Tuni ng means di fferent thi ngs to di fferent peopl e The Tyranny - - PowerPoint PPT Presentation

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Tuni ng means di fferent thi ngs to di fferent peopl e The Tyranny - - PowerPoint PPT Presentation

Tuni ng means di fferent thi ngs to di fferent peopl e The Tyranny of Carlo J. D. Bjorken Another change that I find disturbing is the rising tyranny of Carlo. No, I dont mean that fellow who runs CERN, but the other one, with first


slide-1
SLIDE 1

Tuni ng

means di fferent thi ngs to di fferent peopl e

slide-2
SLIDE 2
  • P. S k a n d s
  • J. D. Bjorken

The Tyranny of Carlo

2

“ Another change that I find disturbing is the rising tyranny of

  • Carlo. No, I don’t mean that fellow who runs CERN, but the other one, with first name

Monte.

slide-3
SLIDE 3
  • P. S k a n d s
  • J. D. Bjorken

The Tyranny of Carlo

2

“ Another change that I find disturbing is the rising tyranny of

  • Carlo. No, I don’t mean that fellow who runs CERN, but the other one, with first name

Monte. The simultaneous increase in detector complexity and in computation power has made simulation techniques an essential feature of contemporary experimentation. The Monte Carlo simulation has become the major means of visualization of not only detector performance but also of physics

  • phenomena. So far so good.
slide-4
SLIDE 4
  • P. S k a n d s
  • J. D. Bjorken

The Tyranny of Carlo

2

“ Another change that I find disturbing is the rising tyranny of

  • Carlo. No, I don’t mean that fellow who runs CERN, but the other one, with first name

Monte. The simultaneous increase in detector complexity and in computation power has made simulation techniques an essential feature of contemporary experimentation. The Monte Carlo simulation has become the major means of visualization of not only detector performance but also of physics

  • phenomena. So far so good.

But it often happens that the physics simulations provided by the the MC generators carry the authority of data itself. They look like data and feel like data, and if one is not careful they are accepted as if they were data. All Monte Carlo codes come with a GIGO (garbage in, garbage out) warning label. But the GIGO warning label is just as easy for a physicist to ignore as that little message on a packet

  • f cigarettes is for a chain smoker to ignore. I see nowadays experimental papers that

claim agreement with QCD (translation: someone’s simulation labeled QCD) and/or disagreement with an alternative piece of physics (translation: an unrealistic simulation), without much evidence of the inputs into those simulations.”

slide-5
SLIDE 5
  • P. S k a n d s
  • J. D. Bjorken

The Tyranny of Carlo

2

“ Another change that I find disturbing is the rising tyranny of

  • Carlo. No, I don’t mean that fellow who runs CERN, but the other one, with first name

Monte. The simultaneous increase in detector complexity and in computation power has made simulation techniques an essential feature of contemporary experimentation. The Monte Carlo simulation has become the major means of visualization of not only detector performance but also of physics

  • phenomena. So far so good.

But it often happens that the physics simulations provided by the the MC generators carry the authority of data itself. They look like data and feel like data, and if one is not careful they are accepted as if they were data. All Monte Carlo codes come with a GIGO (garbage in, garbage out) warning label. But the GIGO warning label is just as easy for a physicist to ignore as that little message on a packet

  • f cigarettes is for a chain smoker to ignore. I see nowadays experimental papers that

claim agreement with QCD (translation: someone’s simulation labeled QCD) and/or disagreement with an alternative piece of physics (translation: an unrealistic simulation), without much evidence of the inputs into those simulations.”

Account for parameters + pertinent cross-checks and validations Do serious effort to estimate uncertainties, by salient MC variations

slide-6
SLIDE 6
  • P. S k a n d s

Resources

Data Preservation: HEPDATA

Online database of experimental results Please make sure published results make it there

Analysis Preservation: RIVET

Large library of encoded analyses + data comparisons Main analysis & constraint package for event generators All your analysis are belong to RIVET

Updated validation plots: MCPLOTS.CERN.CH

Online plots made from Rivet analyses Want to help? Connect to Test4Theory (LHC@home 2.0)

Reproducible tuning: PROFESSOR

Automated tuning (& more)

3

slide-7
SLIDE 7
  • P. S k a n d s

(Test4Theory)

4

New Users/ Day

May June July Aug Sep

July 4th 2012

Monday Feb 18 2013 9:28 PM

The ¡LHC@home ¡2.0 ¡project ¡Test4Theory ¡allows ¡users ¡to ¡par:cipate ¡in ¡running ¡ simula:ons ¡of ¡high-­‑energy ¡par:cle ¡physics ¡using ¡their ¡home ¡computers. The ¡results ¡are ¡submiAed ¡to ¡a ¡database ¡which ¡is ¡used ¡as ¡a ¡common ¡resource ¡by ¡both ¡ experimental ¡and ¡theore:cal ¡scien:sts ¡working ¡on ¡the ¡Large ¡Hadron ¡Collider ¡at ¡CERN.

slide-8
SLIDE 8

(mcplots.cern.ch)

5

mcplots.cern.ch

  • Explicit tables of data & MC points
  • Run cards for each generator
  • Link to experimental reference paper
  • Steering file for plotting program
  • (Will also add link to RIVET analysis)
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SLIDE 9
  • P. S k a n d s

What is Tuning?

The value of the strong coupling at the Z pole

Governs overall amount of radiation

Renormalization Scheme and Scale for αs

1- vs 2-loop running, MSbar / CMW scheme, µR ~ pT2

Additional Matrix Elements included?

At tree level / one-loop level? Using what matching scheme?

Ordering variable, coherence treatment, effective 1→3 (or 2→4), recoil strategy, …

Branching Kinematics (z definitions, local vs global momentum conservation), hard parton starting scales / phase-space cutoffs, masses, non-singular terms, …

6

FSR pQCD Parameters

αs(mZ) αs Running Matching S u b l e a d i n g L

  • g

s

slide-10
SLIDE 10
  • P. S k a n d s

String Tuning

Lund Symmetric Fragmentation Function

The a and b parameters

Scale of string breaking process

IR cutoff and <pT> in string breaks

Mesons

Strangeness suppression, Vector/Pseudoscalar, η, η’, …

Baryons

Diquarks, Decuplet vs Octet, popcorn, junctions, … ?

7 Longitudinal FF = f(z) pT in string breaks Meson Multiplets B a r y

  • n

M u l t i p l e t s

0.2 0.4 0.6 0.8 1.0 0.5 1.0 1.5 0.2 0.4 0.6 0.8 1.0 0.5 1.0 1.5 2.0 0.2 0.4 0.6 0.8 1.0 0.5 1.0 1.5 0.2 0.4 0.6 0.8 1.0 0.5 1.0 1.5 2.0 0.2 0.4 0.6 0.8 1.0 0.5 1.0 1.5 0.2 0.4 0.6 0.8 1.0 0.5 1.0 1.5 2.0

Main String Parameters

slide-11
SLIDE 11
  • P. S k a n d s

Initial-State Radiaton

Value and running of the strong coupling

Governs overall amount of radiation (cf FSR)

Starting scale & Initial-Final interference

Relation between QPS and QF (vetoed showers? cf matching)

I-F colour-flow interference effects (cf ttbar asym) & interleaving

8 αs Size of Phase Space Matching “ P r i m

  • r

d i a l k T ”

Main ISR Parameters

slide-12
SLIDE 12
  • P. S k a n d s

Initial-State Radiaton

Value and running of the strong coupling

Governs overall amount of radiation (cf FSR)

Starting scale & Initial-Final interference

Relation between QPS and QF (vetoed showers? cf matching)

I-F colour-flow interference effects (cf ttbar asym) & interleaving

Additional Matrix Elements included?

