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EW corrections for SM processes
Mathieu PELLEN
University of Freiburg
Physics at TeV Colliders 2021
Les Houches, France
14th of June 2021
Outline:
What are EW corrections ...... and why you want to compute them
Brief review on EW corrections since Les Houches 2019(i.e. arXiv:1906.XXXX)
Overview of each aspects of EW corrections
Aims
Overview of current progress for EW corrections
Input for wishlist
Disclaimer
I might have missed some references (please let me know if so)
Mathieu PELLEN EW corrections for SM processes 2 / 25
Outline:
What are EW corrections ...... and why you want to compute them
Brief review on EW corrections since Les Houches 2019(i.e. arXiv:1906.XXXX)
Overview of each aspects of EW corrections
Aims
Overview of current progress for EW corrections
Input for wishlist
Disclaimer
I might have missed some references (please let me know if so)
Mathieu PELLEN EW corrections for SM processes 2 / 25
Everything You Ever Wanted to Know About EW corrections(But Were Afraid to Ask)
→ Electroweak Radiative Corrections for Collider PhysicsDenner, Dittmaier; 1912.06823
→ reading suggestion for summer... 163 pages with 651 references ...
Mathieu PELLEN EW corrections for SM processes 3 / 25
Everything You Ever Wanted to Know About EW corrections(But Were Afraid to Ask)
→ Electroweak Radiative Corrections for Collider PhysicsDenner, Dittmaier; 1912.06823
→ reading suggestion for summer... 163 pages with 651 references ...
Mathieu PELLEN EW corrections for SM processes 3 / 25
One-slide summary
α2s ∼ α → same order of magnitude as NNLO QCD
Sudakov logarithms in high-energy limit
pT
dσ/dpTLONLO EW
Radiative tails near resonances
m
dσ/dmLONLO EW
Mathieu PELLEN EW corrections for SM processes 4 / 25
One-slide summary
α2s ∼ α → same order of magnitude as NNLO QCD
Sudakov logarithms in high-energy limit
pT
dσ/dpTLONLO EW
Radiative tails near resonances
m
dσ/dmLONLO EW
Mathieu PELLEN EW corrections for SM processes 4 / 25
One-slide summary
α2s ∼ α → same order of magnitude as NNLO QCD
Sudakov logarithms in high-energy limit
pT
dσ/dpTLONLO EW
Radiative tails near resonances
m
dσ/dmLONLO EW
Mathieu PELLEN EW corrections for SM processes 4 / 25
Overview in classes of processes
Top physics
Very active (most of the work)
EW physics (DY, diboson, VBS, triboson, ...)
Mixed QCD/EW corrections for Drell-Yan
NLO EW corrections for tri-boson / VBS and its backgrounds
Jet physics
Nothing since EW corrections for di-jet and tri-jet[Reyer, Schonherr, Schumann; 1902.01763]
Higgs physics
Few (in quantity) because of two-loop amplitudes needed
Mathieu PELLEN EW corrections for SM processes 5 / 25
State of the art (fixed order) - NLO EW corrections
Precise predictions for single-top production: the impact of EW corrections and QCD shower on thet-channel signature Frederix, Pagani, Tsinikos; 1907.12586
Top-quark pair hadroproduction in association with a heavy boson at NLO+NNLL including EWcorrections Broggio et al.; 1907.04343
NNLO QCD + NLO EW with Matrix+OpenLoops: precise predictions for vector-boson pair productionGrazzini et al.; 1912.00068
Next-to-leading-order QCD and electroweak corrections to triple-W production with leptonic decays at theLHC Dittmaier, Knippen, Schwan; 1912.04117 ?Subleading EW corrections and spin-correlation effects in ttW multi-lepton signatures Frederix, Tsinikos;2004.09552
