searching for signs of the second higgs · a simplified parameter space after ewsb there are 9 free...
TRANSCRIPT
![Page 1: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/1.jpg)
Searching for signs of the second Higgs
Nathaniel CraigIAS + Rutgers
Based on work with J. Galloway, S. Thomas; J. Evans, R. Gray, S. Somalwar, S. Thomas.
!"
Emmanuel Contreras-Compana, John Paul Chou, Nathaniel Craig, Jared Evans, Yuri Gershtein, Richard Gray, Yevgeny Kats, Can Kilic, Michael Park, Sunil Somalwar, Matt Walker
Monday, July 1, 2013
![Page 2: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/2.jpg)
The state of EWSB
• We’ve discovered a (more or less) SM-like Higgs at ~126 GeV. Its couplings are SM-like to within ~25%.
• We’ve discovered no evidence thus far for degrees of freedom that could ensure the naturalness of the Higgs mass.
• What do we do now?
Monday, July 1, 2013
![Page 3: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/3.jpg)
Abandon all hope
Monday, July 1, 2013
![Page 4: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/4.jpg)
Abandon all hope
Monday, July 1, 2013
![Page 5: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/5.jpg)
Look for the second Higgs.
Monday, July 1, 2013
![Page 6: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/6.jpg)
1. Fine-tuning is not a meaningful guide, no problem with light scalars.
2. Fine-tuning is a meaningful guide, the weak scale is natural, but we haven’t seen the relevant d.o.f. yet.
3. Fine-tuning is a meaningful guide, the weak scale is tuned, but it’s anthropic.
At the very least, finding a second scalar associated with EWSB could partly differentiate between:
Unlikely that (3.) can explain two light scalars.
Monday, July 1, 2013
![Page 7: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/7.jpg)
• Higgs sector of the MSSM/NMSSM...
• Twin Higgs models and their variants
• Superconformal technicolor
• Composite Higgs models [e.g., SO(6)/SO(4)xSO(2) or Sp(6)/Sp(4)xSU(2)]
Plus additional Higgs scalars often arise in natural theories of EWSB.
Monday, July 1, 2013
![Page 8: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/8.jpg)
Perhaps as important as looking for top partners!(even if we find one, it will be hard to verify its role)
We should look as hard as we can for evidence of additional Higgs scalars.
Monday, July 1, 2013
![Page 9: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/9.jpg)
Today’s talkA compact
parameterization of additional Higgses
Implications of coupling measurements of the SM-like Higgs
Searching in standard channels
Searching in non-standard channels
Monday, July 1, 2013
![Page 10: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/10.jpg)
Today’s talkA compact
parameterization of additional Higgses
Implications of coupling measurements of the SM-like Higgs
Searching in standard channels
Searching in non-standard channels
There is enormous room for improvement here.
Monday, July 1, 2013
![Page 11: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/11.jpg)
Looking for another Higgs
1. Study the couplings of the recently-discovered SM-like Higgs.
2. Search for additional scalars in standard Higgs channels.
3. Search for additional scalars in non-standard Higgs channels.
Useful to develop a concrete framework in which all three avenues are related.
Monday, July 1, 2013
![Page 12: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/12.jpg)
2HDM• For the purposes of this talk, I’ll focus on
extended EWSB sectors whose IR physics is described by two Higgs doublets.
• This covers a broad class of known models and allows for convenient parameterization.
• ...but many of the qualitative features are shared by other extended EWSB sectors.
• I’ll keep the focus on bottom-up phenomena, generalizing beyond SUSY 2HDM.
Monday, July 1, 2013
![Page 13: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/13.jpg)
A simplified parameter space• Need to develop an efficient parameterization. General parameter space of 2HDM is vast, but there are well-motivated simplifying assumptions:
• Flavor limits suggest 2HDM should avoid new tree-level FCNC; satisfied by four discrete choices of couplings to fermions.
• Lack of large CP violation suggests new sources of CP violation coupled to SM are small; motivates focusing on CP-conserving 2HDM potentials.
• Imposing these constraints leads to tractable parameter space for signals & relations between search avenues.
