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i-ri NBS TECHNICAL NOTE 957%*U Of
U.S. DEPARTME
NATIONAL BUREAU OF STANDARDS
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OF STANDARDSLIBRARY .-_.
SEP 2 2 197/
Threshold Photo and Electroproduction
of Pions from Nuclei
&c
±T ^ c^ w \ caJt ftaW w^ . ^^T^
E.T. Dressier
Institute for Basic Standards
National Bureau of Standards
Washington, D.C. 20234
*< ">%.
U.S. DEPARTMENT OF COMMERCE, Juanita M. Kreps, Secretary
Dr. Sidney Harman, Under Secretary
Jordan J. Baruch, Assistant Secretary for Science and Technology
S ,NATIONAL BUREAU OF STANDARDS, Ernest Ambler, Acting Director
Issued September 1977
National Bureau of Standards Technical Note 957Nat. Bur. Stand. (U.S.), Tech. Note 957, 38 pages (Sept. 1977)
CODEN: NBTNAE
U.S. GOVERNMENT PRINTING OFFICEWASHINGTON: 1977
For sale by the Superintendent of Documents, U.S. Government Printing Office, Washington, D.C. 20402
Price $1.50—Stock No. 003-003-01834-0
Contents
Page
1. Introduction 1
2. Pseudoscalar vs. Pseudovector Coupling 2
3. Nonrelativistic Amplitudes .. 5
4. Threshold Photoproduction 12
4.1. Kinematics and Gauge Conditions 12
4.2. Pseudoscalar Photoproduction ... 13
4.3. Pseudovector Photoproduction 15
4.4. Discussion 16
5. Threshold Electroproduction 16
5.1. Current Conservation 16
5.2. Pseudoscalar Electroproduction 17
5.3. Pseudovector Electroproduction 20
6. Cross Section Equations 21
6.1. Coordinate Space Representation 21
6.2. Photoproduction Cross Section 22
6.3. Electroproduction Cross Section 24
7. Discussion of Results 29
8. Appendix 30
9. References '• • 30
ill
Threshold Photo and Electroproductionof Pions from Nuclei
E. T. Dressier
The nonrelativistic amplitudes for photo and electroproduc-tion of pions are derived using effective pseudoscalar and pseudo-vector Lagrangian densities. The results for pseudoscalar andpseudovector coupling are compared at threshold for chargedand neutral pion photo and electroproduction. Cross sectionformulas and kinematical conditions are also presented.
Key words: Effective Lagrangian; electroproduction; impulseapproximation; photoproduction; pseudoscalar and pseudovectorcoupling; threshold pion production.
1. Introduction
In the calculation of any nuclear cross section that involves a
small perturbation to the nuclear system, the standard approach is to usethe impulse approximation,, That means that one assumes that an externalperturbation acts on the nucleons in a nucleus as if they were freeparticles. Using this approximation or model, then if one knows the
amplitude for the reaction off of a single nucleon, we just sum the
contributions from each of the nucleons in the nucleus (a sum correlatedby the nuclear wave functions). The purpose of this paper is to presentthe nonrelativistic amplitudes for photo and electroproduction of pionsthat can be used in an impulse approximation calculation for nuclearprocesses.
To find the amplitude from a single nucleon, one usually starts byconsidering which relativistic Feynman diagrams are important in the
particular energy region under consideration. For the case of a purelyelectromagnetic interaction as in electron scattering, photo or electro-disintegration, or Compton scattering, one can use perturbation theoryand quantum field theory to give the appropriate Feynman diagrams to a
particular order in the coupling constant. However, in photo or electro-production of pions, we now have electromagnetic and strong interactions,and since the coupling constant in strong interactions is large, the
perturbation expansion in powers of the coupling constant will not con-
verge. In spite of this fact, the lowest order term in the expansionusing pseudovector pion-nuclear coupling, gives results which under cer-
tain conditions agree very well with experiment and with the low energy
theorem derived from the theory of the PCAC (partially conserved axial
current) Ll], Therefore, we will use the lowest order perturbation term
as our model for the threshold photo pion production amplitude off of a
nucleon.
Two of the simplest pion-nucleon couplings are pseudoscalar (ps)
and pseudovector (pv) [2J. A comparison of the two couplings is made in
Section 2. In order to use the amplitudes in a nuclear calculation, we
must first make the nonrelativistic approximation of the relativisticFeynman amplitudes. This is done in Section 3. The nonrelativisticamplitudes are then specialized to the cases of threshold photo andelectroproduction in Sections 4 and 5, respectively. In Section 6 thecross section formulas are given.
2. Pseudoscalar vs. Pseudovector Coupling
In the Lagrangian field theory approach to photo pion production,two of the simplest interaction Lagrangian densities between the pion andnuclear fields that one can choose are called the pseudoscalar and pseud-ovector interactions. In the pseudoscalar case, the interaction La-grangian density for the pion-nucleon interaction is
X^ s)= iGN(x) T • 5(X ) y 5
N(x) (1)
whereN(x) = nucleon field operator
cp(x) = pion field operator (a vector in isospin space)
G3
-j— = 15.0 = pion-nucleon coupling constant
T = nucleon isospin operator
For photo pion production, the total interaction Lagrangian densityis
£(ps) = x(ps) + z + z (2)I 7tN yN y%
where
-f,.