At tree level / one-loop level? What matching scheme?

8 αs Size of Phase Space Matching “ P r i m

  • r

d i a l k T ”

Main ISR Parameters

slide-13
SLIDE 13
  • P. S k a n d s

Initial-State Radiaton

Value and running of the strong coupling

Governs overall amount of radiation (cf FSR)

Starting scale & Initial-Final interference

Relation between QPS and QF (vetoed showers? cf matching)

I-F colour-flow interference effects (cf ttbar asym) & interleaving

Additional Matrix Elements included?

At tree level / one-loop level? What matching scheme?

A small additional amount of “unresolved” kT

Fermi motion + unresolved ISR emissions + low-x effects?

8 αs Size of Phase Space Matching “ P r i m

  • r

d i a l k T ”

Main ISR Parameters

slide-14
SLIDE 14
  • P. S k a n d s

Min-Bias & Underlying Event

9 Number of MPI Pedestal Rise Strings per Interaction

Main IR Parameters

slide-15
SLIDE 15
  • P. S k a n d s

Min-Bias & Underlying Event

Infrared Regularization scale for the QCD 2→2 (Rutherford) scattering used for multiple parton interactions

(often called pT0) → size of overall activity

9 Number of MPI Pedestal Rise Strings per Interaction

Main IR Parameters

slide-16
SLIDE 16
  • P. S k a n d s

Min-Bias & Underlying Event

Infrared Regularization scale for the QCD 2→2 (Rutherford) scattering used for multiple parton interactions

(often called pT0) → size of overall activity

Proton transverse mass distribution → difference betwen central (active) vs peripheral (less active) collisions

9 Number of MPI Pedestal Rise Strings per Interaction

Main IR Parameters

slide-17
SLIDE 17
  • P. S k a n d s

Min-Bias & Underlying Event

Infrared Regularization scale for the QCD 2→2 (Rutherford) scattering used for multiple parton interactions

(often called pT0) → size of overall activity

Proton transverse mass distribution → difference betwen central (active) vs peripheral (less active) collisions Color correlations between multiple-parton-interaction systems → shorter or longer strings → less or more hadrons per interaction

9 Number of MPI Pedestal Rise Strings per Interaction

Main IR Parameters

slide-18
SLIDE 18
  • P. S k a n d s

Min-Bias & Underlying Event

Infrared Regularization scale for the QCD 2→2 (Rutherford) scattering used for multiple parton interactions

(often called pT0) → size of overall activity

Proton transverse mass distribution → difference betwen central (active) vs peripheral (less active) collisions Color correlations between multiple-parton-interaction systems → shorter or longer strings → less or more hadrons per interaction

9 Number of MPI Pedestal Rise Strings per Interaction

Main IR Parameters

slide-19
SLIDE 19
  • P. S k a n d s

Fragmentation Tuning

10

Multiplicity Distribution

  • f Charged Particles (tracks)

at LEP (Z→hadrons) Momentum Distribution

  • f Charged Particles (tracks)

at LEP (Z→hadrons)

<Nch(MZ)> ~ 21 ξp = Ln(xp) = Ln( 2|p|/ECM ) Note: use infrared-unsafe observables - sensitive to hadronization (example)

x=2|p|/mZ

slide-20
SLIDE 20
  • P. S k a n d s

Fragmentation Tuning

11

Momentum Distribution

  • f Charged Particles (tracks)

at LEP (Z→hadrons)

ξp = Ln(xp) = Ln( 2|p|/ECM ) Note: use infrared-unsafe observables - sensitive to hadronization (example)

)|

p

/d|Ln(x

ID

> dn

ch

1/<n

0.2 0.4 0.6 0.8 1 1.2 Particle Composition vs Lnx (udsc)

Pythia 8.183

±

π

±

K

±

p Other

V I N C I A R O O T

)|

p

|Ln(x

2 4 6 8

Ratio 0.6 0.8 1 1.2 1.4

Know what physics goes in

slide-21
SLIDE 21
  • P. S k a n d s

Identified Particles

S1/S0, B/M, B3/2/B1/2, strange/unstrange, Heavy

12

>

ch

<n <n>

  • 4

10

  • 3

10

  • 2

10

  • 1

10 1 Baryon Fractions

Pythia 8.181 Data from LEP/PDG/HEPDATA

LEP Pythia (ee:4) Pythia def Pythia (ee:2) Pythia (ee:1)

V I N C I A R O O T

p Λ /p Λ /K Λ

±

Σ Σ Δ

*

Σ

±

Ξ

*0

Ξ Ω

Theory/Data 0.6 0.8 1 1.2 1.4

>

ch

<n <n>

  • 3

10

  • 2

10

  • 1

10 1 10 Meson Fractions

Pythia 8.181 Data from LEP/PDG/HEPDATA

LEP Pythia (ee:4) Pythia def Pythia (ee:2) Pythia (ee:1)

V I N C I A R O O T ±

π π

±

K η ' η

±

ρ ρ

± *

K ω φ

Theory/Data 0.6 0.8 1 1.2 1.4

<n>

  • 4

10

  • 3

10

  • 2

10

  • 1

10 1 10 Heavy Meson Rates

Pythia 8.181 Data from PDG/HEPDATA

LEP Pythia (ee:4) Pythia def Pythia (ee:2) Pythia (ee:1)

V I N C I A R O O T ±

D D

± *

D

± s

D

±

B

±

B

u d s *

B

s

B ψ J /

c 1

χ

3 6 8 5

ψ Υ

Theory/Data 0.6 0.8 1 1.2 1.4

Compare with what you see at LHC Correlate with what you see at LHC Can variations within uncertainties explain differences? Or not?

1σ 2σ 1σ 2σ 1σ 2σ

slide-22
SLIDE 22
  • P. S k a n d s

PYTHIA 8 (hadronization off)

Need IR Corrections?

13

vs LEP: Thrust

1/N dN/d(1-T)
  • 3

10

  • 2

10

  • 1

10 1 10 1-Thrust (udsc)

Pythia 8.165 Data from Phys.Rept. 399 (2004) 71

L3 Pythia

V I N C I A R O O T 1-T (udsc) 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Major)
  • 3

10

  • 2

10

  • 1

10 1 10 Major

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Major 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Minor)
  • 3

10

  • 2

10

  • 1

10 1 10 Minor

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Minor 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(O)
  • 3

10

  • 2

10

  • 1

10 1 10 Oblateness

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T O 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4

Significant Discrepancies (>10%) for T < 0.05, Major < 0.15, Minor < 0.2, and for all values of Oblateness

T = max

  • n
  • i |

pi · n|

  • i |

pi|

  • 1 − T → 1

2

1 − T → 0

Major Minor Oblateness = Major - Minor Minor Major 1-T

slide-23
SLIDE 23
  • P. S k a n d s

PYTHIA 8 (hadronization off)

Need IR Corrections?

