Direct Mass Limits for ${{\mathit H}^{0}}$

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S055H
The mass limits shown below apply to a Higgs boson ${{\mathit H}^{0}}$ with Standard Model couplings whose mass is a priori unknown. These mass limits are compatible with and independent of the observed signal at about 125 GeV. In particular, the symbol ${{\mathit H}^{0}}$ employed below does not in general refer to the observed signal at about 125 GeV.

The cross section times branching ratio limits quoted in the footnotes below are typically given relative to those of a Standard Model Higgs boson of the relevant mass. These limits can be reinterpreted in terms of more general models (e.g.$~$extended Higgs sectors) in which the Higgs couplings to ${{\mathit W}}$, ${{\mathit Z}}$ and fermions are re-scaled from their Standard Model values.

All data that have been superseded by newer results are marked as “not used” or have been removed from this compilation, and are documented in previous editions of this $\mathit Review$ of Particle Physics.

VALUE (GeV) CL% DOCUMENT ID TECN  COMMENT
$\bf{ \text{> 122 and none 128 - 1000}}$
$\mathbf {\text{none } 145 - 1000}$ 95 1
KHACHATRYAN
2015AW
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$ combined
$\text{none 90 - 102, 149 - 172}$ 95 2
AALTONEN
2013L
CDF ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, combined
$\text{none 90 - 109, 149 - 182}$ 95 3
AALTONEN
2013M
TEVA Tevatron combined
$\text{none 90 - 101, 157 - 178}$ 95 4
ABAZOV
2013L
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, combined
$\mathbf {\text{none } 110 - 121.5}, \mathbf {128 - 145}$ 95 5
CHATRCHYAN
2012N
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$ combined
$>114.1$ 95 6
ABDALLAH
2004
DLPH ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit Z}}$
$>112.7$ 95 6
ABBIENDI
2003B
OPAL ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit Z}}$
$\bf{>114.4}$ 95 7, 6
HEISTER
2003D
LEP ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit Z}}$
$>111.5$ 95 6, 8
HEISTER
2002
ALEP ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit Z}}$
$>112.0$ 95 6
ACHARD
2001C
L3 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit Z}}$
• • We do not use the following data for averages, fits, limits, etc. • •
9
AABOUD
2018CJ
ATLS ${{\mathit H}_{{{2}}}^{0}}$ $\rightarrow$ ${{\mathit W}^{+}}{{\mathit W}^{-}}$, ${{\mathit Z}}{{\mathit Z}}$
10
AABOUD
2018CW
ATLS ${{\mathit H}_{{{2}}}^{0}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit H}^{0}}$
$\text{none 132 - 200}$ 95 11
AAD
2015AA
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
12
AAD
2015G
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$
13
AAD
2014AS
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \mu}}{{\mathit \mu}}$
14
AAD
2014J
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit \gamma}}$
$\text{none 114.5 - 119, 129.5 - 832}$ 95 15
CHATRCHYAN
2014AA
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ 4 ${{\mathit \ell}}$
16
CHATRCHYAN
2014AI
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$
$\text{none 127 - 600}$ 95 17
CHATRCHYAN
2014G
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
18
AALTONEN
2013B
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$
19
AALTONEN
2013C
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$
$\text{none }$ 95 20
AALTONEN
2013K
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
21
ABAZOV
2013E
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, 4${{\mathit \ell}}$
22
ABAZOV
2013F
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit \ell}}{{\mathit \tau}}{{\mathit j}}{{\mathit j}}$
$\text{none 159 - 176}$ 95 23
ABAZOV
2013G
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
24
ABAZOV
2013H
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$
25
ABAZOV
2013I
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit \ell}}{{\mathit \nu}}{{\mathit j}}{{\mathit j}}$
26
ABAZOV
2013J
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, leptonic
27
ABAZOV
2013K
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit Z}}{{\mathit X}}$
28
CHATRCHYAN
2013AL
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \tau}}$, ${{\mathit W}}{{\mathit W}^{(*)}}$, ${{\mathit Z}}{{\mathit Z}^{(*)}}$
29
CHATRCHYAN
2013BK
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit \gamma}}$
$\text{none 145 - 710}$ 95 30
CHATRCHYAN
2013Q
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$ combined
31
CHATRCHYAN
2013X
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit t}}{{\overline{\mathit t}}}{{\mathit X}}$
$\text{none 113 - 122, 128 - 133, 138 - 149}$ 95 32
CHATRCHYAN
2013Y
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$
$\text{none 130 - 164, 170 - 180}$ 95 33
CHATRCHYAN
2013Y
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{*}}$
$\text{none 129 - 160}$ 95 34
CHATRCHYAN
2013Y
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{*}}$
$\text{none 111 - 122, 131 - 559}$ 95 35
AAD
2012AI
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$ combined
$\text{none 133 - 261}$ 95 36
AAD
2012AJ
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
37
AAD
2012BU
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$