Monday, July 1, 2013
![Page 14: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/14.jpg)
A simplified parameter space
After EWSB there are 9 free parameters in CP-conserving scalar potential.
mh, mH , mA, mH±
λ5, λ6, λ7
λ6,7 = 0 λ5,6,7 = 0
Useful basis of 4 physical masses, 2 angles, 3 couplings:
tanβ ≡ �Φ2�/�Φ1�
Discrete symm. for flavor: MSSM:
�√2 Re(Φ0
2)− v2√2 Re(Φ0
1)− v1
�=
�cos α sin α−sin α cos α
� �h
H
�
(only appear in trilinear couplings)
Couplings of scalars to fermions, vectors only depend on angles.
Physical d.o.f. are (8-3=5): h, H, A, H±
α :
Monday, July 1, 2013
![Page 15: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/15.jpg)
Alignment limit• Couplings of the observed Higgs
are approximately SM-like
• Strongly suggests proximity to the alignment limit
• In this limit h is the fluctuation around the vev, while remaining scalars are spectators to EWSB
• (Limit obtainable via decoupling or accidentally)
• Useful to expand in
α ≈ β − π/2
δ = β − α− π/2
ggH,ttHµ
-1 0 1 2 3
VBF,
VHµ
0
2
4
6!! "H
WW"H ZZ"H bb"H ## "H
CMS Preliminary -1 19.6 fb$ = 8 TeV, L s -1 5.1 fb$ = 7 TeV, L s
Monday, July 1, 2013
![Page 16: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/16.jpg)
• Scalar self-couplings have additional parametric freedom.
• Gives a map between current fits to the Higgs couplings and the possible size of NP signals.
• H, A are similar d.o.f. in alignment limit
2HDM I 2HDM II 2HDM III 2HDM IV
u Φ2 Φ2 Φ2 Φ2
d Φ2 Φ1 Φ2 Φ1
e Φ2 Φ1 Φ1 Φ2
y2HDM/ySM 2HDM 1 2HDM 2
hV V 1− δ2/2 1− δ2
/2
hQu 1− δ/tβ 1− δ/tβ
hQd 1− δ/tβ 1 + δtβhLe 1− δ/tβ 1 + δtβ
HV V −δ −δHQu −δ − 1/tβ −δ − 1/tβ
HQd −δ − 1/tβ −δ + tβ
HLe −δ − 1/tβ −δ + tβ
AV V 0 0
AQu 1/tβ 1/tβ
AQd −1/tβ tβ
ALe −1/tβ tβ
δ = β − α− π/2
Four discrete 2HDM types. All couplings to SM states fixed in terms of two angles.
Monday, July 1, 2013
![Page 17: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/17.jpg)
(1) Study the couplings
Monday, July 1, 2013
![Page 18: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/18.jpg)
95� ContoursΓΓWW�ZZbb�ΤΤ
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
t Β � 0
t Β � 1
t Β � 10t Β � 100
cos�Β�Α�
Β
Type 1: Fit Breakdown
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
Type 1: Combined Fit �68, 95� CL�
(1) Study the couplings
Monday, July 1, 2013
![Page 19: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/19.jpg)
95� ContoursΓΓWW�ZZbb�ΤΤ
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
t Β � 0
t Β � 1
t Β � 10t Β � 100
cos�Β�Α�
Β
Type 1: Fit Breakdown
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
Type 1: Combined Fit �68, 95� CL�
htt, hbb dropping, hVV takes over total width
(1) Study the couplings
Monday, July 1, 2013
![Page 20: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/20.jpg)
95� ContoursΓΓWW�ZZbb�ΤΤ
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
t Β � 0
t Β � 1
t Β � 10t Β � 100
cos�Β�Α�
Β
Type 2: Fit Breakdown
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
Type 2: Combined Fit �68, 95� CL�
(1) Study the couplings
Monday, July 1, 2013
![Page 21: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/21.jpg)
95� ContoursΓΓWW�ZZbb�ΤΤ
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
t Β � 0
t Β � 1
t Β � 10t Β � 100
cos�Β�Α�
Β
Type 2: Fit Breakdown
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
Type 2: Combined Fit �68, 95� CL�
htt growing/shrinking
hbb growing/shrinking
(1) Study the couplings
Monday, July 1, 2013
![Page 22: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/22.jpg)
0.2
0.2
0.4
0.4
0.60.8 0.81
1.2
1.41.61.8
2
2
�0.6 �0.4 �0.2 0.0 0.2 0.4 0.60
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 1: VBF Σ�Br�h�ΓΓ��Σ�Br�hSM�ΓΓ�
0.2
0.2
0.2
0.4
0.4
0.6
0.6
0.8
0.8
1
1
1
1.2
1.2
1.4
1.4
1.61.82
2.2
2.22.4
1.6
�0.2 �0.1 0.0 0.1 0.20
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 2: VBF Σ�Br�h�ΓΓ��Σ�Br�hSM�ΓΓ�
Monday, July 1, 2013
![Page 23: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/23.jpg)
0.2
0.2
0.4
0.4
0.60.8 0.81
1.2
1.41.61.8
2
2
�0.6 �0.4 �0.2 0.0 0.2 0.4 0.60
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 1: VBF Σ�Br�h�ΓΓ��Σ�Br�hSM�ΓΓ�
0.2
0.2
0.2
0.4
0.4
0.6
0.6
0.8
0.8
1
1
1
1.2
1.2
1.4
1.4
1.61.82
2.2
2.22.4
1.6
�0.2 �0.1 0.0 0.1 0.20
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 2: VBF Σ�Br�h�ΓΓ��Σ�Br�hSM�ΓΓ�
Room for excitementTotal width & hgg drop
but hVV large.