13

vs LEP: Thrust

1/N dN/d(1-T)
  • 3

10

  • 2

10

  • 1

10 1 10 1-Thrust (udsc)

Pythia 8.165 Data from Phys.Rept. 399 (2004) 71

L3 Pythia

V I N C I A R O O T 1-T (udsc) 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Major)
  • 3

10

  • 2

10

  • 1

10 1 10 Major

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Major 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Minor)
  • 3

10

  • 2

10

  • 1

10 1 10 Minor

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Minor 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(O)
  • 3

10

  • 2

10

  • 1

10 1 10 Oblateness

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T O 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4

Significant Discrepancies (>10%) for T < 0.05, Major < 0.15, Minor < 0.2, and for all values of Oblateness

T = max

  • n
  • i |

pi · n|

  • i |

pi|

  • 1 − T → 1

2

1 − T → 0

Major Minor Oblateness = Major - Minor Minor Major 1-T

+ cross checks: different eCM energies (HAD and FSR scale differently)

slide-24
SLIDE 24
  • P. S k a n d s

Need IR Corrections?

14

1/N dN/d(1-T)
  • 3

10

  • 2

10

  • 1

10 1 10 1-Thrust (udsc)

Pythia 8.165 Data from Phys.Rept. 399 (2004) 71

L3 Pythia

V I N C I A R O O T 1-T (udsc) 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Major)
  • 3

10

  • 2

10

  • 1

10 1 10 Major

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Major 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Minor)
  • 3

10

  • 2

10

  • 1

10 1 10 Minor

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Minor 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(O)
  • 3

10

  • 2

10

  • 1

10 1 10 Oblateness

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T O 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4 1

T = max

  • n
  • i |

pi · n|

  • i |

pi|

  • 1 − T → 1

2

1 − T → 0

Major Minor

PYTHIA 8 (hadronization on) vs LEP: Thrust

slide-25
SLIDE 25
  • P. S k a n d s

Need IR Corrections?

14

1/N dN/d(1-T)
  • 3

10

  • 2

10

  • 1

10 1 10 1-Thrust (udsc)

Pythia 8.165 Data from Phys.Rept. 399 (2004) 71

L3 Pythia

V I N C I A R O O T 1-T (udsc) 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Major)
  • 3

10

  • 2

10

  • 1

10 1 10 Major

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Major 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Minor)
  • 3

10

  • 2

10

  • 1

10 1 10 Minor

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Minor 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(O)
  • 3

10

  • 2

10

  • 1

10 1 10 Oblateness

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T O 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4

Note: Value of Strong coupling is αs(MZ) = 0.14

1

T = max

  • n
  • i |

pi · n|

  • i |

pi|

  • 1 − T → 1

2

1 − T → 0

Major Minor

PYTHIA 8 (hadronization on) vs LEP: Thrust

slide-26
SLIDE 26
  • P. S k a n d s

Value of Strong Coupling

15

Note: Value of Strong coupling is αs(MZ) = 0.12

1/N dN/d(1-T)
  • 3

10

  • 2

10

  • 1

10 1 10 1-Thrust (udsc)

Pythia 8.165 Data from Phys.Rept. 399 (2004) 71

L3 Pythia

V I N C I A R O O T 1-T (udsc) 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Major)
  • 3

10

  • 2

10

  • 1

10 1 10 Major

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Major 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Minor)
  • 3

10

  • 2

10

  • 1

10 1 10 Minor

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Minor 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(O)
  • 3

10

  • 2

10

  • 1

10 1 10 Oblateness

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T O 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4

T = max

  • n
  • i |

pi · n|

  • i |

pi|

  • 1 − T → 1

2

1 − T → 0

Major Minor

PYTHIA 8 (hadronization on) vs LEP: Thrust

slide-27
SLIDE 27
  • P. S k a n d s

Value of Strong Coupling

15

Note: Value of Strong coupling is αs(MZ) = 0.12

1/N dN/d(1-T)
  • 3

10

  • 2

10

  • 1

10 1 10 1-Thrust (udsc)

Pythia 8.165 Data from Phys.Rept. 399 (2004) 71

L3 Pythia

V I N C I A R O O T 1-T (udsc) 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Major)
  • 3

10

  • 2

10

  • 1

10 1 10 Major

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Major 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(Minor)
  • 3

10

  • 2

10

  • 1

10 1 10 Minor

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T Minor 0.1 0.2 0.3 0.4 0.5 Theory/Data 0.6 0.8 1 1.2 1.4 1/N dN/d(O)
  • 3

10

  • 2

10

  • 1

10 1 10 Oblateness

Pythia 8.165 Data from CERN-PPE-96-120

Delphi Pythia

V I N C I A R O O T O 0.2 0.4 0.6 Theory/Data 0.6 0.8 1 1.2 1.4

T = max

  • n
  • i |

pi · n|

  • i |

pi|

  • 1 − T → 1

2

1 − T → 0

Major Minor

PYTHIA 8 (hadronization on) vs LEP: Thrust

slide-28
SLIDE 28
  • P. S k a n d s

Wait … is this Crazy?

16

slide-29
SLIDE 29
  • P. S k a n d s

Wait … is this Crazy?

Best result

Obtained with αs(MZ) ≈ 0.14 ≠ World Average = 0.1176 ± 0.0020

16

slide-30
SLIDE 30
  • P. S k a n d s

Wait … is this Crazy?

Best result

Obtained with αs(MZ) ≈ 0.14 ≠ World Average = 0.1176 ± 0.0020

Value of αs depends on the order and scheme

MC ≈ Leading Order + LL resummation Other leading-Order extractions of αs ≈ 0.13 - 0.14 Effective scheme interpreted as “CMW” → 0.13; 2-loop running → 0.127; NLO → 0.12 ?

16

slide-31
SLIDE 31
  • P. S k a n d s

Wait … is this Crazy?

Best result

Obtained with αs(MZ) ≈ 0.14 ≠ World Average = 0.1176 ± 0.0020

Value of αs depends on the order and scheme

MC ≈ Leading Order + LL resummation Other leading-Order extractions of αs ≈ 0.13 - 0.14 Effective scheme interpreted as “CMW” → 0.13; 2-loop running → 0.127; NLO → 0.12 ?

Not so crazy

Tune/measure even pQCD parameters with the actual generator. Sanity check = consistency with other determinations at a similar formal order, within the uncertainty at that order

(including a CMW-like scheme redefinition to go to ‘MC scheme’)

16

slide-32
SLIDE 32
  • P. S k a n d s

Wait … is this Crazy?

Best result

Obtained with αs(MZ) ≈ 0.14 ≠ World Average = 0.1176 ± 0.0020

Value of αs depends on the order and scheme

MC ≈ Leading Order + LL resummation Other leading-Order extractions of αs ≈ 0.13 - 0.14 Effective scheme interpreted as “CMW” → 0.13; 2-loop running → 0.127; NLO → 0.12 ?

