which partially cancel each other: on the one hand, CMS cross sections are higher than those of ATLAS but, on the other hand, ATLAS scenarios tend to have slightly harder jet pT spectrum, leading to a slightly higher acceptance in most of the analyses. The
SUSY Working Groups of the two collaborations agreed to use the same generator for analyses using 8 TeV centre-of-mass energy.
Documentation
SUSY Cross Sections for 8 TeV pp Collisions
Abstract
We summarise the status of the cross section predictions for various supersymmetric processes in pp
collisions at sqrt(s)=8 TeV. This document is based on the agreement between the ATLAS and CMS
collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
the resummation of soft gluon emission at the next-to-leading logarithmic accuracy are used whenever
available. In all other cases we rely on the next-to-leading order in the strong coupling constant. These
cross sections and their uncertainties are provided for various scale and PDF choices.
Documentation
Cross sections for various subprocesses
The cross sections for the associated production of mass degenerate chargino1 and neutralino2 calculated by ATLAS and by CMS differ due to the non-zero higgsino component assumed in the ATLAS model.