Zero in fermion couplings
Monday, July 1, 2013
![Page 24: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/24.jpg)
• We live near the alignment limit, but precisely how near depends sensitively on the 2HDM type.
• This proximity has little to do with directly measuring the coupling to vectors, and a lot to do with the total width and gluon coupling.
• There is room for surprises, especially in future measurement of VBF diphoton.
Monday, July 1, 2013
![Page 25: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/25.jpg)
Look directly for the second Higgs
Monday, July 1, 2013
![Page 26: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/26.jpg)
Second Higgs Doublet Alignment
Decay Topology Limit
H → WW,ZZ −H,A → γγ �H,A → ττ, µµ �
H,A → tt �
A → Zh −H → hh −
t → H±
b �
Monday, July 1, 2013
![Page 27: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/27.jpg)
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
Type 1: Combined Fit �68, 95� CL�
150 200 250 300 350 400 4500.001
0.01
0.1
1
10
MA �GeV�
Σ�Br�pb�
TYPE 1: Inclusive Σ�Br�A�X�, tanΒ�1, cos�Β�Α���0.32
Zh
tt
ZΓ
ΓΓ
gg
ΤΤ
cc
bb
150 200 250 300 350 400 4500.001
0.01
0.1
1
10
MH �GeV�
Σ�Br�pb�
TYPE 1: Inclusive Σ�Br�H�X�, tanΒ�1, cos�Β�Α���0.32, Λ5�0
hhttZΓΓΓggZZWWΤΤccbb
Type 1 2HDM, low tan beta
Monday, July 1, 2013
![Page 28: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/28.jpg)
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
Type 1: Combined Fit �68, 95� CL�
Type 1 2HDM, high tan beta
150 200 250 300 350 400 4500.001
0.01
0.1
1
10
MA �GeV�
Σ�Br�pb�
TYPE 1: Inclusive Σ�Br�A�X�, tanΒ�10, cos�Β�Α���0.43
Zh
tt
ZΓ
ΓΓ
gg
ΤΤ
cc
bb
150 200 250 300 350 400 4500.001
0.01
0.1
1
10
MH �GeV�
Σ�Br�pb�
TYPE 1: Inclusive Σ�Br�H�X�, tanΒ�10, cos�Β�Α���0.43, Λ5�0
hhttZΓΓΓggZZWWΤΤccbb
Monday, July 1, 2013
![Page 29: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/29.jpg)
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
Type 2: Combined Fit �68, 95� CL�
Type 2 2HDM, low tan beta
150 200 250 300 350 400 4500.001
0.01
0.1
1
10
MA �GeV�
Σ�Br�pb�
TYPE 2: Inclusive Σ�Br�A�X�, tanΒ�1, cos�Β�Α���0.11
Zh
tt
ZΓ
ΓΓ
gg
ΤΤ
cc
bb
150 200 250 300 350 400 4500.001
0.01
0.1
1
10
MH �GeV�
Σ�Br�pb�
TYPE 2: Inclusive Σ�Br�H�X�, tanΒ�1, cos�Β�Α���0.11, Λ5�0
hhttZΓΓΓggZZWWΤΤccbb
Monday, July 1, 2013
![Page 30: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/30.jpg)
�1.0 �0.5 0.0 0.5 1.00
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
Type 2: Combined Fit �68, 95� CL�
Type 2 2HDM, high tan beta
150 200 250 300 350 400 4500.001
0.01
0.1
1
10
MA �GeV�
Σ�Br�pb�
TYPE 2: Inclusive Σ�Br�A�X�, tanΒ�10, cos�Β�Α���0.02
Zh
tt
ZΓ
ΓΓ
gg
ΤΤ
cc
bb
150 200 250 300 350 400 4500.001
0.01
0.1
1
10
MH �GeV�
Σ�Br�pb�
TYPE 2: Inclusive Σ�Br�H�X�, tanΒ�10, cos�Β�Α���0.02, Λ5�0
hhttZΓΓΓggZZWWΤΤccbb
Monday, July 1, 2013
![Page 31: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/31.jpg)
• Even in the exact alignment limit, the scalars H and A have large gluon fusion production cross sections, since their top couplings are nonzero.
