EW Physics in High Energy Collisions
LNF: ILC conference October 22, 2006
Denis Comelli
INFN of Ferrara
Work done in collaboration with Paolo Ciafaloni and Marcello Ciafaloni
Perturbation Theory→large log corrections at high energy
∆σ
σ = α
W
Log
2Q
2M
W2+ Log Q
2M
W2| {z }
LHC+ILC
+ 1 + o( m
2Q
2| {z }
LEP
)
IN QCD and QED only single logs (α Log
mQ22) for sufficient inclusive observables! Typical size of one loop logs:
αW
4π Log2(1 T eV )2
MW2 = 6.7%, αW
4π Log(1 T eV )2
MW2 = 1.4%
αW
αS ∼ 0.36, αS
4π Log(1 T eV )2
MW2 = 3.6%
Different kinds of Logs
• (Single Ultraviolet Logs) Running (renormalization) of the EW parameters from MW to Q.
• ( Double + Single Infrared Logs) Mass Singularities (Collinear and Infrared)
• Large αWLog2 Q2
M 2W
corrections from virtual and real W′s for cross sections with Q ≫ MW → Big Impact on LHC and ILC Physics.
• Eventually we need an improved perturbative expansion → all order resummation
• Two classes of Observables:
– Exclusive observables: (σ
e−e+→q ¯q+XQCD) Virtual EW Corrections (EW Sudakov Form factor)
– Inclusive observables: (σe
−e
+→ q ¯ q + X
QCD+ W
′s) Virtual plus Real EW corrections
• Theoretical control of the large logs:
– KLN Theorem, Block-Norsieck Theorem for QED and for QCD
– Violation of Block-Norsieck Theorem for Spontaneously broken theories
• Phenomenology at ILC: e+e− → qq¯+ XQCD + SoftW′s and at LHC: pp → (t¯b, b¯t, t¯t)
| {z }
Q−Scale
+ XQCD + SoftW′s
| {z }
QCD+EW“Background′′
QCD versus EW
• QCD, QED: massless gauge bosons ⇒ real radiation has to be added
• QCD: Confinement ⇒ average over colour charges⇒ compensation of leading double logs and factorization of collinear singularities
• EW: massive gauge bosons ⇒ real radiation not necessarily required
Free non abelian charges ⇒ average over weak charges not required
Not complete cancellation of double logs in inclusive observables, no
simple factorization
Pictorial idea of the transition of a particle (e
−) from “effective” abelian charge (clouds of photons ) for low energies (Q ≤ M
W) to “effective” non abelian charge (clouds of W ’s) at high energies (Q ≫ M
W).
σ
ΗW W
W γ γ
γ γ
γ γ
Unbroken Phase
Q >> M Q < M
Broken Phase: Abelian charge
Non Abelian charge
γ γ
e
−e
+Corrections to σ(e
−e
+→ 2 Jets + X
QCD+ sof t W
′s )
100 400 700 1000
1 3 5
Weak unp.
Weak LL Strong
Q
%
∆σ
σ ≃ α
QCD(Q)
π + α
EW4π Log
2Q
2M
W2Violation of BN Theorem for spontaneously broken U (1) gauge abelian theories
In an unbroken abelian U (1) theory (see QED) mass eigenstates coincide with the gauge eigenstates.
In a broken abelian U (1) theory (see U
Y(1)) mass eigenstates do not coincide necessary with the gauge eigenstates.
Asymptotic states that are a coherent superposition of different gauge eigenstates:
• transverse polarized fermions are a coherent superposition of left and right fermionic gauge charges.
• Z and the photon are a superposition of the B
µand the W
µ3gauge fields.
• In the scalar sector the higgs and the longitudinals goldstone bosons
are a superposition of the gauge doublets Φ and Φ
∗(having opposite
U(1) charges).
ILC with Transverse Polarized e
−e
+beams: σ(e
te
+t→ 2Jets) Asymptotic states: |f
transvi ∝ |f
Li + |f
Ri
Cross section:
hftransv|SS+ |ftransvi = hfL|SS+|fLi + hfR|SS+|fRi + 2hfL|SS+|fRi-1 -0.5 0.5 1 CosHΘL
-4%
-2%
2%
4%
6%
8%
100 DΣ
Σ
Φ= Π
2 Φ= Π
3 Φ= Π
4 , UnP Φ=0
Figure 1: BN Electroweak corrections to the differential cross section for fully transverse polarized beams at √
s = 1 TeV for various values
of φ (azimuthal angle).
EW BN corrections at LHC :
Heavy Quark Production at high energy
P P → Q ¯ Q + X where Q ¯ Q = t¯ t, t¯b, b¯ t, b¯b two kind of observables:
“Sudakov
′′: (P P → tagged final states + X) with W, Z / ∈ X
“BN
′′: (P P → tagged final states + X) with W, Z ∈ X
Cross sections Isospin Structure Tree Level (X = 0) BN corrections δij α2s α2sαw log2sˆ pp → QiQ¯j + X
i 6= j α2w α2sαw log2sˆ
u
d
t
b W
W u t
d b
W
u
u
g W
t b
b
Tree level cross section
Virtual EW corrections
Real EW corrections
αW
α2W
αS
Log2 Q/M2 2
αW Log2 Q2/M2
1000 1500 2000 2500 3000 3500 4000
!!!!s`
-17.5 -15 -12.5 -10 -7.5 -5 -2.5 DΣ
ΣH %
8pT>400 GeV<
DΣBN
ΣH DΣSud
ΣH
Sudakov and BN electroweak corrections at Leading Log order for the process P P → t¯t (similar
results hold for P P → b¯b) in the massless limit. Effects of radiative corrections on dσ
dsˆ, integrated over θ for pt > 400 GeV, ˆs being the partonic c.m. energy (which is also the t¯t invariant mass)
1500 2000 2500 3000 3500 4000
!!!s 5
10 15 20 25 30
ΣBN
ΣSud 9 dΣ
d s` =
PP®tb
PP®bt
√sˆ dependence of the ratio of BN and Sudakov cross sections for p⊥ ≥ 400 GeV. Dashed (red) line for b¯t, continuous (blue) line for t¯b.
