Meson transition form factors from a QCD model field theory

Meson transition form factors from a QCD model field theory

Prog. Port. Nucl. Phys.. Vol. 36, pp. 97-106. 1996 Copyright Q 1996 Elscvier Science Ltd Printed in Great Britain. All rights reserved 0146-6410/96 $3...

694KB Sizes 4 Downloads 119 Views

Prog. Port. Nucl. Phys.. Vol. 36, pp. 97-106. 1996 Copyright Q 1996 Elscvier Science Ltd Printed in Great Britain. All rights reserved 0146-6410/96 $32.00 + 0.00

SO146-6410 (96) 00013-O

Meson Transition Form Factors from a QCD Model Field Theory P. C. TANDY Center/or Nucleor Rescnrch, Deportment ofPhysics. Kent State University, Kent, OH 44242, U.S.A.

Abstract We dircu~s form factors and coupling constants for the 7*x07, pwwand 7rp interactions generated by a model field theory that producea finite rise qg melon modes. The approach implements dressingof the vertiow and propagator8con&tent with dynamical cbiral symmetry breaking, gauge invariance,quark confinement and perturbative QCD.

1

Introduction

We generate meson8 M Qq composites with intrinsic siee from the Global Color Model (GCM). [l, 21 This is a phenomenologically succemful QCD-based model field theory that permits an accessible and covariant description of mteon substructure and interactiona in terme of dynamically dressed quark degrees of freedom. The GCM action is

where j:(2) = rj(2)yrt,q(2). The formulation is in Euclidean space with metric 6,, and in this work, we consider only two flavors (u and d). The GCM represents the gluon sector by a finite range effective gluon twepoint function (Dt,,,(2) = &D(z), in the Feynman-like gauge chosen here), thus formalizing the Abelian approximation to QCD. Nevertheless, the chiral anomalies [2] are properly embedded and this i important for several of the topics addreseed here. A closely related model is that of Nambu and Jona-Laainio [3] where the interaction is a contact one. In practical terms the difference is important. Quark confinement can be incorporated within the GCM and will prevent a spurious gq width for the heavier meeons. Finite E&Xeffects aarociated with dynamical quark seKenergiea and meson BetheSdpeter (BS) amplitudea provide natural regularization of many of the loop integrals for key physical qurntitiea. Studier of merons and baryone within the GCM require hadroni&ion techniques [4] and a recent review [5] is available. For mesons, a brief summary is the following. A functional change of path integration variables allows the recond term of (1) to be eliminated in favor of ~(2)AaBp(2,g)q(~) and a term quadratic in 8. Theae auxiliary booon fieldr 8”(e,v) transform aa &)A”q(2) where A” are the matricer from Fiera reordering of the current-current term. The saddle point configuration of B” yielda a quark &f-energy (equivalent to the ladder Dyson-Schwinger equation (DSE)) and expansion about there identi&s a meeon action in terms of field vruiabla B for propagating modes. The resulting bare inveroe propagator may be ured to generate eigenvectom f+(q, P) for expansion of the bilocd fields

98

P. C. Tandy

88 fjh

1eaving an effective local field variable

PI + rt4q, W(P),

mass-shell, conjugate

the F so defined are solutions to z - y and P is conjugate

To allow for electromagnetic generalized

[6] to account

to the bare quarks. as the quarks.

version

(EM)

coupling

On the

The momentum

coupled

q is

method

can be

(& -+ 8, - idAY)

now dresses the photon-quark

vertex

at the quark level can be translated

for ease of computation,

meson action

the bosonization

field minimally

&[A,]

of the EM coupling

may be adapted

S[A,r,p,...]

equation.

to the meson modes,

electromagnetic

The saddle point configuration

of the resulting

for each meson mode.

b(P)

Bethe-Salpeter

to q.

for a background

Gauge invariance

level. [6] The method simplified

of the ladder

and for our purposes

as well

to the meson

here, the following

shall suffice

Tr~(-)‘[S(i7~~.iTr,+i7~~.P;rp+...)]” n=l n

=

+~I[~~f,D-‘f,a+pf,D-‘T,p+...] t hS[A,p,w]. The trace here is over spin, flavor and color as well as space-time dominant

covariant

(i.e.

