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TRANSCRIPT
Miguel G. Echevarría
QCD Evolution of Sivers Asymmetry
May 12-16, 2014 Santa Fe (NM, US)
QCD Evolution Workshop
1
- QCD Evolution of the Sivers Asymmetry MGE, Ahmad Idilbi, Zhong-Bo Kang, Ivan Vitev. Phys.Rev. D89 (2014) 074013 [arXiv: 1401.5078] !- A Unified Treatment of the QCD Evolution of All (Un-)Polarized TMD Functions: Collins Function as a Study Case MGE, Ahmad Idilbi, Ignazio Scimemi. [arXiv: 1402.0869]
Siver Asymmetry: The Goal
2
• Distribution of unpolarized quarks inside a transversely polarized hadron:
• Improve our understanding of QCD (test theoretical tools: factorization, TMD framework,…) • How? By testing one of the main predictions of the TMD formalism: sign change of Sivers function between SIDIS and DY processes. • We want to extract it from SIDIS and make reliable predictions for DY.
fq/A"(x,k?, ~S) = f
q1 (x, k
2T )� f
?q1T (x, k2T )
(P ⇥ k?) · S?MA
QCD invariant under P and T
f
SIDISq/A" (x,k?, ~S) = f
DYq/A"(x,k?,�~
S)
f
?q1T (x, k2T )
SIDIS = �f
?q1T (x, k2T )
DY
• Different Wilson lines in SIDIS and DY processes • Soft function is universal
QCD Evolution Workshop 2014 (Santa Fe, US)
They include the soft function!
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
The Object
3
• SIDIS cross-section with a transversely polarized hadron:
d�
dxBdydzhd2Ph?
= �0(xB , y,Q2)
hFUU + sin(�h � �s)F
sin(�h��s)UT
i
QCD Evolution Workshop 2014 (Santa Fe, US)
Asin(�h��s)UT =
F sin(�h��s)UT
FUU
e(`) +A"(P ) ! e(`0) + h(Ph) +X
• Sivers asymmetry is defined as:
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
The Object
3
• SIDIS cross-section with a transversely polarized hadron:
d�
dxBdydzhd2Ph?
= �0(xB , y,Q2)
hFUU + sin(�h � �s)F
sin(�h��s)UT
i
QCD Evolution Workshop 2014 (Santa Fe, US)
Asin(�h��s)UT =
F sin(�h��s)UT
FUU
e(`) +A"(P ) ! e(`0) + h(Ph) +X
• Sivers asymmetry is defined as:
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
SIDIS factorization…• Factorization? • Relation with Sivers function? • Evolution? • …
SIDIS Factorization (1/3)
4
• Applying the SCET machinery:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
l(k) +N(P, S) ! l0(k0) + h(Ph, Sh) +X(PX)
JµQCD =
X
q
eq �µ
More details: MGE, Idilbi, Scimemi 1402.0869
JµSCET =
X
q
eq ⇠nWTn ST†
n �µSTn W
T†n ⇠n
T: MGE, Idilbi, Scimemi PRD'11
SIDIS Factorization (1/3)
4
• Applying the SCET machinery:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
l(k) +N(P, S) ! l0(k0) + h(Ph, Sh) +X(PX)
JµQCD =
X
q
eq �µ
Wµ⌫ = H(Q2/µ2)2
Nc
X
q
eq
Zd2kn?d
2kn?d2ks?�
(2)(q? + kn? � kn? + ks?)
⇥ Tr⇥�(0)(x,kn?, S)�
µ �(0)(z,kn?, Sh)�⌫⇤S(ks?)
More details: MGE, Idilbi, Scimemi 1402.0869
�(0)ij (x,kn?, S) =
1
2
Zdy
�d
2y?(2⇡)3
e
�i( 12y
�k+n�y?·kn?) hPS|
h⇠njW
Tn
i(0+, y�,y?)
hW
T†n ⇠ni
i(0) |PSi
�(0)ij (z, P h?, Sh) =
1
2
Zdy
+d
2y?(2⇡)3
e
i( 12y
+k�n �y?·kn?)
⇥ 1
z
X
X
Zh0|
hW
T†n ⇠ni
i(y+, 0�,y?) |X;PhShi hX;PhSh|
h⇠nW
Tnj
i(0) |0i
S(ks?) =
Zd
2y?(2⇡)2
e
iy?·ks?1
Nch0|Tr
hS
T†n S
Tn
i(0+, 0�,y?)
