REPORT s . . i i . ; s
Mil D I I I K U I N M I U M l l I K \ ( I I I I M K M S I N S \ l l
K \ l I ) I \ M ( I \ I ) M : \ l \ M Kl Ml \ l \ l
\ H I K U S \ ( l l \ \ l l < ) \ \ N \ n s i s
I J I' I S.IU.I,,,;!
i J I' I SclUihup i I I \\ Mci l f
DM. ISil>ln <..Y hr.isnuis II W lesi i K.J.I). K.ibk
M M.iv. I"7S
NASIONALE INSTITUUT VIR METALLURGIE
R f P O R l • VFRSLACi V... lf>?K
l l l l - P M H i M I N V l l O N O l TK \ ( > H . K M K M S IN
NA 11 KAl OIAMONDS BY I N M K l M I - N I A I N f l TKOVAC I I V A
HON ANALYSE
1 st \ U \ I T 5
Itmstifiaturs O W Uihliv <' S I risrmis IIW I t s i I j I)
k^t.lc
ISBN 0 86999 176 0
S Y N O P S I S
\ in'*! nt more than 15'M) imliuikal litamiimls. ilisuleil into
'"> samples, nas anals se>i Ihcsc were obtained from three
South African mines Premier, hinwS. anil lagcrstontctn
I * .• presence ot 44 elemental in ihamomls was cstahhshcii from M
isot.iprs .in*! lUMiriumc rcMilis. were otnaineil 1<>r }4
elements.
s \ \i r v A i r i \ Í;
Daar is altcsame 15<M* atsomierhke iliamantr ontiecil ivat in
•>»> monsters icr.iee! «as llirr.lic iliamante was afkotmlii!
ian itne Suiil Unkaansc mvnr Premier, I -insert cn
Ja^rrstuntcin
Die aanwcsi^hcul v.iii 44 clemcrte is in tie diamante vas^cstcl van
M isotope en ilaar is k w a n t i u t i e w resu.tate sir J4
elcmente verkr\
« n v i \ \ r s
1 IS I KOI) ! ( I ! ! > \
.' I \ l " l K IMI N I \ l Ml I HOI) 2 1 M i l l I I O \ Ol 1)1 \ \
K ) \ I ) S 2 2 ( I I \ M \ ( , Ol 1)1 M H i M i s ? > IKK \ l
> ! \ I ION < O N D I I I O N s W D I I I \ « O S I I I I K I
M , 2 I < Ol \ I I N ( , I Ol I I 'MI \ !
2 4 1 \ l H S\»n-::: 2 * -' \ I' K I \\sr< -1-.
2 < 'J l \ l I I \ l l \ I VW>KK 2 (. IJI W I I I M I U 1)1 I
I K M I W I U>\ Ol M I O K I I l \ I I) ISOIOIM s 2 " <Jl \ M
I I \ I I U 1)1 I I KMIN \ I I O N Ol I ON( , I l \ I I) ISOIOIM s
2 ,H i i M I i s o i I » i i i HON 2 •' D M A Kl I ) ! I H O
N
5 KI SI I I s ; i I ( I IKOMH M „ .! 2 M \ \ ( . A M s | I 3 ( Ol '
l ' l K „ í 4 AN I IUON- i " „ ' ? l i \ K I I M „ < ' , ( I KM
M „ »7 V I I I K H I I M „ i X I I I I I K I l ' M
4 DISC I SSION A M ) « O N U I SION
5 \< KNOWI I I K . I M I N I S
f> K l I I K l \ ( I S
fable I Neutron H U M S .«nil cadmium ratios y table 2 Isotopes
positively identif ied in n.itur.il diamonds ') fable ! Kock
standards used I I Table 4 Kadionmlulcs ot sagnititanct- tor
i|iiantnafivc work 12 Table 5 trace elements in Premier diamonds |
J Tiit-lr (i trace elements in I insch diamonds |4 tabic 7 I r a n
elements in larcrslontcin diamonds 15 fable Js I race elements in
diamonds trom unknown sources | n
fable V Decav times alter which the isotopes Wire detected,
standards, and detection | ; l imits
LIST OK ILLUSTRATIONS
l'i|>urt' I Dcc.iv m m tor scandium 4f> IS 11)!iire 2 Dccav
curve lor lanthanum 14(1 and iridium-1'»2 19 l i f iurc J Dccav
curve tor l iarium 151 20 f igure 4 Decav curve for vanadium 52
21
A C f l N O I X A SUMMARV Ol I ' l l I I 'KI VIOUS WORK ON N A T U
R A L DIAMONDS 22
Table I I A nummary o f some elements and compounds detected and
measured in diamonds 23
owing to the diamond % inert and impermeable nature, accidental
inclusions of surrounding magma or co-precipttating minerals arc
not chemically affected bv the diamond's ascent to the f arth's
surface.