$\text{none 319 - 558}$ 95 38
AAD
2012BZ
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$
$\text{none 300 - 322, 353 - 410}$ 95 39
AAD
2012CA
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$
40
AAD
2012CN
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$
41
AAD
2012CO
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}}$
$\text{none 134 - 156, 182 - 233, 256 - 265, 268 - 415}$ 95 42
AAD
2012D
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$
$\text{none 113 - 115, 134.5 - 136}$ 95 43
AAD
2012G
ATLS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$
44
AALTONEN
2012AK
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit t}}{{\overline{\mathit t}}}{{\mathit X}}$
45
AALTONEN
2012AM
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, inclusive 4${{\mathit \ell}}$
46
AALTONEN
2012AN
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$
47
AALTONEN
2012J
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \tau}}$
48
AALTONEN
2012Q
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit Z}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$
$\text{none 100 - 106}$ 95 49
AALTONEN
2012T
TEVA ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$
50
ABAZOV
2012K
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$
51, 52
CHATRCHYAN
2012AY
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}{{\mathit X}}$, ${{\mathit H}^{0}}{{\mathit Z}}{{\mathit X}}$
53
CHATRCHYAN
2012C
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$
54
CHATRCHYAN
2012D
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$
$\text{none 129 - 270}$ 95 55
CHATRCHYAN
2012E
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
56
CHATRCHYAN
2012F
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}{{\mathit X}}$, ${{\mathit H}^{0}}{{\mathit Z}}{{\mathit X}}$
$\text{none 128 - 132}$ 95 57
CHATRCHYAN
2012G
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$
$\text{none 134 - 158, 180 - 305, 340 - 465}$ 95 58
CHATRCHYAN
2012H
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$
$\text{none 270 - 440}$ 95 59
CHATRCHYAN
2012I
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$
60
CHATRCHYAN
2012K
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$
61
ABAZOV
2011G
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
62
CHATRCHYAN
2011J
CMS ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}}$
$\text{none 162 - 166}$ 95 63
AALTONEN
2010F
TEVA ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
64
AALTONEN
2010M
TEVA ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit g}}{{\mathit g}}{{\mathit X}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
65
AALTONEN
2009A
CDF ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$
66
ABAZOV
2009U
D0 ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$
67
ABAZOV
2006
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{*}}$
68
ABAZOV
2006O
D0 ${{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit W}}{{\mathit X}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{*}}$
1  KHACHATRYAN 2015AW search for ${{\mathit H}^{0}}$ production in the decays ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}^{+}}{{\mathit W}^{-}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\mathit q}}$, and ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$ $\rightarrow$ 4 ${{\mathit \ell}}$, ${{\mathit \ell}}$ ${{\mathit \ell}}{{\mathit \tau}}{{\mathit \tau}}$, ${{\mathit \ell}}$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \nu}}$, and ${{\mathit \ell}}{{\mathit \ell}}{{\mathit q}}{{\mathit q}}$ in up to 5.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and up to 19.7 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$=8 TeV in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $145 - 1000$ GeV. See their Fig. 7 for limits on cross section times branching ratio.
2  AALTONEN 2013L combine all CDF searches with $9.45 - 10.0$ fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which corresponds to ($0.45 - 4.8$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $90 - 200$ GeV at 95 $\%$CL. An excess of events over background is observed with a local significance of 2.0 $\sigma $ at ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values between 124 and 203 GeV are excluded at 95$\%$ CL.
3  AALTONEN 2013M combine all Tevatron data from the CDF and D0 Collaborations. A limit on cross section times branching ratio which corresponds to ($0.37 - 3.1$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $90 - 200$ GeV at 95$\%$ CL. An excess of events over background is observed with a local significance of 3.0$\sigma $ at ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values between 121 and 225 GeV are excluded at 95$\%$ CL.
4  ABAZOV 2013L combine all D0 results with up to 9.7 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which corresponds to ($0.66 - 3.1$) times the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $90 - 200$ GeV at 95$\%$ CL. An excess of events over background is observed with a local significance of 1.7$\sigma $ at ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values between 125 and 218 GeV are excluded at 95$\%$ CL.