hS
T†n S
Tn
i(0) |0i
JµSCET =
X
q
eq ⇠nWTn ST†
n �µSTn W
T†n ⇠n
T: MGE, Idilbi, Scimemi PRD'11
• Pure vs. naive collinear (double counting) • Matrix elements suffer from rapidity divergences
SIDIS Factorization (2/3)
5QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
lnS = Rs(bT ,↵s) + 2D(bT ,↵s) ln
✓�+��
Q2µ2
◆ lnS� =1
2Rs(bT ,↵s) +D(bT ,↵s)ln
✓(��)2
⇣Fµ2
◆
lnS+ =1
2Rs(bT ,↵s) +D(bT ,↵s)ln
✓(�+)2
⇣Dµ2
◆
• The soft function can be split (in rapidity space) to all orders as:
⇣F ⇣D = Q4
S = S+ S�dD
dlnµ= �cusp
D ⌘ K See John’s talk
SIDIS Factorization (2/3)
5QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Fij(x,kn?, S; ⇣F , µ2;��) =
Zd
2b? e
ib?·kn? �(0)ij (x, b?, S;µ2;��) S�(bT ; ⇣F , µ
2;��)
Dij(z, P h?, Sh; ⇣D, µ
2;�+) =
Zd
2b? e
�ib?·kn? �(0)ij (z, b?, Sh;µ
2;�+) S+(bT ; ⇣D, µ
2;�+)
lnS = Rs(bT ,↵s) + 2D(bT ,↵s) ln
✓�+��
Q2µ2
◆ lnS� =1
2Rs(bT ,↵s) +D(bT ,↵s)ln
✓(��)2
⇣Fµ2
◆
lnS+ =1
2Rs(bT ,↵s) +D(bT ,↵s)ln
✓(�+)2
⇣Dµ2
◆
• The soft function can be split (in rapidity space) to all orders as:
⇣F ⇣D = Q4
• To cancel rapidity divergences, TMDPDFs and TMDFFs are defined as:
S = S+ S�dD
dlnµ= �cusp
D ⌘ K See John’s talk
SIDIS Factorization (2/3)
5QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Fij(x,kn?, S; ⇣F , µ2;��) =
Zd
2b? e
ib?·kn? �(0)ij (x, b?, S;µ2;��) S�(bT ; ⇣F , µ
2;��)
Dij(z, P h?, Sh; ⇣D, µ
2;�+) =
Zd
2b? e
�ib?·kn? �(0)ij (z, b?, Sh;µ
2;�+) S+(bT ; ⇣D, µ
2;�+)
lnS = Rs(bT ,↵s) + 2D(bT ,↵s) ln
✓�+��
Q2µ2
◆ lnS� =1
2Rs(bT ,↵s) +D(bT ,↵s)ln
✓(��)2
⇣Fµ2
◆
lnS+ =1
2Rs(bT ,↵s) +D(bT ,↵s)ln
✓(�+)2
⇣Dµ2
◆
• The soft function can be split (in rapidity space) to all orders as:
⇣F ⇣D = Q4
• To cancel rapidity divergences, TMDPDFs and TMDFFs are defined as:
This story is regulator IN-dependent!!
⇣F,D 6= ⇣ =(2v · P )2
v2• Straightforward to update the decomposition of TMDs given by [Boer, Mulders PRD’98] to include the soft function.
S = S+ S�dD
dlnµ= �cusp
D ⌘ K See John’s talk
SIDIS Factorization (3/3)
6QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Wµ⌫ = H(Q2/µ2)2
Nc
X
f
ef
Zd2b
(2⇡)2e�ib·P h?/z
⇥h⇣
F[�+]f/N (x, b?, S; ⇣F , µ
2) D[��]h/f (z, b?, Sh; ⇣D, µ2)
+F[�+�5]f/N (x, b?, S; ⇣F , µ
2) D[���5]h/f (z, b?, Sh; ⇣D, µ2)
⌘gµ⌫?
+F[i�i+�5]f/N (x, b?, S; ⇣F , µ
2) D[i�j��5]h/f (z, b?, Sh; ⇣D, µ2)
⇣g{µ?i g
⌫}j � g?ij g
µ⌫?
⌘i
• Fierzing, going to impact parameter space,…
F [�] ⌘ 1
2Tr (F�)
Soft function included in F/D
T (bT ; ⇣, µ2) =
✓⇣b2T
4e�2�E
◆�D(bT ;µ)
CQ/T (bT ;µ
2)⌦ t(µ2) +O (bT⇤QCD)
SIDIS Factorization (3/3)
6QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Wµ⌫ = H(Q2/µ2)2
Nc
X
f
ef
Zd2b
(2⇡)2e�ib·P h?/z
⇥h⇣
F[�+]f/N (x, b?, S; ⇣F , µ
2) D[��]h/f (z, b?, Sh; ⇣D, µ2)
+F[�+�5]f/N (x, b?, S; ⇣F , µ
2) D[���5]h/f (z, b?, Sh; ⇣D, µ2)
⌘gµ⌫?
+F[i�i+�5]f/N (x, b?, S; ⇣F , µ
2) D[i�j��5]h/f (z, b?, Sh; ⇣D, µ2)
⇣g{µ?i g
⌫}j � g?ij g
µ⌫?
⌘i
• Fierzing, going to impact parameter space,…
Known at 3 loops! Depends just on Q!