Sudakov versus BN EW corrections:
• Sudakov EW corrections:
σSud(s) = σH e−LW (s)
P
i(ti(ti+1)+y2
i tan2 θW )
ti, yi : i-th leg isospin and hypercharge, LW(s) ≡ αW4π Log2 s
M 2W
• BN EW corrections: The hard overlap matrix is first decomposed in total t-channel isospin basis:
OH =
X
t1,t2...tn
OH
t1t2...tnPt1t2...tn
OHt1t2...tn → Ot1t2...tn(s) = e− 12LW (s)
P
ni=1 ti(ti+1)
Ot1t2...tnH inclusive (BN) and exclusive (Sudakov) case significantly different patterns of
radiative corrections:
• For Sud ti is the external leg isospin (e.g., ti = 12 for a fermion) while for BN ti is obtained by composing two single-leg isospins (e.g., 12 ⊗ 12 =0 or 1 for a fermion).
• There is a factor 2 of difference in the argument of the exponentials.
• while Sudakov corrections always depress the tree level cross section,
Structure Function approach to EW Correction: Probability to find a parton inside another parton.
σΗ p1 z1
p2 z2
σij(p1, p2, MW) =
Z
dz1 z1dz2 z2
X
kl
Fik(z1, Q, MW) σklH(z1p1, z2p2) Fjl(z2, Q, MW)
Evolution eqs for structure functions:
QCD: f
qi, f
q¯i, f
gEW :f
lL i, f
lR i, f
¯lL i, f
¯lR i, f
qL i, f
qR i, f
q¯L i, f
q¯R i, f
h, f
φa, f
Bµ, f
WµaDue to mixing effects also mixed structure functions: f
BW3, f
LR if
d
logµ2d = +
d d
logµ2= +
b
b b b
f f f
b f
i i
i
i i i
α β α β α β
A B A B A B
Resummation of the tower of logs and structure of the evolution equations:
• QCD : LL α
nSLog
nQ, NLL α
nSLog
n−1Q,...
∂f (x, µ)
∂logµ = α
WZ
1x
dz
z f( x
z , µ) P [z] as t = 0 for EW
• EW : LL α
nSLog
2nQ, NLL α
nSLog
2n−1Q,...
∂f
t=0(x, µ)
∂logµ = α
WZ
1x
dz
z f
t=0( x
z , µ) P
0[z]
∂f
t6=0(x, µ)
∂logµ = α
WZ
1x
dz
z f
t6=0( x
z , µ) (P
1[z] + Log µ M
WP
2[z])
EW Evolution eqs for the system (v, e)
Land (W
±, W
3):
e e
ν
W− W+
e e
e
W
e e
ν ν
W W
e
e e
e
− 3
3
−
W3
5 coupled eqs
− 4παW ∂fν
∂t = fν ⊗ (3PV
f f + P R
f f) + 2fe ⊗ PR
f f + 2f+ ⊗ PR
gf + f3 ⊗ PR gf
− 4παW ∂fe
∂t = fe ⊗ (3PV
f f + P R
f f) + 2fν ⊗ PR
f f + 2f− ⊗ PR
gf + f3 ⊗ PR gf
− 2π αW
∂f+
∂t = f¯e +fν
2 ⊗ PR
f g + f3 ⊗ PR
gg + f+ ⊗ (PR
gg + 2PV gg )
− 2παW ∂f−
∂t = f¯ν +fe
2 ⊗ PR
f g + f3 ⊗ PR
gg + f− ⊗ (PR
gg + 2PV gg )
− 2παW ∂f3
∂t = f¯e +fe +fν +fν¯
4 ⊗ PR
f g + (f− + f+) ⊗ PR
gg + 2f3 ⊗ PV gg
“Diagonalization” of the system of eqs: change of variables
f L
(1) = Tr{t3 F f
} = fν − fe 2
, f g
(0) = f+ + f3 + f−
3
, f g
(1) = f+ − f−
2
, f g
(2) = f+ + f− − 2f3 6
5 factorized eqs.
− ∂
∂t f L
(0) = αW 2π
3 4 f
L
(0) ⊗ (PR
f f + P V
f f) + 3 4 f
g
(0) ⊗ PR gf
− ∂
∂t f g
(0) = αW 2π
2 f g
(0) ⊗ (PR
gg + PV
gg ) + 1 2(f
L
(0) + f L¯
(0)) ⊗ PR f g
− ∂
∂t f L
(1) = αW 2π
f L
(1) ⊗ PV f f −
14 f L
(1) ⊗ (PR
f f + P V
f f) + 12 f g
(1) ⊗ PR gf
− ∂
∂t f g
(1) = αW 2π
f g
(1) ⊗ PV gg + f
g
(1) ⊗ (PR
gg + PV
gg ) + 1 2(f
L
(1) + f L¯
(1)) ⊗ PR f g
− ∂
∂t f g
(2) = αW 2π
3 f g
(2) ⊗ PV gg − f
g
(2) ⊗ (PR
gg + PV gg )