yu-kun song (ustc) 2013.7.29 weihai yks, jian-hua gao, zuo-tang liang, xin-nian wang,...
TRANSCRIPT
Yu-kun Song (USTC)2013.7.29 Weihai
YKS, Jian-hua Gao, Zuo-tang Liang, Xin-Nian Wang, Phys.Rev.D83:054010,2011
YKS, Jian-hua Gao, Zuo-tang Liang, Xin-Nian Wang, to be submitted
Higher twist effects in semi-inclusive DIS
Outline
Introduction to higher twist effects
Collinear expansion extended to SIDIS
Azimuthal asymmetries at twist-3 level
Nuclear effects and higher twist
Conclusions
Partonic picture of nucleon
Nucleon is the eigenstate of → Poincare invariance of induce
momentum/ angular momentum sum rules
→Test of QCD in strong coupling regime
QCDH
• 3 confined quarks• m_q ~ 200-300 MeV• static property• P, J shared by q
• a bunch of free partons• m_q ~ several MeV• hard scattering• P, J shared by q,qbar,g
Quark model(1960s) Parton model(1970s)
QCDL
1 , 1ˆ ˆ ˆ ˆ 2
. q g q gP P J J
Semi-inclusive DIS: a nice probe of nucleon
X
2 2ˆˆ O
Q
O
Sterman-Libby power counting
Leading twist
2
3 43 4ˆ ˆˆ ˆO O
Q Q Q
O
X
Higher twist (1/Q power corrections)
QCD radiative correction→“A clean test of QCD”[Georgi, Politzer, 1978]
Intrinsic [cahn,1978]
→
Power suppressed, higher twist(HT)!Magnitude of higher twist terms
~300 MeV , ~several GeV , ~10%
Not negligible for most SIDIS experiments.
k
2
2
2
2
2(2 ) 1cos
2 2
2 2cos 2
|
2
|
2
y y
y y
y
y y
k
Q
k
Q
k
Q
| |k
Q
Semi-inclusive DIS: a nice probe of nucleon
cos , cos 2 0
Collinear expansion:
Systematic way of calculating higher twist in DIS [Ellis, Furmanski, Petronzio, 1982, 1983; Qiu, 1990]
Extension to SIDIS [Liang, Wang, 2006] QCD multiple gluon scattering
→ gauge link + Higher twist terms
→ nuclear broadening [Liang, Wang, Zhou,2008]
nuclear modification of azimuthal asymmetries
[Liang, Wang, Zhou, 2008]
twist-4 corrections to unpolarized SIDIS
[YKS, Gao, Liang,Wang, 2010]
twist-3 corrections to doubly polarized SIDIS
[YKS, Gao, Liang, Wang, to be submitted]
Higher twist and collinear expansion
(0; )yLk
Leading twist: Collinear approximationBasis of QCD factorization theorem: Sterman-
Libby Power counting [Collins, 2011]
→ Leading contributions ~ Collinear approximation
Example: DISi ik x p
, ] [ , ] ([ )i A G xp A OG kQ
Ap
Ap
…
~ ( ) ( , )
( , ) | (0) (0; ) ( ) |2 2
ixp y
W h x f x k
dyf x k e N L y y N
Gauge invariant parton distribution function
• Collinear approximation• Ward identity
Higher twist: Collinear expansionLeading twist:
Non-leading twist: expansion near collinear limit
Collinear expansion is the natural and systematic way to extract HT effects.
Notice: for a well-defined expansion
, ] [ , ]
[ ,
( )
( ) [ , ] ...[ , ] ]
[
k xpi
i A G xp A
G xp
Q
GG k A k xp G xp AA
G
Ak
k
O
[[ , ] , ]i A GG xpk A
( )n nO
Gauge-invariant,So that they can be measured in Exps.