F [�] ⌘ 1
2Tr (F�)
• TMDs contain perturbative information at large kT (refactorization):
Collinear distribution (PDF, FF, ETQS,…)Perturbative
No divergencesAny TMD PDF/FF
Soft function included in F/D
Universal Evolution
7
• All the 8 TMDPDFs and 8 TMDFFs (leading twist) evolve with the same kernel:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
F
[�]f/N (x, b?, S; ⇣F,f , µ
2f ) = F
[�]f/N (x, b?, S; ⇣F,i, µ
2i ) R
�bT ; ⇣F,i, µ
2i , ⇣F,f , µ
2f
�
D
[�]h/f (z, b?, Sh; ⇣D,f , µ
2f ) = D
[�]h/f (z, b?, Sh; ⇣D,i, µ
2i ) R
�bT ; ⇣D,i, µ
2i , ⇣D,f , µ
2f
�
˜R�b; ⇣i, µ
2i , ⇣f , µ
2f
�= exp
⇢Z µf
µi
dµ
µ�
✓↵s(µ), ln
⇣fµ2
◆�✓⇣f⇣i
◆�D(bT ;µi)
Universal Evolution
7
• All the 8 TMDPDFs and 8 TMDFFs (leading twist) evolve with the same kernel:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
F
[�]f/N (x, b?, S; ⇣F,f , µ
2f ) = F
[�]f/N (x, b?, S; ⇣F,i, µ
2i ) R
�bT ; ⇣F,i, µ
2i , ⇣F,f , µ
2f
�
D
[�]h/f (z, b?, Sh; ⇣D,f , µ
2f ) = D
[�]h/f (z, b?, Sh; ⇣D,i, µ
2i ) R
�bT ; ⇣D,i, µ
2i , ⇣D,f , µ
2f
�
˜R�b; ⇣i, µ
2i , ⇣f , µ
2f
�= exp
⇢Z µf
µi
dµ
µ�
✓↵s(µ), ln
⇣fµ2
◆�✓⇣f⇣i
◆�D(bT ;µi)
lnS = Rs(bT ,↵s) + 2D(bT ,↵s) ln
✓�+��
Q2µ2
◆
The Soft function is universal!!
D(bT ;µi) = DR(bT ;µi) ✓(bTc � bT ) +DNP (bT ) ✓(bT � bTc)
MGE, Idilbi, Scimemi 1402.0869
Universal!!
Known at 3-loops!!
dD
dlnµ= �cusp
See John’s talk
D ⌘ K
The Object (again)
8
• SIDIS cross-section with a transversely polarized hadron:
d�
dxBdydzhd2Ph?
= �0(xB , y,Q2)
hFUU + sin(�h � �s)F
sin(�h��s)UT
i
QCD Evolution Workshop 2014 (Santa Fe, US)
Asin(�h��s)UT =
F sin(�h��s)UT
FUU
FUU =1
2⇡HDIS(Q)
Z 1
0db bJ0(Ph?b/zh)
X
q
e2qfq/A(xB , b;Q)Dh/q(zh, b;Q)
Fsin(�h��s)UT = �HDIS(Q)
Zd2b
(2⇡)2e�iPh?·b/zh P↵
h?X
q
e2qf?q(↵)1T,SIDIS(xB , b;Q)Dh/q(zh, b;Q)
e(`) +A"(P ) ! e(`0) + h(Ph) +X
• Sivers asymmetry is defined as:
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
fq/A(x, b;Q) =
Zd
2k? e
�ik?·bfq/A(x, k
2?;Q)
Dh/q(z, b;Q) =1
z
2
Zd
2pT e
�ipT ·b/zDh/q(z, p
2T ;Q)
f
?q(↵)1T (x, b;Q) =
1
M
Zd
2k? e
�ik?·bk
↵?f
?q1T (x, k2?;Q)
We have set: µ2 = ⇣A = ⇣h = Q2
Sivers Asymmetry: The Strategy
9
Describe unpolarized DY+SIDIS with proper QCD Evolution and a universal non-perturbative model
Miguel G. Echevarría - Nikhef/VU - May 12th 2014QCD Evolution Workshop 2014 (Santa Fe, US)
Model Sivers function and fit it with SIDIS data and using previously extracted parameters
Flip sign to make predictions for planned measurements in DY
1.-
2.-
3.-
• W/Z boson production (CDF, D0, CMS) • DY lepton-pair production at (E288, E605) • SIDIS process (COMPASS, HERMES)
• SIDIS process (JLab, COMPASS, HERMES)
• DY lepton-pair production (Fermilab, CERN) • W boson production (RHIC)
We perform the resummation of large logarithms at NLL accuracy
HDIS,DY (Q2, µ2) = 1 +↵sCF
2⇡
3ln
Q2
µ2� ln2
Q2
µ2� 8 +
⇡2
6+⇡2
�
Unpolarized DY+SIDIS: Perturbative
10
• The necessary perturbative ingredients at NLL are:
LO hard part
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
HDIS,DY (Q2, µ2) = 1 +↵sCF
2⇡
3ln
Q2
µ2� ln2
Q2
µ2� 8 +
⇡2
6+⇡2
�
Unpolarized DY+SIDIS: Perturbative