...
yN 'u£ .. = ieN(x)y Ay (x)N(x) (3)
1YTT
= iecp+(x)(g|- -
-J-)cp(x)Ay (x) (4)
A (x) = electromagnetic field vector
When this interaction Lagrangian density is used in the second order termof the perturbation expansion, one finds that there are three Feynmandiagrams (shown in Figs. 1-3) that can be associated with the secondorder term. (Solid lines are nucleons, wiggly lines are photons, andbroken lines are pions. Each line is labeled by the 4-momenta of the
particle.
)
/*/
Figure 1. Nueleon pole diagram.
Figure 2. Crossed nucleoli pole diagram.
Figure 3. Pion current diagram.
Figures 1-2 are called the nueleon pole contributions to the Borndiagrams. Figure 3 is called the pion current diagram, because it re-
sults from the interaction of the pion's electromagnetic (e-m) currentwith the e-m field operator^ given by £y%.
For pseudovector pion-nucleon coupling, the interaction Lagrangiandensity for the interaction of the pion and nueleon field operators is
given by
t ^if
£<PV) = _JE n(xtcN m (*) yur 5
Td?(x)
N(x) (5)
where fl = °- 08
' (a?-)"= 4* (s%
Now in order to insure gauge invariance of our total interaction La-
grangian density, £ , in the presence of the electromagnetic field,
we have to let [3]
This leads to
, (pv) ,<PV >
&** - ^ + ieA^x)
ttN ttN
fir — -» -» u (Pv )
- e — N(x) y y, T.cp( x)N(x)A^(x) = JC71N + X M (6)m 'p. 5 TtNy
By inspection, we can see that this leads to a new term which has the
interaction of the nucleon, pion, and electromagnetic fields at a point.
There is no term like this in ps coupling, and inserting this into the
perturbation expansion leads to an additional Feynman diagram (fig. 4)
in pv theory.
Figure 4. Point contact or "seagull" diagram*
One should note that although the diagrams in figs. 1-3 are also
present in pv theory, they won't necessarily give the same size contri-
bution as in the ps case, because the form of the 71 - N vertex is dif-
ferent for the two couplings (fig. 5).
y_ for ps
J. yJ for pv
2m
Figure 5. n - N vertex operators for ps and pv coupling.
Even though the size of the contribution to the production amplitude
from each of diagrams 1-3 may be different for the ps and pv cases,
the sum of the contribution from diagrams 1-3 using ps coupling gives
essentially the same result as the sum of the contributions from dia-grams 1-4 using pv coupling for charged pion production at threshold.However, pv and ps couplings give quite different results for tc produc-rion. pv coupling gives the best agreement with experiment and is usual-
ly chosen as the "effective Lagrangian" [4J. In spite of this, we willderive our nonrelativistic amplitudes in the next section using ps cou-pling and show how these amplitudes are modified for the pv case.
3. Nonrelativistic Amplitudes
To calculate the amplitudes corresponding to the diagrams in figs.1-3 using ps coupling, we can use the Feynman rules in appendix B ofref. [5]. The relativistic amplitudes for these diagrams are defined as
Aw 1 T3(*p
- kn )\j _ t(Pi)€
u(7)
\ 2 /Jp' 2 - m2 r 5 a s,T v 1'
/ x C T ,TJ (q' + q)
M?3
PS)= * «sV<V V 5 -V- SV"^f V<V (9>
where a = - 1, + 1, for % , 7t~, and % production, respectively,
o 3
and
T_L|P> = /£ |n> ,
l~T >%1 = T \ - Va
3Ja 3 3 a >
In order to use these amplitudes in a nonrelativistic calculation,
one has to expand these matrices by going from the 4 component Dirac
spinors, U S(P), to the two component Pauli spinors, Xs» This is done
by letting
us;T
(P) = Vl(^)v-(^)v + KS) (10)
where I =<l)and x T
= X XT > X being the spin and XT the isospin Pauli spinors,S a I S ' S I
respectively.
Keeping only terms to
amplitudes by M, where.(j). we denote our nonrelativistic
M(PS
> = -i l«yl k / o' o
/-k \ I 2P -k + ka-k ^ + a.q \i + -^ (ID
+o 2m 2m
P *e ->
i ka«k ( ^-
m 2m / \ 2m
+ie,
( k x q)2m a\ 2 / k
oo \ 2m
+V 2m 2m/ \ 2m/ 2m
^ (fp
+ Kn) + (V K
n) M
M(ps)
. JL.
