| $\bf{> 3900}$ |
95 |
1 |
|
ATLS |
| • • • We do not use the following data for averages, fits, limits, etc. • • • |
|
|
2 |
|
RVUE |
| $> 2810$ |
95 |
3 |
|
ATLS |
| $> 1870$ |
95 |
4 |
|
ATLS |
| $> 938$ |
95 |
5 |
|
CDF |
| $> 923$ |
95 |
6 |
|
D0 |
| $> 488$ |
95 |
7 |
|
RVUE |
| $> 877$ |
95 |
6 |
|
CDF |
| $> 904$ |
95 |
8 |
|
CDF |
| $> 427$ |
95 |
9 |
|
RVUE |
| $> 891$ |
95 |
6 |
|
CDF |
| $> 350$ |
95 |
|
|
ALEP |
| $> 360$ |
95 |
10 |
|
DLPH |
| $> 745$ |
|
6 |
|
CDF |
| $> 720$ |
95 |
11 |
|
CDF |
| $>515$ |
95 |
12 |
|
OPAL |
| $>1600$ |
|
13 |
|
COSM |
| $>310$ |
95 |
14 |
|
DLPH |
| $>329$ |
95 |
15 |
|
ALEP |
| $>619$ |
95 |
16 |
|
RVUE |
| $>365$ |
95 |
17 |
|
RVUE |
| $>87$ |
95 |
18 |
|
RVUE |
| $>620$ |
95 |
19 |
|
CDF |
| $>100$ |
95 |
20 |
|
CHM2 |
| $>125$ |
90 |
21 |
|
VNS |
| $\text{[> 820]}$ |
|
22 |
|
COSM |
| $\text{[> 3300]}$ |
|
23 |
|
ASTR |
| $\text{[> 1040]}$ |
|
22 |
|
COSM |
|
1
AABOUD 2017AT search for resonances decaying to ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV.
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2
BOBOVNIKOV 2018 use the ATLAS limits on $\sigma $( ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit Z}^{\,'}})\cdot{}$B( ${{\mathit Z}^{\,'}}$ $\rightarrow$ ${{\mathit W}^{+}}{{\mathit W}^{-}}$) to constrain the ${{\mathit Z}}-{{\mathit Z}^{\,'}}$ mixing parameter $\xi $. See their Fig. 9 for limits in $\mathit M_{{{\mathit Z}^{\,'}}}−\xi $ plane.
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3
AABOUD 2016U search for resonances decaying to ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV.
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4
AAD 2012CC search for resonances decaying to ${{\mathit e}^{+}}{{\mathit e}^{-}}$, ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV.
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5
AALTONEN 2011I search for resonances decaying to ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$ = 1.96 TeV.
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6
ABAZOV 2011A, AALTONEN 2009T, AALTONEN 2007H, and ABULENCIA 2006L search for resonances decaying to ${{\mathit e}^{+}}{{\mathit e}^{-}}$ in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$ = 1.96$~$TeV.
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7
DEL-AGUILA 2010 give 95$\%$ CL limit on the ${{\mathit Z}}-{{\mathit Z}^{\,'}}$ mixing $-0.0023<\theta <$ 0.0027.
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8
AALTONEN 2009V search for resonances decaying to ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$ = 1.96$~$TeV.
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9
ERLER 2009 give 95$\%$ CL limit on the ${{\mathit Z}}-{{\mathit Z}^{\,'}}$ mixing $-0.0047<\theta <$ 0.0021.
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10
ABDALLAH 2006C give 95$\%$ CL limit $\vert \theta \vert <$ 0.0092. See their Fig. 14 for limit contours in the mass-mixing plane.
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11
ABULENCIA 2005A search for resonances decaying to electron or muon pairs in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$ = 1.96 TeV.
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12
ABBIENDI 2004G give 95$\%$ CL limit on ${{\mathit Z}}-{{\mathit Z}^{\,'}}$ mixing $−$0.00447 $<\theta <$0.00331. See their Fig. 20 for the limit contour in the mass-mixing plane. $\sqrt {s }$ = 91 to 207$~$GeV.
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13
BARGER 2003B limit is from the nucleosynthesis bound on the effective number of light neutrino $\delta \mathit N_{{{\mathit \nu}}}<$1. The quark-hadron transition temperature $\mathit T_{\mathit c}$=150 MeV is assumed. The limit with $\mathit T_{\mathit c}$=400 MeV is $>$3300 GeV.
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14
ABREU 2000S give 95$\%$ CL limit on ${{\mathit Z}}-{{\mathit Z}^{\,'}}$ mixing $\vert \theta \vert <0.0024$. See their Fig.$~$6 for the limit contour in the mass-mixing plane. $\sqrt {\mathit s }$=90 to 189 GeV.
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15
BARATE 2000I search for deviations in cross section and asymmetries in ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ fermions at $\sqrt {\mathit s }$=90 to 183 GeV. Assume $\theta $=0. Bounds in the mass-mixing plane are shown in their Figure$~$18.
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16
CHO 2000 use various electroweak data to constrain ${{\mathit Z}^{\,'}}$ models assuming ${\mathit m}_{{{\mathit H}}}$=100 GeV. See Fig.$~$3 for limits in the mass-mixing plane.
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17
ERLER 1999 give 90$\%$ CL limit on the ${{\mathit Z}}-{{\mathit Z}^{\,'}}$ mixing $-0.0062<\theta <0.0011$.
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18
CONRAD 1998 limit is from measurements at CCFR, assuming no ${{\mathit Z}}-{{\mathit Z}^{\,'}}$ mixing.
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19
ABE 1997S find $\sigma\mathrm {({{\mathit Z}^{\,'}})}{\times }B({{\mathit e}^{+}}{{\mathit e}^{-}},{{\mathit \mu}^{+}}{{\mathit \mu}^{-}})<40~$fb for ${\mathit m}_{{{\mathit Z}^{\,'}}}>600$ GeV at $\sqrt {\mathit s }$= 1.8 TeV.
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20
VILAIN 1994B assume ${\mathit m}_{{{\mathit t}}}$ = 150 GeV and $\theta $=0. See Fig.$~$2 for limit contours in the mass-mixing plane.
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21
ABE 1990F use data for $\mathit R$, $\mathit R_{{{\mathit \ell}} {{\mathit \ell}}}$, and $\mathit A_{{{\mathit \ell}} {{\mathit \ell}}}$. ABE 1990F fix ${\mathit m}_{{{\mathit W}}}$ = $80.49$ $\pm0.43$ $\pm0.24$ GeV and ${\mathit m}_{{{\mathit Z}}}$ = $91.13$ $\pm0.03$ GeV.
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22
These authors claim that the nucleosynthesis bound on the effective number of light neutrinos ($\delta \mathit N_{{{\mathit \nu}}}$ $<~$1) constrains ${{\mathit Z}^{\,'}}$ masses if ${{\mathit \nu}_{{{R}}}}$ is light (${ {}\lesssim{} }~$1 MeV).
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23
GRIFOLS 1990 limit holds for ${\mathit m}_{{{\mathit \nu}_{{{R}}}}}{ {}\lesssim{} }~$1 MeV. See also GRIFOLS 1990D, RIZZO 1991.
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