5  CHATRCHYAN 2012N search for ${{\mathit H}^{0}}$ production in the decays ${{\mathit H}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$, ${{\mathit Z}}$ ${{\mathit Z}^{*}}$ $\rightarrow$ 4 ${{\mathit \ell}}$, ${{\mathit W}}$ ${{\mathit W}^{*}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit \tau}}{{\mathit \tau}}$, and ${{\mathit b}}{{\overline{\mathit b}}}$ in $4.9 - 5.1$ fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and $5.1 - 5.3$ fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. The expected exclusion region for no signal is $110 - 145$ GeV at 99.9$\%$ CL. See also CHATRCHYAN 2013Y.
6  Search for ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit H}^{0}}{{\mathit Z}}$ at $\mathit E_{{\mathrm {cm}}}{}\leq{}$209 GeV in the final states ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$ with ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}}{{\overline{\mathit \ell}}}$, ${{\mathit \nu}}{{\overline{\mathit \nu}}}$, ${{\mathit q}}{{\overline{\mathit q}}}$, ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ and ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ with ${{\mathit Z}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$.
7  Combination of the results of all LEP experiments.
8  A 3$\sigma $ excess of candidate events compatible with ${\mathit m}_{{{\mathit H}^{0}}}$ near 114$~$GeV is observed in the combined channels ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit q}}{{\overline{\mathit q}}}$, ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit \ell}}{{\overline{\mathit \ell}}}$, ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$.
9  AABOUD 2018CJ search for production of a narrow scalar resonance by gluon fusion or vector boson fusion, decaying to ${{\mathit W}^{+}}{{\mathit W}^{-}}$ and ${{\mathit Z}}{{\mathit Z}}$ in various final states in 36.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 13 TeV. See their Fig. 5 for limits on cross section times branching ratio for ${\mathit m}_{{{\mathit H}_{{{2}}}^{0}}}$ = $0.3 - 3.0$ TeV.
10  AABOUD 2018CW search for a narrow scalar resonance decaying to ${{\mathit H}^{0}}$ ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}{{\mathit b}}{{\overline{\mathit b}}}$ in 36.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 13 TeV. See their Fig. 7 for limits on cross section times branching ratios for ${\mathit m}_{{{\mathit H}_{{{2}}}^{0}}}$ = $260 - 1000$ GeV.
11  AAD 2015AA search for ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ in 4.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 20.3 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. A limit on cross section times branching ratio which corresponds to ($0.2 - 6$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 200$ GeV at 95$\%$ CL.
12  AAD 2015G search for ${{\mathit W}}{{\mathit H}^{0}}$ and ${{\mathit Z}}{{\mathit H}^{0}}$ production followed by ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$ in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 20.3 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. A limit on the cross section times branching ratio which corresponds to ($0.8 - 2.6$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 140$ GeV at 95$\%$ CL.
13  AAD 2014AS search for ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ in 4.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 20.3 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. A limit on the cross section times branching ratio which corresponds to ($6.5 - 16.8$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $120 - 150$ GeV at 95$\%$ CL.
14  AAD 2014J search for ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit \gamma}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit \gamma}}$ in 4.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 20.3 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. A limit on cross section times branching ratio which corresponds to ($4 - 18$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $120 - 150$ GeV at 95$\%$ CL.
15  CHATRCHYAN 2014AA search for ${{\mathit H}^{0}}$ production in the decay mode ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$ $\rightarrow$ 4 ${{\mathit \ell}}$ in 5.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 19.7 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. The expected exclusion region for no signal is $115 - 740$ GeV at the 95$\%$ CL. See their Fig. 18 for cross section limits for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 1000$ GeV.
16  CHATRCHYAN 2014AI search for ${{\mathit W}}{{\mathit H}^{0}}$ and ${{\mathit Z}}{{\mathit H}^{0}}$ production followed by ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$ in up to 5.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and up to 18.9 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. A limit on the cross section times branching ratio which corresponds to ($1 - 3$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 135$ GeV at 95$\%$ CL.
17  CHATRCHYAN 2014G search for ${{\mathit H}^{0}}$ production in the decay mode ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \ell}}{{\mathit \nu}}$ in 4.9 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 19.4 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. The expected exclusion region for no signal is $115 - 600$ GeV at the 95$\%$ CL. See their Fig. 21 (left) for cross section limits for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 600$ GeV.
