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Fred Olness 2011 CTEQ School Page 1 Heavy Quark Production Part I: Theoretical Perspective Fred Olness SMU [email protected]

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Page 1: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 1

Heavy Quark ProductionPart I: Theoretical Perspective

Fred OlnessSMU

[email protected]

Page 2: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 2

OUTLINE

➢Statement of the problem➢Status report:

Comparison of Data & Theory

➢How do we make heavy quarks➢Case studies:➢Mass-Independent Evolution

Why is it valid?

➢Conclusions➢Lunch

Page 3: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 3

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Page 4: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 4

Statement of the Problem

Page 5: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 5

A Thought Experiment:

What is the ideal way to learn about quark masses and their effects on a physical process?

As a theorists, I simply run my calculation over the full range of mass values from 0 to ∞,

and study the behavior.

Wouldn't it be great if the experiments could do the same???

Page 6: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 6

What's really in the Fermilab control room ...

Unfortunately, in real life, we can't vary parameters continuously

DO NOT FEED THE OPERATORS

Page 7: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 7

The UP Side

Quark Masses Span Wide Dynamical Range ~ 104

We can't vary the quark mass continuously, but these ``notches'' on our control panel give us a lot of flexibility

U 0.003

D 0.005

S 100

C 1.3

B 4.5

T 173

Page 8: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 8

The DOWN Side

Theorists would much prefer that quark masses only come in 2 varieties:

m = 0: Massless case. Mass plays no dynamic roleWell understood.

m = ∞: Infinite case. Mass Decouples.We can forget about this object

Page 9: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 9

Welcome to the Multi-Scale Problem

... where E is any relevant scale of the problem: Q, PT, E

T,...

Use RGE to solve this.

Single-Scale Problem in Perturbation Theory:Single-Scale Problem in Perturbation Theory:

Multi-Scale Problem in Perturbation Theory:

What do we do if we have 2 scales???

... life gets interesting.

=∑N =1

s LN=∑N =1

∞ { s log E 2

2 }

N

log E2

2 log

M H2

2

d

d log2 = ...

Page 10: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 10

STATUS REPORT: COMPARE DATA & THEORY

Let's start with a historical perspective as things change over time

Page 11: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 11

Hadroproduction of Beauty at Tevatron

Comparison of Run I data with NLO Theory

Data is high by factor of 2x or 3x

... even given µ variation

c,bg

g c,b

HISTORY

Page 12: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 12

Beauty Production at HERA

Comparison of HERA data with NLO Theory

Data is high by factor of 2x or 3x

... even given µ variationHISTORY

Page 13: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 13

Charm is reasonable

Bottom data is high by factor of 2x or 3x

Charm and Bottom Production at LEP

e+

e-

Comparison of LEP data with NLO Theory

γ

γc,b

HISTORY

Page 14: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 14

The Dilemma

Historically, calculation of processes with heavy quarks has been a challenge

Page 15: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 15

Heavy Quarks PDF's

Part of the answer ...

Essential for disparate mass scales

Heavy Quarks: How do we deal with disparate scales???

Heavy Q

uark PDF

DIS production of Heavy Quarks

Page 16: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

16

Heavy Quarks: How do we deal with disparate scales???

Problem: Heavy Quark introduces new scale:

... life gets interesting.log

Q 2

2 log

M H2

2

Solution: Resum Log(MH) in the Heavy Quark PDF's:

...include charm and bottom in the PDFs

DGLAP equation Resums iterative splittings

inside the proton

Heavy Q

uark PDF

Result: We can describe the full kinematic range from low to highthis is the essence of the ACOT renormalization scheme

DIS production of Heavy Quarks

ACOT, PRD 50, 3102

Page 17: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 17

Production of Heavy Quarks: The Problem

Heavy Excitation (HE) Heavy Creation (HC)

If you can't beat 'em, join 'em.

Which is the correct production mechanism?

Quark Channels YESt NOc ???b ???

Quark Channels NOt YESc ???b ???

Page 18: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 18

How to Join without ``Double Counting''???

Heavy Excitation (HE) Heavy Creation (HC)

c,b,t

c,b,t

Wait a minute!Since the heavy quark originally came from

a gluon splitting, these diagrams are Double Counting

Page 19: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 19

How to Join without ``Double Counting''???

