31
EW corrections for SM processes Mathieu PELLEN University of Freiburg Physics at TeV Colliders 2021 Les Houches, France 14 th of June 2021

EW corrections for SM processes

  • Upload
    others

  • View
    1

  • Download
    0

Embed Size (px)

Citation preview

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

Few examples

Mathieu PELLEN EW corrections for SM processes 9 / 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

/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

Summary of each sections

Mathieu PELLEN EW corrections for SM processes 22 / 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