10
• The necessary perturbative ingredients at NLL are:
F
i/h
(x, b;µ) =X
a
Z 1
x
d⇠
⇠
C
i/a
✓x
⇠
, b;µ
◆f
a/h
(⇠, µ) +O(b⇤QCD)
LO hard part
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
HDIS,DY (Q2, µ2) = 1 +↵sCF
2⇡
3ln
Q2
µ2� ln2
Q2
µ2� 8 +
⇡2
6+⇡2
�
Unpolarized DY+SIDIS: Perturbative
10
• The necessary perturbative ingredients at NLL are:
F
i/h
(x, b;µ) =X
a
Z 1
x
d⇠
⇠
C
i/a
✓x
⇠
, b;µ
◆f
a/h
(⇠, µ) +O(b⇤QCD)
Natural scale: c/bfq/A(x, b; c/b) = fq/A(x, c/b) + · · ·
Dh/q(z, b; c/b) =1
z
2Dh/q(z, c/b) + · · ·LO coefficients
c = 2e��E
LO hard part
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Unpolarized DY+SIDIS: Perturbative
11
˜R(b; c/b,Q) = exp
(�Z Q
c/b
dµ
µ
✓�cusp ln
Q2
µ2+ �V
◆)✓Q2
(c/b)2
◆�D(b;c/b)
�(1) = CF
�(2) =CF
2
CA
✓67
18� ⇡2
6
◆� 10
9TRnf
�
�V (1) = �3
2CF
D(1) =CF
2lnµ2b2
c2�! D(1)(b;µ = c/b) = 0
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Unpolarized DY+SIDIS: Perturbative
11
˜R(b; c/b,Q) = exp
(�Z Q
c/b
dµ
µ
✓�cusp ln
Q2
µ2+ �V
◆)✓Q2
(c/b)2
◆�D(b;c/b)
�(1) = CF
�(2) =CF
2
CA
✓67
18� ⇡2
6
◆� 10
9TRnf
�
�V (1) = �3
2CF
D(1) =CF
2lnµ2b2
c2�! D(1)(b;µ = c/b) = 0
↵s(µ)
4⇡=
1
�0x� �1
�
30
lnx
x
2+
�
21
�
50
ln2x� lnx� 1
x
3+
�2
�
40
1
x
3+ · · ·
For NLL
x = lnµ
2
⇤2QCD
We take into account the thresholds and integrate analytically
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Unpolarized DY+SIDIS: Non-Perturbative
12
• Thus, the perturbative part of the TMD PDF/FF is written at NLL as:
• We need to separate and parameterize the non-perturbative large b contributions:
Fpert(x, b;Q) = f(x, c/b) exp
(�Z Q
c/b
dµ
µ
✓�cusp ln
Q
2
µ
2+ �
V
◆)
1/b � ⇤QCD
We use simple gaussian NP input No x/z dependence No flavor-dependence g2 is universal
We use here the b* prescription proposed by CSS
fq/A(x, b;Q) = fq/A(x, c/b⇤) e�gpdf
1 b2exp
(�Z Q
c/b⇤
dµ
µ
✓�cusp ln
Q
2
µ
2+ �
V
◆)✓Q
2
Q
20
◆� 14 g2b
2
Dh/q(z, b;Q) =
1
z
2Dh/q(z, c/b⇤) e
�gff1 b2
exp
(�Z Q
c/b⇤
dµ
µ
✓�cusp ln
Q
2
µ
2+ �
V
◆)✓Q
2
Q
20
◆� 14 g2b
2
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Q20 = 2.4GeV2
b⇤ =bp
1 + (b/bmax
)2
Unpolarized DY+SIDIS: Non-Perturbative
13
• From [Konychev, Nadolsky PLB'06]:
QCD Evolution Workshop 2014 (Santa Fe, US)
0.5 1 1.5 2 2.5 0.5 1 1.5 2 2.5
110
120
130
140
150
0.1
0.15
0.2
0.25
0.3
0
0.1
0.2
0.3
0.4
0.5
0.60
-0.05
-0.1
-0.15
-0.2
a 2!GeV
2 "
bmax !GeV−1"
Renormalonanalysis !Tafat"
a 2!GeV
2 "
a 3!GeV
2 "
bmax !GeV−1"
r2
C3=b0
C3=2 b0
a 1!GeV
2 "
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
g2 = 0.184± 0.018 GeV2
bmax
= 1.5 GeV�1
Extracted from DY and W/Z
Unpolarized DY+SIDIS: Non-Perturbative
13
• From [Konychev, Nadolsky PLB'06]:
QCD Evolution Workshop 2014 (Santa Fe, US)
0.5 1 1.5 2 2.5 0.5 1 1.5 2 2.5
110
120
130
140
150
0.1
0.15
0.2
0.25
0.3
0
0.1
0.2
0.3
0.4
0.5
0.60
-0.05
-0.1
-0.15
-0.2
a 2!GeV
2 "
bmax !GeV−1"
Renormalonanalysis !Tafat"
a 2!GeV
2 "
a 3!GeV
2 "
bmax !GeV−1"
r2
C3=b0
C3=2 b0
a 1!GeV
2 "
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
g2 = 0.184± 0.018 GeV2
bmax
= 1.5 GeV�1
Extracted from DY and W/Z