18  AALTONEN 2013B search for associated ${{\mathit H}^{0}}{{\mathit Z}}$ production in the final state ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \nu}}{{\overline{\mathit \nu}}}$, and ${{\mathit H}^{0}}{{\mathit W}}$ production in ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$ (${{\mathit \ell}}$ not identified) with an improved ${{\mathit b}}$ identification algorithm in 9.45 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which corresponds to ($0.72 - 11.8$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $90 - 150$ GeV at 95$\%$CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 3.06, where 3.33 is expected for no signal.
19  AALTONEN 2013C search for associated ${{\mathit H}^{0}}{{\mathit W}}$ and ${{\mathit H}^{0}}{{\mathit Z}}$ as well as vector-boson fusion ${{\mathit H}^{0}}{{\mathit q}}{{\overline{\mathit q}}^{\,'}}$ production in the final state ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit W}}$ $/$ ${{\mathit Z}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}$ with 9.45 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which is ($7.0 - 64.6$) times larger than the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 9.0, where 11.0 is expected for no signal.
20  AALTONEN 2013K search for ${{\mathit H}^{0}}$ production (with a possible additional ${{\mathit W}}$ or ${{\mathit Z}}$) in the final state ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \ell}}{{\mathit \nu}}$ in 9.7 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which corresponds to ($0.49 - 14.1$) times the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 200$ GeV at 95$\%$ CL. The limit at ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 3.26, where 3.25 is expected for no signal. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values between 124 and 200 GeV are excluded at 95$\%$ CL.
21  ABAZOV 2013E search for ${{\mathit H}^{0}}$ production in four-lepton final states from ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$ and ${{\mathit H}^{0}}{{\mathit Z}}$ in $9.6 - 9.8$ fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which corresponds to ($8.6 - 78.9$) times the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $115 - 200$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 42.3, where 42.8 is expected for no signal.
22  ABAZOV 2013F search for ${{\mathit H}^{0}}$ production in final states ${{\mathit e}}{{\mathit \tau}}{{\mathit j}}{{\mathit j}}$ and ${{\mathit \mu}}{{\mathit \tau}}$ in 9.7 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. The search is sensitive to ${{\mathit H}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \tau}}$ and ${{\mathit H}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$. A limit on cross section times branching ratio which corresponds to ($9.4 - 17.9$) times the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $105 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 11.3, where 9.0 is expected for no signal.
23  ABAZOV 2013G search for ${{\mathit H}^{0}}$ production in final states ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \nu}}{{\mathit \ell}^{-}}{{\mathit \nu}}$ in 9.7 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV and give a limit on cross section times branching ratio for ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 4.1, where 3.4 is expected for no signal. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values between 125 and 218 GeV are excluded at 95$\%$ CL.
24  ABAZOV 2013H search for ${{\mathit H}^{0}}$ production with the decay ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$ in 9.6 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which corresponds to ($8.3 - 25.4$) times the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 12.8, where 8.7 is expected for no signal.
25  ABAZOV 2013I search for ${{\mathit H}^{0}}$ production in the final state with one lepton and two or more jets plus missing $\mathit E_{T}$ with ${{\mathit b}}$ identification in 9.7 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. The search is mainly sensitive to ${{\mathit H}^{0}}$ ${{\mathit W}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\overline{\mathit q}}}$, and ${{\mathit H}^{0}}$ ${{\mathit V}}$ $\rightarrow$ ${{\mathit V}}{{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\overline{\mathit q}}}{{\mathit q}}{{\overline{\mathit q}}}$ (${{\mathit V}}$ = ${{\mathit W}}$, ${{\mathit Z}}$). A limit on cross section times branching ratio which corresponds to ($1.3 - 11.4$) times the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $90 - 200$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 5.8, where 4.7 is expected for no signal. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values between 150 and 188 GeV are excluded at 95$\%$ CL.
26  ABAZOV 2013J search for ${{\mathit H}^{0}}$ production in the final states ${{\mathit e}}{{\mathit e}}{{\mathit \mu}}$, ${{\mathit e}}{{\mathit \mu}}{{\mathit \mu}}$, ${{\mathit \mu}}{{\mathit \tau}}{{\mathit \tau}}$, and ${{\mathit e}^{\pm}}{{\mathit \mu}^{\pm}}$ in $8.6 - 9.7$ fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. The search is sensitive to ${{\mathit W}}{{\mathit H}^{0}}$, ${{\mathit Z}}{{\mathit H}^{0}}$ and gluon fusion production with ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$, ${{\mathit Z}}{{\mathit Z}^{(*)}}$, decaying to leptonic final states, and to ${{\mathit W}}{{\mathit H}^{0}}$, ${{\mathit Z}}{{\mathit H}^{0}}$ production with ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$. A limit on cross section times branching ratio which corresponds to ($4.4 - 12.7$) times the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 200$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 8.4, where 6.3 is expected for no signal.
