bvl-'i^ ' *"* um-p-79/10 bremsstrahlunc and neutral
TRANSCRIPT
Bvl-'i^ ' *"*
UM-P-79/10
BREMSSTRAHLUNC AND NEUTRAL CURRENTS
R. G. Ellis and Bruce H.J. McKellar
School of Physics, University of Melbourne, Parkville, Victoria, Australia 3052
Abstract
The utility of the bremsstrahlung process in detecting
parity violations from V-A weak neutral current interference is
analysed in two ways. Firstly, bremsstrahlung from polarized
lepton-nucleus scattering has an asymmetry with respect to the
polarization of the incident leptons, and secondly, bremsstrahlung
from unpolarized lepton nucleus scattering has a small circular
polarization. The magnitude of each effect is calculated. The
ratio of the parity violating contribution and the parity conserving
contribution to the cross section is shown to be a misleading measure
of the utility of these experiments. A parameter, the figure of
merit, is Introduced and used to discuss the feasibility of possible
experiments.
Work supported by a Commonwealth Postgraduate Research Award.
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1. Introduction
Since the discovery of the neutral currents (CERN-GARGAMELLE
collaboration, 1973) there have been many methods suggested for the
determination of their structure (Adler et al., 1975, Pakvasa and
Rajasekaran. 1975) yet ieveral questions still remain unresolved.
One of the most important questions is the nature of the neutral
current interactions of the charged leptons. In particular, recent
measurements of the parity-non-conserving (PNC) effect in atomic Bi
(P. Baird, et al., 1976) which have been somewhat inconclusive, indicate
that the PNC effect may be smaller than predicted by the Weinberg-
Salam model (Loving, 1975). This model has been rather successful in
the explanation of neutrino neutral current interactions (B.W. Lee, 1976)
and in recent e + d ->• e' + X experiments (Prescott et al., 1978).
Consequently further leptonic experiments to determine the magnitude of
PNC neutral current effects would help resolve the nature of the weak
currents.
To date a number of lepton-hadron and lepton-lepton systems
have been investigated and experimental tests of PNC in neutral current
couplings have been proposed involving e(polarized) + d -*• e' + X
scattering (Prescott et al., 1978), electronic atoms (Bouchait and
Bouchait, 1974, Brodsky and Karl, 1976) muonic atoms (Moskalev, 1974,
Btrnabeu et al., 1974, Feinberg and Chen, 1974), e e annihilation
(Dass and Ross, 1975), lepton-lepton pair production (Mikaelian and
Oakes, 1977) as well as circular polarization in bremsstrahlung
(Jarlskog and Salomonson, 1976). We suggest an alternative method
using lepton-nucleus bremsstrahlung as another process which may yield
information about PNC due to neutral currents (McKellar, 1976).
In particular, the photon cross section for bremsstrahlung
of polarized leptons on a nucleus will be asymmetric with respect to
th« polarization of the incident leptons if parity is not conserved.
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The order of magnitude of this effect will be Gm|/a (McKellar, 1976),
where m» is the mass of the polarized incident lepton: clearly PNC
effects will be largest for muon bremsstrahlung.
The subsequent sections of this paper contain a calculation
of the cross section for this process along with the magnitude of the
FNC effect, and the designation of a new parameter, "the figure of
merit", introduced in order to specify more accurately the viability
of this and similar experiments. The figure of merit is then
maximized to determine the optimum kinematic arrangement for the
observation of PNC. Also included is a reanalysis of a proposed
method for detection of PNC effects based on the PNC origin of
circularly polarized photons resulting from unpolarized-lepton
nucleus bremsstrahlung. This reanalysis is in terms of the figure
of merit, and leads to somewhat different conclusions as to the
optimum experimental conditions.
2. Calculation of the cross section.
We consider bremsstrahlung from a polarized muon in a point
nucleus neglecting recoil corrections, to lowest order in perturbation
theory. In the absence of neutral currents the appropriate Feynman
diagrams are shown in figure 1 which give the parity conserving
amplitude, (Sakurai, 1967).