y2 k o1 ~) + cf-q
'
2Pf«k - k
2mk(12)
+ ^(-K-i+^i).. ^ I m 2m / 2m
, . £'(k x q)+ 1 —aT"^1 + T
37 1- t + —- e a*k2 a k o
o2m
+
> - / oqo k-q \ - r / e.q
2m 2m / \ 2m. e»(k x q)
K+K) ( K - (C ) T \p n/ M P n/ 3 T
2 /a
M<ps> = . ^<q - g re /2 q . k \ . ;. (2 q . k )
y3 / 2k»q - k2 o\ o o/ M
For threshold pion production, we can let q -» which leaves
>]|M <13)
M(ps) _ „ G «k "* -*
i , o
o 2m \ 2m(l + T
3 )
a 2+
m- e
71
o 2mka-k (14)
m
2mt -Ea
V p n/+Vp n /
- K \ TP n y 3
M(ps)
y2
ck -* -»
e„ ~ot; + G#eO Al
k
1 + ^ (X + T
3)
CI m7t -> ->
71 - "*
- e T53— G *k + -sr G *eo 2mk 2m
(<
K + K . K - K Tp n/+\ p n/ 3
2 /a
(15)
M (Ps) .
y3
ack2k m ^~W
O 71
e ( 2m - ko V 71 o
\ + e«k [
IVJ(16)
By replacing eQ
-» kG and e -* k in equations 14 - 16 we see that
M ,P + M « + M , -» , therefore, our nonrelativistic amplitudes
yl y2 y3
are exactly gauge invariant.
Now consider how these amplitudes are modified for the case of pvcoupling. Using eq„ 4d of refo [lJ, the pv amplitudes are given by
M,1 - - u
s, )T ,( Pf ) iy
5 \^-r^1 + T.
H 2
C /(k + K
i_£v
kv K_P n
2m \
+( K - K ]tP n / 3
Us,x(Pi)e "
M(pv)
y2 V,T.<ef>
1 + t;
a
2mk
'n 2
(VM^n) C+ "
fly.T U T
(p.)«l)
2 - m3 "'5 a s,T vri
7
(17)
(18)
M (pv) - , v ,., ,. fra,T3] 1= UQ , T ,( Pf ) (K ff) y, —J- - „, . ggy3 s',T'^f 5 2 q* (19)
(q« + q) Us>T
(p.)^
™ (Pv ) t"t t \ ^ Ta,T3 ] , N p.My4
= V,!'^ —2— V5 Us,T
( Pi)e (20)
Consider now the following identities:
5s',T-<Pf>4r 5-^^=G
s, >T ,<P f)r 5
2m (j6 + m)
p2 - m2
+ 1 (21)
p'3 - rf ^5 Us,T<Pi) =2m(jS' + m)p'2 - m2 + 1 ?5 Us,T^i> (22)
By comparing eqs. 7-9 with eqs. 17 - 19 and using identities 21 -22,
we can see the following:
M .^Mr^v.T. ^y T5 a
(l + T.
V 2(23)
(J I [ K + K )+ K - K
+i JiZ hv
l \ P nj_ \ P
2m a^J U ( P .) e^M (ps)
s,t i'+ M 1
yl yl
M 1PV> = M 1
PS) + 5., T , (p
J
y2 y2 s',T' Nrf
1 + T ) a
V 2 2m(24)
K + K ) + K - K \tp
n/ ip bJ-J^) T y u _ (p.)e^M <
ps)+ M.'
/ a 5 s,t ri v2 v
For M \ * toe usey3
58',T" (P
f} (K
" « ?5US,T (P i
)= ^ U
S ',T' (Pf
} ^5 °s,T <PI ) (25)
Therefore M <pv)
= M <ps)
y3 y3
Taking the nonrelativistic reduction of M' and M 1 givesy2
M' = < - eyl I o
tf'k O'q "P,-+
2m 2m m+ tf.e f T
(1 + T
s)a 2
j. ii^tM, ((Kp+ K
n)+ (%- Kn)
T3)
j o 2m 2m\ a \ 2 /
(26)
My2
-* -» -» -» 0'»D
2m 2m 2mtf-e |
i-
1+T3) T
a
+ ) eo 2m 2m j \ 2 /a
(27)
Combining M 1 and M' with M and MPS
, respectively (eqs. 11, 12),^ ^ ^ ^ (dv) (dv)we can now get the pv nonrelativistic amplitudes to M , and M .
yl y2
M <pv)
= ( •yl 1 o
"2 7* a *P.cr«k *i
m m+ °- q lr +—sp—
/
\ o o I -*
(28)
;.e -2 - 3^i2m 2mk / 2mk
o / o
-» -*/ k«eCJ.q (^—
:
l!V ,.
«•(* '*)2mk mk
o o
'+ i2mk
a 2 o I 2m 2mk )T
\2m 2m 2mk ^L °
+ ;.i;!x +16>(£ * q) T i e n ^ L-£ n
I3
)2mk 2mk a \ 2 /
M(pv)
y2
tf'p,-»f 1
-5r+tf,
« ir+
2p -k + k2
am?o
+2m
+ asH- °- k l5r +0^ asr-sro/ o \ o o
+ie»(k x q)
2mk
1 + t.