27  ABAZOV 2013K search for associated ${{\mathit H}^{0}}{{\mathit Z}}$ production in the final states ${{\mathit \ell}}{{\mathit \ell}}{{\mathit b}}{{\mathit b}}$ with ${{\mathit b}}$ identification in 9.7 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which corresponds to ($1.8 - 53$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $90 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 7.1, where 5.1 is expected for no signal.
28  CHATRCHYAN 2013AL search for ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$, ${{\mathit W}}{{\mathit W}^{(*)}}$, and ${{\mathit Z}}{{\mathit Z}^{(*)}}$ in 5.1 fb${}^{-1}$ and 5.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 and 8 TeV. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values between 110 and 600 GeV are excluded at 99$\%$ CL.
29  CHATRCHYAN 2013BK search for ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit \gamma}}$ $\rightarrow$ ${{\mathit \ell}}$ ${{\mathit \ell}}{{\mathit \gamma}}$ in 5.0 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 19.6 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. A limit on cross section times branching ratio which corresponds to ($4 - 25$) times the expected Standard Model cross section is given in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $120 - 160$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 9.5, where 10 is expected for no signal.
30  CHATRCHYAN 2013Q search for ${{\mathit H}^{0}}$ production in the decays ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}^{+}}{{\mathit W}^{-}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\mathit q}}$ and ${{\mathit H}^{0}}$ $\rightarrow$ $\rightarrow$ 4 ${{\mathit \ell}}$, ${{\mathit \ell}}$ ${{\mathit \ell}}{{\mathit \tau}}{{\mathit \tau}}$, ${{\mathit \ell}}$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \nu}}$, and ${{\mathit \ell}}{{\mathit \ell}}{{\mathit q}}{{\mathit q}}$ in up to 5.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and up to 5.3 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV in the range ${\mathit m}_{{{\mathit H}^{0}}}$ = $145 - 1000$ GeV. Superseded by KHACHATRYAN 2015AW.
31  CHATRCHYAN 2013X search for ${{\mathit H}^{0}}{{\mathit t}}{{\overline{\mathit t}}}$ production followed by ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, one top decaying to ${{\mathit \ell}}{{\mathit \nu}}$ and the other to either ${{\mathit \ell}}{{\mathit \nu}}$ or ${{\mathit q}}{{\overline{\mathit q}}}$ in 5.0 fb${}^{-1}$ and 5.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 and 8 TeV. A limit on cross section times branching ratio which corresponds to ($4.0 - 8.6$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 140$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 5.8, where 5.2 is expected for no signal.
32  CHATRCHYAN 2013Y search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$ in 5.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 5.3 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. The expected exclusion region for no signal is $110 - 144$ GeV at 95$\%$ CL.
33  CHATRCHYAN 2013Y search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{*}}$ $\rightarrow$ 4 ${{\mathit \ell}}$ in 5.0 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 5.3 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. The expected exclusion region for no signal is $120 - 180$ GeV at 95$\%$ CL.
34  CHATRCHYAN 2013Y search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{*}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \ell}}{{\mathit \nu}}$ in 4.9 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV and 5.3 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. The expected exclusion region for no signal is $122 - 160$ GeV at 95$\%$ CL.
35  AAD 2012AI search for ${{\mathit H}^{0}}$ production in ${{\mathit p}}{{\mathit p}}$ collisions for the final states ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$, ${{\mathit \gamma}}{{\mathit \gamma}}$, ${{\mathit W}}{{\mathit W}^{(*)}}$, ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit \tau}}{{\mathit \tau}}$ with 4.6--4.8 fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV, and ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$ $\rightarrow$ 4 ${{\mathit \ell}}$, ${{\mathit \gamma}}{{\mathit \gamma}}$, ${{\mathit W}}$ ${{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit e}}{{\mathit \nu}}{{\mathit \mu}}{{\mathit \nu}}$ with $5.8 - 5.9$ fb${}^{-1}$ at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV. The 99$\%$ CL excluded range is $113 - 114$, $117 - 121$, and $132 - 527$ GeV. An excess of events over background with a local significance of 5.9 $\sigma $ is observed at ${\mathit m}_{{{\mathit H}^{0}}}$ = 126 GeV.