single Dirac matrix)

dressed quark propagator

and in the term CS[A,p,

S[A,]

We have employed only the

The EM field A, appears

’ li near in the indicated w] wh’K h IS

and is at most linear in A, in the more useful approaches. the first term cancels

coordinates.

for each meson mode. When

A, = 0, the n = 1 contribution

Then S = s[O] has ladder DSE content

giving S(p)-’

When A, # 0, rather than expand about the new saddle point configurations, the configurations

that produce

quark-photon

on the choice of I, A central The necessary

vertex

$p,

k)-’

that

of the resulting

calculation

meson mass-shells overall

approach,

the phenomenological parametrized

efforts

input.

amplitudes

ITS(X) = a+)

=

c

action

of meson propagators

in the timelike recent

domain.

and interaction

the dressed

the representation

e-21+ ~~

2(x + 7sL2) - I +

e-+tfiz)

-cme

2( z + ??Z2)2 = XUS, FV = X’UV, ti of quark production

This form is guided by a confining

The

fitted

with pQCD

GeV,

experimental

(232

is complicated momenta

p uv(p’)

by the

to access the

and limitations

as the vehicle

of the

that

carries

we employ the

t as(p’),

?TA scattering

-21

mrr =

(3)

- e-2(z+*2))

,

where m is the bare in S-matrix

momentum amplitudes

model DSE [9] and by the behavior

quantities

lengths

+ -$&I

in the complex

thresholds

m = 6.7 MeV,

physics MeV)3,

= m/X,

in the deep Euclidean

c = 0.0406,

soft chiral

< qq >IGcV~=

functions Euclidean

bsz

This S(p) is an entire function

X = 0.568

is the dressed quark propagator.

propagator

(bl, + b2G)

b12

3s

It is consistent

term of Eq. (2) depends

the capabilities

= -i7.

S(p)

- k) where I’,(p; q) is

k)A,(p

[7]

momentum

to ensure the absence

to complex quark

= Cy.p+E(p)+m.

we study here. vertex

In order to explore

with x = p2/X2, scale.

p-

about

we choose to expand about

The third

for bare hadrons

must be continued

have chosen

Within

for calculations.

to the interactions

effective

fact that the dressed quark propagator

+I’“(+;

= 6(p - k)S(p)-’

is convenient

but it does not contribute

element

from

the 6s term since in that case the meson fields are defined as fluctuations

the saddle point configurations.

a dressed

only in the meson fields

produced

to within

20%.

found in realistic

and X is the sufficient

processes.

[8]

DSE studies.

[lo]

The parameters

are

b4) = (0.118,2.51,0.525,0.169,1

by this parameterization 0.54 fm together =

T:“’

mass

for physical

region up to ln(p2) corrections.

and (bo, bl, b2,4,

140 MeV,

quark

plane, a condition

x

10w4).

are [7] fir = 92.4 MeV, with

reproduction

of the

99

Meson Transition Form Factors

The choice of quark propagator parameters is equivalent to an implicit choice of effective gluon propagator and vertex in the underlying DSE dynamics. [lo] Ghost contributions in DSE studies have been studied iu Landau gauge and shown not to modify the qualitative features of quark and gluon propagators.[ll] Quantitatively, ghosts provide a small (< 10%) effect. We therefore expect that a wellchosen phenomenological quark propagator captures those aspects of the underlying dynamics that is of practical importance for the chiral physics quantities that guide it. Independent applications, such as those contained here, provide important additional tests of this standpoint. In terms of the equivalent representation S(p)-’ = i7 *pA(p') + B(p2) + m, the chiral limit for the pion mass-shell Bethe-Salpeter amplitude is ??,(p; P2 = 0) = i7s.rB(p2, m = 0)/f= since the DSE for B(p2) and the Bethe-Salpeter equation for the pion invariant amplitude become identical. [12] Hence the pion is both a gq bound state and a Goldstone boson. For finite m we use the pseudoscalar form l’,(p;P) M i7~~B(p”,m)/f, consistent with PCAC. We use the Ball-Chiu [13] Ansatz for the dressed quark photon vertex which is I’,(p; q) = @,,(p; q), where $ = f(ro + f) is the quark charge operator, and f,(p;q)

= -ir,&4(~+)

+ 4~4)

+ 37~~(-4(~-)

- A(P+)) + (NP-1

- B(P+))]

(5)

with p& = p f z. This vertex satisfies the Ward-Takahashi identity, transforms correctly and has the correct perturbative limit; but it is not unique. We have investigated several other choices [lo] and found no significant change in our conclusions.