1 o I 2m 2mk 1
V 7
+ 6 e
(k q r -* \_2 . _2 k»q I -* -j* q«e
"2m 2m " 2mk / 2mko/ o
• e*(k x q)-1" 2mk
o
((Kp+KJ +(V K
n)T3) T
\ 2 /a
(29)
10
Taking the nonrelativistic reduction of M , gives
M(pv) =
y4
*i g»k
m 2m 2m- a •e
[Ta'
T3]
(30)
Making the substitutions e -» k and e -» k, the nonrelativistico o
amplitude M <Pv) + My2
(PV) + My3
Cpv)+ K^ (pv)
is also gauge
invariant.
For threshold production, letting q -» 0,
k
o \ 2m 2mk
(31)
e y2m 2m/ a \ 2 /
M(pv) _
y2S
tf ' Pi -- ko> (
1+T3)
, m
o
/m k.
-1 ~*(
It O
2m 2mk /
e\ 2m " 2m
^P + Kn)
+(K - (C
_J2
(32)
n^Va
M
M
(pv)
y3
(pv) =
r? fe f2m - k \+ e .km - k5 oVtc o /O 7X l J
[V T3]
2m m<3* e
[Ta'
T3]
(33)
(34)
We should note at this point that in deriving these expressions, wehave not used any particular gauge or mentioned any specific referenceframe in order to eliminate terms. However, by stating that thresholdmeans "q = o, we are by implication in the center of momentum frame where
k = - p.. In the laboratory frame, q F0 even at threshold.
11
4. Threshold Photoproduction
4.1. Kinematics and Gauge Conditions
For real photons we are free to choose the gauge where e*k = and
e =0. This is the transverse or Coulomb gauge. By inspection of M „,
the contribution from the pion current diagram, we can see that thisterm vanishes at threshold.
Choosing to work in the center of momentum frame of the incomingphoton and the target, gives
k + p. = q + p. (35)1 i
and at threshold
q = = pf
(36)
where p. an^ P^ are the momenta of the initial and final nucleus assum-ri f
ing the final state is a bound nucleus. Then at threshold, using
and
k + E. = m + m£ (37)o 1 71 f
gives
E. = Vm2. + k2 (38)1 1 o
m + mJ - m.
k = \ I *L *(39)
o 2(% + *f )
"""For transitions to continuum states, the kinematics are a bit more
complicated.
12
4.2. Pseudoscalar Photoproduction
+Case 1. y + p -^
tc + n
(ps)The largest contribution comes from M .. as can be seen by consid-
(ps)ering diagram 2 which corresponds to M . In this diagram the proton
has already emitted the % and become a neutron. Since the neutron has
no charge, the incoming photon can only interact with the anomalousmagnetic moment, K .° n
+<M(7t )> = - /2 <(*•£>
- v2
I k \ m
f i . _£) + _E (K + K \
\2m/ 2m I p n)
R<cr«e>
m1 - -- (K + K )
2m p n
(40)
In the cross section we have
+ s
|<M(w )H2 I <c. e:
m1 + -5
m
m
^ (Kp+ V (41)
where we have used
k \-
2m/ m1 +
m
(42)
in order to put the expression in a form which can be compared with the
completely relativistic calculation in ref. [7J.
Since (K + K ) = -.12, the anomalous moment gives only a smallP n +
correction and can be neglected in 7t production.
Case 2. y + n ->-n: +p
13
In this case, the largest contribution comes from M(ps)
y2, since the
isospin operators allow only contributions from the neutron's anomalous
moment part of M(ps)
Again this can be seen intuitively by considering
diagrams 1 and 2 as was done in Case 1.
<M(tc )> = /2 <d
<* */2
JL~*>> mm
<<5'e> L+ 7i + n
. ~ni \ m 2m1 + TC \ L
+ K )
P n
2m
(K + K )P n
(43)
and
|<M(if)>P« 2<tf-e>r
1-+-5m_jm
m m
m *£n p n(44)
where again we have arranged terms to put this in the form of the
relativistic results.
Case 3. y+p^K +p
Diagrams 1 and 2 contribute on an equal footing in this case, how-ever, the leading terms of the C*e operator cancel each other, and we are
left with only higher order terms.
<M(p,7t )> = <(?•£>
k. m
m2 + -2k (45)
|<M(p,7T°)>|2 « \<^>\\^) (1 + K
p>2
(46)
Case 4. y + n -* 71 +n
14
Only the anomalous magnetic moment parts of M , and M „ canyl y2
contribute, because (1 + T ) |n> = 0, which reflects the fact that theneutron has no charge.
o -* -. /m
<M(n,ir )> = - <(S'H^) Kn (47)
|<M(n,7i°)>|2 = l<tf'1>|
af^) ( K
n)2
(48)
By inspection, we can see that charged pion production is mucho o
larger than n production since the n cross sections have an overall
(m
\
2
factor of(
—
) % .02 not present in the charged pion case. Note that the
/
mm V1
ofactor (l + — ) cs .87 is not present in our cross sections for n
\ m /production although it is present in the fully relativistic cross sections
in ref. [6J. This factor would come from corrections of 0( ——)to our
amplitudes which have been neglected in the spirit of our nonrelativisticapproximation. As we can see, these factors are not insignificant, and
obviously a nonrelativistic calculation of ti production is not very
reliable unless terms of 01 —*- have been carefully retained in the
amplitudes from the beginning.
