in terms of the density matrix by The tensor Tkg is only dependent on s, ,u, ,u', k and q and has matrix elements expressed in tenr_s of Clebsch-Gordon coefficients : (-1)8+w C(ssk, p, -p'q) .
(2.2)
In the case of the deuteron, s = 1 and the possible values for k are 0, 1, and 2, which are directly related to the differential cross section, vector polarization and tensor polarization respectively . For the sake of simplicity the initial nucleus is assumed to be unpolarized. The density matrix for an unpolarized nucleus with spin I is given from (2 .1) and (2.2) by putting k = 0, q = 0 and s = I as PM AM ,A
ómAM,A
= (2IA+ 1~
(2 .3)
SPIN-ORBIT EFFECTS IN STRIPPING
49
Using the orthogonality property of Clebsch-Gordan coefficients the deuteron density matrix expanded in terms of the spin tensors
= Ip it,
(2 .5)
where I is the reaction matrix and Tr p' = (vdwp)a(0) . It has been shown 1) that the general form for the reaction matrix including spin-orbit effects is given by IPPMH~ pdMA
X
where
YpTdil (
L Ld p
C IA% IBP
MAIujMB)A (LpLdJpJdlj)
( - 1)w' .W(LpMp) .sl* (LdMP+,uJ+Iup
M p~u~
lud)
X C (Lpjjp , MpypM. p+yp)C( L d l,l d ; Mp+93+Pp-ludYdMP+lui+YP) X C (Jdfx Mp+/uj+lup j -,ufMp+,up),
A (LpLdJjd1j) =
( -1)'P+Ld+Jp+,d8, Ki-a1/31 Ld!dRLPL
dfpJdli x C(L d 1L p , 000)X (L p ~Jp ) l2j. r d 1Jd),
and' denotes (2j+ 1) i. Using the expansions (2 .3) and (2.4) in (2.5), we write the density matrix of the final state in the form -
I
lm
PpMB ; I~dMA
làdlu'd
l~d~'d
Ic'd MA : A'pRI'g'
The density matrix for the emergent protons in the stripping reaction is given from (2 .7) by summing incoherently over the spin projections MB of the final nucleus, i .e. P «ph'p =
MB
P, pMB. P'pM$
The spin polarization of the emergent protons may also be expressed in terms of spin tensors, viz . 14pp'p
of rank R = 0 and 1 . The term Tr p' occu-'s in (2 .8) so as to normalize the final
density matrix p' to unity.
D . 3tOBSON
50
Inserting (2.8) and (2.7) in (2 .8) and summing over MA and VB We obtain the spin tensors
pd
POIPPMpWp
XC(IR , lupT - ppT)C(Lpjp , MpiupMp+lup) X C (Ld 1Jd, MP+9f+iUP IudludMp+lui+lup) C (JdiJp Mp+/uf+lupp lu! Mp+~gp) (2.9) " C(L pL'pp, Ml, --M'P#) -PdM--T--1&) X C(LdL'dq, Pd - Mp_P3 PV M'p+#9 + #p+M-T X C (LIP UP I M' PFP - TM'p+pp - T) 1AjM'p+,up X C(L'd IJ'd, M'p+juf+1tp-T - Pd+MJUd -- MM'p+us+yp -- T)
X C (J'djJ'p j M'p+p3 +,up - T, XYV4 (®kp ,
-
Ok p)Yq (#+T-M)(ekdI Okd) I
where
'
-£ 'd C (LdL'dq , 000 ) C (LPL'pp, 000), fd ~q
B( Pq) = 4n iLd -Lp+ VO-L d LP ~~p
and where we have used the coupling rule for spherical harmonics M B, Y" 6, ( O) LM ( 0) --