Not so crazy

Tune/measure even pQCD parameters with the actual generator. Sanity check = consistency with other determinations at a similar formal order, within the uncertainty at that order

(including a CMW-like scheme redefinition to go to ‘MC scheme’)

16

Improve → Matching at LO and NLO

slide-33
SLIDE 33
  • P. S k a n d s

Sneak Preview:

Multijet NLO Corrections with VINCIA

17

0.1 0.2 0.3 0.4 0.5

1/N dN/d(1-T)

  • 3

10

  • 2

10

  • 1

10 1 10

2

10 1-Thrust (udsc)

Vincia 1.030 + MadGraph 4.426 + Pythia 8.175 Data from Phys.Rept. 399 (2004) 71

L3 Vincia (NLO) Vincia (NLO off) Vincia (LO tune)

V I N C I A R O O T

1-T (udsc)

0.1 0.2 0.3 0.4 0.5

Theory/Data 0.6 0.8 1 1.2 1.4

0.2 0.4 0.6 0.8 1

1/N dN/dC

  • 3

10

  • 2

10

  • 1

10 1 10

2

10 C Parameter (udsc)

Vincia 1.030 + MadGraph 4.426 + Pythia 8.175 Data from Phys.Rept. 399 (2004) 71

L3 Vincia (NLO) Vincia (NLO off) Vincia (LO tune)

V I N C I A R O O T

C (udsc)

0.2 0.4 0.6 0.8 1

Theory/Data 0.6 0.8 1 1.2 1.4

0.2 0.4 0.6 0.8

1/N dN/dD

  • 3

10

  • 2

10

  • 1

10 1 10 D Parameter (udsc)

Vincia 1.030 + MadGraph 4.426 + Pythia 8.175 Data from Phys.Rept. 399 (2004) 71

L3 Vincia (NLO) Vincia (NLO off) Vincia (LO tune)

V I N C I A R O O T

D (udsc)

0.2 0.4 0.6 0.8

Theory/Data 0.6 0.8 1 1.2 1.4

First LEP tune with NLO 3-jet corrections

LO tune: αs(MZ) = 0.139 (1-loop running, MSbar) NLO tune: αs(MZ) = 0.122 (2-loop running, CMW)

Hartgring, Laenen, Skands, arXiv:1303.4974

slide-34
SLIDE 34
  • P. S k a n d s

ISR + Primordial kT

18

T

/dp σ d σ 1/

0.02 0.04 0.06 |<2.4)

µ

η >20, |

µ T

Peak (66<m<116, p

µ µ T bare

p

Pythia 8.181 Data from Phys.Lett. B705 (2011) 415

ATLAS PY8 (Monash 13) PY8 (4C) PY8 (2C)

bins

/N

2 5%

χ 0.1 ± 0.4 0.1 ± 1.3 0.1 ± 1.3

V I N C I A R O O T

7000 GeV

pp

[GeV]

T

p

10 20 30

Theory/Data 0.6 0.8 1 1.2 1.4

T

/dp σ d σ 1/

  • 6

10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

10 |<2.4)

µ

η >20, |

µ T

Peak (66<m<116, p

µ µ T bare

p

Pythia 8.181 Data from Phys.Lett. B705 (2011) 415

ATLAS PY8 (Monash 13) PY8 (4C) PY8 (2C)

bins

/N

2 5%

χ 0.1 ± 0.7 0.0 ± 1.4 0.0 ± 1.3

V I N C I A R O O T

7000 GeV

pp

[GeV]

T

p

100 200 300

Theory/Data 0.6 0.8 1 1.2 1.4

Drell-Yan pT distribution

Peak: primordial kT Tail: alphaS

Note: Q.M. requires physical observable!

slide-35
SLIDE 35
  • P. S k a n d s

Beware Process Dependence!

19

Z

slide-36
SLIDE 36
  • P. S k a n d s

Beware Process Dependence!

19

Z tt

slide-37
SLIDE 37
  • P. S k a n d s

Determine

pT0 : IR regularization scale for MPI Impact-parameter distribution (b-shape), Colour-reconnection strength (~Nhadrons/string)

We use:

P(Nch) pT <pT>(Nch) dNch/dη (~ constant in y, except in forward region) UE (including dNch/d∆φ)

MPI and Beam Remnants

20

slide-38
SLIDE 38
  • P. S k a n d s

36 A MULTIPLE-INTERACTION

MODEL FOR THE EVENT. . .

2031 diffractive system.

Each system

is represented by a string

stretched

between

a diquark

in the

forward end and

a

quark

in the other one.

Except for some tries with a dou-

ble string stretched from a diquark and a quark in the for- ward direction

to a central gluon,

which gave only modest changes in the results, no attempts have been made with more detailed models for diHractive

states.

  • V. MULTIPLICITY DISTRIBUTIONS

The

charged-multiplicity distribution is interesting, despite its deceptive simplicity, since most physical mechanisms

(of those

playing

a role

in minimum

bias events) contribute

to the multiplicity

buildup.

This was illustrated

in Sec. III.

From

now

  • n

we will use the

complete model, i.e., including

multiple

interactions

and varying

impact parameters,

to look more closely at the data.

Single- and double-difFractive events

are now also included;

with the UA5 triggering

conditions

roughly

—,
  • f the generated

double-diffractive events are retained,

while

the contribution from single diffraction

is negligi-

ble.

  • A. Total multiplicities

A final comparison

with the UA5 data at 540 GeV is presented in Fig. 12, for the double

Gaussian matter dis- tribution.

The agreement

is now generally good, although the value at the peak is still a bit high.

In this distribu- tion, the varying

impact parameters

do not play a major role; for comparison,

  • Fig. 12 also includes

the other ex- treme of a ftx overlap

Oo(b) (with

the use of the formal- ism

in Sec. IV, i.e., requiring

at least one semihard

in-

teraction per event, so as to minimize

  • ther

differences).

The three other matter

distributions, solid sphere, Gauss- ian and exponential, are in between, and are all compati- ble with the data. Within the model, the total multiplicity distribution

can be separated into the contribution from

(double-) diffractive events, events with

  • ne

interaction,

events with two interactions, and so on, Fig. 13. While 45% of all events

contain

  • ne interaction,

the low-multiplicity tail

is dominated by double-diffractive events and

the high-multiplicity

  • ne by events

with several interactions.

The

average charged multiplicity increases with the number

  • f interactions,
  • Fig. 14, but not proportionally:

each additional interaction

gives a smaller

contribution than the preceding

  • ne.

This

is

partly because

  • f

energy-momentum-conservation effects, and partly be- cause the additional messing

up"

when new

string pieces are added has less effect when many strings al- ready are present.

The same phenomenon

is displayed

in

  • Fig. 15, here as a function
  • f the "enhancement

factor"

f (b), i.e., for increasingly

central collisions. The multiplicity

distributions

for the 200- and 900-GeV UA5 data

have

not

been published,

but the moments

have, ' and a comparison with these is presented

in Table

  • I. The (n, t, ) value

was brought in reasonable agreement with the data, at each energy

separately,

by a variation

  • f

the pro scale.

The moments

thus obtained

are in reason-

able agreement with the data.

  • B. Energy dependence
10 I I I I I I I

i.

UA5 1982 DATA UA5 1981 DATA

Extrapolating to higher

energies, the evolution

  • f aver-

age charged multiplicity with energy is shown

in Fig. 16.

