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328
LETTERS TO THE EDITOR
B" seems justiGable to assume that the transition to the
ground state is allowed in the usual sense.
The bound
next states
quoefstBion" inisthtehapt -coafptturraensiptirooncsesst. o
excited, The fact
tohfaBt "oinmlyplie1s3%thaotf
all absorptions high excitations
lead to bound states are favored. Appreci-
able formation of excited states would wash out the
orientation in the ground state because of the smearing
over magnetic quantum numbers that occurs in the
process of de-excitation by p-ray emission. Fortunately,
the situation here seems favorable. There are only four
' known excited states below the threshold for particle
emission. While no firm arguments can be made, what is
known of the spins and parities of these states makes
it seem
events
probable that the leading to holed
large states
majonty
of B"
of p,-capture actually go
directly to the ground state.
Another effect which must be considered is possible
B" depolarization of the nucleus due to hyperGne inter-
action with the atomic electrons. Rough estimates
indicate that the atom is probably ionized due to
recoil at the instant of absorption of the p, meson. If the
atom is always ionized and then re-forms again after
it stops, we can calculate the depolarization under the
assumption that the Gne-structure substates are popu-
lated statistically. This gives, for the resultant B"
polarization,
(J)=-;(0.54)(n) =0.36(n).
(2)
3" Thus, if ~(a)~ equals 15%, the final polarization
~(J) ~
of the is probably closer to 5% than to the value of
10% given above.
There is an additional depolarization due to the
environment in which the B"atom 6nds itself. But the
relaxation time for this effect in graphite is presumably
B" longer than the mean life of since metals show
relaxation times of the order of tens of milliseconds.
In any event, such solid-state effects can be essentially
eliminated by a suitable choice of organic material as
target.
*This work was supported, in part, by the Ofhce of Naval Research and the U. S. Atomic Energy Commission.
t Visiting Guggenheim Fellow, on leave of absence from McGill
University, Montreal, Canada.
~T. D. Lee and R. P. Feynman, Proceedings of the Seventh
Annual Rochester Conference on High-Energy Euclear Physics,
'April, 1957 (to be published).
R. L, Garwin, L. Lederman, and co-workers at Columbia have
observed the longitudinal polarization of the electrons in y decay
(L. Lederman, in reference 1).On the basis of a theory of p, decay
the direction of the y meson s polarization can then be inferred. 3 Wu, Ambler, Hayward, Hoppes, and Hudson, Phys. Rev. 105,
1413 (1957). 4 Garwin, Lederman, and Weinrich, Phys. Rev. 105, 1415
(1957). ~ T. N. K. Godfrey, Princeton University thesis, 1954
J J' {u'npubalnisdhed). are the anal and initial nuclear spins respectively,
while 'Ag g is a numerical factor de6ned in the appendix of Jackson, Treiman, and Wyld, Phys. Rev. 106, 517 (1957). For a transition with AJ=O, the polarization of the daughter nucleus is of the
form of Eq. (1) with the factor )p.J replaced by E/(1+5) the coefficients X and b being given in the above reference (with E,=m, and the sign appropriate for electrons).
'' T. D. Lee and C. ¹
Yang, Phys. Rev. 104, 254 (1956).
Since the larger fraction of p, mesons bound in carbon decay
before nuclear capture, the directional asymmetry of the prompt
electrons can be used to measure the magnitude of (e) directly,
while the asymmetry of the delayed electrons will determine (J).
9 F. A. Ajzenberg and T. Lauritsen, Revs. Modern Phys. 27,
77 (1955).
Magnetic Dipole Moment of the Electron
CHARLES M. SO~RPIELD*
IIaruard University, Cambridge, Massachusetts (Received May 6, 1957)
~HE fourth-order radiative corrections to the
magnetic dipole calculated by Karplus
moment and Kroll
of in
1th9e49e.'leTchtreoinr
were result
is contained in the complete expression for the moment,
y, ,/pp = 1+(n/2w) —2.973(n /pr ) = 1.0011454, (1)
where po is the Bohr magneton.
