(Highly) Tentative Conclusions based on the Early LHC Data P. - - PowerPoint PPT Presentation

highly tentative conclusions based on the early lhc data
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(Highly) Tentative Conclusions based on the Early LHC Data P. - - PowerPoint PPT Presentation

(Highly) Tentative Conclusions based on the Early LHC Data P. Skands (CERN TH) 1 The Power of Prediction We are at a unique time in the LHC era Predictions, without foreknowledge, can be tested with totally NEW data This is right


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SLIDE 1

(Highly) Tentative Conclusions based on the Early LHC Data

  • P. Skands (CERN TH)

1

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SLIDE 2

The Power of Prediction

  • We are at a unique time in the LHC era
  • Predictions, without foreknowledge, can be

tested with totally NEW data

  • This is right here and now, once and only
  • Attempt to learn as much as possible from

these “blind” tests, which cannot be repeated

2

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SLIDE 3

The Basic Four

3

900 GeV

ATLAS (N≥1) ALICE (N≥1,NSD)

2.36 TeV

ALICE (N≥1,NSD)

7 TeV

ALICE (N≥1)

P(N) dN/dη

900 GeV ALICE (INEL, NSD) CMS (NSD) ATLAS (N≥1) 2.36 TeV CMS (NSD) ALICE (INEL, NSD) 7 TeV CMS (NSD)

900 GeV

CMS (NSD) ATLAS (N≥1)

2.36 TeV

CMS (NSD)

7 TeV

CMS (NSD)

dN/dp⊥ 〈p⊥〉(N)

900 GeV

ATLAS (N≥1)

2.36 TeV

  • 7 TeV
  • (NSD): physical MB trigger + SD correction w/o physical SD definition
  • C. Zampolli: different model for each of these! “Not satisfactory”

Models should be “universal”. Inability to get universal tune → more physics?

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SLIDE 4

dN/dη

4

  • Really d〈N〉/dη ⇒ most sensitive to first few bins of P(N)
  • 〈N〉 cannot be interpreted without
  • EITHER: a soft/zero trigger + good model of

diffraction

  • OR: a hard trigger that suppresses diffraction
  • Cannot be interpreted at all without physical trigger (NSD!)
  • It is the least useful of the basic four
  • Mixes low-mult (diffractive/peripheral) and high-mult (non-diffractive/

hard-core) physics over its entire range

  • Danger: It is entirely possible to fit this variable while still

mismodeling both diffraction and UE (the two wrongs → right effect)

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SLIDE 5

dN/dη

4

  • Really d〈N〉/dη ⇒ most sensitive to first few bins of P(N)
  • 〈N〉 cannot be interpreted without
  • EITHER: a soft/zero trigger + good model of

diffraction

  • OR: a hard trigger that suppresses diffraction
  • Cannot be interpreted at all without physical trigger (NSD!)
  • It is the least useful of the basic four
  • Mixes low-mult (diffractive/peripheral) and high-mult (non-diffractive/

hard-core) physics over its entire range

  • Danger: It is entirely possible to fit this variable while still

mismodeling both diffraction and UE (the two wrongs → right effect)

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SLIDE 6

dN/dp⊥

5

  • Each track = one entry ⇒ low-mult events

relatively less important

  • Still mixes low-mult (diffractive/peripheral) and high-mult (non-diffractive/

hard-core) physics over its entire range

  • Compare p⊥ spectrum under different trigger conditions
  • Mainly sensitive to (string) fragmentation processes.

Some sensitivity to semi-hard (mini-)jet production

  • Soft models → too soft spectrum?
  • When tuning to 〈p⊥〉(N), important to check tail of dN/dp⊥
  • To maximize fragmentation sensitivity: convert to

x⊥ spectrum? (~ UE-corrected p⊥/E⊥jet)

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SLIDE 7

dN/dp⊥

5

  • Each track = one entry ⇒ low-mult events

relatively less important

  • Still mixes low-mult (diffractive/peripheral) and high-mult (non-diffractive/

hard-core) physics over its entire range

  • Compare p⊥ spectrum under different trigger conditions
  • Mainly sensitive to (string) fragmentation processes.