Expansion parameter
[Ellis, Furmanski, Petronzio, 1982,1983 ;Qiu,1990]
Collinear Expansion:1. Taylor expand at , and decompose
2. Apply Ward Identities
3. Sum up and rearrange all terms,
(0) 2 (0)(0) (0) ' ' ' '
' ' ' '
ˆ ˆ( ) 1 ( )ˆ ˆ( ) ( ) ... 2
H x H x AH k H x k k k A p A
k k k p
Collinear expansion in DIS
( , )ˆ ( )n ciH k i ik x p
(0) (0)1(1, ) (1, )
1 2, 2 1
ˆ ˆ( ) ( )ˆ ˆ( , ), ( , )c L
c L R
H x H xH x x p H x x
k x x i
(0) (0) (1, ) ' (1) (2, ) ' ' (2)1 2 ' 1 2 1 2 ' ' 1 2
, , ,
1 ˆ ˆ ˆˆ ˆ ˆ( ) ( ) ( , ) ( , ) ( , , ) ( , , )2
c c
c L R c L M R
W H x x H x x x x H x x x x x x
A
(0)H
(1, )ˆ cH
(2, )ˆ cH
(0) (0) ˆˆW H (1) (1, )
,
ˆˆ c
c L R
W H
(2) (2, )
, ,
ˆˆ c
c L R M
W H
e N e X
In the low region, we consider the case when final state is a quark(jet)
Compared to DIS, the only difference is the kinematical factor
Collinear expansion is naturally extended to SIDISParton distribution/correlation functions are -
dependent
Collinear expansion in SIDIS e N e q X
3 32 (2 ) ( )k cK E k k q
(0)H
(1, )ˆ cH
(2, )ˆ cH
(0) (0) ˆˆ KW H (1) (1, )
,
ˆˆ c
c L R
W H K
(2) (2, )
, ,
ˆˆ c
c L R M
W H K
k
[Liang, Wang, 2007]
k
Form of hadronic tensor after collinear approximation
: color gauge invariant
Hadronic tensor for SIDIS
(0)
(
(0) (1, ) (2, )
2 2 2 2, , ,
2 (0)(0)
2
2 (11,
, )(1)
2
2 (2,)
)
)(1
2 2
ˆ ( , )
ˆ ( ,
...
1 ˆTr ,2
1 ˆTr ,4
1 ˆTr(2 )
)
[ ]
[ ]
[
c c
c L R c L R M
L
L
NB
L NB
x
dW dW dW d
k
x
W
d k d k d k d k
d Wh
d k
d Wh
d k q p
d Wh
d k q p
k
(2)
2 (2, )(2)
(2, ) (
2 2
2, )
(2, )
ˆTr ,
1 ˆTr
ˆ ˆ( , ) ( , )
ˆ ( ) .(2 )
,
] [ ]
[ ]
L N L NB B
M NB
M
N
d W
x k x k
x khd k q p
2,3,4
3,4,
4,
(0) (0; ) ( ) , (0) (0; ) ( ) ( ) ,
(0) (0) (0) (0; ) ( ) ,
y y y D y y
D D y y
L L
L
: Projection operator
k k xp
(0) (1, ) (2, ) (2, )ˆ , , ,L L M
Structure of correlation matricesExpand in spinor space
Constraints from parity invariance
(0)5
(0) (0)
(2 (0)
( 0) (00) (0)52
)
ˆ ,
1 ˆ ˆTr Tr2
[ ] [ ]d Wh h
d k
(0) 4
4
4
4
( , , ) , (0) ( ) ,
ˆ ˆ ˆ ˆ , (0) ( ) ,
, (0) ( ) ,
, (0) ( )
ik y
ik y
ik y
ik y
p k s d ye p s y p s
d ye p s PP y PP p s
d ye p s y p s
d ye p s y p
(0)
(0) (0)
,
( , , )
( , , ) ( , , )
s
p k s
p k s p k s
Structure of correlation matricesTime reversal invariance relate and
Lorentz covariance + Parity invariance,
† †( ,0 ;0 ,0 ) ( ,0 ;0 ,0 ) ( , ; , )( , ; , ) TL L y y y L L y y y
(0)1 1
(0)1 1
...
