Basics of QCD Lecture 2: higher orders, divergences
Gavin Salam
CERN Theory Unit
ICTP–SAIFR school on QCD and LHC physics July 2015, S˜aoPaulo, Brazil Neither lattice QCD nor perturbative QCD can offer a full solution to using QCD at colliders
What the community has settled on is 1) factorisation of initial state non-perturbative problem from 2) the “hard process,” calculated perturbatively supplemented with 3) non-perturbative modelling of final-state hadronic-scale processes (“hadronisation”).
Gavin Salam (CERN) QCD basics 2 2 / 17 Factorization
Z H Cross section for some hard σ x process in hadron-hadron p 1 2 p x 1 2 collisions
p1 p2 Z Z 2 2 2 σ = dx1fq/p(x1, µ ) dx2fq¯/p(x2, µ )σ ˆ(x1p1, x2p2, µ ) , ˆs = x1x2s
2 I Total X-section is factorized into a ‘hard part’σ ˆ(x1p1, x2p2, µ ) Calculated, e.g. with methods discussed in many of the other courses
2 I and parton distribution functions (PDFs): fq/p(x, µ ) is the probability of finding a quark q inside a proton p, and carrying a fraction x of its momentum. Determined experimentally, cf. later [For now, don’t worry about µ2 “factorisation scale” argument]
Gavin Salam (CERN) QCD basics 2 3 / 17 Factorization
Z H Cross section for some hard σ x process in hadron-hadron p 1 2 p x 1 2 collisions
p1 p2 Z Z 2 2 2 σ = dx1fq/p(x1, µ ) dx2fq¯/p(x2, µ )ˆσ(x1p1, x2p2, µ ) , ˆs = x1x2s
2 I Total X-section is factorized into a ‘hard part’σ ˆ(x1p1, x2p2, µ ) Calculated, e.g. with methods discussed in many of the other courses
2 I and parton distribution functions (PDFs): fq/p(x, µ ) is the probability of finding a quark q inside a proton p, and carrying a fraction x of its momentum. Determined experimentally, cf. later [For now, don’t worry about µ2 “factorisation scale” argument]
Gavin Salam (CERN) QCD basics 2 3 / 17 Factorization
Z H Cross section for some hard σ x process in hadron-hadron p 1 2 p x 1 2 collisions
p1 p2 Z Z 2 2 2 σ = dx1fq/p(x1, µ ) dx2fq¯/p(x2, µ )ˆσ(x1p1, x2p2, µ ) , ˆs = x1x2s
2 I Total X-section is factorized into a ‘hard part’σ ˆ(x1p1, x2p2, µ ) Calculated, e.g. with methods discussed in many of the other courses
2 I and parton distribution functions (PDFs): fq/p(x, µ ) is the probability of finding a quark q inside a proton p, and carrying a fraction x of its momentum. Determined experimentally, cf. later [For now, don’t worry about µ2 “factorisation scale” argument]
Gavin Salam (CERN) QCD basics 2 3 / 17 Factorisation is a term that has several related meanings in QCD.
Intimately connected with infrared divergences
We can start understanding those by studying a process that’s simpler than hadron collisions: e+e− collisions with hadronic final states.