Some sensitivity to semi-hard (mini-)jet production

  • Soft models → too soft spectrum?
  • When tuning to 〈p⊥〉(N), important to check tail of dN/dp⊥
  • To maximize fragmentation sensitivity: convert to

x⊥ spectrum? (~ UE-corrected p⊥/E⊥jet)

slide-8
SLIDE 8

dN/dp⊥

6

10

  • 7

10

  • 6

10

  • 5

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  • 3

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  • 2

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1 5 10 15 20 10

  • 7

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  • 2

10

  • 1

1 5 10 15 20 p !GeV" 1/Nch dNch/dp

Charged Particle p Spectrum (||<2.5, p>0.5GeV)

900 GeV p+p

Inelastic, Non-Diffractive

Pythia 6.423 Data from ATLAS Collaboration, Phys.Lett. B688(2010)21

ATLAS data Perugia 0

  • Fast turnaround. Data propagates quickly into HepDATA!
  • + set of standard MC curves in paper gives us a reproducible counter-

check and benchmark for future comparisons. EXCELLENT!

]

  • 2

[ GeV

T

p d ! /d

ch

N

2

) d

T

p $ 1/(2

ev

N 1/

  • 10

10

  • 9

10

  • 8

10

  • 7

10

  • 6

10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

10 1 10

1 #

ch

n | < 2.5, ! > 500 MeV, |

T

p Data 2009 PYTHIA ATLAS MC09 PYTHIA ATLAS MC09c PYTHIA DW PYTHIA Perugia0 PHOJET

]

  • 2

[ GeV

T

p d ! /d

ch

N

2

) d

T

p $ 1/(2

ev

N 1/

  • 10

10

  • 9

10

  • 8

10

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10

  • 6

10

  • 5

10

  • 4

10

  • 3

10

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10

  • 1

10 1 10 ATLAS = 900 GeV s

[GeV]

T

p 1 10 Ratio 0.5 1 1.5

Data Uncertainties MC / Data

[GeV]

T

p 1 10 Ratio 0.5 1 1.5

b)

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SLIDE 9

dN/dp⊥

6

10

  • 7

10

  • 6

10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1 5 10 15 20 10

  • 7

10

  • 6

10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1 5 10 15 20 p !GeV" 1/Nch dNch/dp

Charged Particle p Spectrum (||<2.5, p>0.5GeV)

900 GeV p+p

Inelastic, Non-Diffractive

Pythia 6.423 Data from ATLAS Collaboration, Phys.Lett. B688(2010)21

ATLAS data Perugia 0

  • Fast turnaround. Data propagates quickly into HepDATA!
  • + set of standard MC curves in paper gives us a reproducible counter-

check and benchmark for future comparisons. EXCELLENT!

]

  • 2

[ GeV

T

p d ! /d

ch

N

2

) d

T

p $ 1/(2

ev

N 1/

  • 10

10

  • 9

10

  • 8

10

  • 7

10

  • 6

10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

10 1 10

1 #

ch

n | < 2.5, ! > 500 MeV, |

T

p Data 2009 PYTHIA ATLAS MC09 PYTHIA ATLAS MC09c PYTHIA DW PYTHIA Perugia0 PHOJET

]

  • 2

[ GeV

T

p d ! /d

ch

N

2

) d

T

p $ 1/(2

ev

N 1/

  • 10

10

  • 9

10

  • 8

10

  • 7

10

  • 6

10

  • 5

10

  • 4

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  • 1

10 1 10 ATLAS = 900 GeV s

[GeV]

T

p 1 10 Ratio 0.5 1 1.5

Data Uncertainties MC / Data

[GeV]

T

p 1 10 Ratio 0.5 1 1.5

b)

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SLIDE 10

P(N)

7

  • One entry for each N: low-mult events clearly

distinguishable from high-mult

  • Low peak sensitive to diffraction, dominated by

peripheral (LEP-like) collisions (?), no collective effects?

  • Falloff of high-N tail sensitive to UE, dominated by

hard, central collisions. Departures from LEP fragmentation? Collective effects?