Q 2 L q2-*"2 q' 2-^ \l
Where Q is the 3-momentum transfer to the nucleus of charge Z, and the
intermediate 4-momenta are q « p - k , q ' - p ' + k . p',p are the 4-
momenta of the initial and final muons of mass m, and u and u' are the
corresponding spinors. The metric, spinor normalization and notation
are set out in Sakurai (1967).
- 4 -
Replacing the photon in figure 1 by the neutral weak boson Z yields che Feyninan diagram for the neutral current contribution, figure "*.. The interaction Lagrangian for the Z can be written,
L z = *l V P ( Y V 5
} V O ( 2 - 2 )
o J=Vi,P,n J v J J 5 J p where the summation is over the couplings of the Z to the muon and nucleons in the nucleus, with a. and b. being coupling constants. This yields the effective Lagrangian, L --, for the Z interaction shown in figure 3, as,
Leff - i Vx ( VVs ) M. i j ' V v V V V ^ L ( 2 - 3 )
j P »n o
where we have taken the limit Q 2 « B £ where m is the mass of the o o
neutral boson, and the summation extends over all protons and neutrons in the nucleus.
If we assume an approximately random spin distribution amongst the nucleons, then the only term which will sum coherently will be,
i ? 4iY *ii«4i " Za + Na r-P,n j h i j p n
where Z and N are the proton and neutron numbers of the nucleus, respectively.
Furthermore, taking only the parity violating part of Leff w c m a y w r i t * »
-ib L - —H. (Zfl + N a )- Y y * (2.4)
e f f p v nr% P n ^ 5 V Li 0
- 5 -
Thus, the amplitude corresponding to the PNC part of figure 2 will be,
M . ?J - i ^ ' L . u r 4+im ^(a) . ,(q) d'+jm -, ( s ) , M • -Ze u' (p )£ LY Y a t + i 3 y y i u (p) P V - 5 q2-hn2 q'2^2 k 5
(2.5)
1 b
where £ - -^ (Za + Na ) . Ze2 m| P n
o In the Weinberg-Salam model
4ira 4Z where 6 , is the Weinberg angle, G and a are the Fermi and iine structure constants. The magnitude of E is typical of predictions made by other similar models, (Bjorken, 1977). Experimental attempts to determine E have been inconclusive, (Kayser, 1977), however, recent results from e(polarized) +d -»e'+x inelastic scattering favour the w-S prediction, (Prescott et al, 1978).
The cross section resulting from the combination of the PC and PNC amplitudes is of the form
do" do ± do ± for + ve helicity muons. c v
Here, do is the usual parity conserving cross section given by, (Koch and Mbtz, 1959).
Z 2 « 3 |p'|du dO. d?> ,2u 2 {-2cc ,Q 2[2(E 2+E , 2>c ,+c-Q 2-2m2]+ do. * P'
C 4ir |p | u Q* ( c c ' ) 2
(c 2+c' 2)(cc ,+2m 2Q 2)-8m 2(c ,E ,+cE) 2}
(2.7)
- 6 -
Whilst, do is the PNC contribution to the breasstrahlung differential v cross section, and is given by,
Z2a32£|p1du> d£L dfi ,u 2 , _ do —E { - (EQ 2+E'm 2+2Em 2 - — ) +
V it |p| U Q 2 c' 2
-^EQ 2+Em 2+3E'm 2- C-^)+ ~K ttQ2+2»2) (-EQ 2+2p 2(E+E')-2EE ,u)-m 2Q 2
u] c z cc
+ I _ B2(4p2. Q2 ) l. J_ Lm 2E ,(4p , 2-Q 2)4A» 2EE ,u+Ec ,m 2]} (2.8) c.2 c2
and c - -2p.k » 2(Eu-pu>cose) ; c' = 2pJk = •^(E'ui-p'ucose') and Q 2 - |p-p'-k|2 * p2+p,2+w2-2pu>cose+2p,u>cose,-2pp,(cos9cos6,+
cos$Sine'Sin6). The angles 6,6',4 are defined in figure 4. Integrating over the angle coordinates 6' and $ of the scattered muon yields the differential cross section in photon energy and direction do(k,u) which can again be separated in PC and PNC components.