The stance
calculation has been using the mass-operator
redone in formalism
the of
Spcrhesweinntgeri.n-'
We consider a single electron moving in a constant
(in space and time) electromagnetic field. The expectation value of the mass operator in the lowest state
represents the self or proper energy of the electron. The magnetic moment is identified from that part of the
self-energy which is linear in the external Geld.
The electron Green's function 6, the photon Green's
function 8, and the interaction operator I', which
appear in the symbolic expression for the mass operator,
+ M =m, te' TryGI'g,
are computed in the presence of (as functions of) the
external held. To do this it is sufficient to replace the
— electron's momentum
by the combination
operator, p,
II=p eA,
where it
provided
occurs, by that full
account is taken of the commutation properties of II.
Units are such that A=c=i. Renormalized quantities
are used throughout the perturbation calculation.
The fourth-order contribution to the moment is
found to be
— + li. '4'
n' (197
~' +-',t'(3) —-'m, '
q
ln2
= —0.328n—' ,
(2)
dup m' (144 12
~
where l'(3) is the Riemann zeta function of 3. Thus
p,/pp = 1.0011596.
The discrepancy between (1) and (2) has been traced to the term iir+ii'r' of Karplus and Kroll. In
other words, terms li"' and iirr'+ii"" appear unchanged
in the new result. A further point-by-point comparison of the two answers is not readily accomplished because the grouping of the terms divers markedly in the two cases. The present calculation has been checked several times and all of the auxiliary integrals have been done
in at least two different ways.
LETTERS TO THE E D I TOR
329
The theoretical magnetic moment may be compared
with the experimental moment; it is also used in
determining the 6ne-structure constant 0. , and it contributes to the Lamb shift. The magnetic moment is
measured by determining p,/p~ and p„/p&, where p~ is
the proton been quite
moment. accurate.
'
The On
measurements the other hand,
of p,/p~ have
there are two
confhcting experimental determinations" of p„/p, s,
which result in two diferent values for the magnetic
moment:
References
3and4
3 and 5
It e/Po
1.001146+0.000012 1.001165~0.000011.
The theoretical value' for the hyper6ne splitting in hydrogen is proportional to the quantity
=(—0.53+0.37)os/ss, which is consistent with the
value presented above.
'*RN.atKioanrapllusScaienndceNF. oMun.dKatrioolnl,
Predoctoral Phys. Rev.
Fellow.
77, 536 (1950).
2
'
J. Schwinger, Proc. Natl. Acad. Sci.
Koenig, Prodell, and Kusch, Phys.
37, 452, 455 (1951). Rev. 88, 191 (1952);
R.
Be'riJn.gHer.
and M.
Gardner
A. Heald, Phys R.ev. 95,
and E. M. Purcell, Phys.
1474 Rev.
(1954). 76, 1262
(1949);
J.
'''HAP. ..GFCarr.adnZniememrn,acPha,hnydPs.hSyR.sL.eviRe.be8evs3.,,
Cohen, DuMond, Layton,
996 Jr., 104,
and
(1951). Phys. Rev. 104, 1197 1771 (1956).
Rollet, Revs. Modern
(1956). Phys.
27, 363 (1955}.
"s
'
E. T.
E. Salpeter,
Fulton and
"W. Aron and
Phys. Rev. 89, 92 (1953). P. C. Martin, Phys. Rev. 95, 811 (1954).
A. J. Zuchelli, Phys. Rev. 105, 1681 (1957).
Triebwasser, Dayhoff, and Lamb, Phys. Rev. 89, 98 (1953).
""NHo.vSicuku,ra
Lipworth, and Yergin,
and E. H. Wichmann,
Phys. Rev. 100, 1153 (1955). Phys. Rev. 105, 1930 (1957};
A."PAete.rPmeatenrnm, anPnhys(.priRveavte.
105, 1931 (1957). communication) (to
be
published).
present value of e,v to determine a new value. This turns out to be
1/n = 137.039.
