SCALE LIMITS for Contact Interactions: $\Lambda\mathrm {({{\mathit \mu}} {{\mathit \mu}} {{\mathit q}} {{\mathit q}})}$

INSPIRE   JSON  (beta) PDGID:
S054CTS
$\Lambda_{LL}^+({\mathrm {TeV}}$) $\Lambda_{LL}^-({\mathrm {TeV}}$) CL% DOCUMENT ID TECN  COMMENT
$ \bf{>23.3} $ >40.0 95 1
SIRUNYAN
2021N
 CMS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$)
• • We do not use the following data for averages, fits, limits, etc. • •
$ > 8.5 $ > 8.5 95 2
AAD
2021AU
 ATLS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit b}}{{\mathit s}}$)
$ > 22.3 $ > 32.7 95 3
AAD
2021Q
 ATLS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$)
$ >22.3 $ >32.7 95 4
AAD
2020AP
 ATLS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$)
$ >20.4 $ > 30.4 95 5
SIRUNYAN
2019AC
 CMS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$)
$ >20 $ > 30 95 6
AABOUD
2017AT
 ATLS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$)
$ >15.8 $ >21.8 95 7
AABOUD
2016U
 ATLS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$)
$ > 12.0 $ >15.2 95 8
KHACHATRYAN
2015AE
 CMS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$)
$ > 12.5 $ > 16.7 95 9
AAD
2014BE
 ATLS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$)
$ > 9.6 $ > 12.9 95 10
AAD
2013E
 ATLS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$) (isosinglet)
$ > 9.5 $ > 13.1 95 11
CHATRCHYAN
2013K
 CMS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$) (isosinglet)
$ > 8.0 $ > 7.0 95 12
AAD
2012AB
 ATLS (${{\mathit \mu}}{{\mathit \mu}}{{\mathit q}}{{\mathit q}}$) (isosinglet)
1  SIRUNYAN 2021N limits are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV.
2  AAD 2021AU search for new phenomena in final states with ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ and one or no ${{\mathit b}}$-tagged jets in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limits assume ${{\mathit g}_{{{*}}}^{2}}$ = 4 $\pi $.
3  AAD 2021Q limits are from ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. A frequentist statistical framework is used to remove the prior dependence.
4  AAD 2020AP limits are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV.
5  SIRUNYAN 2019AC limits are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV.
6  AABOUD 2017AT limits are from ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit uses a uniform positive prior in 1/${{\mathit \Lambda}^{2}}$.
7  AABOUD 2016U limits are from ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit uses a uniform positive prior in 1/${{\mathit \Lambda}^{2}}$.
8  KHACHATRYAN 2015AE limit is from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV.
9  AAD 2014BE limits are from ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The quoted limit uses a uniform positive prior in 1/${{\mathit \Lambda}^{2}}$.
10  AAD 2013E limis are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV.
11  CHATRCHYAN 2013K limis are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV.
12  AAD 2012AB limis are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV.
References