I ' I ' I tl 10 1P 3— C

O

  • 3
10 10-4 I I t 10 i j 1 j ~ j & j & I 1

20 40 60 80

100 120 10 0 I 20 I I 40 I I 60 I I I ep I I 100 120
  • FIG. 12. Charged-multiplicity

distribution

at 540 GeV, UA5

results

(Ref. 32) vs multiple-interaction

model with variable im-

pact parameter:

solid line, double-Gaussian matter distribution; dashed line, with fix impact parameter

[i.e., 00(b)]

  • FIG. 13. Separation
  • f multiplicity

distribution at 540 GeV

by number

  • f interactions

in event for double-Gaussian

matter distribution. Long dashes, double diffractive; dashed-dotted

  • ne interaction;

thick solid line, two interactions;

dashed line, three interactions; dotted line, four or more interactions; thin solid line, sum of everything.

Why dN/dη is useless (by itself)

w

Sjöstrand & v. Zijl, Phys.Rev.D36(1987)2019

Number of Charged Tracks Number of Charged Tracks

21

Can get <N> right with completely wrong models. Need RMS at least.

slide-39
SLIDE 39
  • P. S k a n d s

Underlying Event

UE - LHC from 900 to 7000 GeV - ATLAS

22

… until you reach a plateau (“max-bias”) Interpreted as impact-parameter effect Qualitatively reproduced by MPI models As you trigger on progressively higher pT, the entire event increases … Relative size of this plateau / min-bias depends on pT0 and b-profile

slide-40
SLIDE 40
  • P. S k a n d s

Image Credits: istockphoto

Matching

23

slide-41
SLIDE 41

P . Skands

Born + Shower

Example: .

24

2 2

+

Shower Approximation to Born + 1

+ …

slide-42
SLIDE 42

P . Skands

Born + Shower Born + 1 @ LO

Example: .

24

2 2

+

+

2

Shower Approximation to Born + 1

+ …

slide-43
SLIDE 43

P . Skands

Born + Shower Born + 1 @ LO

1

Example: .

25

2

+= g2

s 2CF

 2sik sijsjk + 1 sIK ✓ sij sjk + sjk sij ◆ = g2

s 2CF

 2sik sijsjk + 1 sIK ✓ sij sjk + sjk sij + 2 ◆

2

+ …

slide-44
SLIDE 44

P . Skands

Born + Shower Born + 1 @ LO

1

Example: .

25

2

+= g2

s 2CF

 2sik sijsjk + 1 sIK ✓ sij sjk + sjk sij ◆ = g2

s 2CF

 2sik sijsjk + 1 sIK ✓ sij sjk + sjk sij + 2 ◆ Total Overkill to add these two. All I really need is just that +2 …

2

+ …

slide-45
SLIDE 45

P . Skands

Adding Calculations

Born × Shower X+1 @ LO

26

X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … … … Fixed-Order Matrix Element Shower Approximation …

Fixed-Order ME above pT cut & nothing below

X+1(2) … X+1(1) X+2(1) X+3(1) … X+1(0) X+2(0) X+3(0) …

(see lecture 3) (with pT cutoff, see lecture 2)

slide-46
SLIDE 46

P . Skands

Born × Shower X+1 @ LO × Shower

27

X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … … … Fixed-Order Matrix Element Shower Approximation …

Fixed-Order ME above pT cut & nothing below

X+1(2) … X+1(1) X+2(1) X+3(1) … X+1(0) X+2(0) X+3(0) …

Adding Calculations

(see lecture 3)

Shower approximation above pT cut & nothing below

(with pT cutoff, see lecture 2)

slide-47
SLIDE 47

P . Skands

→ Double Counting

Born × Shower + (X+1) × shower

28

… … Fixed-Order Matrix Element Shower Approximation X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … Double Counting of terms present in both expansions Worse than useless …

Double counting above pT cut & shower approximation below

slide-48
SLIDE 48

P . Skands

Interpretation

29

► A (Complete Idiot’s) Solution – Combine

  • 1. [X]ME + showering
  • 2. [X + 1 jet]ME + showering
  • 3. …

► Doesn’t work

  • [X] + shower is inclusive
  • [X+1] + shower is also inclusive

Run generator for X (+ shower) Run generator for X+1 (+ shower) Run generator for … (+ shower) Combine everything into one sample What you get What you want Overlapping “bins” One sample

slide-49
SLIDE 49

P . Skands

Cures

30

slide-50
SLIDE 50

P . Skands

Tree-Level Matrix Elements

PHASE-SPACE SLICING (a.k.a. CKKW, MLM, …) UNITARITY (a.k.a. multiplication, PYTHIA,

VINCIA, …)

X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) …

Cures

30

slide-51
SLIDE 51

P . Skands

Tree-Level Matrix Elements

PHASE-SPACE SLICING (a.k.a. CKKW, MLM, …) UNITARITY (a.k.a. multiplication, PYTHIA,

VINCIA, …)

NLO Matrix Elements

SUBTRACTION (a.k.a. MC@NLO) UNITARITY + SUBTRACTION (a.k.a. POWHEG,

VINCIA)

X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) …

Cures

30

slide-52
SLIDE 52

P . Skands

Tree-Level Matrix Elements

PHASE-SPACE SLICING (a.k.a. CKKW, MLM, …) UNITARITY (a.k.a. multiplication, PYTHIA,

VINCIA, …)

NLO Matrix Elements

SUBTRACTION (a.k.a. MC@NLO) UNITARITY + SUBTRACTION (a.k.a. POWHEG,

VINCIA)

+ WORK IN PROGRESS …

NLO + multileg tree-level matrix elements NLO multileg matching Matching at NNLO

X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) …

Cures

30

slide-53
SLIDE 53

P . Skands

Tree-Level Matrix Elements

PHASE-SPACE SLICING (a.k.a. CKKW, MLM, …) UNITARITY (a.k.a. multiplication, PYTHIA,

VINCIA, …)

NLO Matrix Elements

SUBTRACTION (a.k.a. MC@NLO) UNITARITY + SUBTRACTION (a.k.a. POWHEG,

VINCIA)

+ WORK IN PROGRESS …

NLO + multileg tree-level matrix elements NLO multileg matching Matching at NNLO

X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X +1(2) … X(1) X +1(1) X +2(1) X +3(1) … Born X +1(0) X +2(0) X +3(0) … X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) …

Cures

30

slide-54
SLIDE 54
  • P. S k a n d s

Matching 1: Slicing

31

Examples: MLM, CKKW, CKKW-L

slide-55
SLIDE 55
  • P. S k a n d s

Matching 1: Slicing

31

First emission: “the HERWIG correction”

Use the fact that the angular-ordered HERWIG parton shower has a “dead zone” for hard wide-angle radiation (Seymour, 1995)

Many emissions: the MLM & CKKW-L prescriptions

F @ LO×LL-Soft (HERWIG Shower)

` (loops) 2

(2) (2)

1

. . .

1

(1) (1)

1

(1)

2

. . . (0) (0)

1

(0)

2

(0)

3

. . .

1 2 3

. . .

k (legs)

+

F+1 @ LO×LL (HERWIG Corrections)

` (loops) 2

(2) (2)

1

. . .

1

(1) (1)

1

(1)

2

. . . (0) (0)

1

(0)

2

(0)

3

. . .