Heavy Excitation (HE) Heavy Creation (HC)

TOT = HE + (HC − SUB)

Formally, NLO

Subtraction (SUB)

SUB removes the overlapping regions of phase space where the

t-channel quark is collinear and on shell

collinear on-shell

large PT

off-shell

How do we actually derive???

Page 20: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 20

There is a rigorous factorization proof ...

A formal proof was constructed by numerous

groups.

This proof was explicitly extended to the case of

massive quarks (Collins,1998)

Though Experiment:To keep things simple, let's consider scattering

off a parton target.

Page 21: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 21

Application of Factorization Formula at Leading Order (LO)

Basic Factorization Formula

At Zeroth Order:

0= f 0

⊗0⊗d 0

O 2/Q2

0= f 0⊗0⊗d 0=⊗0⊗=0

Use: f0 = δ and d0 = δ for a parton target.

Therefore:

Warning: This trivial result leads to many misconceptions at higher orders

f0 f1

for parton target

0=

0

Note: not m2/Q2

Page 22: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 22

Application of Factorization Formula at Next to Leading Order NLO)

Basic Factorization Formula

At First Order:

We used: f0 = δ and d0 = δ for a parton target.

Therefore:

σ1 f1 ⊗ σ0 σ0 ⊗ d1

f0 f1

1= f 1

⊗0⊗d 0

f 0⊗

1⊗d 0

f 0⊗

0⊗d 1

1= f 1

⊗0

1

0⊗d 1

1=1− f 1⊗0−0⊗d 1Not just

Page 23: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 23

HOMEWORK PROBLEM: NNLO WILSON COEFFICIENTS

Use the Basic Factorization Formula

At Second Order (NNLO):

Therefore:

Compute ω2 at second order.Make a diagrammatic representation of each term.

2=???

Page 24: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 24

HOMEWORK PROBLEM: CONVOLUTIONS

Part 1) Show these 3 definitions are equivalent; work out the limits of integration.

Part 2) Show convolutions are the ``natural'' way to multiply probabilities.

If f represents the heads/tails probability distribution for a single coin flip, show that the distribution of 2 coins is f⊕f and 3 coins is f⊕f⊕f.

BONUS: How many processes can you think of that don't factorize?

f ⊕g=∫ f x g y z− x ydx dy

f x=121−x1x

Page 25: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 25

ACOT is a minimal massive extension of the MS-bar scheme

In particular, m0 limit of ACOT yields MS-Bar

no finite renormalization

*Aivazis, Collins, Olness, Tung

Extensions of MS-Bar

Page 26: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 26

Compare S-ACOT with MS-Barx=0.1, Q=10NC charm F2

ACOT m0 limit yields MS-Bar: No finite renormalization

mass

F2

ACOT

MS-bar

Page 27: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 27

Compare S-ACOT with MS-Barx=0.1, Q=10NC charm F2

ACOT m0 limit yields MS-Bar: No finite renormalization

mass

F2

ACOTMS-bar

Not just a theoretical statement!!!

Page 28: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 28

x=0.1, Q=10 GeVNC charm F2

σ1 f1 ⊗ σ0

ln(m 2)

mass

F2

ACOT m0 limit yields MS-Bar: No finite renormalization

Page 29: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 29

Application of Factorization Formula at Next to Leading Order (NLO)

Combined Result:

f1 ⊗ σ0

σ0 ⊗ d1

TOTSUB

HCHE

TOT = HE + HC − SUB

Heavy Excitation Heavy

Excitation

Subtraction

01=01−{ f 1⊗00⊗d 1 }

DoubleCountingResolved

Page 30: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 30

Interaction of the separate contributions vs. energy scale

SUB

HC

HE

Heavy Excitation

Heavy Excitation Subtraction

HC

HE

TOT TOT

TOT = + -

Reduced dependence

DoubleCountingResolved

Energy Scale

Cro

ss S

e cti

on

After Subtraction

Before Subtraction

Energy Scale

Cro

ss S

e cti

on

Page 31: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 31

When do we need to worry about Heavy Quark PDFs???

Why do c(x,µ) and b(x,µ) increase so quickly???