Precise predictions for double-Higgs production via vector-boson fusion Dreyer, MP et al.; 2005.13341
RIP Hbb: how other Higgs production modes conspire to kill a rare signal at the LHC Pagani, Shao, Zaro;2005.10277
NLO QCD+EW predictions for tHj and tZj production at the LHC Pagani, Tsinikos, Vryonidou;2006.10086
Electroweak corrections to the angular coefficients in finite-pT Z-boson production and dilepton decayFrederix, Vitos; 2007.08867
NLO QCD and EW corrections to vector-boson scattering into ZZ at the LHC Denner, MP et al.;2009.00411 ?Probing the spin correlations of tt production at NLO QCD+EW Frederix, Tsinikos, Vitos; 2105.11478
Combined NLO EW and QCD corrections to off-shell tt-W production at the LHC Denner, Pelliccioli;
2102.03246 ?Automated EW corrections with isolated photons: ttγ, ttγγ and tγj as case studiesPagani et al.; 2106.02059
? In the Les Houches wishlist 2019
Mathieu PELLEN EW corrections for SM processes 6 / 25
State of the art (fixed order)
Two-loop mixed corrections
Mixed QCD×QED corrections to on-shell boson production at the LHC Delto et al.; 1909.08428 ?NNLO QCD×EW corrections to Z production in the qq channel Bonciani et al.; 1911.06200 ?Mixed QCD-electroweak corrections to on-shell Z production at the LHC Buccioni et al.; 2005.10221 ?Mixed QCD×QED corrections to exclusive Drell Yan production using the qT-subtraction method Cieri etal.; 2005.01315 ?Next-to-leading order corrections to light-quark mixed QCD-EW contributions to Higgs boson productionBecchetti et al.; 2010.09451
Two-loop mixed QCD-EW corrections to gg→ Hg Bonetti et al.; 2007.09813
Next-to-next-to-leading order mixed QCD-electroweak corrections to on-shell Z production Bonciani et al.;2007.06518 ?Mixed NNLO QCD×electroweak corrections of O (Nf αsα)
to single-W/Z production at the LHC Dittmaier, Schmidt, Schwarz; 2009.02229 ?Mixed QCD-electroweak corrections to W-boson production in hadron collisions Behring et al.; 2009.10386?Mixed QCD-EW corrections to pp→ `ν` + X at the LHC Buonocore et al.; 2102.12539 ?Estimating the impact of mixed QCD-electroweak corrections on the W-mass determination at the LHCBehring et al.; 2103.02671 ?Mixed EW-QCD two-loop amplitudes for qq→ `+`− and γ5 scheme independence of multi-loopcorrections Heller et al.; 2012.05918 ?
Mathieu PELLEN EW corrections for SM processes 7 / 25
State of the art (beyond fixed order)Combination with QCD/QED shower
An event generator for same-sign W-boson scattering at the LHC including electroweak corrections Chiesa,MP et al.; 1906.01863
Fixed-order and merged parton-shower predictions for WW and WWj production at the LHC
including NLO QCD and EW corrections Brauer, MP et al.; 2005.12128 ?NLO QCD+NLO EW corrections to diboson production matched to parton shower Chiesa, Oleari, Re;2005.12146
WWγ production at hadron colliders with NLO QCD+EW corrections and parton shower effects Zhu etal.; 2005.10707
EW shower
Multipole photon radiation in the Vincia parton shower Skands, Verheyen; 2002.04939
Collinear electroweak radiation in antenna parton showers Kleiss, Verheyen; 2002.09248
Automated evaluation of electroweak Sudakov logarithms in Sherpa Bothmann, Napoletano; 2006.14635
Four lepton production and the accuracy of QED FSR Gutschow, Schonherr; 2007.15360
EW corrections and PDF/Fragmentation functions
PineAPPL: combining EW and QCD corrections for fast evaluation of LHC processes Carrazza et al.;2008.12789