Gavin Salam (CERN) QCD basics 2 4 / 17 p1 p1 −ie γ −ie γ µ k ,ε µ k ,ε
p2 p2
[e+e− → qq¯] [Soft-collinear emission] Soft gluon amplitude Start with γ∗ → qq¯: p1
−ieγ µ Mqq¯ = −u¯(p1)ieqγµv(p2)
p2 Emit a gluon:
A i Mqqg¯ =u ¯(p1)igs /t ieqγµv(p2) p/1 + /k i A − u¯(p1)ieqγµ igs /t v(p2) p/2 + /k
Make gluon soft ≡ k p1,2; ignore terms suppressed by powers of k: A p1. p2. p/v(p) = 0, Mqqg¯ ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k p//k + /kp/ = 2p.k
Gavin Salam (CERN) QCD basics 2 5 / 17 [e+e− → qq¯] [Soft-collinear emission] Soft gluon amplitude Start with γ∗ → qq¯: p1
−ieγ µ Mqq¯ = −u¯(p1)ieqγµv(p2)
p2 Emit a gluon:
p p A i 1 1 M =u ¯(p )ig /t ie γ v(p ) −ie γ −ie γ qqg¯ 1 s p/ + /k q µ 2 µ k ,ε µ 1 k ,ε i A p p − u¯(p1)ieqγµ igs /t v(p2) 2 2 p/2 + /k
Make gluon soft ≡ k p1,2; ignore terms suppressed by powers of k: A p1. p2. p/v(p) = 0, Mqqg¯ ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k p//k + /kp/ = 2p.k
Gavin Salam (CERN) QCD basics 2 5 / 17 [e+e− → qq¯] [Soft-collinear emission] Soft gluon amplitude Start with γ∗ → qq¯: p1
−ieγ µ Mqq¯A= −iu¯(p1)ieqγµv(p2) p/1 + /k A u¯(p1)igs /t ieqγµv(p2) = −igs u¯(p1)/ 2 eqγµt v(p2) p/1 + /k (p1 + k) p Use /A/B = 2A.B − /B/A: 2 Emit a gluon:
1 A = −igs u¯(p1)[2.(p1 + k) − (p/ + /k)/] eqγpµt v(p2) p A i 1 2 1 1 M =u ¯(p )ig /t ie γ v(p ) (p1−ie+ γ k) −ie γ qqg¯ 1 s p/ + /k q µ 2 µ k ,ε µ 1 k ,ε Useu ¯(p1)p/1 i= 0 and k p1 (p1, k massless) − u¯(p )ie γ ig /t Av(p ) p2 p2 1 q µ p/ + /k s 2 2 1 A ' −igs u¯(p1)[2.p1] 2 eqγµt v(p2) Make gluon soft ≡ k p1,2; ignore(p terms1 + k) suppressed by powers of k: p1. A = −igs u¯(p1)eqγµt v(p2) p .k p1. p2. p/v(p) = 0, M ' u¯(p )ie γ t1Av(p|) g {z − } qqg¯ 1 q µ pure2 QEDs spinor structure p1.k p2.k p//k + /kp/ = 2p.k
Gavin Salam (CERN) QCD basics 2 5 / 17 [e+e− → qq¯] [Soft-collinear emission] Soft gluon amplitude Start with γ∗ → qq¯: p1
−ieγ µ Mqq¯ = −u¯(p1)ieqγµv(p2)
p2 Emit a gluon:
p p A i 1 1 M =u ¯(p )ig /t ie γ v(p ) −ie γ −ie γ qqg¯ 1 s p/ + /k q µ 2 µ k ,ε µ 1 k ,ε i A p p − u¯(p1)ieqγµ igs /t v(p2) 2 2 p/2 + /k
Make gluon soft ≡ k p1,2; ignore terms suppressed by powers of k: A p1. p2. p/v(p) = 0, Mqqg¯ ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k p//k + /kp/ = 2p.k
Gavin Salam (CERN) QCD basics 2 5 / 17 [e+e− → qq¯] [Soft-collinear emission] Squared amplitude
2 2 X A p1. p2. |Mqqg¯ | ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k A,pol 2 2 2 p1 p2 2 2 2p1.p2 = −|Mqq¯|CF gs − = |Mqq¯|CF gs p1.k p2.k (p1.k)(p2.k) Include phase space:
3~ 2 2 d k 2 2p1.p2 dΦqqg¯ |Mqqg¯ | ' (dΦqq¯|Mqq¯|) 3 CF gs 2E(2π) (p1.k)(p2.k) | {z } dS Note property of factorisation into hard qq¯ piece and soft-gluon emission piece, dS. dφ 2α C 2p .p θ ≡ θ dS = EdE dcos θ · s F 1 2 p1k 2π π (2p1.k)(2p2.k) φ = azimuth
Gavin Salam (CERN) QCD basics 2 6 / 17 [e+e− → qq¯] [Soft-collinear emission] Squared amplitude