~~' C'LL' , MM' lu) C (LL' , 000)Y ) p ( ~) :;14 h ,
L
In connection with (2.9) it should be noted that only a single sum over t occurs due to parity considerations. a and a' denote collectively the projectile quantum numbers. With the help of known sum rules s) we carry out the summations over spin projections Yd , ,up and yp and also over the projections Mp and Mp.. We find
x
Tr p'
_
(2IB+ 1) (2IA+ 1)
(_1) Vp+Ld+p+tpq rt
.1 < T" >
A (a, lj)A (á , lj)B (Pq) (2j+ 1 ) pfd .%'d(2t+1)(2Jp+1)(2J'p+1)
rM
aa'lßpq
1
X W (J'pjtJd ; J'dJP) W (pRgI; tr)X (LdL'dq, 11I, JdJ'dt) xX(LpL'pp, JJR, JPJ'pt)C(RIr, T, -MT-M) (-- 1) T C(_Pqr, ;q, -,u+M--T, M--T)YDO(®kp,
For R =
I
Okp)Yq-11+M-T(ekd,
(2.10) Okd) "
this formula determines the polariza~ion of the protons. The
51
SPIN-ORBIT EFFECTS IN STRIPPING
components of the polarization vector are related to the spin tensors < TRA > by Pa .= {Tll>-
P, = i «T">+
and P£ = -1/2
1
(a',
A (oc,
lj)p Ij)B(pq) (2IA-+-1 ) IM `,aa'ljpQ (2j+ l ) h ( -1 ) Ld+p- FD-1YgJ d1 'd(2JP+ 1 ) (2J'p+ l) W(J'piPJd ; J'aJP)
x X (LaL'aq~ i<
C
11I, JdJ'dP)W (L'pLpj'pjp ,
P
qI, ju, --,u+1VIM)YP ~& (ekp, OkpWQ
2 )
p+ISf
(ekd Okd) . ,9
Formulae (2.10) and (2.11) are the most general cases for the polarization and angular distribute -n of the protons emergent from a stripping reaction involving arbitrarily polarized deuterons. In the particular case when the deuterons are unpolarized, we find, putting
(--1)pYp*4 (ekp '
Okp ) Yp
p (0kd ' Okd)'
and the polarization for unpolarized deuterons JRT
>o{Tr P'}o
_-.
(2IA+ 1 A l) Y 1) (2j+ (2IB+ aa'Ijp 1) _
_
(oc,
lj )A
(a', lj) B (pp )
X (-- 1)J 'd+Jd+L'd+L' p$ (2p+1)JdJ'd(2Jp+1)(2Jp'+1)
X W(PL'dJd l ; LdJ ' d)W (J'JPJd3 J'dJp)x(LpL'pp' 1 2 R ; Jpj'pp) ( -1)TC(PPR, p, -p-T ^T)YD~z ( okp 3 Okp) Yp -p-T (ekd' 0kd)
From (2 .11), (2.12) and (2.13) we can write Tr p' in the form 1/6H(aaa'ljp)G(p, 1)F(p, 0) aca'I,fP
(2 .1 )
n. Rossaa
52
in which H(aoc'ljp)
G (q, I)
F(p, R)
_ -
(2IB+I) (21A+'1)(;41-+-1)
A (a, lj)A (a', lj)$(pq)l(--I)Ld-Jp-~ X J dJ od(2Jp+ 1) (2J,p+ 1) W(J 0 pjPJd r J'dJP ) 9
fiX (Ld L' d q,
111, JdJ'dP) = (-I)Jn0+'p 0~X(LL'pp, IJ R, Jpj'pq),
and lu, (-'I)9C(pgI, Plm --
lu+M' M)yp #( ItD
D)Ya + 'M (e kd
Y'k
Y'kd)'
From (2 .14) we see that the angular distribution for a polarized incident beam in which spin-orbit effects are incuded, is of the general form [a(®)Jpol
_ Ca(8 )]unpol{I+f(oca'ljp)pp'
pd+g(«a'ljpq),j
P2arr
and hence [a(8)]pol depends on the tensor polarization comport(;nts
3(21B+
1)
( 21A+ I)
IM
XMW(J1ll ; tj)X
X
(I R , Iti, 1I1)
