Heavy Vector T riplets: Bridging Theory and Data
Andrea Thamm
Benasque, 17 April 2014 École Polytechnique Fédérale de Lausanne in collaboration with D. Pappadopulo, R. Torre, A. Wulzer based on arXiv:1402.4431
Heavy Vector T riplets: Bridging Theory and Data Andrea Thamm - - PowerPoint PPT Presentation
Benasque, 17 April 2014 Heavy Vector T riplets: Bridging Theory and Data Andrea Thamm cole Polytechnique Fdrale de Lausanne in collaboration with D. Pappadopulo, R. Torre, A. Wulzer based on arXiv:1402.4431 Outline 1. Motivations
Benasque, 17 April 2014 École Polytechnique Fédérale de Lausanne in collaboration with D. Pappadopulo, R. Torre, A. Wulzer based on arXiv:1402.4431
Andrea Thamm 3
Andrea Thamm 3
✤ aim: phenomenological Lagrangian for heavy spin-1 resonances
to bridge between experimental data and theoretical models
✤ idea:
present bounds in terms of simplified model parameters any model can be matched to simplified Lagrangian
Theory yDatay Ls ⃗ c(⃗ p) L(⃗ c)
✤ indirect probes of new physics very important ✤ at LHC also many direct probes, for example:
Weakly coupled Strongly coupled SPIN 1 Z’ models, sequential W’ ,… Composite Higgs models very difficult to reinterpret
Andrea Thamm 3
LV = −1 4D[µV a
ν]D[µV ν] a + m2 V
2 V a
µ V µ a
+ i gV cHV a
µ H†⌧ a ↔
D
µ
H + g2 gV cF V a
µ Jµ a F
+ gV 2 cV V V ✏abcV a
µ V b ν D[µV ν] c + g2 V cV V HHV a µ V µ aH†H − g
2cV V W ✏abcW µ ν aV b
µV c ν
V =
LV = −1 4D[µV a
ν]D[µV ν] a + m2 V
2 V a
µ V µ a
+ i gV cHV a
µ H†⌧ a ↔
D
µ
H + g2 gV cF V a
µ Jµ a F
+ gV 2 cV V V ✏abcV a
µ V b ν D[µV ν] c + g2 V cV V HHV a µ V µ aH†H − g
2cV V W ✏abcW µ ν aV b
µV c ν
V =
∼ gV cH Vµ
WL , ZL, h WL , ZL, h
Coupling to SM Vectors
Vµ f ¯ f ∼ g2 gV cF
cF V · JF → clV · Jl + cqV · Jq + c3V · J3 Jµ a
F
= X
f
f Lγµτ afL
Coupling to SM fermions
LV = −1 4D[µV a
ν]D[µV ν] a + m2 V
2 V a
µ V µ a
+ i gV cHV a
µ H†⌧ a ↔
D
µ
H + g2 gV cF V a
µ Jµ a F
+ gV 2 cV V V ✏abcV a
µ V b ν D[µV ν] c + g2 V cV V HHV a µ V µ aH†H − g
2cV V W ✏abcW µ ν aV b
µV c ν
V =
LV = −1 4D[µV a
ν]D[µV ν] a + m2 V
2 V a
µ V µ a
+ i gV cHV a
µ H†⌧ a ↔
D
µ
H + g2 gV cF V a
µ Jµ a F
+ gV 2 cV V V ✏abcV a
µ V b ν D[µV ν] c + g2 V cV V HHV a µ V µ aH†H − g
2cV V W ✏abcW µ ν aV b
µV c ν
V =
Couplings among Vectors
✤ do not contribute to V decays ✤ do not contribute to single production ✤ only effects through (usually small) VW mixing
LV = −1 4D[µV a
ν]D[µV ν] a + m2 V
2 V a
µ V µ a
+ i gV cHV a
µ H†⌧ a ↔
D
µ
H + g2 gV cF V a
µ Jµ a F
+ gV 2 cV V V ✏abcV a
µ V b ν D[µV ν] c + g2 V cV V HHV a µ V µ aH†H − g
2cV V W ✏abcW µ ν aV b
µV c ν
V =
typical strength of V interactions gV gV ∼ g ∼ 1 Weakly coupled model Strongly coupled model gV ≤ 4π dimensionless coefficients ci cH ∼ cF ∼ 1 cH ∼ −g2/g2