Quark and Gluon Contents of a Lepton at High Energies; Han, Ma, Xie; 2103.09844
On factorisation schemes for the electron parton distribution functions in QED; Frixione; 2105.06688
Initial conditions for electron and photon structure and fragmentation functions; Frixione; 1909.03886
Low-virtuality photon transitions γ∗ → f f and the photon-to-jet conversion function; Denner, MP et al.;1907.02366
Mathieu PELLEN EW corrections for SM processes 8 / 25
Combined NLO EW and QCD corrections to off-shell tt-W production at the LHC; Denner, Pelliccioli; 2102.03246
α2sα
6αsα
7 α8
α3sα
6 α2sα
7 αsα8 α9
QCD QCD QCDEW EW
LOQCD
NLO1 NLO2 NLO3 NLO4
LOEW
Computation of full off-shell NLO1, NLO2, and NLO3 for ...... pp→ e+νeτ
+ντµ−νµ b b
First NLO EW 2→ 8 computation→ First time virtual with 10-point functions forphenomenology applications
τ+
ντ
µ−
νµ
W
bb
b
Z/γ
W
Z/γ
u
d
d
e+ νe
νµ
τ
νe
g
Mathieu PELLEN EW corrections for SM processes 10 / 25
Differential distributions
10 6
10 5
10 4
10 3
d/d
p T,t
[fb/
GeV]
p p e+ e + b b, s = 13 TeV, 0 = (MT, t MT, t)1/2/2LOQCDLOEW (×10)LOQCD + NLO1LO+NLO
0.30.20.10.00.10.20.3
ratio
[/LO
QCD]
LOEWNLO1
NLO2NLO3
100 200 300 400 500 600 700pT, t [GeV]
0.951.001.051.101.15
ratio
[/ L
O QCD
+NL
O 1]
LOQCD + NLO1 LO + NLO
10 5
10 4
10 3
10 2
10 1
d/d
Mt [
fb/G
eV]
p p e+ e + b b, s = 13 TeV, 0 = (MT, t MT, t)1/2/2LOQCDLOEW (×10)LOQCD + NLO1LO+NLO
0.40.20.00.20.40.60.81.0
ratio
[/LO
QCD]
LOEWNLO1
NLO2NLO3
160 170 180 190Mt [GeV]
0.951.001.051.101.15
ratio
[/ L
O QCD
+NL
O 1]
LOQCD + NLO1 LO + NLO
Non-trivial cancellation between different orders[Frederix, Pagani, Zaro; 1711.02116]
→ Importance of full NLO predictions in realistic final state
Mathieu PELLEN EW corrections for SM processes 11 / 25
Automated EW corrections with isolated photons: ttγ, ttγγ and tγj as case studies; Pagani, Shao, Tsinikos, Zaro; 2106.02059
NLO EW corrections for processes with final state photon ...... not yet fully automatised→ Solution: modified renormalisation, adapted FKS counterterms,photon isolation with democratic jets(no fragmentation function)→ Automation of full NLO corrections in MadGraph5 aMC@NLO
Application
Full NLO predictions for
ttγ
ttγγ
tγj
Mathieu PELLEN EW corrections for SM processes 12 / 25
Differential distributions
dσ
/dp
T [pb/G
eV
]
NLONLOQCD
LO
10−7
10−6
10−5
10−4
10−3
10−2
10−1 tt
γ, LHC13
total unc. scale unc. PDF unc.
0.8
1
1.2 NLO
pT(γ1) [GeV]
NLOQCD total unc.
NLO/NLOQCD
NLOQCD+EW/NLOQCD
0.8
1
1.2
0 100 200 300 400 500 600 700 800 900d
σ/d
pT [pb/G
eV
]
NLOQCD+EWNLOQCD
LO
10−7
10−6
10−5
ttγγ, LHC13
total unc. scale unc. PDF unc.
0.8
1
1.2 NLOQCD+EW
pT(γ1) [GeV]
NLOQCD total unc. NLOQCD+EW/NLOQCD
0.8
1
1.2
0 100 200 300 400 500 600
In this case, expected hierarchy of EW correctionsB Fully automatised computation / publicly available
Mathieu PELLEN EW corrections for SM processes 13 / 25
Mixed NNLO QCD×electroweak corrections of O (Nf αsα) to single-W/Z production at the LHC
Dittmaier, Schmidt, Schwarz; 2009.02229
V Nfαsα1PI
V ′VNfαsα
1PI
V Nfαsα1PI
Drell-Yan: best measured process at the LHC
Highest theoretical precision required
In addition to QCD and EW corrections→ mixed corrections of O (ααs) for pp→ 2` are needed
First step in this direction: O (nFααs) corrections
NB: Very recently, complete two-loop amplitude for the neutralcurrent dilepton process obtained [Heller et al.; 2012.05918]
Mathieu PELLEN EW corrections for SM processes 14 / 25
Differential distributions
1st+2nd gen.