2

The n’+y+y Form Factor

The pion charge form factor for space-like momenta is one of the simplest but non-trivial testing grounds for applications of QCD to hadronic properties. A closely related quantity that has received less attention is the 7*x0 + 7 transition form factor. [14] Here the photon momentum dependence maps out a particular off-shell extension of the axial anomaly. [15] P resently available data for this transition form factor in the space-like region Q2 < 2.5 GeV’ is from the CELLO [M] collaboration at the PETRA storage ring where the process e+e- -+ e+e-x0 was measured with geometry requiring one of the two intermediate photons to be almost real. There is renewed interest in this transition form factor due to the prospect of obtaining higher precision data over a broader momentum range via virtual Compton scattering from a proton target at CEBAF. [17] Feat ures distinguishing the present work [18] from a previous quark loop study [19] are: quark confinement (thus eliminating spurious quark production thresholds), dressing of the photon-quark vertex, and the dynamical relation between the pion BetheSalpeter amplitude and the quark propagator. The latter elements are crucial for producing the correct maso-shell axial anomaly independently of model details. The relevant part of the action (2) is identified by expansion to second order in A,. Only the first term (with R = 1) contributes and we find s[x”77] = -Tr[Sl?,A,Sr,A,Sl?,~“]. That is

where the vertex function is given by the integral

A,,(P, Q) =

-tr J

$$

S(k - P - Q)I’,(k xr,(k

- ;

- f;

-P

- f$ Q)S(k - Q)l”,(& - ;

- Q)S(k) - Q; P).

(7)

100

P. C. Tandy

Figure 1: The quark triangle diagram for the generalized impulse approximation to the +y*rr’yvertex. The momentum assignments are shown in the quark triangle diagram of Fig. 1. The general form of the vertex allowed by CPT is h,,(P, Q) = -ik cfluapPaQpg(Q’, P’, P - &) where ~4123 = 1, a! is the fine-structure constant, fir is the pion decay constant, and g is the off-mass-shell invariant amplitude. With the one photon mass-shell condition (P + Q)’ = 0, the invariant amplitude, denoted by g(Q2, P’), is the object of the present work. For a physical pion the shape of the 7*z” -+ 7 transition form factor is given by g(Q2, -ml). The chiral limit for the physical x0 + 77 decay amplitude is fixed at $ by the axial anomaly [ZO]which gives an excellent account of the 7.7 eV width and requires g(0,0) = l/2. This follows only from gauge invariance and chiral symmetry in quantum field theory and provides a stringent check upon model calculations. The “‘77 vertex function in (7) is now completely specified in terms of the quark propagator. An exactly parallel situation holds for the spacelike pion charge form factor and this model has previously been shown to provide an excellent description of the data. [7] No adjustment of parameters is made in the present application. At Q2 = 0, our numerical evaluation yields grDrr = g(0, -ml) = 0.496, in agreement with the previous application of this model [7] and in good agreement with the experimental value 0.504 & 0.019. The chiral limit of this approach has been shown (71 to correctly incorporate the exact result g(O,O) = l/2 p ro d uced by the axial anomaly independent of the form and details of the quark propagator. The obtained form factor F(Q2) = g(Q’, -mz)/g(O, -m:) at the pion mass-shell is displayed as Q2F(Q2) in Fig. 2 by the solid line along with the CELLO data. [16] We calculate a “radius” or interaction size, defined via (r$+ ) = -6 F’(Q2)Io2=s, of 0.47 fm while a monopole fit to the data yields [16] 0.65 f 0.03 fm. The insert compares our low Q’ result with a recent result from a QCD sum rule approach [2I], and a monopole form [22] that interpolates from the leading asymptotic behavior F(Q2) + gn2f:/Q2 argued from the pQCD factorization approach. [23] In the latter two approaches there is ambiguity due to: A) the unknown momentum scale at which perturbative behavior should set in; and B) assumptions for the pion wavefunction and how it should evolve with the momentum scale. 121) Within the present approach, both the photon coupling and the pion wavefunction evolve with Q2 in a way determined by the evolution of the dressed quark propagators. This produces, in a single expression, both the ultra-violet behavior required by pQCD and the infra-red limit dictated by the axial anomaly. We note that the employed pion Bethe-Salpeter amplitude B(p’,m)/f* has the correct leading power law behavior mX2/p2f, which implements the hard gluon contribution that