2 2 X A p1. p2. |Mqqg¯ | ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k A,pol 2 2 2 p1 p2 2 2 2p1.p2 = −|Mqq¯|CF gs − = |Mqq¯|CF gs p1.k p2.k (p1.k)(p2.k) Include phase space:
3~ 2 2 d k 2 2p1.p2 dΦqqg¯ |Mqqg¯ | ' (dΦqq¯|Mqq¯|) 3 CF gs 2E(2π) (p1.k)(p2.k) | {z } dS Note property of factorisation into hard qq¯ piece and soft-gluon emission piece, dS. dφ 2α C 2p .p θ ≡ θ dS = EdE dcos θ · s F 1 2 p1k 2π π (2p1.k)(2p2.k) φ = azimuth
Gavin Salam (CERN) QCD basics 2 6 / 17 [e+e− → qq¯] [Soft-collinear emission] Squared amplitude
2 2 X A p1. p2. |Mqqg¯ | ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k A,pol 2 2 2 p1 p2 2 2 2p1.p2 = −|Mqq¯|CF gs − = |Mqq¯|CF gs p1.k p2.k (p1.k)(p2.k) Include phase space:
3~ 2 2 d k 2 2p1.p2 dΦqqg¯ |Mqqg¯ | ' (dΦqq¯|Mqq¯|) 3 CF gs 2E(2π) (p1.k)(p2.k) | {z } dS Note property of factorisation into hard qq¯ piece and soft-gluon emission piece, dS. dφ 2α C 2p .p θ ≡ θ dS = EdE dcos θ · s F 1 2 p1k 2π π (2p1.k)(2p2.k) φ = azimuth
Gavin Salam (CERN) QCD basics 2 6 / 17 [e+e− → qq¯] [Soft-collinear emission] Squared amplitude
2 2 X A p1. p2. |Mqqg¯ | ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k A,pol 2 2 2 p1 p2 2 2 2p1.p2 = −|Mqq¯|CF gs − = |Mqq¯|CF gs p1.k p2.k (p1.k)(p2.k) Include phase space:
3~ 2 2 d k 2 2p1.p2 dΦqqg¯ |Mqqg¯ | ' (dΦqq¯|Mqq¯|) 3 CF gs 2E(2π) (p1.k)(p2.k) | {z } dS Note property of factorisation into hard qq¯ piece and soft-gluon emission piece, dS. dφ 2α C 2p .p θ ≡ θ dS = EdE dcos θ · s F 1 2 p1k 2π π (2p1.k)(2p2.k) φ = azimuth
Gavin Salam (CERN) QCD basics 2 6 / 17 [e+e− → qq¯] [Soft-collinear emission] Squared amplitude
2 2 X A p1. p2. |Mqqg¯ | ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k A,pol 2 2 2 p1 p2 2 2 2p1.p2 = −|Mqq¯|CF gs − = |Mqq¯|CF gs p1.k p2.k (p1.k)(p2.k) Include phase space:
3~ 2 2 d k 2 2p1.p2 dΦqqg¯ |Mqqg¯ | ' (dΦqq¯|Mqq¯|) 3 CF gs 2E(2π) (p1.k)(p2.k) | {z } dS Note property of factorisation into hard qq¯ piece and soft-gluon emission piece, dS. dφ 2α C 2p .p θ ≡ θ dS = EdE dcos θ · s F 1 2 p1k 2π π (2p1.k)(2p2.k) φ = azimuth
Gavin Salam (CERN) QCD basics 2 6 / 17 [e+e− → qq¯] [Soft-collinear emission] Squared amplitude
2 2 X A p1. p2. |Mqqg¯ | ' u¯(p1)ieqγµt v(p2) gs − p1.k p2.k A,pol 2 2 2 p1 p2 2 2 2p1.p2 = −|Mqq¯|CF gs − = |Mqq¯|CF gs p1.k p2.k (p1.k)(p2.k) Include phase space:
3~ 2 2 d k 2 2p1.p2 dΦqqg¯ |Mqqg¯ | ' (dΦqq¯|Mqq¯|) 3 CF gs 2E(2π) (p1.k)(p2.k) | {z } dS Note property of factorisation into hard qq¯ piece and soft-gluon emission piece, dS. dφ 2α C 2p .p θ ≡ θ dS = EdE dcos θ · s F 1 2 p1k 2π π (2p1.k)(2p2.k) φ = azimuth
Gavin Salam (CERN) QCD basics 2 6 / 17 [e+e− → qq¯] [Soft-collinear emission] Soft & collinear gluon emission
Take squared matrix element and rewrite in terms of E, θ,