V
and cF ∼ 1
1 2 3 4 5 10-13 10-12 10-11 10-10 10-9 10-8 10-7 10-6 10-5 10-4 10-3 10-2 10-1 100 s ` = MV @TeVD dLêds ` @pbD WL
+ZL HV+L
WL
+WL
WL
8 TeV
CTEQ6L1 Hm2 = MW
2 L
1 2 3 4 5 10-7 10-6 10-5 10-4 10-3 10-2 10-1 100 101 102 103 104 s ` = MV @TeVD dLêds ` @pbD uid j HV+L uiuj HV0L did j HV0L diuj HV-L
8 TeV
CTEQ6L1 Hm2 = s `L
✤ DY and VBF production
model independent model dependent
✤ can compute production rates analytically! ✤ easily rescale to different points in parameter space ✤ VBF subleading in motivated part of parameter space
σDY = X
i,j ∈ p
ΓV → ij MV 4π2 3 dLij dˆ s
s=M 2
V
σV BF = X
i,j ∈ p
ΓV → WL iWL j MV 48π2 dLWL iWL j dˆ s
s=M 2
V
ΓV±→ff
0 ' 2 ΓV0→ff ' Nc[f]
✓g2cF gV ◆2 MV 96π , ΓV0→W +
L W − L
' ΓV±→W ±
L ZL
' g2
V c2 HMV
192π ⇥ 1 + O(ζ2) ⇤ ΓV0→ZLh ' ΓV±→W ±
L h
' g2
V c2 HMV
192π ⇥ 1 + O(ζ2) ⇤
500 1000 1500 2000 2500 3000 3500 4000 0.02 0.04 0.06 0.08 0.10 0.12
M0 @GeVD BRHV0 Æ 2 XL
W+W- Zh uu dd ll è nn bb tt è gV = 1 Model A 500 1000 1500 2000 2500 3000 3500 4000 10-3 10-2 10-1
M0 @GeVD BRHV0 Æ 2 XL
W+W- Zh uu dd ll è nn bb tt è gV = 3 Model B
✤ relevant decay channels: di-lepton, di-quark, di-boson
gV cH ' g2cF /gV ' g2/gV gV cH ' gV , g2cF /gV ' g2/gV
Weakly coupled model Strongly coupled model
Andrea Thamm 3
✤ want limits on since model-independent ✤ must stay in a window around the peak,
σ × BR
due to steep fall of parton luminosities at large energies
Effect of interference -1 < y < 1 SM + BW Hwêo interferenceL sHpp Æ V0L â BRHV0 Æ l+l-L + sSMHpp Æ l+l-L SM + Signal Hwêo interferenceL sHpp Æ V0 Æ l+l-L + sSMHpp Æ l+l-L Signal BW sHpp Æ V0L â BRHV0 Æ l+l-L Signal only sHpp Æ V0 Æ l+l-L SM sSMHpp Æ l+l-L ✤ large distortion for non-negligible widths ✤ still under control in window around the peak ✤ but large tail
Di-lepton searches for
2600 2800 3000 3200 3400 3600 3800 1 2 3 4 Ml+ l- @GeVD dsêdMl+ l- @10-7pbêGeVD
0.0 0.5 1.0
y 1-sFullêsBW H%L
LHCû8TeV MV = 3.5 TeV GêMV = 11 %
BW 2 → 2 V0
1200 1400 1600 1800 2000 2200 2 4 6 8 Ml+ l- @GeVD dsêdMl+ l- @10-7pbêGeVD
0.0 0.5 1.0
10 20 y 1-sFullêsBW H%L
LHCû8TeV MV = 2 TeV GêMV = 10 %
[M − Γ, M + Γ]
[Accomando, Becciolini, Balyaev, Moretti, Shepherd, arXiv:1304.6700 ] [Accomando, Becciolini, de Curtis, Dominici, Fedeli, Shepherd, arXiv:1110.0713]
σ × BR
Effect of interference -1 < y < 1 SM + BW Hwêo interferenceL sHpp Æ V0L â BRHV0 Æ l+l-L + sSMHpp Æ l+l-L SM + Signal Hwêo interferenceL sHpp Æ V0 Æ l+l-L + sSMHpp Æ l+l-L Signal BW sHpp Æ V0L â BRHV0 Æ l+l-L Signal only sHpp Æ V0 Æ l+l-L SM sSMHpp Æ l+l-L ✤ depends on S/B ratio ✤ can be a large effect ✤ tail strongly model dependent, not
