un-ki yang, manchester 1 modeling neutrino structure functions at low q 2 arie bodek university of...
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Un-ki Yang, Manchester 1
Modeling Neutrino Structure Functions at low Q2
Arie BodekUniversity of Rochester
Un-ki YangUniversity of Manchester
NuInt 2009, Barcelona, Spain, May 18 – 22, 2009
Un-ki Yang, Manchester 2
A Model for all Q2 region?
The high Q2 region of lepton-nucleon scattering is well understood in terms of quark-parton model by a series of e/m/n DIS experiments.
But the low Q2 region is relatively poorly understood in neu-trino scattering: very important for neutrino oscillation ex-periments. Many interesting issues… PDFs at high x? Non-perturbative QCD? target mass, higher twist effects? Duality works for resonance region? Axial vector contribution? Different nuclear effects (e/ m vs )n ?
Build up a model for all Q2 region
Un-ki Yang, Manchester 3
Challenges at Low Q2
GRV
F2
A model to describe all Q2 region for e/m/n scatterings [ DIS, resonance, even photo-production(Q2=0) ]
• Resonance region is overlapped with a DIS region• Hard to extrapolate DIS contribution to low Q2 region
from high Q2 data, because of non-pQCD effects Describe DIS+resonance together using quark-parton
model
Resonance scattering in terms of quark-parton model?
Duality works, many studies by JLab
Higher twist effects, PDFs at high x? SLAC, JLab data
Un-ki Yang, Manchester 4
Effective LO Approach
Quark-Parton model:• NLO pQCD +TM+HT,
and NNLO pQCD+TM: good for DIS and res-onance
• A HT extracted from the NLO analysis: ~ NNLO pQCD term: in-dep. of e/ /m n
Effective LO approach: Use a LO PDFs with a new
scaling variable to absorb TM, HT, higher orders• A reference for (,d):
study nuclear effect
ξW =Q2 + B
{Mν [1+ (1+Q2 / ν 2 )] + A}
Q2
Q2 +CF2 (ξw ,Q2 )[LO]
mf=M*(final state)
P=M
q
Un-ki Yang, Manchester 5
Use GRV98 LO x w= [Q2+B ] / [ Mn (1+(1+Q2/n2)1/2 ) +A]
Different K factors for valence and sea
Ksea = Q2/[Q2+Csea] Kval = [1- GD
2 (Q2) ] *[Q2+C2V] / [Q2+C1V], GD
2 (Q2) = 1/ [ 1+Q2 / 0.71 ] 4
Freeze the evolution at Q2 = 0.8
Very good fits are obtained using SLAC/NMC/BCDMS p, d
with low x HERA/NMC F2
A=0.418, B=0.222, Csea = 0.381
C1V = 0.604, C2V= 0.485 2/DOF= 1268 / 1200
Fit with xw DIS F2(d)
Un-ki Yang, Manchester 7
F2(p) resonance
Photo-production (p)
(s g-proton) = 4 /pa Q2 * F2(w, Q2)
where F2(w, Q2)
= Q2 /(Q2 +C) * F2(w )
Resonance and photo-production data
Not included in the fit
2xF1 data
All DIS e/ F2 data are well described
Photo-production data (Q2=0) also work: thus included in the lat-est fit
2xF1 data (Jlab/SLAC) also work:
using F2(w)+R1998
Jlab 2xF1
Comparison with neutrino data
• Assume vector = axial • Apply nuclear corrections
using e/ scattering data Underestimated at low x=0.015 Total anti-neutrino cross section
lower by 5%?
: red, : blue,(w) ---- (x)
CCFR diff cross at En= 55 GeV
Un-ki Yang, Manchester 10
NLO Correction to xF3?
Scaling variable, w absorbs higher order effect on F2 , but not xF3; F2 data used in the fitting
Check double ratio
=> not 1 but indep. of Q2
xF3(NLO)
xF3(LO)/F2 (NLO)
F2 (LO)
NLO ratio: using VFS
Un-ki Yang, Manchester 11
Effect of xF3 NLO correction
Parameterized xF3 correction as a function of x
Neutrino cross section down by 1%
Anti-neutrino cross section up by 3%
Un-ki Yang, Manchester 12
Axial-vector contribution
In our neutrino cross section model
assumed Kaxial = Kvector
Toward axial-vector contribution• Kaxial = 1• Extract Kaxial using existent neutrino data (underway)
Un-ki Yang, Manchester 13
Axial-vector contribution
CCFR diff. cross at En= 55 GeV
Kaxial = Q2/(Q2+C) Kaxial = 1
Un-ki Yang, Manchester 14
Axial-vector contribution
CCFR diff. cross at En= 35 GeV
Kaxial = Q2/(Q2+C) Kaxial = 1
Un-ki Yang, Manchester 15
Summary and Discussions
Effective LO model with w describes all DIS and resonance data as well as photo-production data:
• Provide a good reference for neutrino cross section, (,d)
• Possible studies for axial vector contribution at Q2<1 and diff. nuclear effect
• High energy neutrino data at low Q2 is in favor of addi-tional axial vector contribution
Things to do
• Need to tune axial vector contribution using existent neutrino data and possibly with coming MINERnA
• Different nuclear effects (e vs n, F2 vs xF3):
Jlab and MINERnA data are very crucial