2p1.p2 1 = 2 2 (2p1.k)(2p2.k) E (1 − cos θ) So final expression for soft gluon emission is 2α C dE dθ dφ dS = s F π E sin θ 2π NB:
I It diverges for E → 0 — infrared (or soft) divergence
I It diverges for θ → 0 and θ → π — collinear divergence
Soft, collinear divergences derived here in specific context of e+e− → qq¯ But they are a very general property of QCD
Gavin Salam (CERN) QCD basics 2 7 / 17 [e+e− → qq¯] [Soft-collinear emission] Soft & collinear gluon emission
Take squared matrix element and rewrite in terms of E, θ,
2p1.p2 1 = 2 2 (2p1.k)(2p2.k) E (1 − cos θ) So final expression for soft gluon emission is 2α C dE dθ dφ dS = s F π E sin θ 2π NB:
I It diverges for E → 0 — infrared (or soft) divergence
I It diverges for θ → 0 and θ → π — collinear divergence
Soft, collinear divergences derived here in specific context of e+e− → qq¯ But they are a very general property of QCD
Gavin Salam (CERN) QCD basics 2 7 / 17 [e+e− → qq¯] [Soft-collinear emission] Soft & collinear gluon emission
Take squared matrix element and rewrite in terms of E, θ,
2p1.p2 1 = 2 2 (2p1.k)(2p2.k) E (1 − cos θ) So final expression for soft gluon emission is 2α C dE dθ dφ dS = s F π E sin θ 2π NB:
I It diverges for E → 0 — infrared (or soft) divergence
I It diverges for θ → 0 and θ → π — collinear divergence
Soft, collinear divergences derived here in specific context of e+e− → qq¯ But they are a very general property of QCD
Gavin Salam (CERN) QCD basics 2 7 / 17 [e+e− → qq¯] [Soft-collinear emission] Soft & collinear gluon emission
Take squared matrix element and rewrite in terms of E, θ,
2p1.p2 1 = 2 2 (2p1.k)(2p2.k) E (1 − cos θ) So final expression for soft gluon emission is 2α C dE dθ dφ dS = s F π E sin θ 2π NB:
I It diverges for E → 0 — infrared (or soft) divergence
I It diverges for θ → 0 and θ → π — collinear divergence
Soft, collinear divergences derived here in specific context of e+e− → qq¯ But they are a very general property of QCD
Gavin Salam (CERN) QCD basics 2 7 / 17 If probability of gluon emission diverges, then how can you calculate anything beyond leading order?
Kinoshita-Lee-Nauenberg theorem tells as that if you sum over allowed states, then result must be finite.
Gavin Salam (CERN) QCD basics 2 8 / 17 2α C Z dE Z dθ σ = σ 1 + s F R(E/Q, θ) tot qq¯ π E sin θ 2α C Z dE Z dθ − s F V (E/Q, θ) π E sin θ
[Total cross sections] [Real-virtual cancellation] Real-virtual cancellations: total X-sctn
Total cross section: sum of all real and virtual diagrams
2 p1 −ie γ −ie γ ie γ µ k ,ε +µ x µ
p2
Total cross section must be finite. If real part has divergent integration, so must virtual part. (Unitarity, conservation of probability)
I R(E/Q, θ) parametrises real matrix element for hard emissions, E ∼ Q. I V (E/Q, θ) parametrises virtual corrections for all momenta (a “physical fudge” — exact way is to do calc. in dim. reg.)