C (RIt, -TMM-T)
x Fam Fm+M-T*' Tr P' - 3 (2IB+ I)
lit
82 (- 1) R-T+j+j+t sa
m
(-1)m C(llt, -mm+M-TM--T)
0,21 (-1)s+1
(21A+ 1) IM ßa X W (le Ïll ; ij)W (I Ilj ; ij) (2 X
m
(2.16)
(-I)''C(III, -mm+MM)FI-Fam+as* .9
_ (2IB + 1) a R-T+J +J W( ll ; R (2,A+ 1 ) sa ®sa(-I) X W(J J ; R1) ( -1)'mC(IIR, -mm--T, --T)
.17)
>o{Tr Pr}o
x FamFIm-T
,
m
(2 .13)
SPIN-ORBIT EFFECTS IN STRIPPING
and
{Tr P10
where E
m
OLylLp YaMnp
f
=1
(21B+ l )
' IF1m i 2~ 112(2IA+1) (21+1)
53
012
(2.19)
vp(kpr)u1(r)Z-1Y1m (0n .,On)*Vd(kdr)dr
(2.00)
contains the phenomenological part of the mechanism. These relations are slightly simpler than the corresponding ones derived in ref. 2 ) in which the channel spin formalism was employed. We have used --j coupling throughout . Putting R = 1 and T = 0 in (2 .18) yields the polarization of the protons for an unpolarized deuteron beam (-1)'-1-1831(2j+ (2j+1)-'(?1+1)-! 2 ,V mi FI -1 m = 21 (2.21) p 3 12 p$r I FZ m 831(21 + l )-1 1 i1
m
in agreement with Huby el al. , ; ). The analogous expression to (2.15) is obtained from (2 .17), (2.18) and (2.19) as CQ(8 )Jpol = ( 1 + 3 Pip ®
d)[11(8)lunpol "
Comparing (2 .15) and (2.22), we see that (2.22) is a special case of (2 .15) where the coefficient g is zero and the coefficient f is a pure number. If (2.22) is valid one can conclude that this relation yields an alternative procedure for determining the polarization of the emergent protons in a stripping reaction . The validity of (2 .22) is investigated in the next section for the C 12 (d, p)C I3 reaction. esults for C11(d, ))C11 using 9
eV Deuterons
We may express (2.22) in two alternative forms which are more amenable to discussion, viz. and
(a
+ -.6- ) /6QQ)
d1 ; (30. 2 )
in which a + and a- are the cross section- for deuterons polarized along and against the direction d x kp respectively, and ao is the cross section for un® polarized deuterons. Here for simplicity of calculation we assume completely polarized deuterons : ; d 1 = 1 .
a+, a- and aQ are calculated including spin-orbit effects and Pp then predicted from (3 .1). This prediction is compared in fig. 1 with the polarization calculated exactly. The parameters used for these distorted wave calculations are the 0.75 0.50 0.25
-0.25
(1) Prediction forPp from(3.1) (2)Exact Calculation of Pp
-0-50
.:
-0.75
Fig. 1 . Polarization in the stripping reaction C 1 s(d, p)C18, Q = 2.72 MeV for 8.9 MeV deuterons. (1) is thepredicted curve for Ppusing (3.1) and (2) is the predicted curve for Ppcalculated directly. The optical parameters used are shown in table 1.