1 2 3

. . .

k (legs)

=

F @ LO1×LL (HERWIG Matched)

` (loops) 2

(2) (2)

1

. . .

1

(1) (1)

1

(1)

2

. . . (0) (0)

1

(0)

2

(0)

3

. . .

1 2 3

. . .

k (legs)

F @ LO×LL-Soft (excl)

` (loops) 2

(2) . . .

1

(1) (1)

1

. . . (0) (0)

1

(0)

2

1 2 k (legs)

+

F+1 @ LO×LL-Soft (excl)

` (loops) 2

(2) . . .

1

(1) (1)

1

. . . (0) (0)

1

(0)

2

1 2 k (legs)

+

F+2 @ LO×LL (incl)

` (loops) 2

(2) . . .

1

(1) (1)

1

. . . (0) (0)

1

(0)

2

1 2 k (legs)

=

F @ LO2×LL (MLM & (L)-CKKW)

` (loops) 2

(2) . . .

1

(1) (1)

1

. . . (0) (0)

1

(0)

2

1 2 k (legs)

Examples: MLM, CKKW, CKKW-L

(Mangano, 2002) (CKKW & Lönnblad, 2001) (+many more recent; see Alwall et al., EPJC53(2008)473)

slide-56
SLIDE 56
  • P. S k a n d s

Z→udscb ; Hadronization OFF ; ISR OFF ; udsc MASSLESS ; b MASSIVE ; ECM = 91.2 GeV ; Qmatch = 5 GeV SHERPA 1.4.0 (+COMIX) ; PYTHIA 8.1.65 ; VINCIA 1.0.29 (+MADGRAPH 4.4.26) ; gcc/gfortran v 4.7.1 -O2 ; single 3.06 GHz core (4GB RAM)

Slicing: The Cost

32

0.1s 1s 10s 100s 1000s 2 3 4 5 6

Z→n : Number of Matched Emissions

1s 10s 100s 1000s 10000s 2 3 4 5 6

Z→n : Number of Matched Emissions

  • 1. Initialization time

(to pre-compute cross sections and warm up phase-space grids)

SHERPA+COMIX SHERPA (CKKW-L)

  • 2. Time to generate 1000 events

(Z → partons, fully showered &

  • matched. No hadronization.)

1000 SHOWERS

(example of state of the art)

slide-57
SLIDE 57

P . Skands

Classic Example

33

W + Jets

Number of jets in pp→W+X at the LHC From 0 (W inclusive) to W+3 jets PYTHIA includes matching up to W+1 jet + shower With ALPGEN, also the LO matrix elements for 2 and 3 jets are included But Normalization still

  • nly LO

mcplots.cern.ch With Matching Without Matching

RATIO

ETj > 20 GeV |ηj| < 2.8 Number of Jets W+Jets LHC 7 TeV

slide-58
SLIDE 58

P . Skands

Classic Example

33

W + Jets

Number of jets in pp→W+X at the LHC From 0 (W inclusive) to W+3 jets PYTHIA includes matching up to W+1 jet + shower With ALPGEN, also the LO matrix elements for 2 and 3 jets are included But Normalization still

  • nly LO

mcplots.cern.ch With Matching Without Matching

RATIO

ETj > 20 GeV |ηj| < 2.8 Number of Jets W+Jets LHC 7 TeV

slide-59
SLIDE 59

P . Skands

Slicing: Some Subtleties

Choice of slicing scale (=matching scale)

Fixed order must still be reliable when regulated with this scale → matching scale should never be chosen more than ~

  • ne order of magnitude below hard scale.

Precision still “only” Leading Order Choice of Renormalization Scale

We already saw this can be very important (and tricky) in multi-scale problems. Caution advised (see also supplementary slides & lecture notes)

34

slide-60
SLIDE 60

P . Skands

Choice of Matching Scale

35

→ A scale of 20 GeV for a W boson becomes 40 GeV for something weighing 2MW, etc … (+ adjust for CA/CF if g-initiated) → The matching scale should be written as a ratio (Bjorken scaling) Using a too low matching scale → everything just becomes highest ME Caveat emptor: showers generally do not include helicity correlations

25 50 75 100 Born (exc) + 1 + 2 (inc)

Reminder: in perturbative region, QCD is approximately scale invariant

Low Matching Scale

slide-61
SLIDE 61
  • P. S k a n d s

Matching 2: Subtraction

LO × Shower NLO

36

X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … … …

Fixed-Order Matrix Element Shower Approximation

X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … Examples: MC@NLO, aMC@NLO

slide-62
SLIDE 62
  • P. S k a n d s

Matching 2: Subtraction

LO × Shower NLO - ShowerNLO

37

X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … … …

Fixed-Order Matrix Element Shower Approximation

Fixed-Order ME minus Shower Approximation (NOTE: can be < 0!)

X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) …

Expand shower approximation to NLO analytically, then subtract:

Examples: MC@NLO, aMC@NLO

slide-63
SLIDE 63
  • P. S k a n d s

Matching 2: Subtraction

LO × Shower (NLO - ShowerNLO) × Shower

38

X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) … … …

Fixed-Order Matrix Element Shower Approximation

Fixed-Order ME minus Shower Approximation (NOTE: can be < 0!)

X(1) X(1) … X(1) X(1) X(1) X(1) … Born X+1(0) X(1) X(1) … …

Subleading corrections generated by shower off subtracted ME

Examples: MC@NLO, aMC@NLO

slide-64
SLIDE 64
  • P. S k a n d s

Matching 2: Subtraction

39

Combine → MC@NLO

Consistent NLO + parton shower (though correction events can have w<0) Recently, has been almost fully automated in aMC@NLO X(2) X+1(2) … X(1) X+1(1) X+2(1) X+3(1) … Born X+1(0) X+2(0) X+3(0) …

NLO: for X inclusive LO for X+1 LL: for everything else Note 1: NOT NLO for X+1

Note 2: Multijet tree-level matching still superior for X+2 NB: w < 0 are a problem because they kill efficiency: Extreme example: 1000 positive-weight - 999 negative-weight events → statistical precision of 1 event, for 2000 generated (for comparison, normal MC@NLO has ~ 10% neg-weights)

Frederix, Frixione, Hirschi, Maltoni, Pittau, Torrielli, JHEP 1202 (2012) 048 Frixione, Webber, JHEP 0206 (2002) 029

Examples: MC@NLO, aMC@NLO

slide-65
SLIDE 65
  • P. S k a n d s

Matching 3: ME Corrections

40

Double counting, IR divergences, multiscale logs

slide-66
SLIDE 66
  • P. S k a n d s

Standard Paradigm:

Have ME for X, X+1,…, X+n; Want to combine and add showers → “The Soft Stuff”

Matching 3: ME Corrections

40

Double counting, IR divergences, multiscale logs

slide-67
SLIDE 67
  • P. S k a n d s

Standard Paradigm:

Have ME for X, X+1,…, X+n; Want to combine and add showers → “The Soft Stuff”

Works pretty well at low multiplicities

Still, only corrected for “hard” scales; Soft still pure LL.