4.3. Pseudovector Photoproduction
For pv pion-nuclear coupling, there are three terms which contributeto the cross section at threshold,
M(PV) = M(pv)
+ M ( Pv) +(pv)
(49)y yl y2 y4
Within the approximations we have been using, we can see that the
anomalous moment parts vanish. This does not have any significant effectfor charged pion production; however, it makes the cross section for
oy + n -* n + n equal to 0.
Case 1. y+p-»7i +n
15
The largest contribution now comes from diagram 4 as opposed to the
ps case where diagram 1 gave the largest term
<M(7t+)> = .. V 2 <5.> (l -75;) (50)
Case 2. y + n -* 71 +p
Again diagram 4 is the largest contribution with a small correctioncoming from diagram 2.
<M(ti")> /2 <tf->(i + 2^)(51)
oCase 3. y + p -» 71 +p
givesDiagram 4 can't contribute in this case, and M + I
(pv) (pv)
yl y2
m<M(p,7C°)> = — <tf-e> (52)
m
4.4. Discussion
In the ps case, if we neglect the very small anomalous moment cor-rections to the charged pion cross sections, we get exactly the sameresult as with pv coupling. However, for 7t° production, the ps crosssections give results much closer to the experimental values (See ref.
[6] for numerical values) even using our approximate amplitudes. In con-
clusion, we can say that for threshold photoproduction of charged pions,either eqs. 14-16 or eqs. 31-34 can be used. For 71° production, these
equations can be in error by as much as 207» due to neglect of terms of
0(p2 /m2 ).
5. Threshold Electroproduction
5.1. Current Conservation
For electroproduction of pions where the incident photon is now—> —>
virtual (k2
7^0), we. can no longer use k«e = to eliminate terms. This
means that we now have contributions from the pion current diagram (fig.
3) even at threshold. However, we can use current conservation of the
electron and nucleon currents to eliminate the e terms. For electropro-
duction, e^ now represents the electrons current and is not the polariza-
tion vector of a real photon.
16
as
We cati define a nuclear current J by writing our matrix elements
M = e^J = e «J - e'J ,
H o o(53)
then current conservation gives
k^s = k e - k«e =[I o o
k^j = k J - k.J =u o o
(54)
(55)
Using eqs. 54-55 to solve for e and J , we can writeo o
M-—— - e.J= e.|k rro o \ o
(56)
Therefore- we need not consider the terms in M that have eo
5.2. Pseudoscalar Electroproduction
For electroproduction of pions the incident photon in figs. 1-3 is
virtual (k2^0), therefore, we have to introduce form factors at each of
the vertices that a photon is attached. Eqs. 7-9 now become.
M (ps) _ ~ rT
/ \ A, T (f$ + m)Mel - ^sV^V *5 a P
2 - m^
FS+ T F
Vrl 3
fl
cj ( FS + T F
v
+ij£ kU
\ 2Q
322m 2
US,T^i)£t
(57)
M(ps)
e22mU
s(p)
FS+ T f
v)
a (fs+ T F
V
1 Vy+ i _b£hi k
Uil2__3_2ru 2
+ X2m
k2
(58)
17
{£ + m)r«T u (p,)^
Me3
PS>= «.., T -<'f> V5
^le^^> F„U. „<p.)'2 - m3 t,; s J *17C
(59)
where
F^k2 ) = FP + F^ (60)
F^) = FP.
F«
(61)
FS
2(k
2 )=K pFP + KnF^ (62)
F>2
>=VP
2-V2 (63)
Fj(o) = FP(o) = Fg(o) = 1 (64)
n,F (o) = (65)
Rearranging terms, we can let [lJ
(PS) = M 5
PS) + M <ps)
+ M < ps) = U , ,( Pf ) J- y F^el e2 e3 s ,t' f ' 5) V 1
<2q - k).. r^rj <2h + k)u
(f; + T3F[)
2" * p3 - m3 a 2
Mv K^l
q 2 - nr ti
"fl
2 > - nf3To\ 2 2 /
+
(66)
p' 2 - m2 2 2 p' 2 - m2 \ 2
Jr«pSL| rtT<p,
2 / a[ s,T i
If we use the test for gauge invariance on this amplitude, we findv
that we must let F, = F . Since all of the form factors are assumed to1 TC
be independent, an alternate way to make M(ps)
[auge invariant is to
make each term in eq. 66 independently gauge invariant. This can bedone by letting
y F7v i
v.kk: t
k2 (67)
(2q
-k)u
n ' 2 _ m2(2q-k)
(2q-k)»kk
k2 Jq 7^ mc (68)
(2P
l+ k
) ,
p2 - m2 (2Pl + k)
.