0 1 2 3 4 5 6 bTHGeV-1L0.00.20.40.60.81.01.21.4
HQf êQiL-2Dg2=0.16
DR NLL
Qi = 2.4 GeVQf = 2 GeV
✓Qf
Qi
◆�2hD(b⇤;µb)+
R Qiµb
dµµ �cusp+ 1
4 g2b2i
✓Qf
Qi
◆�2DR(b;Qi)
• We choose g2=0.16 for bmax=1.5:
MGE, Idilbi, Schafer, Scimemi EPJC'13
Unpolarized DY+SIDIS: Non-Perturbative
14
• Regarding the intrinsic widths:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
hk2?iQ0 = 0.25� 0.44 GeV2
hp2T iQ0 = 0.16� 0.20 GeV2 gpdf1 =hk2?iQ0
4
g↵1 =hp2T iQ0
4z2
Schweitzer, Teckentrup, Metz PRD'10 Torino group
Good description of HERMES data
Unpolarized DY+SIDIS: Non-Perturbative
14
• Regarding the intrinsic widths:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
hk2?iQ0 = 0.25� 0.44 GeV2
hp2T iQ0 = 0.16� 0.20 GeV2 gpdf1 =hk2?iQ0
4
g↵1 =hp2T iQ0
4z2
• The tuned parameters that give a good global description of DY+SIDIS are:
Schweitzer, Teckentrup, Metz PRD'10 Torino group
Good description of HERMES data
hk2?iQ0 = 0.38 GeV2
hp2T iQ0 = 0.19 GeV2
g2
= 0.16 GeV2
bmax
= 1.5 GeV�1
Unpolarized DY+SIDIS: Non-Perturbative
14
• Regarding the intrinsic widths:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
hk2?iQ0 = 0.25� 0.44 GeV2
hp2T iQ0 = 0.16� 0.20 GeV2 gpdf1 =hk2?iQ0
4
g↵1 =hp2T iQ0
4z2
• The tuned parameters that give a good global description of DY+SIDIS are:
Schweitzer, Teckentrup, Metz PRD'10 Torino group
Good description of HERMES data
hk2?iQ0 = 0.38 GeV2
hp2T iQ0 = 0.19 GeV2
g2
= 0.16 GeV2
bmax
= 1.5 GeV�1
• TMD factorization works for qT<Q, so we consider data accordingly!!
Unpolarized DY+SIDIS: Non-Perturbative
14
• Regarding the intrinsic widths:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
hk2?iQ0 = 0.25� 0.44 GeV2
hp2T iQ0 = 0.16� 0.20 GeV2 gpdf1 =hk2?iQ0
4
g↵1 =hp2T iQ0
4z2
• The tuned parameters that give a good global description of DY+SIDIS are:
Schweitzer, Teckentrup, Metz PRD'10 Torino group
Good description of HERMES data
hk2?iQ0 = 0.38 GeV2
hp2T iQ0 = 0.19 GeV2
g2
= 0.16 GeV2
bmax
= 1.5 GeV�1
• TMD factorization works for qT<Q, so we consider data accordingly!!
Plots…
15
0
0.02
0.04
0.06
0.08
0 5 10 15 20
CMS Zp+p 3s=7 TeV
pT (GeV)
1/m
dm
/dp T
(GeV
-1)
0
200
400
600
800
0 5 10 15 20
CDF Z run 1D0 Z
p+p– 3s=1.8 TeV
pT (GeV)
dm/d
p T (p
b/G
eV)
0
500
1000
1500
2000
2500
0 5 10 15 20
D0 Wp+p
– 3s=1.8 TeV
pT (GeV)
dm/d
p T (p
b/G
eV)
• W/Z boson production at Tevatron (D0 and CDF) and LHC (CMS)
QCD Evolution Workshop 2014 (Santa Fe, US)
Unpolarized DY+SIDIS: Plots (1/4)
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
16
• DY lepton-pair production at Fermilab (E288 and E605)
10-2
10-1
1
10
0 0.2 0.4 0.6 0.8 1 1.2 1.4
E288 3s=19.4 GeV
pT (GeV)
Edm
/d3 p
(pb/
GeV
2 )
10-2
10-1
1
10
0 0.2 0.4 0.6 0.8 1 1.2 1.4
E288 3s=23.8 GeV
pT (GeV)
Edm
/d3 p
(pb/
GeV
2 )
10-2
10-1
1
10
0 0.2 0.4 0.6 0.8 1 1.2 1.4
E288 3s=27.4 GeV
pT (GeV)
Edm
/d3 p
(pb/
GeV
2 )
10-2
10-1
1
0 0.2 0.4 0.6 0.8 1 1.2 1.4
E605 3s=38.8 GeV
pT (GeV)
Edm
/d3 p
(pb/
GeV
2 )
QCD Evolution Workshop 2014 (Santa Fe, US)
Data from top to bottom correspond to different invariant mass Q.
