• • • We do not use the following data for averages, fits, limits, etc. • • • |
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1 |
|
HAWC |
|
|
2 |
|
CMS |
$<0.0008$ |
95 |
3 |
|
ATLS |
|
|
4 |
|
CMS |
$\text{<(0.043 - 0.17)}$ |
95 |
5 |
|
OPAL |
$\text{<(0.05 - 0.8)}$ |
95 |
6 |
|
OPAL |
$\text{<(2.5 - 0.5)}$ |
95 |
7 |
|
OPAL |
$\text{<(1.6 - 0.9)}$ |
95 |
8 |
|
OPAL |
1
ALBERT 2018C search for WIMP annihilation in Sun to long-lived, radiatively decaying mediator; no signal; limits set on $\sigma {}^{SD}$( ${{\mathit \chi}}{{\mathit p}}$ ) assuming long-lived mediator.
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2
KHACHATRYAN 2017D search for new scalar resonance decaying to ${{\mathit Z}}{{\mathit \gamma}}$ with ${{\mathit Z}}$ $\rightarrow$ ${{\mathit e}^{+}}{{\mathit e}^{-}}$ , ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at 8 and 13 TeV; no signal seen.
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3
AAD 2016AI search for excited quarks (EQ) and quantum black holes (QBH) in 3.2 fb${}^{-1}$ at 13 TeV of data; exclude EQ below 4.4 TeV and QBH below 3.8 (6.2) TeV for RS1 (ADD) models. The visible cross section limit was obtained for 5 TeV resonance with ${{\mathit \sigma}_{{G}}}/{{\mathit M}_{{G}}}$ = 2$\%$.
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4
KHACHATRYAN 2016M search for ${{\mathit \gamma}}{{\mathit \gamma}}$ resonance using 19.7 fb${}^{-1}$ at 8 TeV and 3.3 fb${}^{-1}$ at 13 Tev; slight excess at 750 GeV noted; limit set on RS graviton.
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5
ABBIENDI 2000D associated production limit is for ${\mathit m}_{{{\mathit X}^{0}}}$= $90 - 188$ GeV, ${\mathit m}_{{{\mathit Y}^{0}}}$=0 at $\mathit E_{{\mathrm {cm}}}$=189 GeV. See also their Fig.$~$9.
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6
ABBIENDI 2000D pair production limit is for ${\mathit m}_{{{\mathit X}^{0}}}$ = $45 - 94$ GeV, ${\mathit m}_{{{\mathit Y}^{0}}}$=0 at $\mathit E_{{\mathrm {cm}}}$=189 GeV. See also their Fig.$~$12.
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7
ACKERSTAFF 1997B associated production limit is for ${\mathit m}_{{{\mathit X}^{0}}}$ = $80 - 160$ GeV, ${\mathit m}_{{{\mathit Y}^{0}}}$=0 from $10.0~$pb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 161 GeV. See their Fig.$~$3(a).
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8
ACKERSTAFF 1997B pair production limit is for ${\mathit m}_{{{\mathit X}^{0}}}$ = $40 - 80$ GeV, ${\mathit m}_{{{\mathit Y}^{0}}}$=0 from $10.0~$pb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 161 GeV. See their Fig.$~$3(b).
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