EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH
4 Decemb er 1995
CERN{PPE/95{178
NUCLEON SPIN STRUCTURE FROM POLARIZED DEEP INELASTIC
MUON-NUCLEON SCATTERING AT CERN
Vernon W. Hughes
(On b ehalf of the Spin Muon Collab ora tio n)
Physics Department, Yale University, 260 Whitney Avenue, 465 J.W. Gibbs,
New Haven, CT 06520-8121 , USA
E-mail: [email protected]
Abstract
Polarized deep inelastic inclusivemuon-nucleon scattering has b een measured at
+
CERN by the Spin Muon Collab oration (SMC) with incident energies of 100
and 190 GeV and with p olarized proton and deuteron targets in an x interval of 0.003
2 2
to 0.7, with Q ranging from 1 to 60 GeV . The spin dep endent structure functions
g have b een determined for the proton, deuteron and neutron. The fundamental
1
Bjorken p olarization sum rule has b een con rmed, and the Ellis-Ja e sum rules have
b een found to b e invalid, with the consequences that the fraction of the nucleon
spin contributed by the quark spins is small and strange quarks have a net negative p olarization.
1 INTRODUCTION
The spin structure of the nucleon can b e studied from p olarized deep inelastic inclu-
sivemuon-nucleon scattering [1{5]. Spin structure functions have not yet b een calculated
from basic QCD, but are useful for testing nucleon mo dels. With their rst moments a
basic test of QCD is made and imp ortant information ab out the comp osition of nucleon
spin is obtained. The intrinsic nucleon spin angular momentum of 1/2 must equal the
sum of the spin contributions from the quark spins , from the gluon spins G, and
from the orbital angular momentum L of quarks and gluons, i.e.
1
+G+L =1=2 (1)
z
2
The quark contribution has b een obtained.
The kinematics and variables for p olarized inclusivemuon-proton scattering in the
2 2
single photon exchange approximation are given in Fig. 1. G (; Q ) and G (; Q ) are
1 2
spin dep endent structure functions. They are related in the scaling limit to the two spin
dep endent structure functions g (x) and g (x).
1 2
2 2
M G (; Q )= g (x)
1 1
2 2
M G (; Q )= g (x)
2 2
Spin dep endent structure functions are determined by measuring di erences or asymme-
tries in the di erential scattering cross sections for the antiparallel and parallel spin cases.
These determine the virtual photon-proton absorption asymmetry A .
1
The counting rate asymmetry is related to the intrinsic muon-proton scattering
cross-section asymmetry as shown in Fig. 2. A is a virtual photon-proton asymmetry
2
arising from the interference of longitudinal and transverse photon p olarizatio ns, and the
kinematic factor is small for longitudinal muon and proton p olarizations. The kine-
matic dep olarization factor D relates the muon b eam p olarizatio n to the virtual photon
p olarizatio n. A should scale, and p ositivity limits are indicated for A and A . The usual
1 1 2
+
expressions for F and g in the quark-parton mo del are given, in which q (x)[q (x)] is
1 1
i i
the probability that a quark of avour i has its spin parallel [antiparallel] to the proton
spin.
Spin p olarization sum rules are given in Fig. 3. The Bjorken p olarization sum rule
is a rigorous consequence of QCD in the scaling limit, indep endent of the mo del of the
nucleon [6]. Perturbative QCD corrections to the Bjorken sum rule are given [7]. This sum
rule assumes only that a general quark-parton picture of the nucleon applies and that the
weak interactions of quarks and leptons are the same.
The Ellis-Ja e sum rules for the rst moments of the proton and neutron structure
functions separately are mo del-dep endent and assume that strange quarks in the nucleon
sea are unp olarized and that SU(3) symmetry applies [8]. Perturbative QCD corrections
F
are given [9].
Formulae are given in Fig. 4 for the rst moments of the proton and neutron spin
structure functions based on the op erator pro duct expansion which is basically a p er-
2
turbative QCD approach excluding non-p erturbativelowQ e ects. Assuming isospin
invariance and SU(3) symmetry and using measured values for g =g from neutron b eta
F A V
decay and of F/D from hyp eron b eta decay, the fraction of the nucleon spin contributed
by the spins of all quarks, , can b e determined. Also the fractional angular momenta
due to u,d, and s quarks separately can b e evaluated. 1 k, sµ ′ Polarized k Scattered muon muon Virtual q photon P, S Px Hadron final state Polarized Wµν nucleon
Wµν (F1, F2, G1, G2)
Kinematic variables
(Lab oratory frame)
m muon rest mass
M proton rest mass
s electron spin-four-vector
S =(O; S ) proton-spin four-vector
k =(E; k) four-momentum of incidentmuon
0 0 0
k =(E ;k ) four-momentum of scattered muon
P =(M; O) four-momentum target proton
0
q = k k =(; q ) four-momentum transfer
2
2 2 0 2
Q = q =4EE sin (=2) {(invariant mass) of virtual photon
0
energy of the virtual photon in the lab oratory = P q=M = E E
scattering angle in the lab oratory
2
x = Q =2M Bjorken scaling variable
y = =E fractional energy loss of scattered electron
P four-momentum of hadronic nal state
x
0 1
"
2 2
2
B C
a cos
d F F
2 1
2 2 0
2
B C
= + 2 tan 2 tan (E + E cos )
@ A
0
d dE 2 M 2
2 4
4E sin
2
#
+(A)
0 2 2
MG 8EE tan sin G
1 2
2 2