• Even close to the exact alignment limit, processes such as H>VV can be appreciable because the competition is only with H > bb below the top pair threshold.
Monday, July 1, 2013
![Page 32: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/32.jpg)
(2) Look in standard Higgs channels
Monday, July 1, 2013
![Page 33: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/33.jpg)
17
(GeV)Hm200 400 600 800 1000
SM!/
!95
% C
L lim
it on
-110
1
10
210ObservedExpected
! 1±Expected ! 2±Expected
-1=8 TeV, L=5.3 fbs -1=7 TeV, L=5.1 fbsCMS
" 2l2# ZZ #H
Figure 9: Observed (solid line) and expected (dashed line) 95% CL upper limit on the ratio ofthe product of the production cross section and branching fraction to the SM expectation forthe Higgs boson in the H → ZZ → 2�2ν channel.
(GeV)Hm200 400 600 800 1000
SM!/
!95
% C
L lim
it on
-110
1
10
210 Expected 2l 2q" ZZ "H
qq# l" WW "H # 2l 2" WW "H
# 2l 2" ZZ "H $ 4l + 2l 2" ZZ "H
Combined
-15.3 fb%=8 TeV, Ls -1 5.1 fb%=7 TeV, LsCMS
(GeV)Hm200 400 600 800 1000
SM!/
!95
% C
L lim
it on
-110
1
10
210 Observed 2l 2q" ZZ "H
qq# l" WW "H # 2l 2" WW "H
# 2l 2" ZZ "H $ 4l + 2l 2" ZZ "H
Combined
-1 5.3 fb%=8 TeV, Ls -1 5.1 fb%=7 TeV, LsCMS
Figure 10: (left) Expected and (right) observed 95% CL limits for all individual channels andtheir combination. The horizontal dashed line at unity indicates the SM expectation.
0.01
0.01
0.05
0.05 0.05
0.1
0.1
0.1
0.5
0.5
1
1
5
5
5
�0.6 �0.4 �0.2 0.0 0.2 0.4 0.60
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 1: Inclusive Σ�Br�H�VV��Σ�Br�HSM�VV�, mH�300 GeV, Λ5�0
0.01 0.01
0.05
0.050.05
0.1
0.1
0.5
0.5
1
1
�0.2 �0.1 0.0 0.1 0.20
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 2: Inclusive Σ�Br�H�VV��Σ�Br�HSM�VV�, mH�300 GeV, Λ5�0
H > WW, ZZ
Monday, July 1, 2013
![Page 34: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/34.jpg)
17
(GeV)Hm200 400 600 800 1000
SM!/
!95
% C
L lim
it on
-110
1
10
210ObservedExpected
! 1±Expected ! 2±Expected
-1=8 TeV, L=5.3 fbs -1=7 TeV, L=5.1 fbsCMS
" 2l2# ZZ #H
Figure 9: Observed (solid line) and expected (dashed line) 95% CL upper limit on the ratio ofthe product of the production cross section and branching fraction to the SM expectation forthe Higgs boson in the H → ZZ → 2�2ν channel.