dc(k,u) H do (k,ui)±do (k,u>)
Z 2 a 3 du dn p' m^i^Sit^e (2E2-hn2) (p 2 -u 2 ) where do (k,«) « 5 GJ2{ 5-5 m2 _-? ?— +
c ir u w- p l p z c H T z c z
E'm2 tt2(5E2+2EE'+3m2) ^ L_ r S m ^ S i n ^ Q u a ^ E ' ) _,_ 2m2E2(E2+E'2) p'cw p^c* pp' p z c H p*c z
+ «2(E2+EE'-m2) ] . »!S_ + J-L_r [» 2- 7E 2
+3EE'-E' 2] + eTC^4 - 2 " 2p*c* p'cu p^p'c* c* c
T 2 c J » (2.9) and the parity violating contribution yields -
- 7 -
da (k,u) = i-2_ c i u *L 2a,2 4 {^-T C — + » 2(5 + I 1 ) -2(E2+E'2-hn2)]+ v ir ui k p* vcwp tu E
T ^-T^ [2E4*E'+- (E'p,2+EE,a))+ \ „- 2(c-2m 2) (c^m^EE') ] + ^ g U E E ' m + E p ' 2
cp T c n i p pc
2. .,2 Ec . Ec 2 n 3E . 4E 2 4E'rf 8Em2 , 2E , 0_, w m K p zE - E*p z - -=- + -r-y J - —y + 7s- 5— + ̂ 5—(c-2E'ui)( —) r r 2 8m z ur wc c* c z T zc c 2
^ - T j - l W - E'(EE' -a 2)] wcp "
where E - in (|^) ; e T - In (f-|~) ; T - |p - k| - ^ + 0 " ; E _ P 1-p
The results of these calculations are shewn in figure 5 where da c
(k,u) and do (k,u) are drawn on the same axes to illustrate the magnitude of the PNC effect, for a muon of energy 3 Gev and photon energy 1.5 and 0.5Gev.
In figure 6 we show the ratio, R , of the PNC and PC contribution to the differential photon cross section, ie.-
»«)
R (k,u) -\ J *V*" J J d 2o cU,c A u A f i k (2.11)
Where the intergrals are over the element (Afi.,Au ) about (k,u>). R (k,u) is the parameter usually associatad with the feasibility of process yielding experimental Information about ?NC effects. We have
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included it for comparison with other calculations but emphasize
that R is not a true indication of the experimental feasibility
of the process under consideration. Instead we introduce another
parameter,"the figure of merit", which is a more realistic measure
of the observability of PNC effects.
3. THE FIGURE OF MERIT.
Measurements of the PNC effects require the determination
of the different AN between the number of photons observed with one
orientation of muon spin and the number with the other orientation.
If N is the total number of photons observed in solid angle Aft, and
in energy range Au about u then-
AN
Ne Afl, Aw k
dzo Aft. Au k (3.1)
Where e ia the degree of muon polarization. To establish the
existence of a real effect as distinct from a statistical fluctu
ation we require-
or
AN * N'
d*< Aft. Au h k N* j
w 4
d*< Aft. Au k (3.2)
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Fur ther , the t o t a l number of photons, N, can be r e l a t e d t o the
number of incident auons N by-
\ { f ^cV*- (3.3)
Where N. is the number of atoms per urlt volume of the target
material and t is the thickness of the target.
Substituting (3.3) into (3.2),
F = y
I! * AwAft.
f J J AwAft,
d2c £ AH N.-t.E*
M A (3.4)
Where Aft. ,Aw becomes the solid angle of acceptance and energy
resolution of the photon detector, and e' has been introduced as
the detector efficiency.