(2p + k)-kk1 u
k2 3s - m2 (69)
(2p - k),
,•2 mc(2Po - k),
(2p2
- k) - klvk2 Jp 1 m2 (70)
The fourth and sixth terms in eq . 66 are already gauge invariant. Note
that these "gauge corrections" only enter into the longitudinal part of
the cross section since their 3 - momentum part is always in the longi-tudinal direction, i.e., along k.
Keeping terms of 0(p/m) and letting q -», the current operator to
be used in eq. 56 is
19
fCps) _/_ z -. ^Tt
'tt 1 2k m
I~1
,k "2 7*1 a 3 _v ojt
\ ks / 2 1 /2km -
k (?»k
k2 \ k2
r' T
3la 3|
F2 7C
(71)
2m / 1 + m
I an
m
(F1+ T
3FI)
,(FS T^V+ T F2 3 2
2m~
1 - ZEE2mk
(i+_vl) ,
F2+ Vl,+2 I "a
it
5.3. Pseudovector Electroproduction
From eq. 5.2 of ref. [l], the amplitude for electroproduction usingpseudovector coupling is
Mi
Pv):=5s',T-<Pf>r 5
j. rFA Lp] +an (f^i 'H A 2 q 2 - m
T ,Ta 3JL F
q' 2 - m2 % 2(72)
/2P
1+ k
)u T (F1+T
3FD
"w ps - m2 a 2
idl - k) T i(livL) + (I1V22 p2 - m2 a\ 2 2
+ (2p 2
'
k) u /
Fi+ T
3FI.
T+p' 2 - m2 * 2 a
2 p' 2 - m2
-^^.i^k*20
Eq. 72 is made gauge invariant by making the substitutions in eqs.67 - 70.
In ref. [l], Dombey and Read identify F^(k2 ) with the nucleon axialvector form factor. Expressions for this form factor and the other formfactors in eq. 72 are given in the appendix.
;(pv)
In the nonrelativistic limit at threshold, the current operator is
= [a + r-5- cr-k L a 3
F"-1 F.
2k m7t K Ck
2k m - k2 \ k2O 71
L« 3J2 \ (73)
ko
2m
1 + ^)
• S V \ / s VFl+T
3Fl)
,(F2+T
3F1
\ 2 2
2m/
m71
2m
+2m
k?
2mk
livD + (livI
s VF T + F2 a 2
IV^}
6. Cross Section Equations
6.1. Coordinate Space Representation
The amplitudes given in the previous sections are in a momentumspace representation. It is convenient in order to use known nuclearwave functions to express these matrix elements in a coordinate spacerepresentation. This is done by using the fact that each of the ampli-
tudes has a 3-momentum conserving ^-function which multiplies it. For
production off of a single nucleon, we can let
!3(VVvV x»',t'" xS,T(74)
J
-IP »X .7* -» _3 e Ff -ik »x T
d xV8t?"
xs',t-Mx
s,te
r
.r* -» ip.«Xik «x e i
V87?"
21
~ip *x *'
's ip *x —'
-
'
where e " f /• 87c3 and e i /V8TC3 are now the final and initial nucleon
wave functions in coordinate space. To generalize this to a system of Anucleons, one has to replace
T ip^x ip.*xe f e 1
X„i T i
" ' and X .. by the appropriate initial and final' /87U3 /87T3
S,T
state nuclear wave functions and let /d3x ->^T]/d
3x ... d'\When we separate out the center of mass part of the initial and finalstate nuclear wave functions, then the integration over the center ofmass coordinate gets back a 3-momentum conserving 6-function,
6 (P + k - P. - k.), where P. and P^ are the momenta of the centerf 7C 1 1 1 r
of mass of initial and final nucleus. All that is left in the coordinatespace matrix element is the integration over the internal coordinates ofthe nucleus.
If we include interactions of the^outgoing pion with the final state- i q • r
nucleus, then we can no longer use e i as the pion wave function—
*
— 1 Q * TT*
where r. represents a relative coordinate. We let e i -» cp (r.) where1 TCI
(p (r.) is now distorted by Coulomb and strong final state interactions.71 1
This is called the distorted wave impulse approximation (DWIA). There is
no general agreement as to how to generate these wave functions, and the
investigation of this part of the problem is beyond the scope of this
paper. However, an understanding of these final state interactions could
be the most important and interesting aspect of photo pion production
from nuclei.
6.2. Photoproduction Cross Section
Assuming the initial and final nuclear states are bound states, the
photoproduction cross section can be written |_8J
y=
~5. a
\^J (2E%ko
> T _ v \° vt
£T \ ' *i
_ nr
*° = k {^) ^^^^^ + E- " E= -
E"' < 75 >
63(P
f+ q - Pi - k)d
3Pfd q
22
where |<M(r)>| c includes the sum and average over the projections of theangular momentum of the final and initial states and the coordinatespace integrations.
vThe flux factor |— - 1 | can be evaluated in the center of momentum
frame where
v =m, m. cc
andv
1 + ^r>k 1 >
3 3The integration over d P is done using 6 ( ) . Letting
A3d q = J% EdEdfi»(he)2 71 % 7t
(76)
the integration over dE can be performed using 6(E r + E E.- E ). But&7t
& vf 7t i y
E,- is now a function of E so that we cannot use the 6-function directlyf 71
Ef ~ m
f+ *r
f= m
f+
E3- m2
71 71
2m.(77)
Then
6(E, + E - E. - E )dE =f 71 1 V 71
E2
- m2
m r + —~-—— + E - E. - Ef 2m, 71 i y
dE = (78)
'( E* - E°)
1 +
dEE \ 71
_7C
m,
23
where E is the result one gets by setting [ J = and solving for E .
