1997
DOI: 10.1016/s0550-3213(97)80027-2
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Squark and gluino production at hadron colliders

Abstract: We h a v e determined the theoretical predictions for the cross-sections of squark and gluino production at p p and pp colliders (Tevatron and LHC) in next-to-leading order of supersymmetric QCD. By reducing the dependence on the renormalization/factorization scale considerably, the theoretically predicted values for the cross-sections are much more stable if these higher-order corrections are implemented. If squarks and gluinos are discovered, this improved stability translates into a reduced error on the mas… Show more

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Cited by 757 publications
(1,008 citation statements)
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References 51 publications
(64 reference statements)
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“…SUSY signal cross sections are calculated to next-toleading order (NLO) in the strong coupling constant using PROSPINO2 [49]. The inclusion of the resummation of soft gluon emission at next-to-leading-logarithmic (NLL) accuracy (NLO þ NLL) [49][50][51][52][53] is performed in the case of strong sparticle pair production.…”
Section: Monte Carlo Simulationsmentioning
confidence: 99%
See 1 more Smart Citation
“…SUSY signal cross sections are calculated to next-toleading order (NLO) in the strong coupling constant using PROSPINO2 [49]. The inclusion of the resummation of soft gluon emission at next-to-leading-logarithmic (NLL) accuracy (NLO þ NLL) [49][50][51][52][53] is performed in the case of strong sparticle pair production.…”
Section: Monte Carlo Simulationsmentioning
confidence: 99%
“…The inclusion of the resummation of soft gluon emission at next-to-leading-logarithmic (NLL) accuracy (NLO þ NLL) [49][50][51][52][53] is performed in the case of strong sparticle pair production. For neutralino, chargino, slepton and sneutrino production, the NLO cross sections used are in agreement with the NLO þ NLL calculation within ∼2% [54][55][56].…”
Section: Monte Carlo Simulationsmentioning
confidence: 99%
“…similar to the ME cut R j,j > 0. 4. By looking at p T,j /p T,ME in generated dijet samples, we checked explicitly that out-of-cone corrections are too small to affect our study significantly.…”
Section: Mssm Searches and Jetsmentioning
confidence: 99%
“…The SUSY production cross sections for a given spectrum can be computed using Prospino 2.0 [60] at next-to-leading order in QCD. With a gluino scale mg ∼ 900 GeV and the spectra of figure 2 and 3, the dominant production cross-sections are σgg ∼ 0.53 − 0.54 pb, σqg ∼ 2.9 − 3.0 pb and σqq ∼ 1.4 − 1.5 pb.…”
Section: Collider Model and Data Generationmentioning
confidence: 99%