reducible
O(Nfαsα)
Mℓℓ[GeV]
δ[%]
√s = 14 TeV
pp → Z/γ → ℓ−ℓ+ + X
12011010090807060
2
1.5
1
0.5
0
−0.5
−1
−1.5
−2
1st+2nd gen.
reducible
O(Nfαsα)
Mℓℓ[GeV]
δ[%]
√s = 14 TeV
pp → Z/γ → ℓ−ℓ+ + X
1000900800700600500400300200100
2.5
2
1.5
1
0.5
0
−0.5
−1
−1.5
−2
Size of corrections: phenomenologicaly relevant→ relevant for W/Z mass determination
Mathieu PELLEN EW corrections for SM processes 15 / 25
Fixed-order and merged parton-shower predictions for WW and WWj production at the LHC
including NLO QCD and EW corrections; Brauer, Denner, MP, Schonherr, Schumann; 2005.12128
Inclusion of EW corrections in (QCD) merged predictions→ Merged PS effects with approximate EW corrections(included via virtual EW approximation)
Fixed-order analysis at NLO QCD+EW→ for off-shell pp→ µ+νµe−νe
→ for off-shell pp→ µ+νµe−νej
Inclusive sample with:
Merged predictions + PS + approximate EW corrections→ pp→ µ+νµe−νe + 0, 1j@NLO + 2, 3j@LO
→ Can be studied with nj = 0 (WW) or nj = 1 (WWj)
NB: [Chiesa, Oleari, Re; 2005.12146]
→ no approximation but restricted to WW
Mathieu PELLEN EW corrections for SM processes 16 / 25
Ratio W+W−j/W+W−: fixed order vs. beyond fixed order
Sher
pa+R
eco
la
LONLO QCD
NLO QCD+EWNLO QCD×EWNLO QCD×EWapprox
0
2
4
6
8
10
12
14pp → µ+νµe−νe(+jet) + X @ 13 TeV
R1j 0j(p
T,µ
+e−
)
0 50 100 150 200 250 300 350 400
0.20.40.60.8
11.21.41.61.8
pT,µ+e− [GeV]
R1j 0j
/R
1j 0j,N
LO
QC
D
Sher
pa+R
eco
la
MEPS@NLO pp → µ+νµe−νe + 0,1j@NLO + 2,3j@LO
LONLO QCDNLO QCD + EWapproxNLO QCD × EWapprox
0
2
4
6
8pp → µ+νµe−νe + jets @ 13 TeV
R1j 0j
(pT,
µ+
e−)
0 50 100 150 200 250 300 350 400
0.9
1.0
1.1
pT,µ+e− [GeV]R
1j 0j/
R1j 0j
,ME
PS@
NL
OQ
CD
Very large ratios between WWj and WW (sensitive to jet veto)→ Ratio motivated by ATLAS measurement [1608.03086]
For multi-jet merged parton-shower: much more stable ratios
Mathieu PELLEN EW corrections for SM processes 17 / 25
Collinear electroweak radiation in antenna parton showers; Kleiss, Verheyen; 2002.09248
EW parton shower: received less attention
B Phenomenologically relevant
B Complications due to EW theory (chiral, massive particles,resonances ...)