Meson Transition

101

Form Factors

---BL

.I

.o

-. em sum ~~~~I~~.~l”~‘I”~‘I’~”

0.0

0

2

0.5

1.0

4

1.5

R”lC

2.0

6

Limit

2.5 6

10

Q2(GeV2) Figure 2: The r*r07 transition form factor. dominates pQCD. The dotted straight line in Fig. 2 is the pQCD factorization [23] limit Q*F(Q*) + 8s*f,2 = 0.67 GeV’. Although our non-factorized calculation reaches this value near Q’ = 3 GeV’, we find a slow decrease with higher Q2 consistent with a logarithmic correction. An excellent fit to the numerical results for 3.3 GeV2 5 Q” < 10 GeV’ is provided by F(Q2) = A [l.O + B Q2 ln(C Q’)]-‘, where A = 1.021, B = 0.461 /rni = 0.777 GeV2 and C = 1.16 / rn: = 1.45 GeV2. (We have neglected the anomalous dimension of the quark propagator in this calculation, which would modify the power of the In-correction.) The logarithmic correction to the anticipated l/Q2 asymptotic behavior can be attributed to the persistent nonperturbative nature of the coupling to the final state soft photon in this exclusive process. [18] Numerically we find that, if a bare coupling were to be used for both photons as is implicit The turn-over in in the pQCD factorization approach, F(Q’) would eventually approach 8r’f,‘/Q”. Q2F(Q2), near 3 GeV’ predicted in Fig. 2 is barely within the Q2 limit of 4 GeV’ anticipated for measnrements at CEBAF if a 6 GeV electron beam becomes available. [17] This turn-over and the logarithmic corrections generated by the loop integral are features also found in the parallel approach to the pion charge form factor.[‘l] For a study of the behavior of the vertex function off the pion mass shell, as needed for the anticipated CEBAF experiment, see Ref. [18].

The prr Form Factor

3

From (2) we identify S [par] = -Tr [S’T~? - P;f’,( Sirs+’ - a,)“],

S[pm]

=i/$&

(Q). G(-P -

which yields

f) x S(P -

$,(P,Q)

(8)

where the vertex is

W,Q)=/pqi

PPNP-E

d4kj+p

(k

+

f;

Q)r,(k

+

!$ -P -

$(k

- ;; p -

;)T,(k, P,8)

(9)

P. C. Tandy

102

with Z’,,(k,P,Q)

= tr [S(k+

f + $S(k+

f

$]

- $S(k-

From symmetry properties, it is not difficult to show that A,(P, Q) = -A,(-P, requires the general form A,(P,

Q) = A,(P, -Q),

Q2,(f’ *Q)'),

Q) = -P,FF,(P2, Q2, (P . Q)“) - &,A’ . QfL(Pz>

(10) which

(11)

With both pions on the mass-shell, (P - t)” = (P + T)” = -mg. Equivalently, P . Q = 0 and p2 = -m; - !$ so that only the first term of (11) survives. The corresponding form factor F,,.&Q2) contains the coupling constant as its mass-shell value, i.e. Fprr(Q2 = -m:) = gp,_. If the form factor is held at this value for all momenta, one obtains the point coupling limit which can be expressed in the standard form S [p**] = -gprrrr i?(z) x d,17(c). (12)

JSz,;(z).