Gavin Salam (CERN) QCD basics 2 9 / 17 2α C Z dE Z dθ − s F V (E/Q, θ) π E sin θ
[Total cross sections] [Real-virtual cancellation] Real-virtual cancellations: total X-sctn
Total cross section: sum of all real and virtual diagrams
2 p1 −ie γ −ie γ ie γ µ k ,ε +µ x µ
p2
Total cross section must be finite. If real part has divergent integration, so must virtual part. (Unitarity, conservation of probability) 2α C Z dE Z dθ σ = σ 1 + s F R(E/Q, θ) tot qq¯ π E sin θ
I R(E/Q, θ) parametrises real matrix element for hard emissions, E ∼ Q. I V (E/Q, θ) parametrises virtual corrections for all momenta (a “physical fudge” — exact way is to do calc. in dim. reg.)
Gavin Salam (CERN) QCD basics 2 9 / 17 [Total cross sections] [Real-virtual cancellation] Real-virtual cancellations: total X-sctn
Total cross section: sum of all real and virtual diagrams
2 p1 −ie γ −ie γ ie γ µ k ,ε +µ x µ
p2
Total cross section must be finite. If real part has divergent integration, so must virtual part. (Unitarity, conservation of probability) 2α C Z dE Z dθ σ = σ 1 + s F R(E/Q, θ) tot qq¯ π E sin θ 2α C Z dE Z dθ − s F V (E/Q, θ) π E sin θ
I R(E/Q, θ) parametrises real matrix element for hard emissions, E ∼ Q. I V (E/Q, θ) parametrises virtual corrections for all momenta (a “physical fudge” — exact way is to do calc. in dim. reg.)
Gavin Salam (CERN) QCD basics 2 9 / 17 [Total cross sections] [Real-virtual cancellation] Total X-section (cont.)
2α C Z dE Z dθ σ = σ 1 + s F (R(E/Q, θ) − V (E/Q, θ)) tot qq¯ π E sin θ
I From calculation: limE→0 R(E/Q, θ) = 1. I For every divergence R(E/Q, θ) and V (E/Q, θ) should cancel:
lim (R − V ) = 0 , lim (R − V ) = 0 E→0 θ→0,π Result:
I corrections to σtot come from hard (E ∼ Q), large-angle gluons
I Soft gluons don’t matter: 2 I Physics reason: soft gluons emitted on long timescale ∼ 1/(Eθ ) relative to collision (1/Q) — cannot influence cross section. I Transition to hadrons also occurs on long time scale (∼ 1/Λ) — and can also be ignored.
I Correct renorm. scale for αs: µ ∼ Q — perturbation theory valid.
Gavin Salam (CERN) QCD basics 2 10 / 17 [Total cross sections] [Real-virtual cancellation] Total X-section (cont.)
2α C Z dE Z dθ σ = σ 1 + s F (R(E/Q, θ) − V (E/Q, θ)) tot qq¯ π E sin θ
I From calculation: limE→0 R(E/Q, θ) = 1. I For every divergence R(E/Q, θ) and V (E/Q, θ) should cancel:
lim (R − V ) = 0 , lim (R − V ) = 0 E→0 θ→0,π Result:
I corrections to σtot come from hard (E ∼ Q), large-angle gluons
I Soft gluons don’t matter: 2 I Physics reason: soft gluons emitted on long timescale ∼ 1/(Eθ ) relative to collision (1/Q) — cannot influence cross section. I Transition to hadrons also occurs on long time scale (∼ 1/Λ) — and can also be ignored.
I Correct renorm. scale for αs: µ ∼ Q — perturbation theory valid.
Gavin Salam (CERN) QCD basics 2 10 / 17 [Total cross sections] [Real-virtual cancellation] Total X-section (cont.)
2α C Z dE Z dθ σ = σ 1 + s F (R(E/Q, θ) − V (E/Q, θ)) tot qq¯ π E sin θ
I From calculation: limE→0 R(E/Q, θ) = 1. I For every divergence R(E/Q, θ) and V (E/Q, θ) should cancel:
lim (R − V ) = 0 , lim (R − V ) = 0 E→0 θ→0,π Result:
I corrections to σtot come from hard (E ∼ Q), large-angle gluons
I Soft gluons don’t matter: 2 I Physics reason: soft gluons emitted on long timescale ∼ 1/(Eθ ) relative to collision (1/Q) — cannot influence cross section. I Transition to hadrons also occurs on long time scale (∼ 1/Λ) — and can also be ignored.