Unpolarized DY+SIDIS: Plots (2/4)
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
17
• SIDIS Multiplicities at CERN (COMPASS)
10-1
1
10
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8
COMPASSDeuteron h+
�xB� = 0.093�Q2�=7.57 GeV2
pT (GeV)
dN/d
z d2 p T
(GeV
-2)
10-2
10-1
1
10
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8
COMPASSDeuteron h-
�xB� = 0.093�Q2�=7.57 GeV2
pT (GeV)
dN/d
z d2 p T
(GeV
-2)
Data from top to bottom correspond to different z regions
QCD Evolution Workshop 2014 (Santa Fe, US)
Unpolarized DY+SIDIS: Plots (3/4)
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
18
• SIDIS Multiplicities at DESY (HERMES)
10-1
1
10
0 0.1 0.2 0.3 0.4 0.5 0.6
HERMESProton /+
�xB� = 0.117
�Q2�=2.45 GeV2
pT (GeV)
dN/d
z d2 p T
(GeV
-2)
10-2
10-1
1
10
0 0.1 0.2 0.3 0.4 0.5 0.6
HERMESProton /-
�xB� = 0.117
�Q2�=2.45 GeV2
pT (GeV)
dN/d
z d2 p T
(GeV
-2)
QCD Evolution Workshop 2014 (Santa Fe, US)
Unpolarized DY+SIDIS: Plots (4/4)
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Data from top to bottom correspond to different z regions
18
• SIDIS Multiplicities at DESY (HERMES)
10-1
1
10
0 0.1 0.2 0.3 0.4 0.5 0.6
HERMESProton /+
�xB� = 0.117
�Q2�=2.45 GeV2
pT (GeV)
dN/d
z d2 p T
(GeV
-2)
10-2
10-1
1
10
0 0.1 0.2 0.3 0.4 0.5 0.6
HERMESProton /-
�xB� = 0.117
�Q2�=2.45 GeV2
pT (GeV)
dN/d
z d2 p T
(GeV
-2)
QCD Evolution Workshop 2014 (Santa Fe, US)
Unpolarized DY+SIDIS: Plots (4/4)
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
We have a good description of SIDIS+DY data
Data from top to bottom correspond to different z regions
Sivers Function: Parameterization
19
• Sivers function is OPEd onto the Qiu-Sterman matrix element:
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
f
↵SIDIS1T f/P (z, bT ; ⇣F , µ) =
X
j
✓ib
↵?2
◆Z 1
z
dx1 dx2
x1 x2Cf/j(z/x1, z/x2, bT ; ⇣F , µ)TF j/P (x1, x2;µ) +O(bT⇤QCD)
• With evolution and non-perturbative model:
µ2 = ⇣F
Q20 = 2.4GeV2
• We parameterize the Qiu-Sterman function as:
Tq,F (x, x, µ) = Nq(↵q + �q)(↵q+�q)
↵
↵qq �
�q
q
x
↵q (1� x)�qfq/A(x, µ)
f↵SIDIS1T f/P (z, bT ; c/bT ) =
✓ib↵?2
◆TF f/P (z, z; c/bT ) + · · ·
˜f↵SIDIS1T f/P (z, b;Q) =
✓ib↵
2
◆TF f/P (z, z; c/b⇤)e
�gsivers1 b2
⇥ exp
(�Z Q
c/b⇤
dµ
µ
✓�cusp ln
Q2
µ2+ �V
◆)✓Q2
Q20
◆� 14 g2b
2
Kouvaris, Qiu, Vogelsang, Yuan PRD’06
Sivers Function: Fit
20
• We use the parameters obtained from the analysis of the unpolarized DY+SIDIS:
QCD Evolution Workshop 2014 (Santa Fe, US)
�
2/d.o.f. = 1.3
↵u = 1.051+0.192�0.180 ↵d = 1.552+0.303
�0.275
↵sea = 0.851+0.307�0.305 � = 4.857+1.534
�1.395
Nu = 0.106+0.011�0.009 Nd = �0.163+0.039
�0.046
Nu = �0.012+0.018�0.020 Nd = �0.105+0.043
�0.060
Ns = 0.103+0.548�0.604 Ns = �1.000±1.757
hk2s?i = 0.282+0.073�0.066 GeV2
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
hk2?iQ0 = 0.38 GeV2
hp2T iQ0 = 0.19 GeV2
g2
= 0.16 GeV2
bmax
= 1.5 GeV�1
• We fit 11 parameters, chi2/dof=1.3:
gsivers1 =hk2s?i4
Sivers Function: Fit