We define the LBS as the "figure of merit", F , for this
experimental situation and observe that maximization of F corresponds
to the optimum kinematic arrangement for the observation of PNC effects.
The kinematic arrangement obtained in this way is quite different
to that suggested by maximizing R which is the more usual procedure.
In order to evaluate the figure of merit It is necessary
to lntergrate d 2o over Aft. . Explicitly,
- 10 -
r do r do v - . I i !L_ J - _ I _ y _ -» = <; i n f t , . _ ~2 i • 2w i 2EE'c
j di^du, ~*k " j di^du **Sin8d« - * • ' « - ^ pT 1 - ^ T - COSO -r k ~
inc.eE <2(E24E'2-»«2)-«2<54 | 1 } ) + ejfmi ( E + 3 £ . } + 8«£ ( _ e +
Pw P'pu PP'w 4p' 2
p'<T 2 -p 2 )
r»f»»2*rpi„\ / . _ 2 P - T -"*
( T 2 - p ' 2 ) pp , 2 w T 4p* p ' pw T
2 p , l n ( I ^ ) + p , 6 ) + ^ - + ^T)(2EE'-4m2)+ ^ j ^ E E ' u + E p ' ^ E - E ' p 2 )
• 1 ? « * *&> <£-,>"> + " + ^ < ^ ' < - , - 2 » 1 (35) and
k
C^e + l £ 2 S i . * , . 5E2+2EE'+3,n2
+ 2E£L ( E 2 + £ , 2 ) +
p 3p* c pp c
+ «!!£_ ( B 2 . 7 E +3EE'-E'2) PP c
T.2 • <£ - V • i E ! ^ > + ̂ >'<<£,-> «'+ ? $ £ v 2 T 2 2
2p'
2m 2p 2 3e p 2 , ( P 2 - U 2 ) _ ? , 6 e_ _ c — } ( 3 6 )
T 2 - p ' 2
where fi - «i ( K —) T 2
- 11 -
As a typical case the figure of Merit has been plot ted in
figure 7 for auons of energy 3Gev, photon energy 1.5 and O.SGev with
energy range 4w = 0.05Gev and small s o l i d angle Aft. * w/ ftsr.
Comparison of figure 6 and figure 7 show that for the same
conditions the maxima of F and R occur at s ign i f i cant ly dif ferent Y Y
values of 0. Maximization of R is misleading and use of the figure
of merit is necessary for proper optimization of the kinematic
arrangement of the experimental situation.
Maximization of F (k,u,AP~ Aw) I ,„ indicates that the Y n e * juev
optimum kinematic arrangement occurs for observation of the complete
photon energy range and photons in solid angle A&. extending from
polar angle 8 - 40° to 180° and all azimuthal angles c. The figure
of merit is shown for several different solid angles in figure 8
which yields,
\»ax '3Gev ' Z ^ 2.16xl0~2 (3.7)
Rearranging (3.4),
N V n - J F 2 N t c» < 3' 8 )
W a
N is approximately inversely proportional to Z since F is
proportional to Z and N is approximately inversely proportional to
Z. Thus, a high Z target material will increase the feasibility
of this experiment.
The following typical values can be used to estimate N u 2 tnin, ( i ) e , the degree of polarization of the incident
nuons 'v 90%
- 12 -
giving
( i i ) e , the photon detector e f f ic iency •<. 20*
( i i i ) S , for a Pb target -. 3.3 x 1 0 2 2 cm"3
( i v * t , target thickness *- 10 cm
( v > £, from the Veinberg-Salam model (Sin 2 9 * 0.25) -. t 6.91xlO~5Gev 2
v M . > 3.2 x 1 c 1 1 (3 Q\ • i n V J * * '
Thus, maximization of the figure of merit has given the minimum
number of suons repaired in order to observe a s t a t i s t i c a l l y
s ign i f i cant PMC e f f e c t , as well as determining the optimum kinematic
arrangement for t h i s observation.