36  AAD 2012AJ search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit \ell}}{{\mathit \nu}}$ with 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which corresponds to ($0.2 - 10$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 600$ GeV at 95$\%$ CL.
37  AAD 2012BU search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ with 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which is ($2.9 - 11.7$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 150$ GeV at 95$\%$ CL.
38  AAD 2012BZ search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}{{\mathit \nu}}{{\overline{\mathit \nu}}}$ with 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which corresponds to (0.2--4) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $200 - 600$ GeV at 95$\%$ CL.
39  AAD 2012CA search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}{{\mathit q}}{{\overline{\mathit q}}}$ with 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which corresponds to (0.7--9) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $200 - 600$ GeV at 95$\%$ CL.
40  AAD 2012CN search for associated ${{\mathit H}^{0}}{{\mathit W}}$ and ${{\mathit H}^{0}}{{\mathit Z}}$ production in the channels ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}$, ${{\mathit \nu}}{{\overline{\mathit \nu}}}$, and ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, with 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which is ($2.5 - 5.5$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 130$ GeV at 95$\%$ CL.
41  AAD 2012CO search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\overline{\mathit q}}}$ with 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which is (1.9--10) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $300 - 600$ GeV at 95$\%$ CL.
42  AAD 2012D search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$ $\rightarrow$ 4 ${{\mathit \ell}}$ in 4.8 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV in the mass range ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 600$ GeV. An excess of events over background with a local significance of 2.1 ${{\mathit \sigma}}$ is observed at 125 GeV.
43  AAD 2012G search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$ in 4.9 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV in the mass range ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 150$ GeV. An excess of events over background with a local significance of 2.8 ${{\mathit \sigma}}$ is observed at 126.5 GeV.
44  AALTONEN 2012AK search for associated ${{\mathit H}^{0}}{{\mathit t}}{{\overline{\mathit t}}}$ production in the decay chain ${{\mathit t}}$ ${{\overline{\mathit t}}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}}{{\mathit b}}{{\mathit b}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\mathit q}}{{\mathit b}}{{\mathit b}}$ with 9.45 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which is ($10 - 40$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 20.5, where 12.6 is expected.
45  AALTONEN 2012AM search for ${{\mathit H}^{0}}$ production in inclusive four-lepton final states coming from ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$, ${{\mathit H}^{0}}$ ${{\mathit Z}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}{{\mathit \ell}}{{\mathit \ell}}$, or ${{\mathit H}^{0}}$ ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \tau}}{{\mathit \ell}}{{\mathit \ell}}$, with 9.7 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which is ($7.2 - 42.4$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $120 - 300$ GeV at 95$\%$ CL. The best limit is for ${\mathit m}_{{{\mathit H}^{0}}}$ = 200 GeV.
46  AALTONEN 2012AN search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$ with 10 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which is (7.7--21.3) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 17.0, where 9.9 is expected.
47  AALTONEN 2012J search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ (one leptonic, the other hadronic) with 6.0 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which is ($14.6 - 70.2$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 150$ GeV at 95$\%$ CL. The best limit is for ${\mathit m}_{{{\mathit H}^{0}}}$ = 120 GeV.
48  AALTONEN 2012Q search for associated ${{\mathit H}^{0}}{{\mathit Z}}$ production in the final state ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}$ with 9.45 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which corresponds to ($1.0 - 37.5$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $90 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 7.1, where 3.9 is expected. A broad excess of events for ${\mathit m}_{{{\mathit H}^{0}}}$ $>$ 110 GeV is observed, with a local significance of 2.4 $\sigma $ at ${\mathit m}_{{{\mathit H}^{0}}}$ = 135 GeV.
49  AALTONEN 2012T combine AALTONEN 2012Q, AALTONEN 2012R, AALTONEN 2012S, ABAZOV 2012O, ABAZOV 2012P, and ABAZOV 2012K. An excess of events over background is observed which is most significant in the region ${\mathit m}_{{{\mathit H}^{0}}}$ = $120 - 135$ GeV, with a local significance of up to 3.3 $\sigma $. The local significance at ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 2.8 $\sigma $, which corresponds to ($\sigma ({{\mathit H}^{0}}{{\mathit W}}$) + $\sigma ({{\mathit H}^{0}}{{\mathit Z}}$)) B(${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$)) = ($0.23$ ${}^{+0.09}_{-0.08}$) pb, compared to the Standard Model expectation at ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV of $0.12$ $\pm0.01$ pb.