First implementation of collinear electroweak radiation Vincia→ include all possible final-state collinear EW branchings→ collinear vector boson emissions off the initial stateincluded
Mathieu PELLEN EW corrections for SM processes 18 / 25
Differential distributions
0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000
[GeV]hardp
0.25−
0.2−
0.15−
0.1−
0.05−
0
To
tal
σ
EW
σ
Vincia (No QCD)
Vincia (QCD)
Pythia (No QCD)
Pythia (QCD)
j+ W→pp
0 500 1000 1500 2000 2500 3000 3500 4000 4500 5000 [GeV]hardp
3−10
2−10
1−10
Avera
ge n
um
ber
of bra
nchin
gs
(Vincia)+W (Pythia)+W
(Vincia)
W (Pythia)
W
Z (Vincia) Z (Pythia)
h (Vincia)
j (EW + QCD Shower)+ W→pp
Noticeable impact at high energy(in Pythia, only radiation of electroweak gauge bosons and no spin information kept)
→ particularly relevant for future colliders
Mathieu PELLEN EW corrections for SM processes 19 / 25
PineAPPL: combining EW and QCD corrections for fast evaluation of LHC processes;
Carrazza, Nocera, Schwan, Zaro; 2008.12789
PineAPPL:
library producing fast-interpolation grids of cross sections
to be interfaced with any Monte Carlo generator→ Application to MadGraph5 aMC@NLO
Applicable for all higher order (QCD, EW, mixed)B Crucial for global PDF fits to include EW corrections
→ https://n3pdf.github.io/pineappl
Mathieu PELLEN EW corrections for SM processes 20 / 25
Validation plot
0.0
0.1
0.2
Pin
eAP
PL
/M
C-
1[‰
] CMS Z boson production at√s = 13 TeV
Central scale
Lower scale
Upper scale
0.8
0.9
1.0
1.1
EW
on/
EW
off(P
DF
un
cert
ainty
)
NLO QCD+EW
NLO QCD
Data uncertainty
0.8
0.9
1.0
1.1
EW
on/
EW
off(S
cale
un
cert
ainty
)
102 103
p`¯
T [GeV]
0.8
0.9
1.0
1.1
EW
on/
EW
off(M
Cu
nce
rtai
nty
)
MC reproduced extremely precisely (sub-permille)
Next step: inclusion of EW corrections in global PDF fits!
Mathieu PELLEN EW corrections for SM processes 21 / 25
State of the art (fixed order)
NLO EW corrections
Up to 2→ 8 processes
B Tools not always publicB Computations can be extremely CPU intensiveB Processes with photon in the final stateB Loop-induced processes (e.g. gg→ H) requires two-loop EW
amplitudes
Mixed QCD/EW or NNLO EW corrections
Up to 2→ 2
B Main bottleneck: two-loop EW amplitudes
Mathieu PELLEN EW corrections for SM processes 23 / 25
State of the art (beyond fixed order)
Combination with QCD/QED shower
Up to 2→ 6 processes
B Treatment of mixed corrections not yet accounted
EW shower
First steps in direction of a full treatment
B No matching of weak corrections to EW shower
EW corrections and PDF/Fragmentation functions
Great progresses
B More studies in this directions to be expected
Mathieu PELLEN EW corrections for SM processes 24 / 25
Summary
Significant progress on EW corrections in the Standard Model
Any process @ NLO EW can be computed
Challenges:
Two-loop amplitudes with massive EW particlesCombination of EW corrections with QCD/QED/EW PS... and make all this publicly available/usable
Remarks:
The wishlist may not be restricted to fixed order
Processes on wishlist are strong motivations for theorists
→ If you want EW corrections for your favourite process:
Put it on the wishlist!
Mathieu PELLEN EW corrections for SM processes 25 / 25
Summary
Significant progress on EW corrections in the Standard Model
Any process @ NLO EW can be computed
Challenges:
Two-loop amplitudes with massive EW particlesCombination of EW corrections with QCD/QED/EW PS... and make all this publicly available/usable
Remarks:
The wishlist may not be restricted to fixed order
Processes on wishlist are strong motivations for theorists
→ If you want EW corrections for your favourite process:
Put it on the wishlist!
Mathieu PELLEN EW corrections for SM processes 25 / 25
Summary
Significant progress on EW corrections in the Standard Model
Any process @ NLO EW can be computed
Challenges:
Two-loop amplitudes with massive EW particlesCombination of EW corrections with QCD/QED/EW PS... and make all this publicly available/usable
Remarks:
The wishlist may not be restricted to fixed order
Processes on wishlist are strong motivations for theorists
→ If you want EW corrections for your favourite process:
Put it on the wishlist!
Mathieu PELLEN EW corrections for SM processes 25 / 25