-0.5

0.0

0.5

1.0

Q’(GeV’) Figure 3: Behavior of the prz form factor with p momentum in the viscinity of the mass-shell at -0.6 GeV’. The previous study [24] within the GCM made the approximation gprr E Fm,(P = Q = 0) in order to avoid the occurrence of complex momenta in the arguments of the propagators snd vertex functions in the integral (9). Complex momenta are unavoidable when a Euclidean formulation is continued to handle timelike external momenta. However when propagators and BS amplitudes are produced numerically it is a difficult and lengthy matter to extend such solutions to the complex plane. The utility of the parameterized representation, (3) and (4), of the quark propagator is that the continuations required to properly implement mass-shell constraints as needed for extraction of gprs and other quantities are a simple matter. Since the propagator parameters have so far been constrained only by pion physics,

103

Meson Transition Form Factors

there is ao guarantee that continlrrtion cd S(p) away from the real p2 axis by an amount proportional to rni will be correct. The present exploratory calculations involving vector mesons constitute a first investigation of this matter. The investigation here is limited &me we have not made an independent calculation of the p BS amplitude r,(p). Thie requinm knowledge of the effective gluon propagator II(r) compatible, in a ladder DSE sense, with the given quark propagator. Although come progress haa recently been made in this direction, [25,26] iu the preoent work we directly parameteriae r,,(#) o( e-d/“. Thie has proved to be effective in a related study. [27] The strength is set by the canonical normatiuation condition [20] which is equivalent to ensuring that the residue at the pok of the p propagator is unity. Only the quadratic p dependence from the first term of (2), i.e. the quark loop contribution te the p inverse propagator, is ueeded to implement this. The range a is then adjusted to reproduce the empirical value gzt = 6.2. This requires a = 0.208 CeV2. The corresponding p + ra decay width, given by 2 r

P-r*

=

4* !Em,

312 12

11-L

rnz 4m2

1

(13)



is 151 MeV. The calculated form factor F’v(Q’) is shown in Fig. 3 for timelike and spacelike momenta in the viscinity of the mass-shell. The main conclusion from this cakulation is that the previous approximation of using zero momentum to extract a coupling constant [24] can underestimate the value by almost a factor of 2.

4

The 7xrp Form Factor

The empirical p BS amplitude set by gparraa above enables a parameter-free prediction for the yrp vertex. Apart from being a consistency check in this manner, the yrp interaction together with the 7vx, 77x, and the purr processes, provide important guidance for extending the present approach to nonperturbative QCD modeling of meson physics to phenomena not dictated by third symmetry. Within nuclear physics, the associated iaoscalar 7*vp meson-exchange current contributes signi6cautly to ekctron scattering from light nuclei. In particular, our understanding of the deuteron EM structure functions for Q2 % 2 - 4 CeV’ is presently hindered by uncertainties in the behavior of this form factor. [Zs]. Expansion of (2) to first order in the EM fidd yields the 7vp interaction as the pair of contributions sf7xp] = -Tr(ST,A,Si7$. With a vertex function &(I’, s[77rp1=

ti,S;7,1.

&fp] - Tr[Sr,A,S&y,F

- i;yFp%y5G~i#,].

(14)

Q) de&ad by -J

$

UQF'(-J'- $W-

$v(P,Q),

(15)

one may combme the two terms in (14) to obtain the integral

4w(P,Ql

=

f/&

X

tr[S(k+ - ~)rJk+;Q}S(k+

r,(k + ;; -P -

;)r,(k- f$P - g, + ~)i7JS(k_Ji7P].