50  ABAZOV 2012K search for associated ${{\mathit H}^{0}}{{\mathit Z}}$ production in the final state ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \nu}}{{\overline{\mathit \nu}}}$, and ${{\mathit H}^{0}}{{\mathit W}}$ production with ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$ (${{\mathit \ell}}$ not identified) with 9.5 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. A limit on cross section times branching ratio which is ($1.9 - 16.8$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $100 - 150$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 4.3, where 3.9 is expected.
51  CHATRCHYAN 2012AY search for associated ${{\mathit H}^{0}}{{\mathit W}}$ and ${{\mathit H}^{0}}{{\mathit Z}}$ production in the channels ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}$, and ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}}{{\mathit \tau}}$, ${{\mathit W}}{{\mathit W}^{(*)}}$, with 5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which is ($3.1 - 9.1$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 200$ GeV at 95$\%$ CL.
52  CHATRCHYAN 2012AY combine CHATRCHYAN 2012F and CHATRCHYAN 2012AO in addition and give a limit on cross section times branching ratio which is ($2.1 - 3.7$) times larger than the expected Standard Model cross section for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 170$ GeV at 95$\%$ CL. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 125 GeV is 3.3.
53  CHATRCHYAN 2012C search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}{{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ in 4.7$~$fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which is ($4 - 12$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $190 - 600$ GeV at 95$\%$ CL. The best limit is at ${\mathit m}_{{{\mathit H}^{0}}}$ = 200 GeV.
54  CHATRCHYAN 2012D search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}{{\mathit q}}{{\overline{\mathit q}}}$ in 4.6$~$fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which corresponds to ($1 - 22$) times the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $130 - 164$ GeV, $200 - 600$ GeV at 95$\%$ CL. The best limit is at ${\mathit m}_{{{\mathit H}^{0}}}$ = 230 GeV. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values in the ranges ${\mathit m}_{{{\mathit H}^{0}}}$ = $154 - 161$ GeV and $200 - 470$ GeV are excluded at 95$\%$ CL.
55  CHATRCHYAN 2012E search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \nu}}{{\mathit \ell}^{-}}{{\overline{\mathit \nu}}}$ in 4.6 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV in the mass range ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 600$ GeV.
56  CHATRCHYAN 2012F search for associated ${{\mathit H}^{0}}{{\mathit W}}$ and ${{\mathit H}^{0}}{{\mathit Z}}$ production followed by ${{\mathit W}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}$, ${{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}$, ${{\mathit \nu}}{{\overline{\mathit \nu}}}$, and ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}$, in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which is ($3.1 - 9.0$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 135$ GeV at 95$\%$ CL. The best limit is at ${\mathit m}_{{{\mathit H}^{0}}}$ = 110 GeV.
57  CHATRCHYAN 2012G search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit \gamma}}$ in 4.8 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV in the mass range ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 150$ GeV. An excess of events over background with a local significance of 3.1 ${{\mathit \sigma}}$ is observed at 124 GeV.
58  CHATRCHYAN 2012H search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}^{(*)}}$ $\rightarrow$ 4 ${{\mathit \ell}}$ in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV in the mass range ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 600$ GeV. Excesses of events over background are observed around 119, 126 and 320 GeV. The region ${\mathit m}_{{{\mathit H}^{0}}}$ = $114.4 - 134$ GeV remains consistent with the expectation for the production of a SM-like Higgs boson.
59  CHATRCHYAN 2012I search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit Z}}{{\mathit Z}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}{{\mathit \nu}}{{\overline{\mathit \nu}}}$ in 4.6 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV in the mass range ${\mathit m}_{{{\mathit H}^{0}}}$ = $250 - 600$ GeV.
60  CHATRCHYAN 2012K search for ${{\mathit H}^{0}}$ production in the decay ${{\mathit H}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ with 4.6 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. A limit on cross section times branching ratio which is ($3.2 - 7.0$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 145$ GeV at 95$\%$ CL.
61  ABAZOV 2011G search for ${{\mathit H}^{0}}$ production in 5.4 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV in the decay mode ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \nu}}{{\mathit q}}{{\overline{\mathit q}}^{\,'}}$ (and processes with similar final states). A limit on cross section times branching ratio which is ($3.9 - 37$) times larger than the expected Standard Model cross section is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $115 - 200$ GeV at 95$\%$ CL. The best limit is at ${\mathit m}_{{{\mathit H}^{0}}}$ = 160 GeV.