O 71
Now the dE integration can be done simply.
dgV- 1 /G \
siq, (he)* |<M(r)>|»
dQ 4ti 2mc2 V 1 / eTT E ^wy;
/ i + _lJ/l + *m.c3
JI m c2
Note that the kinematical factors in the denominator of eq. 79 werederived assuming a bound final state in a particular frame and are notnecessarily present or of this form for all photoproduction processes.
6.3. Electroproduction Cross Section
From eq. 56 we saw that the electroproduction amplitudes could be
written as
M = e-lk^r - J
Defining a new current operator J 1 by
3 ' iN^- - 3 >(80)
the electroproduction cross section can be written [8]
a2 LGf fel)&T 1 Jfe .<j.>\ fr .<j.>"\ (81)
(2mc2) LdEfdfi , leicHanc2 / \k / E k4 i\ e / \ e
e e N ' \ e / n
+ ^e-<J ,
>*Yk;»<J,>\- |-<J»>'<J'>*| 6(E
f+ E^ + E
e , - E. - Ee
)
24
6 (p-c + q + k' - P .- k )vrf ^ e r
i e
where E and E , are the initial and final electron energies, k and k'e e & ' e e
are the initial and final electron momenta, and
k2 = (k - k')2 = (k - k' )2
- (k - k')2
(82)e e eo eo e e
The longitudinal part of the current J* is given by
-» k*j' -» k2 -*
JL =^ k =-i? J
L < 83 >
k o
and the transverse current by
J^ = JT
(84)
From eq. 73, we can see that the contribution to J from the pion currentdiagram is in the k direction. Therefore, this diagram only contributesto the longitudinal current and need not be considered in J .
Assuming the final state to be a state with one definite angularturn, the longitudinal- 1:
interference terms disappear.momentum, the longitudinal- transverse and transverse- transverse-
2 This is a safe assumption since we are considering only threshold
production.
25
The cross section can now be written as
dc?
dE ,dQe e
:
=
4 m(^j ¥^^ "\ «<*f
- h> «& - ^) (85)
E.L.-2 k*k o
2 (ke.k) (k;.k) - ^k2 k2
|k-<I >
+"2k
2 k ,2 sin2 6e e e kf_
2
['e+ .<J
T>r + U_-<jt
>
where e+ =e +ie
/2
and 8 is the angle between k and k' . Neglecting the electron mass,e e e
we can write for the coefficient of the longitudinal current
k o L o(1 - e)
(86)
and for the coefficient of the transverse current
2k2k'
2 sin2e e k2
i?
k2 i
2 (1 - e)(87)
Dividing through by k2 , the cross section can now be written
dtf
dE ,dO ,
e e
2, r
87T3
( G \a(K\ (hcf <fq 3p L
e)(88)
26
[iv<yi* + I'.-^i'l k= nlk«< T > 2
64 (P, - P )
jl'-+ " T ' "
'"-~T
'J - e ^ - -ki.
f i;
I 2sk2 -
2k
_i
.- 2p- tan2 7p )
It is useful for the purpose of comparing with photoproduction datato express parts of the cross section in center of mass variables (vari-ables in the photon- target center of mass system will be denoted by a *)
[9]. The rest of the cross section will be evaluated in the lab system.
It is known that
.a cfp, ,3 * d3P
6*<pf_P.) = £a__l 6*(p*-P*) (90)
\ Ef E
71 f
If we transform to a system where k is in the z- direction, then we knowthe transverse terms won't change and
v^i 2 + r^.-<jT>|2 = Iv<j
t|2 + \*--<3
t i
2(91)
The longitudinal current transforms by
^V' 2 A\2 |k-<j>,v
|
2
L1 ° \ h (92)
k2 \k / k2
If we assume the electron and pion are detected, the cross section is
_of./G \3
(
ke\ (hc|q"|) 1
87T3 [Z^?] UJ WT (1 - e)
d£ _JL( G \2
eUhcjq 1) 1 1(93)
dE ,dQ , dQ \ / \ e/ ' / E
e e' 7CN '
i +mfc2
27
[lV^/l 5+ Ie.-<J
T>*| 8
1o |k.<J> p
k 2k3
(93)
(cont.
)
where
k =o
: An. + k ^
m. + k1 o
k2 2(94)
_>+ km.k* = -p-
m + k \2
- k2(95)
Let
k'
r = S-ls.t 2ti2 \ k
g
h _1 1_Tk2! (1 - e) (he)
Then
dtf
dE ,dfi ,dQe
1 e' 7i
r _s / G f (hc )
2lq"l
t 4ti \2mc2y Kl v-
1 +m c*
(96)
V <JT>
I
2 + K^V- |k.<X>*| 2r.