20
• We use the parameters obtained from the analysis of the unpolarized DY+SIDIS:
QCD Evolution Workshop 2014 (Santa Fe, US)
�
2/d.o.f. = 1.3
↵u = 1.051+0.192�0.180 ↵d = 1.552+0.303
�0.275
↵sea = 0.851+0.307�0.305 � = 4.857+1.534
�1.395
Nu = 0.106+0.011�0.009 Nd = �0.163+0.039
�0.046
Nu = �0.012+0.018�0.020 Nd = �0.105+0.043
�0.060
Ns = 0.103+0.548�0.604 Ns = �1.000±1.757
hk2s?i = 0.282+0.073�0.066 GeV2
Miguel G. Echevarría - Nikhef/VU - May 12th 2014
hk2?iQ0 = 0.38 GeV2
hp2T iQ0 = 0.19 GeV2
g2
= 0.16 GeV2
bmax
= 1.5 GeV�1
• We fit 11 parameters, chi2/dof=1.3:
gsivers1 =hk2s?i4
Plots…
Sivers Asymmetry: Fit
21
• COMPASS proton target
-0.1
-0.05
0
0.05
0.1
AU
T
Sive
rsh-
COMPASS Proton
-0.1
-0.05
0
0.05
0.1
10 -2 10 -1
xB
AU
T
Sive
rs
h+
0.25 0.5 0.75 1zh
0.2 0.4 0.6 0.8ph� (GeV)
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Sivers Asymmetry: Fit
22
• COMPASS deuteron target
-0.1
-0.05
0
0.05
0.1
AU
T
Sive
rs
/-
COMPASS Deuteron
-0.1
-0.05
0
0.05
0.1
10 -2 10 -1
xB
AU
T
Sive
rs
/+
0.25 0.5 0.75 1zh
0.2 0.4 0.6 0.8ph� (GeV)
-0.1
-0.05
0
0.05
0.1
AU
T
Sive
rs
K-
COMPASS Deuteron
-0.1
-0.05
0
0.05
0.1
10 -2 10 -1
xB
AU
T
Sive
rs
K+
0.25 0.5 0.75 1zh
0.2 0.4 0.6 0.8ph� (GeV)
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Sivers Asymmetry: Fit
23
• HERMES proton target
-0.1
-0.05
0
0.05
0.1AU
T
Sive
rs
/0
HERMES Proton
-0.1
-0.05
0
0.05
0.1AU
T
Sive
rs
/-
-0.1
-0.05
0
0.05
0.1
10 -1
xB
AU
T
Sive
rs
/+
0.2 0.4 0.6zh
0.2 0.4 0.6ph� (GeV)
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Sivers Asymmetry: Fit
24
-0.1
-0.05
0
0.05
0.1
0.15A
UT
Sive
rsK-
HERMES Proton
-0.1
-0.05
0
0.05
0.1
0.15
10 -1
xB
AU
T
Sive
rs
K+
0.2 0.4 0.6zh
0.2 0.4 0.6ph� (GeV)
• HERMES proton target
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Sivers Asymmetry: Fit
25
• JLAB neutron target
-0.2
0
0.2AU
T
Sive
rs
/-JLAB Neutron
-0.2
0
0.2
0.1 0.2 0.3 0.4xB
AU
T
Sive
rs/+
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Sivers Asymmetry: Fit
26
• Qiu-Sterman function:
-0.1
-0.05
0
0.05
0.1
10 -3 10 -2 10 -1
u
d
x
x T q,
F(x,
x)
10 -3 10 -2 10 -1
u–
d–
x10 -3 10 -2 10 -1 1
s
s–
x
• SIDIS data only constrain u and d quark flavours. Sea quarks are not constrained.
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Tq,F (x, x, µ) = Nq(↵q + �q)(↵q+�q)
↵
↵qq �
�q
q
x
↵q (1� x)�qfq/A(x, µ)
Q20 = 2.4GeV2
Sivers Asymmetry: Predictions for DY
27
• DY at RHIC: proton(polarized)-proton at √s=510GeV
-0.04
-0.03
-0.02
-0.01
0
0.01
-4 -3 -2 -1 0 1 2 3 4y
AN
Integrate: pT: [0,1]GeV Q: [4,9]GeV
Integrate: pT: [0,3]GeV
-0.03-0.02-0.01
00.010.020.030.04
-2 -1.5-1 -0.5 0 0.5 1 1.5 2
W+
y
AN
0
0.01
0.02
0.03
0.04
-2 -1.5-1 -0.5 0 0.5 1 1.5 2
W<
y
AN
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Forward rapidity region Prediction: 2%-3%
Prediction: 2%-3%
Sivers Asymmetry: Predictions for DY
28
• DY at CERN (COMPASS): 190GeV Pi- beam to scatter on polarized proton target. √s=18.9GeV.