Matching 3: ME Corrections

40

Double counting, IR divergences, multiscale logs

slide-68
SLIDE 68
  • P. S k a n d s

Standard Paradigm:

Have ME for X, X+1,…, X+n; Want to combine and add showers → “The Soft Stuff”

Works pretty well at low multiplicities

Still, only corrected for “hard” scales; Soft still pure LL.

At high multiplicities:

Efficiency problems: slowdown from need to compute and generate phase space from dσX+n, and from unweighting (efficiency also reduced by negative weights, if present) Scale hierarchies: smaller single-scale phase-space region Powers of alphaS pile up

Matching 3: ME Corrections

40

Double counting, IR divergences, multiscale logs

slide-69
SLIDE 69
  • P. S k a n d s

Standard Paradigm:

Have ME for X, X+1,…, X+n; Want to combine and add showers → “The Soft Stuff”

Works pretty well at low multiplicities

Still, only corrected for “hard” scales; Soft still pure LL.

At high multiplicities:

Efficiency problems: slowdown from need to compute and generate phase space from dσX+n, and from unweighting (efficiency also reduced by negative weights, if present) Scale hierarchies: smaller single-scale phase-space region Powers of alphaS pile up

Better Starting Point: a QCD fractal?

Matching 3: ME Corrections

40

Double counting, IR divergences, multiscale logs

slide-70
SLIDE 70
  • P. S k a n d s

(shameless VINCIA promo)

41

(plug-in to PYTHIA 8 for ME-improved final-state showers, uses helicity matrix elements from MadGraph)

LO: Giele, Kosower, Skands, PRD84(2011)054003 NLO: Hartgring, Laenen, Skands, arXiv:1303.4974

slide-71
SLIDE 71
  • P. S k a n d s

Interleaved Paradigm:

Have shower; want to improve it using ME for X, X+1, …, X+n.

(shameless VINCIA promo)

41

(plug-in to PYTHIA 8 for ME-improved final-state showers, uses helicity matrix elements from MadGraph)

LO: Giele, Kosower, Skands, PRD84(2011)054003 NLO: Hartgring, Laenen, Skands, arXiv:1303.4974

slide-72
SLIDE 72
  • P. S k a n d s

Interleaved Paradigm:

Have shower; want to improve it using ME for X, X+1, …, X+n.

Interpret all-orders shower structure as a trial distribution

Quasi-scale-invariant: intrinsically multi-scale (resums logs) Unitary: automatically unweighted (& IR divergences →

multiplicities)

More precise expressions imprinted via veto algorithm: ME corrections at LO, NLO, … → soft and hard corrections No additional phase-space generator or σX+n calculations → fast

(shameless VINCIA promo)

41

(plug-in to PYTHIA 8 for ME-improved final-state showers, uses helicity matrix elements from MadGraph)

LO: Giele, Kosower, Skands, PRD84(2011)054003 NLO: Hartgring, Laenen, Skands, arXiv:1303.4974

slide-73
SLIDE 73
  • P. S k a n d s

Interleaved Paradigm:

Have shower; want to improve it using ME for X, X+1, …, X+n.

Interpret all-orders shower structure as a trial distribution

Quasi-scale-invariant: intrinsically multi-scale (resums logs) Unitary: automatically unweighted (& IR divergences →

multiplicities)

More precise expressions imprinted via veto algorithm: ME corrections at LO, NLO, … → soft and hard corrections No additional phase-space generator or σX+n calculations → fast

Automated Theory Uncertainties

For each event: vector of output weights (central value = 1) + Uncertainty variations. Faster than N separate samples; only

  • ne sample to analyse, pass through detector simulations, etc.

(shameless VINCIA promo)

41

(plug-in to PYTHIA 8 for ME-improved final-state showers, uses helicity matrix elements from MadGraph)

LO: Giele, Kosower, Skands, PRD84(2011)054003 NLO: Hartgring, Laenen, Skands, arXiv:1303.4974

slide-74
SLIDE 74
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-75
SLIDE 75
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-76
SLIDE 76
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element

X

ai → |MF+1|2 P ai|MF|2 ai →

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-77
SLIDE 77
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element Unitarity of Shower

P | | Virtual = − Z Real

X

ai → |MF+1|2 P ai|MF|2 ai →

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-78
SLIDE 78
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element Unitarity of Shower

P | | Virtual = − Z Real

Correct to Matrix Element

Z |MF|2 → |MF|2 + 2Re[M 1

FM 0 F] +

Z Real

X

ai → |MF+1|2 P ai|MF|2 ai →

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-79
SLIDE 79
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element Unitarity of Shower

P | | Virtual = − Z Real

Correct to Matrix Element

Z |MF|2 → |MF|2 + 2Re[M 1

FM 0 F] +

Z Real

X

ai → |MF+1|2 P ai|MF|2 ai →

R e p e a t

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-80
SLIDE 80
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element Unitarity of Shower

P | | Virtual = − Z Real

Correct to Matrix Element

Z |MF|2 → |MF|2 + 2Re[M 1

FM 0 F] +

Z Real

X

ai → |MF+1|2 P ai|MF|2 ai →

R e p e a t

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-81
SLIDE 81
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element Unitarity of Shower

P | | Virtual = − Z Real

Correct to Matrix Element

Z |MF|2 → |MF|2 + 2Re[M 1

FM 0 F] +

Z Real

X

ai → |MF+1|2 P ai|MF|2 ai →

R e p e a t

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-82
SLIDE 82
  • P. S k a n d s

Matching 3: ME Corrections

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element Unitarity of Shower

P | | Virtual = − Z Real

Correct to Matrix Element

Z |MF|2 → |MF|2 + 2Re[M 1

FM 0 F] +

Z Real

X

ai → |MF+1|2 P ai|MF|2 ai →

R e p e a t

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-83
SLIDE 83
  • P. S k a n d s

Matching 3: ME Corrections

First Order

PYTHIA: LO1 corrections to most SM and BSM decay processes, and for pp → Z/W/H (Sjöstrand 1987) POWHEG (& POWHEG BOX): LO1 + NLO0 corrections for generic processes (Frixione, Nason, Oleari, 2007)

Multileg NLO:

VINCIA: LO1,2,3,4 + NLO0,1 (shower plugin to PYTHIA 8; formalism for pp soon to appear) (see previous slide) MiNLO-merged POWHEG: LO1,2 + NLO0,1 for pp → Z/W/ H UNLOPS: for generic processes (in PYTHIA 8, based on POWHEG input) (Lönnblad & Prestel, 2013)

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element Unitarity of Shower

P | | Virtual = − Z Real

Correct to Matrix Element

Z |MF|2 → |MF|2 + 2Re[M 1

FM 0 F] +

Z Real

X

ai → |MF+1|2 P ai|MF|2 ai →

R e p e a t

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-84
SLIDE 84
  • P. S k a n d s

Matching 3: ME Corrections

First Order

PYTHIA: LO1 corrections to most SM and BSM decay processes, and for pp → Z/W/H (Sjöstrand 1987) POWHEG (& POWHEG BOX): LO1 + NLO0 corrections for generic processes (Frixione, Nason, Oleari, 2007)

Multileg NLO:

VINCIA: LO1,2,3,4 + NLO0,1 (shower plugin to PYTHIA 8; formalism for pp soon to appear) (see previous slide) MiNLO-merged POWHEG: LO1,2 + NLO0,1 for pp → Z/W/ H UNLOPS: for generic processes (in PYTHIA 8, based on POWHEG input) (Lönnblad & Prestel, 2013)