Herekk = k f f. The7vpEMcurrent (-(2*)‘~~willbeconPared~a~onlcqanctoQmrintrining EM gauge invariance at the quark level. Explicitly, PIG of the Ward-Tahahashi identity QJ&

Q) =

P. C. Tandy

104

QS-r(k - +) - QS-*(k + f), in (16) immediately gives Q,A,(P,Q) = 0. The general form of the vertex function can be shown by symmetries to be &(P, Q) = -i-&c,,,+POIQ~ gpv f(Q*, P2, P . Q), as is expected for a coupling arising from the chiral anomaly. We have used the standard definition of the coupling constant so that, at the triple mass-shell point, the form factor f = 1. Our numerical evaluation yields glz,, = 0.5. The experimental p+ + x+7 partial width (67 f 7 keV) determines the empirical value g$ = 0.54 f 0.03. The 77rp form factor obtained with on-mass-shell A and p, and weighted by Q2, is shown by the solid curve in Figure 4. Also shown for comparison is the vector dominance model (VDM) phenomenology initially used to include such meson exchange effects in electron scattering analysis, [29] as well as the result from a free constituent quark loop with bare photon coupling. (28,301 The quark-based results produce a much softer form factor than is produced by the VDM assumption. Above 50 fme2, which is readily accessible in electron scattering, the differences are serious. .6

____ ---.-

VMD IG

~

THIS WORK

i

.l

.O 0

50

100

150

200

Q’ (fm-‘) Figure 4: The photon momentum dependence of the 7xp form factor from the on-shell approximation for both mesons.

5

Discussion

The photon-quark vertex employed in this work does not contain an explicit vector meson pole. The absence of the vector meson dominance mechanism in the explicit photon vertex is, in fact, consistent with the tree-level nature of the action (2). The n = 1 part of the first term, in combination with the third term, produces direct coupling of the photon with vector mesons. When the analysis is carried to first-order in meson loope, EM coupling mediated by a vector menon propagator will be produced

105

Meson Transition Form Factors

consistently as an additional mechanism to that considered here. More detailed exploration of this point is the subject of a future article. [31] At the photon mass-shell point, the coupling constants obtained here at tree-level for both 7rr7 and 7zp are within 10% of experiment. Our calculation for 7rp is equivalent to the O’* term in the meson loop expansion. An estimate of the meson-loop corrections to our result would be interesting. At this stage we can only remark that, within the same approach to the pion EM form factor, pionloop corrections were seen to contribute at the level of < 15% to the charge radius. [32] Similarly, the pion-loop contribution to the p mass has the correct sign and magnitude to generate most of the p - w mass splitting [33] and is a 2% dfect. The emerging picture is that a representation of low-mass mesons in terms of dynamically dressed quarks may capture the dominant quantum loop effects. Subsequent meson loop dressing would have to overcome distributed coupling produced by finite size effects. Instead of considering the underpinnings of the present investigations to be a result of bosonization of the GCM action to the bare meson level, there is a more general viewpoint. [lo] Selected truncation of the tower of coupled Dyson-Schwinger equations of QCD, together with use of a generalized impulse approximation, points to the same end result for the processes we consider here. However, the road to higher order effects is different in each. Progression through the loop expansion in the effective action approach defmes a rigid ordering of physics content. There is potentialIy more freedom to develop au efllcient ordering with the second approach as one moves beyond the impulse approximation and with less severe DSE truncation. We have taken the former viewpoint to emphasize the immediate relevance to e&ctive hadronic field theory models. It is becoming quite feasible to generate such models with many of the previously phenomenological coupling form factors now given a quark basis that, although approximate, captures the dominant influence on dynamics at the hadron size scale. Acknowledgments This work has drawn upon a number of valuable previous collaborations with K.L. Mitchell, C.D. Roberts and M.R. Frank. I also thank Amand F53ler for the organization of a fine program at Erice. This work was supported in part by the National Science Foundation under Grant Nos. INT92-15223 and PHY94-14291.

References [l] R. T. Cahill and C. D. Roberts, Phys. Rev. D32,2419

(1985).

[2] J. Praschifka, C. D. Roberts, and R. T. Cahill, Phyr. Rev. D38,209 [3] Y. Nambu and G. Jona-Lasinio, Phys. Rev. 122,345 Nucl. Phyr. 27, 195 (1991).

(1987).

(1961); U. Vogel and W. Weise, Prog. Part.

[4] R. T. Cahill, Aust. J. Phye. 42, 171 (1989); H. Reinhardt, Phys. Lett. B244,316 [5] R. T. Cahill, Nucl. Phys. A543,63c

(1990).