  • Intermediate region (shape) sensitive to proton

mass distribution

slide-11
SLIDE 11

10

  • 5

10

  • 4

10

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  • 1

1 20 40 60 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1 20 40 60 Nch (||<1.5, all p, Nch5) Probability(Nch)

Charged Particle Multiplicity (||<1.5, all p, Nch5)

900 GeV p+pbar

Inelastic, Non-Diffractive

Pythia 6.423 Data from UA5 Collaboration, Z Phys 43(1989)357

UA5 data (NSD)

<13.9>

Perugia 0

<17.7>

Pro-pTO

<17.8>

Pro-Q2O

<17.2>

DW

<16.1>

P(N)

8

  • Extrapolations from Tevatron have ~ too low tail already at

900 GeV (cf UA5) - gets worse when we go → 2.36 → 7 TeV

  • From C. Zampolli’s talk
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SLIDE 12

10

  • 5

10

  • 4

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  • 2

10

  • 1

1 20 40 60 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1 20 40 60 Nch (||<1.5, all p, Nch5) Probability(Nch)

Charged Particle Multiplicity (||<1.5, all p, Nch5)

900 GeV p+pbar

Inelastic, Non-Diffractive

Pythia 6.423 Data from UA5 Collaboration, Z Phys 43(1989)357

UA5 data (NSD)

<13.9>

Perugia 0

<17.7>

Pro-pTO

<17.8>

Pro-Q2O

<17.2>

DW

<16.1>

P(N)

8

  • Extrapolations from Tevatron have ~ too low tail already at

900 GeV (cf UA5) - gets worse when we go → 2.36 → 7 TeV

  • So! They already knew! Why didn’t they (we) lift the tail higher?

From C. Zampolli’s talk

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SLIDE 13

P(N)

9

Tevatron tail tension. E.g., Perugia 0 already slightly high at both Tevatron energies - (more LHC data at ~ 2-3 TeV would be useful)

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SLIDE 14

〈p⊥〉(N)

10

  • One entry for each N: low-mult events clearly

distinguishable from high-mult

  • Low N sensitive to diffraction, dominated by peripheral (LEP-

like) collisions (?), no collective effects?

  • High N sensitive to UE, dominated by hard, central collisions.

Departures from LEP fragmentation? Collective effects?

  • Intermediate region (shape) sensitive to proton mass

distribution

  • Appears to be a sensitive probe of infrared
  • dynamics. Higher moments also sensitive?
slide-15
SLIDE 15
  • average transverse momentum <pT>

At N >60 model shows a rise not

〈p⊥〉(N)

11

  • Non-trivial energy dependence.
  • A (partial) tradeoff with 〈N〉 appears possible. Sufficient?

10 20 30 40 50 60 [ GeV ] %

T

p & 0.6 0.7 0.8 0.9 1 1.1 1.2 1.3

1 #

ch

n | < 2.5, ! > 500 MeV, |

T

p Data 2009 PYTHIA ATLAS MC09 PYTHIA ATLAS MC09c PYTHIA DW PYTHIA Perugia0 PHOJET

10 20 30 40 50 60 [ GeV ] %

T

p & 0.6 0.7 0.8 0.9 1 1.1 1.2 1.3 ATLAS = 900 GeV s

ch

n 10 20 30 40 50 60 Ratio 0.8 0.9 1 1.1

Data Uncertainties MC / Data

ch

n 10 20 30 40 50 60 Ratio 0.8 0.9 1 1.1

d)

slide-16
SLIDE 16

Conclusions

  • Question marks concerning energy scaling
  • Apparent tensions with Tevatron: not certain that “trivial”

retunings sufficient to span all energies?

  • What is the cause?
  • Energy-dependent energy dependence?
  • Different scaling law?
  • Different scaling for diffraction vs non-diffractive?
  • Energy- vs x- dependence?
  • Other energy- or x-dependent phenomena? (e.g., mass

distributions? collective effects? … ?)

12

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SLIDE 17

Concrete Steps

  • A complete data set (~107 events) at an intermediate

energy of 2-3 TeV would add highly valuable information (+ aid confrontation with Tevatron constraints)

  • Tuning: map out actual ECM-dependence. E.g., separate tunings

at each ECM using complete data sets [LPCC/MCnet project: H. Schulz]

  • Bring in data from Tevatron, RHIC (!), SPS, ISR, …
  • Continue to probe 900 GeV and 7 TeV with increased

number of observables and trigger conditions

  • E.g., zero bias → INEL → diffractive and ND-enhanced triggers, with

N≥1,2,3,...→ high-N / high-p⊥ → UE, …. , study scaling of each sample

  • Correlations, identified-particle fragmentation functions

13