• DY at Fermilab: 120GeV proton beam to scatter on proton target. Either polarized beam or polarized target. √s=15.1GeV.
-0.04
-0.03
-0.02
-0.01
0
-0.6 -0.4 -0.2 -0 0.2 0.4 0.6xF
AN
-0.02
-0.01
0
0.01
0.02
-0.6 -0.4 -0.2 -0 0.2 0.4 0.6xF
AN
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
xF = xa � xb
Polarized hadronProjected measurement at xF=-0.2 Prediction: 3%-4%
Polarized target Polarized beam
Prediction: 1%-2%
Integrate: pT: [0,1]GeV Q: [4,9]GeV
Integrate: pT: [0,1]GeV Q: [4,9]GeV
Conclusions & Outlook
29
• TMDs should contain the soft function to be well-defined.
• The evolution of all the 8 TMDPDFs and 8 TMDFFs is driven by the same evolution kernel.
• We know the perturbative ingredients to get resummation up to NNLL.
!• We found a simple non-perturbative model that can describe reasonably well all SIDIS, DY and W/Z boson data.
• Using that model and proper QCD evolution, we fit the Sivers asymmetry in SIDIS and made reliable predictions for DY and W boson to be compared with coming measurements (RHIC, CERN (COMPASS), Fermilab).
!• Improvements: NLL to NNLL, different models, and different ways to avoid the Landau pole.
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
See Stefano's talk
Conclusions & Outlook
29
• TMDs should contain the soft function to be well-defined.
• The evolution of all the 8 TMDPDFs and 8 TMDFFs is driven by the same evolution kernel.
• We know the perturbative ingredients to get resummation up to NNLL.
!• We found a simple non-perturbative model that can describe reasonably well all SIDIS, DY and W/Z boson data.
• Using that model and proper QCD evolution, we fit the Sivers asymmetry in SIDIS and made reliable predictions for DY and W boson to be compared with coming measurements (RHIC, CERN (COMPASS), Fermilab).
!• Improvements: NLL to NNLL, different models, and different ways to avoid the Landau pole.
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
See Stefano's talk
Back up slides
30QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Unpolarized DY+SIDIS
31
• SIDIS process:
• We measure the hadron multiplicity:
e(`) +A(P ) ! e(`0) + h(Ph) +X
dN
dzhd2Ph?
=d�
dxBdQ2dzhd
2Ph?
�d�
dxBdQ2
d�
dxBdQ2= �
DIS0
X
q
e
2qfq/A(xB , Q)
d�
dxBdQ2dzhd2Ph?=
�DIS0
2⇡HDIS(Q)
X
q
e2q
Z 1
0db bJ0(Ph?b/zh)fq/A(xB , b;Q)Dh/q(zh, b;Q)
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Unpolarized DY+SIDIS
31
• SIDIS process:
• We measure the hadron multiplicity:
e(`) +A(P ) ! e(`0) + h(Ph) +X
dN
dzhd2Ph?
=d�
dxBdQ2dzhd
2Ph?
�d�
dxBdQ2
d�
dxBdQ2= �
DIS0
X
q
e
2qfq/A(xB , Q)
d�
dxBdQ2dzhd2Ph?=
�DIS0
2⇡HDIS(Q)
X
q
e2q
Z 1
0db bJ0(Ph?b/zh)fq/A(xB , b;Q)Dh/q(zh, b;Q)
Collins 11 MGE, Idilbi, Scimemi JHEP’12, PLB'13
Well-defined TMDsDepends just on Q
See John’s talkWe have set: µ2 = ⇣A = ⇣h = Q2
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014
Unpolarized DY+SIDIS
32
• Drell-Yan process:
A(PA) +B(PB) ! [�⇤ !]`+`�(y,Q, p?) +X
• W/Z boson production:
A(PA) +B(PB) ! W/Z(y, p?) +X
d�
dQ2dyd2p?=
�DY0
2⇡HDY (Q)
X
q
e2q
Z 1
0db bJ0(p?b)fq/A(xa, b;Q)fq/B(xb, b;Q)
d�W
dyd2p?=
�W0
2⇡HDY (Q)
X
q,q0
|Vqq0 |2Z 1
0db bJ0(q?b)fq/A(xa, b;Q)fq0/B(xb, b;Q)
d�Z
dyd2p?=
�Z0
2⇡HDY (Q)
X
q
�V 2q +A2
q
� Z 1
0db bJ0(q?b)fq/A(xa, b;Q)fq0/B(xb, b;Q)
QCD Evolution Workshop 2014 (Santa Fe, US) Miguel G. Echevarría - Nikhef/VU - May 12th 2014