62  CHATRCHYAN 2011J search for ${{\mathit H}^{0}}$ production with ${{\mathit H}}$ $\rightarrow$ ${{\mathit W}^{+}}{{\mathit W}^{-}}$ $\rightarrow$ ${{\mathit \ell}}{{\mathit \ell}}{{\mathit \nu}}{{\mathit \nu}}$ in 36 pb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV. See their Fig. 6 for a limit on cross section times branching ratio for ${\mathit m}_{{{\mathit H}^{0}}}$ = $120 - 600$ GeV at 95$\%$ CL. In the Standard Model with an additional generation of heavy quarks and leptons which receive their masses via the Higgs mechanism, ${\mathit m}_{{{\mathit H}^{0}}}$ values between 144 and 207 GeV are excluded at 95$\%$ CL.
63  AALTONEN 2010F combine searches for ${{\mathit H}^{0}}$ decaying to ${{\mathit W}^{+}}{{\mathit W}^{-}}$ in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV with 4.8 fb${}^{-1}$ (CDF) and 5.4 fb${}^{-1}$ (${D0}$).
64  AALTONEN 2010M combine searches for ${{\mathit H}^{0}}$ decaying to ${{\mathit W}^{+}}{{\mathit W}^{-}}$ in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV with 4.8 fb${}^{-1}$ (CDF) and 5.4 fb${}^{-1}$ (${D0}$) and derive limits ${\mathit \sigma (}{{\mathit p}}$ ${{\overline{\mathit p}}}$ $\rightarrow$ ${{\mathit H}^{0}}{)}\cdot{}$ B(${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}^{+}}{{\mathit W}^{-}}$) $<$ ($1.75 - 0.38$) pb for ${\mathit m}_{{{\mathit H}}}$ = $120 - 165$ GeV, where ${{\mathit H}^{0}}$ is produced in ${{\mathit g}}{{\mathit g}}$ fusion. In the Standard Model with an additional generation of heavy quarks, ${\mathit m}_{{{\mathit H}^{0}}}$ between 131 and 204 GeV is excluded at 95$\%$ CL.
65  AALTONEN 2009A search for ${{\mathit H}^{0}}$ production in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ =1.96 TeV in the decay mode ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$ $\rightarrow$ ${{\mathit \ell}^{+}}{{\mathit \ell}^{-}}{{\mathit \nu}}{{\overline{\mathit \nu}}}$. A limit on ${\mathit \sigma (}{{\mathit H}^{0}}{)}$ $\cdot{}$ B(${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{(*)}}$) between 0.7 and 2.5 pb (95$\%$ CL) is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $110 - 200$ GeV, which is $1.7 - 45$ times larger than the expected Standard Model cross section. The best limit is obtained for ${\mathit m}_{{{\mathit H}^{0}}}$ = 160 GeV.
66  ABAZOV 2009U search for ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ with ${{\mathit \tau}}$ $\rightarrow$ hadrons in 1 fb${}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV. The production mechanisms include associated +${{\mathit H}^{0}}$ production, weak boson fusion, and gluon fusion. A limit (95$\%$ CL) is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $105 - 145$ GeV, which is $20 - 82$ times larger than the expected Standard Model cross section. The limit for ${\mathit m}_{{{\mathit H}^{0}}}$ = 115 GeV is 29 times larger than the expected Standard Model cross section.
67  ABAZOV 2006 search for Higgs boson production in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV with the decay chain ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{*}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \nu}}{{\mathit \ell}^{'\mp}}{{\overline{\mathit \nu}}}$. A limit ${{\mathit \sigma}}({{\mathit H}^{0}})\cdot{}B({{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{*}}$) $<$ ($5.6 - 3.2$) pb (95 $\%$CL) is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $120 - 200$ GeV, which far exceeds the expected Standard Model cross section.
68  ABAZOV 2006O search for associated ${{\mathit H}^{0}}{{\mathit W}}$ production in ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 1.96 TeV with the decay ${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{*}}$, in the final states ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{'\mp}}{{\mathit \nu}}{{\mathit \nu}^{\,'}}{{\mathit X}}$ where ${{\mathit \ell}}$ = ${{\mathit e}}$, ${{\mathit \mu}}$. A limit ${\mathit \sigma (}{{\mathit H}^{0}}{{\mathit W}}{)}\cdot{}$ B(${{\mathit H}^{0}}$ $\rightarrow$ ${{\mathit W}}{{\mathit W}^{*}}$) $<$ ($3.2 - 2.8$) pb (95 $\%$CL) is given for ${\mathit m}_{{{\mathit H}^{0}}}$ = $115 - 175$ GeV, which far exceeds the expected Standard Model cross section.
References