V0 σ × BR
✤ want limits on since model-independent ✤ must stay in a window around the peak,
Di-lepton searches for
2600 2800 3000 3200 3400 3600 3800 1 2 3 4 Ml+ l- @GeVD dsêdMl+ l- @10-7pbêGeVD
0.0 0.5 1.0
y 1-sFullêsBW H%L
LHCû8TeV MV = 3.5 TeV GêMV = 11 %
1200 1400 1600 1800 2000 2200 2 4 6 8 Ml+ l- @GeVD dsêdMl+ l- @10-7pbêGeVD
0.0 0.5 1.0
10 20 y 1-sFullêsBW H%L
LHCû8TeV MV = 2 TeV GêMV = 10 %
constructive destructive background
[Accomando, Becciolini, Balyaev, Moretti, Shepherd, arXiv:1304.6700 ] [Accomando, Becciolini, de Curtis, Dominici, Fedeli, Shepherd, arXiv:1110.0713]
1200 1400 1600 1800 2000 2200 2 4 6 8 Ml+ l- @GeVD dsêdMl+ l- @10-7pbêGeVD
0.0 0.5 1.0
10 20 y 1-sFullêsBW H%L
LHCû8TeV MV = 2 TeV GêMV = 10 %
σ × BR
✤ searches only sensitive to the peak can be easily reused
(give bounds on )
✤ searches sensitive to the tail only valid in the assumed model, not reusable Effect of interference -1 < y < 1 SM + BW Hwêo interferenceL sHpp Æ V0L â BRHV0 Æ l+l-L + sSMHpp Æ l+l-L SM + Signal Hwêo interferenceL sHpp Æ V0 Æ l+l-L + sSMHpp Æ l+l-L Signal BW sHpp Æ V0L â BRHV0 Æ l+l-L Signal only sHpp Æ V0 Æ l+l-L SM sSMHpp Æ l+l-L
V0 σ × BR
✤ want limits on since model-independent ✤ must stay in a window around the peak,
Di-lepton searches for
2600 2800 3000 3200 3400 3600 3800 1 2 3 4 Ml+ l- @GeVD dsêdMl+ l- @10-7pbêGeVD
0.0 0.5 1.0
y 1-sFullêsBW H%L
LHCû8TeV MV = 3.5 TeV GêMV = 11 %
[Accomando, Becciolini, Balyaev, Moretti, Shepherd, arXiv:1304.6700 ] [Accomando, Becciolini, de Curtis, Dominici, Fedeli, Shepherd, arXiv:1110.0713]
ATLAS CMS
both neglect interference effects bounds set assuming a Z’ tail Gaussian shape around the peak for very narrow resonance not ok, since tail is considered
reusable for very narrow resonance
no bound on σ × BR
[ATLAS-CONF-2013-017] [CMS-PAS-EXO-12-061]
✤ ATLAS di-boson search using the simplified model ✤ ideally, also bounds on model parameters should be given
Andrea Thamm 3
1000 2000 3000 4000 10-4 10-3 10-2 10-1 100 101 102 103 104 MV @GeVD sHpp Æ VL @pbD
theoretically excluded
CMS AgV=1
Weakly coupled model Strongly coupled model
similar bounds for ATLAS
✤ excluded for masses < 3 TeV ✤ di-lepton most stringent ✤ di-boson searches < 1-2 TeV ✤ reach of LHC at 14 TeV: 6 TeV ✤ reach of FCC at 100 TeV: 30 TeV ✤ excluded for masses < 1.5 TeV
unconstrained for larger
✤ di-boson most stringent ✤ in excluded region , not
reproduced
✤ reach of LHC at 14 TeV: 3-4 TeV ✤ reach of FCC at 100 TeV: 15-20 TeV
1000 2000 3000 4000 10-4 10-3 10-2 10-1 100 101 102 103 104 MV @GeVD sHpp Æ VL @pbD
theoretically excluded
CMS BgV=3
gV
pp Æ V0 pp Æ V+ V0 Æ tt V0 Æ WW Æ jj V0 Æ WW Æ lnqq