Page 32: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 32

``Standard'' Evolution

SUB

HC

HETOT

Energy Scale

Cro

ss S

e cti

on

Page 33: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 33

Why does fb(x,µ) increase so quickly???

On occasion, certain factors can accelerate

evolution

Why does fb(x,µ) increase so quickly???

Page 34: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 34

SUB

PDF

When do we need to consider heavy quark PDF evolution ???

Page 35: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 35

B-Hadroproduction: A Case Study

Page 36: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 36

The Basic Contributions to Heavy Flavor Production

Leading Order Next to LO

Hea

vy

Cre

ati o

nH

eavy

E

xcit

a tio

n

Fixe

d-F

lavo

r S

che m

e

Var

iab l

e-F

lavo

r S

chem

e

Nason, Dawson, EllisBeenakker, Kuijf, Van Neerven, Smith

Surprise: NLO / LO ~ 2But, theory still below data

Page 37: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 37

Compare Fixed & Variable Flavor Scheme

Variable Flavor Scheme

Fixed Flavor Scheme

● To NLO, different schemes are comparable.

● K-Factor very different.

● Suggestion: VFS may provide more efficient organization of perturbation series than FFS.

● Recall: Choice of expansion point x

0 in Taylor series.

K-Factor

K-Factor

+

Page 38: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 38

The Moral

You don't have to choose which expansion point you use; by using the Heavy Quark PDF,

QCD will compensate

In practice ...

Using the heavy quark PDF's we can accommodate quark masses of any values: e.g., 10-150 to 10+150

Page 39: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 39

An Example: How the separate pieces can conspire

σ1

f1 ⊗ σ0

TOT SUBHCHE

σ0

TOT = HE + HC − SUB

Expand f(x)=x in Taylor Series about x0.

For x0=0: f(ε) = 0 + (ε− 0) + ... = ε

For x0=1: f(ε) = 1 + (ε− 1) + ... = ε

Subtraction

Heavy Excitation

Heavy Excitation

Page 40: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 40

Hadroproduction of Beauty at Tevatron: Current Understanding

B.A. Kniehl, G. Kramer, I. Schienbein, H. SpiesbergerPhysRevD.77.014011

Page 41: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 41

W/Z PRODUCTION

Page 42: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 42

Heavy Quark contribution to W/Z Production

Heavy Quark components play anincreasingly important role at the LHC

tot

cs

us

ud

cd

d/d

y(W

+)

at L

HC

y

Heavy quark PDFs essential ingredient

tot

cs

us

ud

cd

y

d/d

y(W

+)

at T

e vat

ron

Tevatron LHC

Page 43: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 43

HIGGS PRODUCTION

Page 44: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 44

Higgs Production via Heavy Quark PDFs

Page 45: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 45

INTRINSIC CHARM

& BOTTOM

Page 46: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 46

D. Duggan (D0) arXiv:0906.0136

Heavy Quarks at the Tevatron: +c and +b

Page 47: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 47

Are there Intrinsic Heavy Quarks???

b-quark1%

2 %M

omen

tum

Fr a

ctio

n

µ (GeV)

CTEQ-6.6

c-quark

∗ Most sensitive near threshold* What happens if we allow the evolution to determine charm?

Zero: No intrinsic charmPositive: Intrinsic charmNegative: Inconsistent

mbm

c

Are there Intrinsic Heavy Quarks??? Do they matter???

Page 48: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 48

SINGLE TOP

Page 49: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 49

Single Top

s-channelassociated Wt-channel

Page 50: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 50

Mass-Independent Evolution.

Why is it valid?

Page 51: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 51

DGLAP Equation and the Heavy Quark PDF

DGLAP equation Resums iterative splittings inside

the proton

DGLAP Equation

Splitting Function

HE=∫ f P a⊗ac

df i

d log2 =s

21 P j i⊗ f j ...

1 P g q =12[ x2

1−x2] M H2

2 [ x 1−x ]

Page 52: Heavy Quark Production - High Energy Physicshep.wisc.edu/cteq11/lectures/Olness_HeavyQuarks.pdf · 2011-07-14 · Fred Olness 2011 CTEQ School Page 7 The UP Side Quark Masses Span

Fred Olness 2011 CTEQ School Page 52

Effect of Heavy Quark Mass in the Calculation

valid near threshold (MH~Q)

In Summary:

Near threshold(MH~Q), mass effects cancel between HE and SUB

Above threshold(MH<<Q), mass effects can be ignored

1P splittings must match

SUB=∫ f P g ⊗ P1 g a⊗ a c

≈ f P g ⊗ P1 g a

HE=∫ f P a⊗ac

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Fred Olness 2011 CTEQ School Page 53

Effect of Heavy Quark Mass in the Calculation is Trivial

SUB=∫ f P g ⊗ P1 g a⊗ a c

HE=∫ f P a⊗ac HC=∫ f P g ⊗ gc

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Fred Olness 2011 CTEQ School Page 54

Variation of σ vs. renormalization scale µ

LO = HE result is very sensitive to the choice of scale (i.e., µ2=Q2 or Q2/4)TOT result (higher order) is stable w.r.t. the choice of scale

An accurate calculation must be stable as the renormalization scale varies

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Fred Olness 2011 CTEQ School Page 55

Outlook & Conclusions 55

The race is not always to the swift, nor the battle to the strong - but that’s the way to bet.

Runyon's Law

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Fred Olness 2011 CTEQ School Page 56

Charm & Bottom Quark Production

An interesting subject because:● Lots of data at present; more in near future● Theoretical issues of multi-scale problem

A fascinating subject because:● Theory & data not fully consistent● This should be a region we can compute

Fred Olness [email protected]

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Fred Olness 2011 CTEQ School Page 57

Keep an open mind!!!

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Fred Olness 2011 CTEQ School Page 58

LEFTOVERS

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Fred Olness 2011 CTEQ School Page 59

Dynamics & Kinematics

e γ

cN

X

cD

Heavy Quarks

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Fred Olness 2011 CTEQ School Page 60

Effect of Kinematic Mass Re-Scaling

ACOT (Aivazis, Collins, Olness, Tung) A general framework for including the heavy quark components.Phys.Rev.D50:3102-3118,1994.

S-ACOT (Simplified-ACOT) ACOT with the initial-state heavy quark masses set to zero.Phys.Rev.D62:096007,2000.

ACOT- & S-ACOT-: As above with a generalized slow-rescalingPhys.Rev.D62:096007,2000.

Q Scale

n=0n=1n=2

c

Kinematic Masses are more important than Dynamical Masses (in general)

c

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61

scale (GeV)

F2charm

m=0m0

S-ACOT-

X=0.1

F2 Charm in the threshold region

Kinematic Masses are more important than Dynamical Masses (in general)

LO

LO

Dynamic mass

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62

scale (GeV)

F2

charm

LO

NLO (m=0)

FFSGluon only

S-ACOT-

ACOTS-ACOT

X=0.1

F2 Charm in the threshold region

A man with one watch knows what time it is; a man with two is never sure.

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63

Les Houches 2009

Comparative Studies

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Fred Olness 2011 CTEQ School Page 64

LO

NLO

NNLO

Q < mH

Q > mH

Q = mH

Q = mH

Q = mH

constant term

TR type schemes

+

+

+

+

+

LO

NLO

NNLO

Q < mH

Q > mH

constant term

ACOT type schemes

+

+

+

64Schematic Summary of ACOT & TR Schemes 64

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Fred Olness 2011 CTEQ School Page 65

S-ACOTTR

S-ACOTTR

Comparison of ACOT & TR Schemes

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Fred Olness 2011 CTEQ School Page 66

Les Houches Comparative Study

ACOT & S-ACOTessentially identical

... it's all in the kinematics

FONNL & S-ACOTnumerically similar

chi(χ) prescription enforces threshold

MSTW09uses different

threshold definition

different schemedifferent

intermediate result

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Fred Olness 2011 CTEQ School Page 67

A comment about schemes

Set # pts 6HQ 6MZEUS 104 0.91 0.98 2.84 3.72

H1 484 1.02 1.04 1.50 1.22TOTAL 1925 1.04 1.06 1.26 1.30

6M GM 6HQ ZM

2/DOF

Consistent Schemes Mixed Schemes

Essential to match PDF with (hard) cross section in proper schemes!!!

2 420 2 500

Just because the PDFs or (hard) cross

sections do not match, for a consistent

scheme, the physical observable should be

invariant to O(S

N+1)

S-ACOTTR