I Correct renorm. scale for αs: µ ∼ Q — perturbation theory valid.
Gavin Salam (CERN) QCD basics 2 10 / 17 [Total cross sections] [Real-virtual cancellation] Total X-section (cont.)
2α C Z dE Z dθ σ = σ 1 + s F (R(E/Q, θ) − V (E/Q, θ)) tot qq¯ π E sin θ
I From calculation: limE→0 R(E/Q, θ) = 1. I For every divergence R(E/Q, θ) and V (E/Q, θ) should cancel:
lim (R − V ) = 0 , lim (R − V ) = 0 E→0 θ→0,π Result:
I corrections to σtot come from hard (E ∼ Q), large-angle gluons
I Soft gluons don’t matter: 2 I Physics reason: soft gluons emitted on long timescale ∼ 1/(Eθ ) relative to collision (1/Q) — cannot influence cross section. I Transition to hadrons also occurs on long time scale (∼ 1/Λ) — and can also be ignored.
I Correct renorm. scale for αs: µ ∼ Q — perturbation theory valid.
Gavin Salam (CERN) QCD basics 2 10 / 17 [Total cross sections] [Real-virtual cancellation] Total X-section (cont.)
2α C Z dE Z dθ σ = σ 1 + s F (R(E/Q, θ) − V (E/Q, θ)) tot qq¯ π E sin θ
I From calculation: limE→0 R(E/Q, θ) = 1. I For every divergence R(E/Q, θ) and V (E/Q, θ) should cancel:
lim (R − V ) = 0 , lim (R − V ) = 0 E→0 θ→0,π Result:
I corrections to σtot come from hard (E ∼ Q), large-angle gluons
I Soft gluons don’t matter: 2 I Physics reason: soft gluons emitted on long timescale ∼ 1/(Eθ ) relative to collision (1/Q) — cannot influence cross section. I Transition to hadrons also occurs on long time scale (∼ 1/Λ) — and can also be ignored.
I Correct renorm. scale for αs: µ ∼ Q — perturbation theory valid.
Gavin Salam (CERN) QCD basics 2 10 / 17 [Total cross sections] [Real-virtual cancellation] Total X-section (cont.)
2α C Z dE Z dθ σ = σ 1 + s F (R(E/Q, θ) − V (E/Q, θ)) tot qq¯ π E sin θ
I From calculation: limE→0 R(E/Q, θ) = 1. I For every divergence R(E/Q, θ) and V (E/Q, θ) should cancel:
lim (R − V ) = 0 , lim (R − V ) = 0 E→0 θ→0,π Result:
I corrections to σtot come from hard (E ∼ Q), large-angle gluons
I Soft gluons don’t matter: 2 I Physics reason: soft gluons emitted on long timescale ∼ 1/(Eθ ) relative to collision (1/Q) — cannot influence cross section. I Transition to hadrons also occurs on long time scale (∼ 1/Λ) — and can also be ignored.
I Correct renorm. scale for αs: µ ∼ Q — perturbation theory valid.
Gavin Salam (CERN) QCD basics 2 10 / 17 [Total cross sections] [Real-virtual cancellation] Total cross section at NLO
Our treatment so far was a bit rough: designed to emphasize physical nature of divergences.
In practice calculations will be done in 4 + dimensions and infrared divergences translate to powers of 1/.