4 . FOEMPACTOR EFFECTS.
Formfactor e f f e c t s are expected to be s igni f icant in
strahlung. The formfactor can be included by replacing.
II do with j [ F(Q2)do
Where F(Q 2) is the formfactor. Analytical treatment becomes difficult
with the inclusion of the formfactor and the results of a numerical
analysis are shown in figures 6 and 7. The dipole type fomf actor
2 F(Q 2) - <JZ^Q7> 2 **e re « 2 * 0- 7* <* v 2
was used and is at least approximately verified at low Q 2 by existing
data. (Schreiner, 1974), (Kirk et al, 1973, Hanson et al, 1973, Bartel
et al, 1973). Maximization of the figure of merit F (k,*,Afl K » A u ^ 3 G e v
with the formfactor included, indicates that the optlmun kinematic
arrangement for the detection of a photon asymmetry occurs for
observation of the complete photon energy range and photons In solid
- I:
angle &JL extending from polar angle 6-8 to 148 and all azimuthal
angles, <j>. The figure of merit with the formfactor included is
shown in figure 8 for the optiaium solid angle. This yields,
which gives,
F
Y l 3Gev = Z S x l . S x l O " 3
m a X (FT)
NM . > 4.6 x 1 0 1 3
min F F
Hence detection of a statistically significant PNC effect requires
at least 4.6 x 10 1 3 muons. It remains to be seen if N 'vSxlO 1 3 is u
experimentally feasible.
5. CIRCULAR POLARIZATION OF ELECTRON BREMSSTRAHLUNG.
A reanalysis has been made of a related calculation by
Jarlskog and Salomonson in terms of the figure of merit. They have
calculated the magnitude of circular polarization of bremsstrahlung
from unpnlarized lepton-nucleus scattering. This circular polarization
has its origin in the PNC interaction. Figures 9 and 10 show the
figure of merit, F J g, and the circular polarization, R.g, which is the
difference between the right circularly polarized cross section,
da_ and the left circularly polarized cross section, da , over the
total cross section, ie,
do R-do L
RJS 5 do R+da L ( 5 A )
Figures 9 and 10 are shown for 30 Mev electrons with bremsstrahlung
photon energy 15 Mev ± 0.75 Mev and 6 Mev ±0.75 Mev and solid angle
of acceptance Aft. "*5 sr. In this case figure 10 indicates that the
optimum kinematic arrangement for the observation of circular
polarization will be with the detector centre at about 12 from
- 14 -
the forward direction. At this position R _ is about 2% of maximum,
thereby illustrating the necessity of a figure of merit calculation
to optimize the experimental arrangement.
The figure of merit has been maximized with respect to
solid angle and photon energy range and the results shown in figure
11. The optimum kinematic arrangement occurs for observation of the
complete photon energy range and photons in the solid angle,
Aft. , extending from polar angle, 9, between 30° and 180° and all
azimuthal angles $ (cf figure 4).
From figure 11,
-5 -1 F - Z C x 6.13 x 10 Gev max
In this type of experiment equation (3.8) becomes
N 1
max
where (i) e • polarization analysing efficiency ^ 5%
(ii) e' » photon detector efficiency *\. 20%
For a Pb target with thickness Iran N 2 2
\in * ̂ 3 X 1 0
Again, maximization of the figure of merit has given the optimum
kinematic arrangement for observation of PNC effects. In this case
the minimum number of electrons required to ensure that the PNC
effect will be significant has been estimated to be 1.) x 10 2 2.
With a beam current of 300 uA, this would take approximately
2,000 hours.
Formfactor effects will not be significant at 30Mev because
- 15 -
of the much lover momentum transfer than in the previous calculation
involving muons.
6. CONCLUSION.
The feasibility of two experiments which could yield
significant information on the nature of the neutral current interaction
of charged leptons has been analysed.