The theoretical Lamb shifts in hydrogen, deuterium,
and singly ionized helium are aRected by the changes
in both n and p, Incorporating these changes into the
' calculations of Salpeter,
recoil corrections of Fulton
along with and Martin,
t'heandprtohteonp-rreoctoonil-
" structure corrections of Aron and Zuchelli, we obtain
the following results in Mc/sec:
Theoretical
Experimental
Reference
SH
1057.99+0.13
1057.77m 0.10
11
SDS—DSH
1059.23~0.13 1.24&0.04
1059.00~ 0.10 11 1.23~ 0.15 11
" SHe
14055.9 &2.1
The experimental values"
14043 w13.0
12
have been listed for
comparison. There remain several uncomputed theoreti-
cal e8ects which are expected to be of the same order
of magnitude as the indicated theoretical uncertainties.
" The magnetic moment of the p, meson, as computed
by Suura and Wichmann, and Petermann, would be
changed to read
— —. — o.
n'q eh
p„= i
1+ 2~
+0.75
x')
i
2ns„c
I J. would like to thank Professor Schwinger, Pro-
fessor P. C. Martin, Professor E. M. Purcell, and
Professor R. J. Glauber, and Dr. K. A. Johnson for
their helpful comments and discussion related to this
— work. Note added its proof. Petermann" has placed upper and lower bounds on the separate terms of Karplus and Kroll. He 6nds that their value for pIIc does not lie within the appropriate bounds. Assuming the other terms to be correct, he concludes that p'/ps
P. F. ZWEIPEL
Knolls Atomic Power Laboratory, * Schenectady,
(Received April 18, 1957)
Sew Fork
' 'N a previous paper, ' tables of allowed X capture-
- - positron branching ratios were presented. However,
it was pointed. out by Wapstra' and Perlman' that
numerical errors existed in the table. These errors
appear in the first, third, and fifth columns of Table II
of reference 1, each entry of which should be multiplied.
by the factors of 0.5018, 1.2244, and 0.6462, respec-
I tively. In Table of this communication, the corrected
E table of allowed
to positron branching ratios is
given. In this work, the eftect of the 6nite nuclear size
' on the bound electron wave functions, which was
ignored in reference 1, was taken into account. This
eGect, which is negligible for low Z, reduces the branch-
ing ratio by about 10% for Z=84 and by about 15% for Z=92. EBects of finite size on the positron wave
' functions was ignored, since it is a considerably smaller
effect.
As in reference 1, the bound electron wave functions
were taken from Reitz's thesis' except for Z=16, for
E TABLE I. Allowed to positron branching ratios.
W0/mC2+g
1.28 1.44 1.60 1.76 1.92 2.08 2.40 2.88 8.84 4.80 5.76 6.72 7.68 8.64 9.60 10.56 11.52 12.48
29
46.6
707
1.208X104 4.56X105 8.92X105
8.65
112
1.58X108 4.50X104 8.41X104
2.83
38.6
425
1.08X104 1.84X104
1.24
18.9
164
8.57X108 5.01X108
0.641
6.91
77.6
1.57X108 2.67X108
0.378
8.91
42.8
807
1.86X108
0.190
1.60
16.4
289
479
0.0613
0.597
5.86
96.4
158
0.0169
0.160
1.51
28.6
89.0
7.00X10 8 0.0648
0.608
9.10
15.7
8.56X10 8 0.0828
0.802
4.82
8.05
2.06X10 8 0.0188
0.178
2.82
4.75
1.30X10 8 0.0118
0.109
1.80
8.06
8.85X10 4 V.93X10 8 0.0729
1.28
2.10
6.29X10 4 5.60X10 8 0.0513
0.879
1.52
4.48X10 4 4.09X10 8 0.0377
0.652
1.18
8.37X10 4 3.07X10 8 0.0281
0.498
0.869
2.60X10 4 2.37X10 8 0.0219
0.893
0.685