- e
k*3
k2o
>
= ^<V e<,L>
whe re JL is the equivalent real photon energy in the lab system,
28
where
( G
V&nc2
Dv<v>
(97)
(5, = a2mc2
(he)' 1 +mfcc
|k«<J >"| :
1j
(98)
7. Discussion of Results
In order to see where the nonrelativistic current operators are nolonger valid, the electroproduction cross section off of a proton pro-ducing a n+ is calculated using the fully relativistic operator in eq
.
72 and compared with the nonrelativistic results from eq. 73. In fig. 6,
we see that the nonrelativistic results are not very good beyondk2 = - .l(GeV/c) 2
. In figs. 7 and 8 are plotted the transverse andlongitudinal cross sections.
In order to get better agreement between the two results, one wouldhave to include terms which depend on the initial and final 3 - momentumof the nucleon. This is no problem for pion production off of a single
—>—* —
>
nucleon, because P. = - k and P_ = 0. But for pion production off ai _^ f
nucleon in a nucleus P.^*k and Pf^0 and these terms greatly complicate
the calculation.
The author thanks Dts. James O'Connell and Leonard Maximon for
proofreading the manuscript and for helpful suggestions and discussions
29
8. Appendix
From ref. [l] and [7], the form factors to be used in eq . (71) and(73) are
FA= 1
, mA=l.
1k2
<£=
(1 + K )
Pk2
1 ".71
°£= 1
k21 ".71
GM
"Kn
1k2
".71
nGE=
(1
T Gn
M+ 4T) J 4m2
The pion form factor is
_1_
.-
F = r-g— , m = 0.765 GeVtc , k3 p
m2P
9. References
[l] Dombey, N., and Read, B. J., Nucl. Phys. B60, 65 (1973).
[2] Mandl, F. , Introduction to Quantum Field Theory, pp. 75-78(Interscience Publishers, Inc., New York, 1960).
[3] Sakurai, J. J., Invariance Principles and Elementary Particles,
pp. 178-184 (Princeton University Press, Princeton, New Jersey,
1964).
[4] 01s son, M. G., and Osypawski , Nucl. Phys. B87 , 399 (197 5).
[5] Bjorken, J. D. , and Drell, S. D. , Relativistic Quantum Mechanics
,
pp. 285-290 (McGraw-Hill, Inc., New York, 1964).
30
[6] DeBaenst, P., Nucl. Phys . B24, 633 (1970).
[7] Read, B. J., Nucl. Phys. B74, 482 (1974).
[8] Derived with Dr. E. L. Tomusiak.
[9] Dalitz, R. H., and Yennie, D. R., Phys. Rev. 105, 1598 (1957)
31
200
-J
b
+
6
it: cr
150
100
50
NONRELATIVISTIC
RELATIVISTIC
02 .04 .06
|K2
| (GeV/c)2
.08 .10
+ ,
Figure 6. Comparison of cross section slope for e(p,e'7C )n using fully
relativistic and nonrelativistic amplitudes.
32
300
I K 1 (GeV/c)'
Figure 7. Slope of the transverse and longitudinal cross sectionsusing nonrelativistic amplitudes.
33
300
250
200
=1150
100
K | (GeV/c)'
Figure 8. Slope of the transverse and Longitudinal cross sections
using fully relativistic amplitudes.
34
NBS-114A (REV. 7-73)
U.S. DEPT. OF COMM.BIBLIOGRAPHIC DATA
SHEET
1. PUBLICATION OR REPORT NO.
NBS T^957
2. Gov't AccessionNo.
3. Recipient's Accession No.
4. TITLE AND SUBTITLE
Threshold Photo and Electroproduction of Pions from Nuclei
5. Publication Date
September 1977
6. Performing Organization Code
7. AUTHOR(S)E. T. Dressier
8. Performing Organ. Report No.
9. PERFORMING ORGANIZATION NAME AND ADDRESS
NATIONAL BUREAU OF STANDARDSDEPARTMENT OF COMMERCEWASHINGTON, D.C. 20234
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24u4?T111. Contract/Grant Nc
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Same as item 9.
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Final
14. Sponsoring Agency Code
15. SUPPLEMENTARY NOTES
16. ABSTRACT (A 200-word or less (actual summary of most significant information. If document includes a significant
bibliography or literature survey, mention it here.)
The nonrelativistic amplitudes for photo and electroproduction of pions arederived using effective pseudoscalar and pseudovector Lagrangian densities. Theresults for pseudscalar and pseudovector coupling are compared at threshold forcharged and neutral pion photo and electroproduction. Cross section formulas andkinematical conditions are also presented.
17. KEY WORDS (six to twelve entries; alphabetical order; capitalize only the first letter of the first key word unless a proper
name; separated by semicolons)
Effective Lagrangian; electroproduction; impulse approximation; photoproduction;pseudoscalar and pseudovector coupling; threshold pion production.
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