(GeV)Hm200 400 600 800 1000
SM!/
!95
% C
L lim
it on
-110
1
10
210 Expected 2l 2q" ZZ "H
qq# l" WW "H # 2l 2" WW "H
# 2l 2" ZZ "H $ 4l + 2l 2" ZZ "H
Combined
-15.3 fb%=8 TeV, Ls -1 5.1 fb%=7 TeV, LsCMS
(GeV)Hm200 400 600 800 1000
SM!/
!95
% C
L lim
it on
-110
1
10
210 Observed 2l 2q" ZZ "H
qq# l" WW "H # 2l 2" WW "H
# 2l 2" ZZ "H $ 4l + 2l 2" ZZ "H
Combined
-1 5.3 fb%=8 TeV, Ls -1 5.1 fb%=7 TeV, LsCMS
Figure 10: (left) Expected and (right) observed 95% CL limits for all individual channels andtheir combination. The horizontal dashed line at unity indicates the SM expectation.
0.01
0.01
0.05
0.05 0.05
0.1
0.1
0.1
0.5
0.5
1
1
5
5
5
�0.6 �0.4 �0.2 0.0 0.2 0.4 0.60
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 1: Inclusive Σ�Br�H�VV��Σ�Br�HSM�VV�, mH�300 GeV, Λ5�0
0.01 0.01
0.05
0.050.05
0.1
0.1
0.5
0.5
1
1
�0.2 �0.1 0.0 0.1 0.20
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 2: Inclusive Σ�Br�H�VV��Σ�Br�HSM�VV�, mH�300 GeV, Λ5�0
Contours are essentially just Htt, not HVV
H > WW, ZZ
Monday, July 1, 2013
![Page 35: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/35.jpg)
H,A > tau tau
[GeV]Am200 400 600 800
tan
05
101520253035404550 CMS -1 = 7+8 TeV, L = 17 fbsPreliminary,
= 1 TeVSUSY
scenariomaxhMSSM m
ObservedExpected
expected 1 expected 2
LEP
95% CL Excluded Regions
M
[GeV]Am200 400 600 800
!ta
n
0
5
10
15
20
25
30
35
40
45
50CMS -1, L=17 fb""# Preliminary, H
Expected LimitB-TagNo B-TagCombined
Sum of h, H, A signals(no mass resolution)
Sensitivity at large tan beta coming from enhanced
production modes, rather than decay couplings.
Monday, July 1, 2013
![Page 36: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/36.jpg)
(GeV)Hm110 115 120 125 130 135 140 145 150
SM!/
!95
% C
L lim
it on
0.0
0.5
1.0
1.5
2.0ObservedExpected (68%)Expected (95%)
-1 = 8 TeV, L = 19.6 fbs -1 = 7 TeV, L = 5.1 fbsCMS
CMS preliminary (MVA)"" #H
1
10
51
100
1
150 200 250 300 350 400 450 500
0
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
mA�GeV�
Β
TYPE 1: Inclusive Σ�Br�A�ΓΓ� �fb�
H,A > diphoton
mA (GeV)
51 fb
10 fb
1 fb
One of the most promising channels at low tan beta in alignment limit!
Monday, July 1, 2013
![Page 37: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/37.jpg)
H,A > t tbar?
[TeV]ttM0.5 1 1.5 2 2.5 3
x B
[pb]
Z'!
Upp
er L
imit
-210
-110
1
10
210Expected (95% CL)
Observed (95% CL)
Z' 10.0% width
1 s.d.±Expected
2 s.d.±Expected
= 8 TeVs, -1CMS, L = 19.6 fb Z' with 10% Decay Width
Another final state we don’t typically pursue because subdominant to VV in SM-like heavy Higgs.
But at low tan beta the cross section for H, A > ttbar can be large! Needs further study.
200 400 600 800 1000
0.05
0.10
0.50
1.00
5.00
10.00
200 400 600 800 1000
0.05
0.10
0.50
1.00
5.00
10.00
200 400 600 800 1000
0.05
0.10
0.50
1.00
5.00
10.00
Monday, July 1, 2013
![Page 38: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/38.jpg)
• H>VV is useful even quite near the alignment limit, since the coupling must be radically suppressed before it’s beaten by light fermions.
• Ditau and diphoton are the best states for the exact alignment limit. But H,A > tau tau only works at large tan beta in Type 2 2HDM.
• So we desperately need to extend our reach in diphoton past 150 GeV.
• Top pairs???