The first of these experiments involved detection of an
asymmetry in the breinsstrahlung photon cross section with respect
to the helicity of a polarized incident beam of muons. It was shown
that at least 4.6 x 10 3 3Gev muons would be required for the asymmetry
to be statistically significant.
The second of these experiments (previously considered by
Jarlskog and Salomonson) involves the detection of circular
polarization in the bremsstrahlung photon cross section from
unpolarized electrons. It was shown that at least 1.3 x 10 2 2 30Mev
electrons would be required for statistical significance. The
existence of the asymmetry and circular polarization which these
experiments respectively attempt to detect are PNC in origin.
It should be emphasized that these calculations made on the
basis of maximization of the figure of merit, yield the minimum
number of leptons required for detection of a statistically
significant PNC effect. Clearly in most experimental situations
greater lepton intensities will be required if the conditions for
maximization of the figure of merit cannot be experimentally achieved.
However, a smaller number of leptons than specified cannot yield any
significant information.
In conclusion, the detection of PNC effects of neutral current
V - A interference in bremsstrahlung would considerably stretch the
- 16 -
present state of the art. Whether either of these experiments are
feasible remains to be seen. In this paper, one criterion, the required
number of incident leptons, has been calculated and this must be
satisfied before further investigation using either of these two
experiments should be undertaken.
- 17 -
APPENDIX. This appendix contains the equations used in the calculation
of the figure of merit, FT_, and the ratio R , f or the circular Jo JS
polarization experiment. The matrix elements and Feynraan diagrams will be the same
as expression and figure 2. The cross section resulting from combination of the parity conserving and parity violating amplitudes will have the form,
do - do„ + doT R L
where do- is the right hand polarized photon cross section and doT
is the left hand polarized cross section. A difference in do R and doT indicates parity violation. Hence in this case,
do • do„ - do, while do * do„ + doT VJS R L CJS R L
where do v is parity violating in origin and do c is just the total bremsstrahlung cross section which will be the same as in the asymmetry calculation.
Squaring the amplitudes yields*
Zo 3 |p'| dm dn.dflp' d 0 . 5 * u2 {2m 2(c-c')( Jt+- i) 2 "
VJS ir* !P I « Q 2 C C
* 2"<7r + 7>(?r + ?1> +^Ccc'-2(Ea-E'2)3--ir(c2-c'2)} 'c' C *c' c ' cc' ' cc
in analogy with equation (2.8) Intergrating over the angles of the scattered electron yields (c.f. equation 2.10)
- 18 -
v J g TT u> k p W l c m2^ '+
c+2(EE'-m 2 ) p ' - 8m2o)E r - c + 2 p ' 2 ( E E ' - m 2 ) r . , c+2(EE'-m 2 ) p ' . , 2c p p'2p m^UlC 2c"2" p
2m2
r 2(c-E'u)) c + 2 ( E E ' - m 2 ) e T
A 2(c-E'u)) ( c + 2 ( E E ' - m 2 ) ) e T ^ L , T^~ ( " ^ VTc + ~ c " F p ^ ^ " ^ " (
2 ^ . ^ ^ . 1 ) + ^ ( . _ ^ ! . 4 ^ ) _ ^ ( 1 . 1 ( E 2 . E , 2 ) ^
do
I n t e g r a t i n g do (k,u>) over Afi, , (cf equat ion ( 3 . 5 ) ) , V J S k
'JS dQ, du> k
2irSin6d6
. Z 2 0 3 C ^ S p J . ^ { g 2 _ « c o s e + ^ ^ ^ E ^ < « ; - * ) u> k p P P p a) p m^oj
^ L . L , „ „ , 2 x „ x 2m 2 E , . 2 p ' 2 (EE'-m 2 ) „ , + 7 c o s e " T^7 (EE'-m 2 ) Znc) - - f r j U n c - - * — - V * * ' 2 top P ' P - nro>
?nc
p'L (EE'-m 2) n , n e T m2 4m 2 E t , e T
t T e T p '
.•2 * (fcp-7T»
J y ( . S L , n c . Z s i i l + E H , c o £ 6 . _ e _ ( c o 8 9 + ( E 2 - E , 2 ) ^ c pp» 2pu pc 2 uip' 2 pu '
, m 2 i + T3~"
p p *o>
PP
2 T 2
[,-Z P ; ^ + 6] + - P - [•*= f ^-] - - V - (EE»-m2)[- V + (T^-p'O p'ptu T p' P pw 4 m 2E' r P * 2 . .-. . m 2 r e 1 . 6
+ f e T
+ 5]
- 19 -
M + — I - + 2TT— ((T+p') In (T+p')-(T+p,)+ ̂ e T + p'6)-
,EE'-m 2we T . 6 . 2 ,
pu>p T p p'o '
These expressions together with the parity conserving
equations (2.7), (2.9), (3.6) are sufficient to evaluate R and YJS
F YJS.