Full final answer for σtot at next-to-leading order (NLO) is, for massless quarks, 3 α C σ = σ 1 + s F + O α2 tot qq¯ 4 π s
Gavin Salam (CERN) QCD basics 2 11 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
x x x x x x x 0 loops (tree−level)
o o o o 1 loop
ø ø 2 loops
0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
x x x x x x x 0 loops (tree−level) α 0 s o o o o 1 loop α 1 s 2 ø ø Z 2 loops α 2 s α 3 i j s 0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
x x x x x x x 0 loops (tree−level) α 0 s o o o o 1 loop α 1 s ø ø Z Z 2 loops X α 2 s α 3 j i i j s 0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
x x x x x x x 0 loops (tree−level) α 0 s o o o o 1 loop α 1 s ø ø Z Z 2 loops X α 2 s α 3 j i i j s 0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
x x x x x x x 0 loops (tree−level) α 0 s o o o o 1 loop α 1 s 2 ø ø Z 2 loops α 2 s α 3 i j s 0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
x x x x x x x 0 loops (tree−level) α 0 s o o o o 1 loop α 1 s ø ø Z Z 2 loops X α 2 s α 3 j i i j s 0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
Z @ LO
x x x x x x x 0 loops (tree−level) α 0 s o o o o 1 loop α 1 s ø ø Z 2 loops α 2 s α 3 i j s 0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
Z @ NLO
x x x x x x x 0 loops (tree−level) α 0 s o o o o 1 loop α 1 s ø ø Z 2 loops α 2 s α 3 i j s 0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 [Total cross sections] [Beyond NLO] Beyond NLO: e.g. NNLO
Z @ NNLO
x x x x x x x 0 loops (tree−level) α 0 s o o o o 1 loop α 1 s ø ø Z 2 loops α 2 s α 3 i j s 0 1 2 3 4 5 6
ij → Z + n partons
To get NpLO you need the Born (LO) diagram supplemented with all combination of n loops and p − n extra emissions, with 0 ≤ n ≤ p.
Gavin Salam (CERN) QCD basics 2 12 / 17 Exercise: substitute αs(MZ ) = 0.118 to get a feel for the quality of the expansion.
Question: did we have to write the result as a function of αs(Q)? Actually, it is standard to write results as a function of αs(µR ), where µR is the renormalisation scale, to be taken µR ∼ Q.
[Total cross sections] [Beyond NLO] total X-section (cont.)
Dependence of total cross section on only hard gluons is reflected in ‘good behaviour’ of perturbation series:
α (Q) α (Q)2 α (Q)3 σ = σ 1 + 1.045 s + 0.94 s − 15 s + tot qq¯ π π π Λ4 + O α4 + O s Q4
(Coefficients given for Q = MZ )
Gavin Salam (CERN) QCD basics 2 13 / 17 Question: did we have to write the result as a function of αs(Q)? Actually, it is standard to write results as a function of αs(µR ), where µR is the renormalisation scale, to be taken µR ∼ Q.
[Total cross sections] [Beyond NLO] total X-section (cont.)
Dependence of total cross section on only hard gluons is reflected in ‘good behaviour’ of perturbation series:
α (Q) α (Q)2 α (Q)3 σ = σ 1 + 1.045 s + 0.94 s − 15 s + tot qq¯ π π π Λ4 + O α4 + O s Q4
(Coefficients given for Q = MZ )
Exercise: substitute αs(MZ ) = 0.118 to get a feel for the quality of the expansion.
Gavin Salam (CERN) QCD basics 2 13 / 17 [Total cross sections] [Beyond NLO] total X-section (cont.)
Dependence of total cross section on only hard gluons is reflected in ‘good behaviour’ of perturbation series:
α (Q) α (Q)2 α (Q)3 σ = σ 1 + 1.045 s + 0.94 s − 15 s + tot qq¯ π π π Λ4 + O α4 + O s Q4
(Coefficients given for Q = MZ )
Exercise: substitute αs(MZ ) = 0.118 to get a feel for the quality of the expansion.
Question: did we have to write the result as a function of αs(Q)? Actually, it is standard to write results as a function of αs(µR ), where µR is the renormalisation scale, to be taken µR ∼ Q.
Gavin Salam (CERN) QCD basics 2 13 / 17 [Total cross sections] [Scale dependence] Scale dependence
Let’s express NLO results for arbitrary µR in terms of αs(Q):
nlo σ (µR ) = σqq¯ (1 + c1 αs(µR )) µ = σ 1 + c α (Q) − 2c b ln R α2(Q) + O α3 qq¯ 1 s 1 0 Q s s