# Difference: SUSYCrossSections (39 vs. 40)

#### Revision 402019-07-12 - AlexanderMann

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# LHC SUSY Cross Section Working Group

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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.

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• 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.)

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## Overview

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
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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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.
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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
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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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.
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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
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collaborations, as well as with the LPCC SUSY cross section working group. Calculations including
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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.
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### 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

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