_'V±Æ W±Z Æ 3l±n V±Æ W±Z Æ jj V0 Æ ll V±Æ l±n V0 Æ tt V± Æ tb
GF mZ
0.0 0.5 1.0
2 4 6
cH cF
*
BgV=1
ú
AgV=1 MV = 2 TeV gV=1
0.0 0.5 1.0
2 4 6
cH cF
*
BgV=3
ú
AgV=3 MV = 2 TeV gV=3
0.0 0.5 1.0
2 4 6
cH cF
*
BgV=6
ú
AgV=6 MV = 2 TeV gV=6
✤ experimental limits converted into plane
(cH, cF )
yellow: CMS analysis dark blue: CMS light blue: CMS black: bounds from EWPT WZ → jj WZ → 3lν l+ν
✤ dominates ✤ EWPT not competitive ✤ only
allowed lν −1 . cF . 1
✤ EWPT become comparable ✤ di-bosons more and more relevant ✤ strongly coupled model evades bounds from
direct searches
[Pappadopulo, Thamm, Torre, Wulzer, arXiv:1402.4431 ]
500 1000 1500 2000 2500 3000 3500 1 2 3 4 5
MV @GeVD gV
Model A 500 1000 1500 2000 2500 3000 3500 1 2 3 4 5
MV @GeVD gV
Model B
theoretically excluded
yellow: CMS analysis dark blue: CMS light blue: CMS black: bounds from EWPT WZ → jj WZ → 3lν l+ν
✤ experimental limits converted into plane
(MV , gV )
✤ similar exclusions at low , leptonic final state dominates ✤ very different for larger coupling
gV
[Pappadopulo, Thamm, Torre, Wulzer, arXiv:1402.4431 ]
model-independent, reusable way.
shell signal region.
model parameters which can be easily matched to any preferred model. σ × BR
LV = −1 4D[µV a
ν]D[µV ν] a + m2 V
2 V a
µ V µ a
+ i gV cHV a
µ H†⌧ a ↔
D
µ
H + g2 gV cF V a
µ Jµ a F
+ gV 2 cV V V ✏abcV a
µ V b ν D[µV ν] c + g2 V cV V HHV a µ V µ aH†H − g
2cV V W ✏abcW µ ν aV b
µV c ν
V =
✤ including only dim-4 operators is well justified in:
weakly coupled models strongly coupled models that obey SILH power counting
✤ if higher dim. operators are unsuppressed:
parametrisation insufficient
✤ generalised custodial relation after rotation to mass basis
m2
W M 2 + = cos2 θW m2 ZM 2 0 .
mW,Z M+,0 . 10−1 ⌧ 1
✤ require hierarchy
M 2
+ = M 2 0 (1 + O(%))
✤ degeneracy
expect comparable production rates phase space suppressed cascade decays
✤ naturally small mixing angles ✤ EWPT to ensure compatibility with experiment
θN,C ' cH gV ˆ v 2 mW,Z m2
V
. 10−1 g|exp = g + O( ˆ m2
W /µ2 V ),
g0|exp = g0 + O( ˆ m2
W /µ2 V )
v2|expˆ v2 ✓ 1 − c2
H
g2
V ˆ
v2 4µV ◆ ˆ S = γ2
Hz2 ˆ
m2
W
µ2
V
− γHγF ˆ m2
W
µ2
V
, W = γ2
F
g2 g2
V
m2
W
µ2
V
✤ to include corrections we fix
(mZ, M0, GF ) → (v, mV , g)
0.0 0.5 1.0
0.0 0.5 1.0
cH cVVW
MV = 2 TeV cF = 4 gV = 3
0.0 0.5 1.0
0.0 0.5 1.0
cH cVVV
MV = 2 TeV cF = 4 gV = 3
0.0 0.5 1.0
0.0 0.5 1.0
cH cVVHH
MV = 2 TeV cF = 4 gV = 3
yellow: CMS analysis dark blue: CMS light blue: CMS black: bounds from EWPT WZ → jj WZ → 3lν l+ν
✤ experimental limits converted into plane
(cH, cV V V )
✤ affect exclusion only marginally
cV V W , cV V V and cV V HH
[Pappadopulo, Thamm, Torre, Wulzer, arXiv:1402.4431 ]