·...( ) ( )
T T T L
L T
ks ks i ii i
ksT T
iLi
f p k M s k
k sp k Ms k
M
f f f f f
g g g g g g
1 1 1 1, , ,
, ,
: twist-2 parton distribution functions
: twist-3 parton correlation funct, i, , ons, ,
T L T
T T L T T L
f f g g
f f f f g g g g
y
SIDISDY
SIDISf DYf
TMD PDF and correlation functionsTwist-2 TMD parton distribution functions
Twist-3 TMD parton correlation functions
2·
3
2·
3
1
31
·51
2
| (0) (0; ) ( ) | ,2(2 )
, | (0) (0; ) ( ) | , ,2(2 )
, | (0) (0;2(2 )
( , )
( , )
( , )
ixp y ik y
ixp y ik yks
ixp yL
i
T
k y
dy d ye p y y p
dy d
f x k
f x k
g
y Me p s y y p s
dy d yx k e p y
L
L
L
2· 5
31
) ( ) | , ,
, | (0) (0; ) ( ) | , ,2(2 )
( , ) ixp y ikT
y
y p
Mg x
dy d ye p s y y p s
k sk
L
Unpolarized PDF
Sivers
Helicity distribution
Worm-gear
2·
3 2
2·
3
2·
3
( , )
(
| (0) (0; ) ( ) | ,2(2 )
, | (0) (0; ) ( ) | , ,2(2 )
,2(2 )
, )
( , )
ixp y ik y
ijj iixp y ik y
ixp y ik y
T
T
p dy d y ke p y y p
k
kdy d yp
f x k
f x e p s y y p sM k s
p dy d ye p
k
sf x k
L
L
2·
3 2
| (0) (0; ) ( ) | , ,
, | (0) (0; ) ( ) | , ,2( )
( , )2
ks
ijj iixp y ik y
L
sy y p s
k s
kp dy d ye p y y p
kf x k
L
L
color gauge invariant !
Structure of correlation matricesSimilar for
QCD equation of motion, ,induce relations
(1, ) (1, ) (1, )
(1, )
(1, )
5
...
ˆ
...
( )
( )
ks i ii
L L L
LT T L
LT T
i
Lks i
i
p k M s k
ip k Ms k
0i D
Re ,
Re ,
Re ,
Re ,
( )( )( )( )
T T
L L
T T
T
L
T
x
x
x
x
f
f
f
f
Im ,
Im ,
Im ,
Im .
( )( )( )( )
T T
L L
T T
T
L
T
g
g
g
x
x
x
xg
(1, ) (1, ),L R
Relations from QCD EOMSum up and , one has (up to twist-3)
Explicit color gauge invariance for and .Explicit EM gauge invariance
(0)W (1, ) (1, ),L RW W
2
{ }2
{ } { }
[
1
]
1
1 1
1( 2 )
·
( 2 ) ( 2 )· ·
· ( 2 )
·
( ) ( )
( ) ( )
ks ksT B
i iB i B i
ks
T
T L
L T TB
f f f f
f f
d Wd k q x p
d k p q
Mq x p s q x p k
p q p q
k s ii k q x p
Mg g
qg
pg
[ ] [ ] ( 2 ) ( 2 )· ·B i B iT
i iLg
iM iq x p s q x p k
p q qg
p
(0)
20
dW
dq
k
if ig
Consistency to DISIntegration over , one has
where
because of Time-reversal invariance.For DIS at twist-3 only contribute.
2d k
1 { }
1 [ ]
( ) ( 2 ) ( )·
( ) ( 2 ) ( )2 ·
iB i T
iL B i T
MW d f x q x p s f x
p q
iMi g x q x p s g x
p q
22
2
22
2
( ) ( , ) ( , ) ,2
( ) ( , ) ( , ) .2
[ ]
[ ]
T T T
T T T
kf x d k f x k f x k
M
kg x d k g x k g x k
M
( ) 0Tf x
( )Tg x
Azimuthal asymmetries at twist-3 levelCross section for
Twist-3 parton correlation function
QCD equation of motion implies
e e XN q
2 2 2 2
4 4
2
2 2 | |{ ( ) ( ) cos
( , )
(
..
co, )
2(
.