(1992).

[tl] M. R. Frank and P. C. Tandy, Phys. Rev. C49,478

(1994).

[7] C. D. Roberts, in Cl&al Dynamics: Theory and Ezpcriment, A. M. Bernstein and B. R. Holstein (Eds.), Lecture Notes in Physics, 452, p. 68 (Springer, Berlin 1995). [8] C. D. Roberts, A. G. Wiiams

and G. Krein, Int. J. Mod. Phye. A7,5607

[9] C. J. Burden, C. D. Roberts and A. G. Williams, Phye. Lett. B285,347

(1992). (1992).

106 (lo] C. D. Roberts and A. G. Wiiams,

P. C. Tandy Prog. Part. Nucl. Phys. 33, 477 (1994).

[ll] N. Brown and M. R. Pennington, Phys. Lett. B202, 257 (1988); Phys. Rev. D38, 2266 (1988); Phys. Rev. D39 2723 (1989). [12] R. Delbourgo and M. D. Scadron, J. Phys. G5, 1631 (1979). [13] J. S. Bali and T.- W. Chiu, Phys. Rev. D22, 2542 (1980). [14] Ll. AmetIIer, J. Bijnens, A. Bramon and F. Cornet, Phys. Rev. D45, 986 (1992); W. Jaus, Phys. Rev. D44, 2851 (1991). (151 S. Adler, Phys. Rev. 177, 2426 (1969); J. BeII and R.Jackiw, Nuovo Cimento A60, 47 (1969). [16] H. J. Behrend et al. (CELLO CoIIab.), Z. Phys. C 49, 401 (1991). [17] A. Afanasev, in Proc. of the Workshop on CEBAF at Higher Energies, Eds. N. Isgur and P. Stoler, (CEBAF, Newport News, 1994), P.185; A. Af anasev, J. Gomez, and S. Nanda, CEBAF Letter of Intent # LOI-94/005, unpublished. [18] M. R. Frank, K. L. Mitchell, C. D. Roberts and P. C. Tandy, Phys. Lett. B359, 17 (1995). [19] H. Ito, W. W. Buck, and F. Gross, Phys. Lett. B287, 23 (1992); I. V. Ax&in, M. A. Ivanov, N. B. Kuhmanova and V. E. Lyubovitskij, Yad. Fiz. [Sov. J. Nucl. Phys.] 57, 1082 (1994). [20] C. Itzykson and J. R. Zuber, Quantum Field Theory, McGraw-Hill, New York, 1980, p. 550. [21] A. V. Radyushkin, in Proc. of the Workshop on CEBAF at Higher Energies, Eds. N. Isgur and P. Stoler, (CEBAF, Newport News, 1994), P.273. [22] S.J. Brodsky and G.P. Lepage, Phys. Rev. D24, 1808 (1981). [23] G. P. Lepage and S. J. Brodsky, Phys. Rev D22, 2157 (1980). [24] J. Praschifka, C. D. Roberts, and R. T. Cahill, Int. J. Mod. Phys. A2, 1797 (1987). [25] R. T. Cahii and S. M. Gunner, Phys. Lett. B359,281

(1995).

[26] C. J. Burden, Lu Qian, C. D. Roberts, P. C. Tandy and M. J. Thomson, in preparation, November, 1995. [27] K. L. Mitchell, P. C. Tandy, C. D. Roberts, and R. T. Cahill, Phys. Lett. B335,282

(1994).

[28] H. Ito and F. Gross, Phys. Rev. Lett. 71, 2555 (1993). [29] E. Hummel and T. J. Tjon, Phys. Rev. C42, 423 (1990). [30] H. Ito, W. W. Buck, and F. Gross, Phys. Rev. C45, 1918 (1992). [31] P. C. Tandy, in preparation, November 1995. [32] R. Alkofer, A. Bender and C. D. Roberts, Int. J. Mod. Phys. AlO, 3319 (1995). [33] K. L. Mitchell, Ph.D. Dissertation, Kent State University, 1995; K. L. Mitchell and P. C. Tandy, in preparation, November 1995.