same as in the preceding article 1) and are shown in table 1 using the same notation. TASLz 1 Parameters used to calculate a+, a-, aro and Pp
Protons
45 MeV
vp =
10 MeV
Deuterons
55 laM=
15 MeV
Wp =
8 keV
ap = 0.5 x 10-18 cm
Rp = 1.2 x 10-18 Afcm
08MeV
0.7 x 10-18 cm
1.59 x 10-18 Ai cm
Ve
=
The polarization predicted from (3.1) when spin-orbit effects are included has the correct sign at the stripping peak but is reduced in magnitude. At large angles (3.1) is obviously inadequate. The calculated values of a+, a- and ao are also inserted in (3 .2) . The result is shown in fig. 2 and indicates that at the stripping peak there is at least an error of 10-20 % if spin-orbit effects are included, and at backward angles (3 .2) is also invalid. Since the polarizations around the stripping peak are usually only 10-20 % we must conclude that the use of (2.22), or the alternative forms (3.1) and (3 .2), could easily lead to erroneous spin assignments in naclear spectroscopy. If the polarization of the product of a stripping reaction
SPIN-ORBIT EFFECTS IN STRIPPING
5.5
are to be measured correctly, it must be determined directly using a second scatterer.
10
0.5
30
60
90
120
150
9scatt (
Fig. 2. Predicted curves for the quantity S = a+-}-a-/2ao in the stripping reaction Cl$(d, p) C'3, Q = 2.72 MeV for 8.9 MeV deuterons. The straight line at S = 1 is for (3.2) and the curve i:> the theoretical prediction for S calculated directly. The optical parameters used are shown in table 1.
The use of polarized beams would be very useful for determining the importance of spin-dependent distortion such as spin-orbit coupling . An example of this is shown in fig. 3 where, we show the theoretical prediction for the polarization of protons, for completely polarized deuterons, in which spin-orbit effects
v
v
+05
;
~;
Stripping Peak
v
P(el
v
-05
v v (1) =P+ (2) = P
,
30
I
1
60
90
-
`1
I
120 150 O scatt
Fig. 3. Polarization in the stripping reaction C'$ (d, p) C'3, Q = 2.72 MeV for completely polarized. deuterons at 8.9 MeV. The two curves, (1) and (2), are the theoretical predictions for Pd = $1 and --1 respectively . The optical parameters used are shown in table 1 .
56
D.
Rossai
are included. If spin-orbit effects are neglected and completely polarized deuterons used, then the protons emerge fully polarized. If spin-orbit effects are included, spin-flip transitions are possible . Fig. 3 shows that "spin-flips' are unimportant at the stripping peak, but become very important at backward angles. These 'spin-flip' transitions were neglected by Cheston 7) but fortunately the present calculation shows that this is a good approximation at angles close to the stripping peak. . Discussion The results of the investigations carried out in both the present paper and a preceding paper 1) suffice to prove that the effects of spin-orbit interactions in stripping are important. The fact that polarizations of 50 % are found e) experimentally at angles where the stripping mechanism almost completely predominates is sufficient evidence for the necessity of including some form of spin-dependent forces. We have shown that the probable explanation of large polarizations is due to spin-orbit effects in both incident and final channels. From the present paper it is evident that the use of polarized beams is unlikely to be re'iable as a tool for nuclear spectroscopy. The use of polarized beams in stripping could be useful in the investigation of spin-dependent forces and possibly higher spin moments of the incident particles. The author wishes to thank Dr. F. Hirst and his computer staff for their help in the operation of CSIRAC, and Associate Professor C. B. O. Mohr for his continued interest in this work. He would also like to thank Mr. B. A. Robson for programming the complex Schrödinger equation. References 1) 2) 3) 4) 5) 6) 7) 8)
D. Robson, Nuclear Physics 22 (1961) 34 G. L. Vysotskii and A. G. Sitenko, JETP (USSR) 4 (1959) 812 G. R. Satchler, Nuclear Physics 6 (1958) 543 B. A. Robson and D. Robson, Proc. Phys. Soc. (to be published) M. E. Rose, Elementary th,.,ory of angular momentum (Wiley, New York, 1957) R. Huby, M. Y. Refai and G. R. Satchler, Nuclear Physics 9 (1958/59) 94 W. B. Cheston, Phys. Rev. 96 (1954) 1590 P. Hillman, Phys . Rev. 104 (1956) 176