2s
}(2 )
) 1
2 2B
e
B
m q BB
B
e dx dQ p dk d k kd A y B y x
Qf f
x f x k
f x
y
Q
y
y Q k
k
y
2
3 2(0) (0;( , ) ) ( )
(2 ) 2ix y
Bp ik yp dy d y k
e N L y y Nf kk
x
(1)
(1
2
3 2
2
53 2)
( , )
( , )
( )(0) (0; ) ( )
(2 ) 2
( )(0) (0; ) ( )
(2 ) 2
ixp y ik y
iji jixp y ik
B
By
dy d y k D ye N L y y N
k
k D ydy d ye N L y y N
k
x k
x k
[Liang,Wang,2007]
(1) (1)Re( )Bx f
Azimuthal asymmetries at twist-4 level
Cross section for
Twist-4 parton correlation functions
(1) (1)2 2
(
2 2em 2
2
1) (1)
2
2
2
2 22 2
2
2
2 | |[1 (1 ) ] 4(2 ) 1 cos
|
( ,
|4(1 ) [ ]cos 2
| | 28(1 )
) ( , )
( , ) ( , )
( , ( , )])[
qBB
BB
B
B B
B
B
e kdy y y x
dxdyd k Q y Q
ky x
Q
d
dxdyd k
d
dxdyd
f x k f x k
x k x k
x k xy kk x
xQk
( )
(2, )2
2
22
2 2
2
2
| |2[1 (1
( , )
( , )) ]
B
B
B
LB
f x k
d
dxd
M
Q
ky
yd k Qxx k
(1) (1)2
22
2
2
( , ) ( , )cos
| | [ ]2(12
(( ,) )
)
1 1B B
B
Bk xy x k x k
f xy kQ
(1)2
(1)2
2 2
4 3
2{ } 5
4 3
2, (0) (0( , )
( , )
) (0; ) ( ) ,(2 ) 2
, (0) (0) (0; ) ( ) ,(2 ) 2
ixp y ik y
ix
B
kB
p y i y
k k k g dy d ye p s D L y y p s
k
ik k dy d ye p s D L yx k y s
k
x k
p
19
[YKS, Gao, Liang, Wang,2011] e N e q X
Doubly polarized at twist-3 e N e q X
[YKS, Gao, Liang, Wang, to be published]( ) ),(le N e q Xs
2 2em
1
2
2
1
2
2 2
2
2,
2 | |( ) ( ) ,
| | 2( ) ( ) ,
2 2
2 | |( )
cos
sin sin sin(2 )
sin ,
2
[( ) ]
UU l LU UT UL l LL l LT
UU
UT
q
B
B
B
B
T T Ts s
B
sT
L
L
LU
U
ed
dx dyd k Q y
x kA y B y
Q
k x M k kA y B y
M
F F s F F F s F
F f f
F
F
F
f f f f
f
Q M M
x kB y
Q
x
2 2
1
21 2
| |( ) ,
2 | |( ) ( ) ,
| | 2( ) ( )
sin
cos
cos2 2
cos cos 2[( ) ]
L LB
LL
LT s sT TB
T T s
kD y
Q
x kC y D y
Q
k x M k kC y
g
g g
g D yM Q M
g g gM
F
F
Leading twist
Twist-3 asymmetries
broadening of PDF in a nucleus
QCD multiple scattering cause broadending.
The form of broadening is simplified whenLocal color confinementA>>1Weak correlation between nucleons
If nucleon PDF take Gaussian form,
( , )qAf x k
22( ) /2
2
( , ) ( , )Fk l
F
Nq qA A
f x k d l e f x l
[Liang, Wang, Zhou, PRD2008]
2 /
( , ) ( )NqN
k
q
ef x k f x
2
2( )
2
/
, ((
( ) ))
FN
qF
kA
q
ef x k Af x
Tk
Tk
2 ˆ( )F d q
2F Broadening!
Nuclear modification of Nuclear twist-3/4 parton correlation function
Gaussian ansatz for distributionTake identical Gaussian parameter for parton
distribution/correlation functions
cc oos s, 2
22
22
( ) /2
2
( ) /(1)
2
22 (1)
2
2
222
( , ) ( , )
(ˆ2( )
, ) ( , )
F
F
k lA Nq q
l
F
A
F
k N
Af x k d l e f x l
Ax k d l e
k l
k
kl
l l
kx
2
2 2
cos cos 2,
cos cos 2eA eA
N F e Fe N
Tk
Suppressed!
Nuclear modification for
depend on dependence
Nuclear modification of sin LU
2F
2 22
2 2 2
sin 1 1 1 1exp .
sin( ) [( ) ]
eALU FeNLU F F F
k
sin LU
2(twist-2), (twist-3), F
dependence
Tk
Nuclear modification of sin LU
Sensitive to the ratio of ! /
Conclusions & outlooks Collinear expansion is naturally extended to SIDIS. Cross
section and azimuthal asymmetries for doubly polarized
are obtained up to twist-3, and unpolarized SIDIS up
to twist-4.
Much more abundant azimuthal asymmetries at high twist,
and their gauge invariant expressions are obtained.
Azimuthal asymetries act as a good probe of nuclear
properties. They are sensitive to Gaussian parameters of
HT correlation fuctions.
Numeric study of HT correlation functions, HT effects in
fragmentation functions, ,…, are underway.
ee q XN
Thanks for your attention!
e XN he