42

Illustrations from: PS, TASI Lectures, arXiv:1207.2389

Legs Loops +0 +1 +2 +0 +1 +2 +3

|MF|2

Generate “shower” emission

|MF+1|2 LL ∼ X

i∈ant

ai |MF|2

Correct to Matrix Element Unitarity of Shower

P | | Virtual = − Z Real

Correct to Matrix Element

Z |MF|2 → |MF|2 + 2Re[M 1

FM 0 F] +

Z Real

X

ai → |MF+1|2 P ai|MF|2 ai →

R e p e a t

Start at Born level

Virtues: No “matching scale” No negative-weight events Can be very fast

Examples: PYTHIA, POWHEG, VINCIA

slide-85
SLIDE 85
  • P. S k a n d s

Time to generate 1000 showers (seconds) 0.1 1 10 100 1000 10000 2 3 4 5 6 Z→n : Number of Matched Legs Initialization Time (seconds) 0.1 1 10 100 1000 2 3 4 5 6 Z→n : Number of Matched Legs

Hadronization Time (LEP)

Global Sector SHERPA Old Global Old Sector SHERPA 1.4.0 VINCIA 1.029

Z→udscb ; Hadronization OFF ; ISR OFF ; udsc MASSLESS ; b MASSIVE ; ECM = 91.2 GeV ; Qmatch = 5 GeV SHERPA 1.4.0 (+COMIX) ; PYTHIA 8.1.65 ; VINCIA 1.0.29 + MADGRAPH 4.4.26 ; gcc/gfortran v 4.7.1 -O2 ; single 3.06 GHz core (4GB RAM)

Speed

43

  • 1. Initialization time

(to pre-compute cross sections and warm up phase-space grids)

SHERPA+COMIX PYTHIA+VINCIA

  • 2. Time to generate 1000 events

(Z → partons, fully showered &

  • matched. No hadronization.)

VINCIA (GKS)

(example of state of the art)

Larkoski, Lopez-Villarejo, Skands, PRD 87 (2013) 054033

seconds

SHERPA (CKKW-L)

polarized unpolarized

1000 SHOWERS

sector global

slide-86
SLIDE 86
  • P. S k a n d s

1/N dN/d(1-T)

  • 3

10

  • 2

10

  • 1

10 1 10

L3 Vincia

1-Thrust (udsc)

Data from Phys.Rept. 399 (2004) 71 Vincia 1.027 + MadGraph 4.426 + Pythia 8.153

Rel.Unc.

1

Def R µ Finite QMatch Ord

2 C

1/N

1-T (udsc)

0.1 0.2 0.3 0.4 0.5

Theory/Data

0.6 0.8 1 1.2 1.4

Uncertainty Estimates

44

Plot from mcplots.cern.ch

Giele, Kosower, PS; Phys. Rev. D84 (2011) 054003 PS, Phys. Rev. D82 (2010) 074018

a) Authors provide specific “tune variations”

Run once for each variation→ envelope

b) One shower run

+ unitarity-based uncertainties → envelope VINCIA + PYTHIA 8 example Vincia:uncertaintyBands = on PYTHIA 6 example Perugia Variations µR, KMPI, CR, Ecm-scaling, PDFs

slide-87
SLIDE 87
  • P. S k a n d s

0.1 0.2 0.3 0.4 0.5

1/N dN/d(1-T)

  • 3

10

  • 2

10

  • 1

10 1 10

L3 Vincia

1-Thrust (udsc)

Data from Phys.Rept. 399 (2004) 71 Vincia 1.027 + MadGraph 4.426 + Pythia 8.153

0.1 0.2 0.3 0.4 0.5

Rel.Unc.

1

Def R µ Finite QMatch Ord

2 C

1/N

1-T (udsc)

0.1 0.2 0.3 0.4 0.5

Theory/Data

0.6 0.8 1 1.2 1.4

a) Authors provide specific “tune variations”

Run once for each variation→ envelope

Uncertainty Estimates

45

Plot from mcplots.cern.ch

Giele, Kosower, PS; Phys. Rev. D84 (2011) 054003 PS, Phys. Rev. D82 (2010) 074018

b) One shower run

+ unitarity-based uncertainties → envelope Matching reduces uncertainty VINCIA + PYTHIA 8 example Vincia:uncertaintyBands = on PYTHIA 6 example Perugia Variations µR, KMPI, CR, Ecm-scaling, PDFs

slide-88
SLIDE 88
  • P. S k a n d s

Summary

QCD phenomenology is witnessing a rapid evolution:

Driven by demand of high precision for LHC environment Exploring physics: infinite-order structure of quantum field

  • theory. Universalities vs process-dependence.

Emergent QCD phenomena: Jets, Strings, Hadrons

Non-perturbative QCD is still hard

Lund string model remains best bet, but ~ 30 years old Lots of input from LHC

“Solving the LHC” is both interesting and rewarding

New ideas evolving on both perturbative and non-perturbative sides → many opportunities for theory-experiment interplay Key to high precision → max information about the Terascale

46

slide-89
SLIDE 89
  • P. S k a n d s

MCnet Studentships

47

MCnet projects:

  • PYTHIA (+ VINCIA)
  • HERWIG
  • SHERPA
  • MadGraph
  • Ariadne (+ DIPSY)
  • Cedar (Rivet/Professor)

Activities include

  • summer schools

(2014: Manchester?)

  • short-term studentships
  • graduate students
  • postdocs
  • meetings (open/closed)

training studentships

3-6 month fully funded studentships for current PhD students at one of the MCnet nodes. An excellent opportunity to really understand and improve the Monte Carlos you use!

www.montecarlonet.org for details go to:

Monte Carlo

London CERN Karlsruhe Lund D u r h a m

Application rounds every 3 months.

MARIE CURIE ACTIONS funded by:

M a n c h e s t e r L

  • u

v a i n G ö t t i n g e n

slide-90
SLIDE 90

Oct 2014 → Monash University Melbourne, Australia

Come to Australia

p p

Establishing a new group in Melbourne Working on PYTHIA & VINCIA NLO Event Generators Precision LHC phenomenology & soft physics Support LHC experiments, astro-particle community, and future accelerators Outreach and Citizen Science

slide-91
SLIDE 91
  • P. S k a n d s

Jets vs Parton Showers

Jet clustering algorithms

Map event from low E-resolution scale (i.e., with many

partons/hadrons, most of which are soft) to a higher E-

resolution scale (with fewer, hard, IR-safe, jets)

49 Jet Clustering (Deterministic*) (Winner-takes-all) Parton Showering (Probabilistic)

Q ~ Λ ~ mπ ~ 150 MeV Q ~ Qhad ~ 1 GeV Q~ Ecm ~ MX

Parton shower algorithms

Map a few hard partons to many softer ones Probabilistic → closer to nature.

Not uniquely invertible by any jet algorithm*

Many soft particles A few hard jets Born-level ME Hadronization

(* See “Qjets” for a probabilistic jet algorithm, arXiv:1201.1914) (* See “Sector Showers” for a deterministic shower, arXiv:1109.3608)