Monday, July 1, 2013
![Page 39: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/39.jpg)
(3) Look in non-standard Higgs
channels
Monday, July 1, 2013
![Page 40: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/40.jpg)
Second Higgs Doublet Alignment
Decay Topology Limit
H → WW,ZZ −H,A → γγ �H,A → ττ, µµ �
H,A → tt �
A → Zh −H → hh −
t → H±
b �
Monday, July 1, 2013
![Page 41: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/41.jpg)
0.001
0.008
0.01
0.05
0.05
0.05
0.1 0.1
0.1
0.5 0.5
0.5
1
1
1
5
5
10
10
10
1
�0.6 �0.4 �0.2 0.0 0.2 0.4 0.60
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 1: Inclusive Σ�Br�H�hh� �pb�, mH�300 GeV, Λ5�0
0.0080.008
0.1
0.1
0.5
0.51
1
1
55
5
1010
1010
�0.2 �0.1 0.0 0.1 0.20
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 2: Inclusive Σ�Br�H�hh� �pb�, mH�300 GeV, Λ5�0
H > hh
Appreciable rates (~1000 x SM) consistent with
fits and VV limits.
Monday, July 1, 2013
![Page 42: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/42.jpg)
H > hh while we wait• Two promising ways to look for
resonant H>hh: in diphoton+bb, and in multileptons.
• Resonant production from a heavier state pushes events out to lower-background channels. 400 600 800 10005
6
7
8
9
10
mH �GeV�
Σ�Br�H�
hh��pb�
95� Observed Exclusion
• Using 5/fb, 7 TeV CMS multilepton results (no b-tags, no had. taus), observed limit is ~6pb. Using full 8 TeV set + b-tags, expect closer to ~3pb.
• With this motivation, CMS is doing a dedicated hh search in above channels with 8 TeV data. Sensitivity should be at ~few pb level.
Monday, July 1, 2013
![Page 43: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/43.jpg)
0.0050.0050.10.1
0.40.4
0.50.5
1 1
5 5
1010
5050
�0.6 �0.4 �0.2 0.0 0.2 0.4 0.60
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 1: Inclusive Σ�Br�A�Zh� �pb�, mA�300 GeV
0.0010.005 0.0050.1 0.1
0.40.4
0.50.511
55
10 10
�0.2 �0.1 0.0 0.1 0.20
Π2
3 Π8
Π4
Π8
tΒ � 0
tΒ � 1
tΒ � 10tΒ � 100
cos�Β�Α�
Β
TYPE 2: Inclusive Σ�Br�A�Zh� �pb�, mA�300 GeV
A > Zh
Appreciable rates (~few x SM) consistent with
fits and Zh cross section limits (~3 x SM).
Monday, July 1, 2013
![Page 44: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/44.jpg)
A > Zh while we wait
400 600 800 10002
3
4
5
6
7
mA �GeV�
Σ�Br�A�
Zh��pb�
95� Observed Exclusion• Most promising way to look for A>Zh is in ll+WW, with approx. kinematic reconstruction. But pure multi-leptons also not bad.
• Resonant production from a heavier state pushes events out to lower-background channels.
• Using 5/fb, 7 TeV CMS multilepton results (no b-tags, no had. taus), observed limit is ~2.5pb. Slightly worse than 8 TeV Zh cross section limit.
• With this motivation, CMS is doing a dedicated Zh search with 8 TeV data. Sensitivity should be at ~pb level, better than Zh cross section limit.
Monday, July 1, 2013
![Page 45: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/45.jpg)
• There can be appreciable rates for H>hh and A>Zh even quite close to the alignment limit, for the same reason as H>VV.
• We are not (yet, publicly) searching in these channels, but there can be observation-level rates consistent with the couplings of h.
• Sensitivity is currently in the range of ~pb using only crude search techniques, so there’s considerable room for refinement.
Monday, July 1, 2013
![Page 46: Searching for signs of the second Higgs · A simplified parameter space After EWSB there are 9 free parameters in CP-conserving scalar potential. m h,m H,m A,m H ± λ 5, λ 6, λ](https://reader034.vdocuments.mx/reader034/viewer/2022050600/5fa7a4208cd1fa087852d973/html5/thumbnails/46.jpg)
Today’s talkA compact
parameterization of additional Higgses
Implications of coupling measurements of the SM-like Higgs
Searching in standard channels
Searching in non-standard channels
(Close to alignment limit but with room for surprises)
(We look in H>VV, H,A > tau tau, but given prox. to alignment,
crucial to look in H,A > diphoton )
(Look in H>hh, A>Zh!)
Monday, July 1, 2013