- 20 -
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- 21 -
Figure Captions
Fig. 1.
Lowest order diagrams contributing to electromagnetic
bremsstrahlung. A represents the nucleus.
Fig. 2.
Lowest order diagrams contributing to parity non conserving
matrix elements in bremsstrahlung. The cross represents the nucleus and
the dot the neutral current interaction. Z is the neutral intermediate o
vector boson.
Fit. 3.
Feynman diagram for the interaction betwen the muon and the
nucleon via the intermediate vector boson, Z . In the static limit
this reduces to the neutral current interaction of Fig. 2.
Fig. 4.
Defines the angles 6, 8',<fr. p, p', k are the incident muon
momentum, the scattered muon momentum and the photon momentum respectively.
Illustrates the relative magnitude of I do_ • PC
Aft, Au k
c
and I I da • PV where the integral i s
Aft.Au
over Aw - 0.05 GeV « - ±,2 GeV Aftfc « ^ sr and E - 3GeV.
**g- *• It as a function of polar angle 6; Au> * 0.05 GeV Y
Lt\ * 16 ,r* u " 1*6, °' 6 G e V E " 3G*V*
- 22 -
Figure Captions (Contd.)
Fig. 7.
Fig. 8.
F as a function of 9. ;Aw,An >u>,E as in Fig. 6. T kt
Maximization of F as a function of solid angle magnitude
and direction. The curve labelled 140 _ corresponds to maximization Fr
of F with formfactor included. The labels 3, 30, 60, 90 etc. correspond
to the polar angle A6, over which Aft, extends. 6 defines the angle about which AH, is centred. k Fig. 9.
Fig. 10.
m- n-
R as a function of 6. E » 30MeV Au> - 0.75 MeV
AG. - "2Q sr u * 15, 6
F as a function of 6. E, Aw, Afik, u> as in Fig. 9.
F maximized as a function of solid angle magnitude and YJS
direction. The labels 3, 30, 60 etc., as in Fig. 8.
1
ot
LL
CO
Fig. L
CROSS SECTION //do-/ / <
< CD
-15 o O 1 cn 0
PHOTON e
i i • i i • i i i i 0 PHOTON
e
-
ANGLE [degrees]
ro /
r ro/
"0 / °/ 1
r n
T — i — i — i — i — r
PHOTON ANGLE 0 [degrees]
180
' Fig. 6.
0 T I I i i I T
PHOTON ANGLE 180 - 9 [degrees]
• Fig. 7.
1
10 H n ,
M10"2 -
E UJ
£ 10"3
o Li.
-4 10 H — i — i — i — i — i — i — i — i —
0 PHOTON ANGLE 180 6 [degrees]
Fig.8.
T — i — i — i — r
PHOTON ANGLE 9 [degrees]
180
Fig.9.
1
-4x10 T — i — i — r PHOTON ANGLE
6 [degrees]
Fig. 10.
T 1 — i — i — r PHOTON ANGLE
6 [degrees] 180
Fig. 11.