The amounts ot impurities present in diamonds can »ar\
vonside'alii» 1 p to several per ceil o: minerals have been found
in boart stones ' and nitrogen !r»r!s r.ighrr than "siMipp ;:i h u
e bs-en sletertnincil Nitrogen is responsible tor man» of the
spectra! properties nt .ti.i-Tion,! and is in tact used to classify
diamonds into different tvpes 'la. lb. and III Koron is thought to
I,.- response e fir the Semi-conducting property ot type lib
diamonds '
Diamonds that are regarded as inclusion free have a total impurity
content ot A few parts per million, anil the purest stones analysed
in this investigation had in impurity content ••' >ess than I
p.p.m.
the development and improvement ot analytical techniques have led
to the determination of more elements at lower levels. I he
earliest analyses of diamond were done In wet-! hemic»! methods on
the ash left alter the combustion of the diamond in oxygen 1'" With
the advent of optical spectrograph», a tar more sensitive too!
became available for diamond analvsis. requiring smaller samples
and less preparation" '. The volatile impurities found in diamond,
which a n he liberated if the diamond is burnt 1 0 or crushed' ',
have been studied bv mass spectrometry Infrared spectrometry ha»
also been used in the determination ot l l : ( ) and <:0, in the
outer mat ot a diamond1*. I lie electron rrmroprobe has l>cen
applied to the analysis of colloid-si/ed inclusions v v , ' and
;<> larger crystalline inclusions after thev ha»c l>ecn
removed from their diamond matrix' ' ' I he strain patterns
associated with the distribution of impurities have been studied by
X-ra» topography ''', and the crystal structures of inclusions bv v
rav diffraction The results of previous work are summarized in the
Appendix.
The most powerful technique used to date for the determination of
impurities m diamond is neutron-activation analysis'*"" In a
preliminary study l-esq rr .< : 1 , proved instrument.;!
neutron-activation analysis to be an extremely sensitive techiiiquc
for the analysis of diamond. particular!» because little or no
matrix activation occurs and the real Itmits of detection anproach
the theoretically possible limits.
A ma|or advantage of instrumental neutron-activation analysis
compared with other techr* ,ucs is that it is non-destructive, in
that, although the sample suffers considerable radiation damage, it
is available for re analysis This nondestructive aspect is
understandably of considerable importance with rare or expensive
samples such as diamonds
In this work, instrumental ncutron-acttvation analysis was applied
to a large suite of carefully selected diamonds. The initial aims
of the project were to studv the pcochemistrv of diamonds, to
investigate anv possible correlation between the colour of diamonds
and their chemistry, and to study the chemistry of the inclusions.
The suites of diamonds analysed were selected with these aims in
mind and are believed to be the largest, best selected (for the
above purposes), and best described suites from specific sources
that have been analysed to date.
2. KXPKKIMKNTAI. METHOD 2.1. SM.HCTIO\ Ol MAWtSDS
The diamonds analysed in this work were taken from one month's
production of three South African kiml-erlitc mines: Premier in the
Transvaal, Tinsch in the Cape ITovince, ami Jagersfontetn in ihc
Orange l-ree State. A total of over 1500 stones were grouped into
96 samples, each sample weighing about I gram and consisting of 10
to 25 stones in the sue range 0,25 u- 0.5 carats. All the diamonds
in one sample wcie se'ectcd so that they were as nearly identical
as possible in colour and quality, and, in the better grades, in
size. The samples were divided into eight earegorie* according to
colour and the presence or absence of visible inclusions, shades of
colour forming sub-categories.
The four main colour categories generally recognized are
colourless, yellow, brown, and green, the first three colours being
common to most mines. No green stones were available from
Jagersfontein, where they are found very rarely. Most of the green
stones found in I'insch owe their colour to a thin outer green
skin, which is generally accepted as being due to radiation damage
2' from naturally occurring radioactive isotopes.
In practice, the colours found in diamonds do not form clearly
separate colour groups, and diamond» vary in colour from colourless
through yellow to brown. Similarly, variations of colour from
yellow through yellow-green to brown have been found. Diamonds from
different mines vary in shade.
1
IRAt l I I I M f M S l \ m.VMOM»
and experience»I diamond sorter* can identify large parn-K oi
diamonds from ditícrent sources l>v means of thc.r colour land
morphological i characteristics
'Inclusion-tree' stones were defined in this work as stones in
which no inclusion*, or strain fields associated with them, could
be observed al ><• times magnification with polarucd light.
'Inclusion-containing' stones were selected as those having
inclusions that wcr. re.'.lily visible to the naked esc So attempt
was made to distinguish between graphitic and non-graphitic
inclusions, or between clean inclusions and graphite coated or
sulphide-coated tnclusioi s
At the same time as the inclusion free anvl inclusion containing
stones were selected, all stones were examined for surface «.racks
Stones with cracks were reacted since there was a possibility that
the kimberlite mains would enter the bods ot the stone and would
IK- extremely difficult to remove.
Hoart samples were also selected, and were grouped with the brown
-.amplcs. However, it was realized that boart consists ot a miss
!<f fused crystallites ot diamond, which can be expected to
include relativeiv large amounts of magma, and which mav a'so be
somewhat porous.
The predominant morphology of the better quality stones was
dodcvahedral. with some octahedral stones In the poorer-quality
samples teg txurt). there were more cleavages iv.A
misshapenness,
\ o attempt was made to type these stones according to optical and
conduction characteristics into the four accepted categories.
However, because natural diamonds arc predominantly type la . the
stones used ir, this work ire probably of that type One exception
may be sample P", which, irom its orange colour, possibly contains
some type lb stones
2.2. ( 7 M V / V . . Ol DIAMOSDS The purity of high-qualitv
diamonds KÍU be exceptional, less than 1 p.p.m. of impurities
other
than oxygen and possibly nitrogen be.ng tound m some of the diamond
samples analysed. I he meticulous cleaning of the diamond surface
is therefore essential if meaningful results are to be obtained,
the cleaning is made difficult by the presence of trigons and other
growth and dissolution features, or micro-cracks 10 to 20 ^m deep,
which are possibly due to percussion damage3 .
However, owing to the good chemical resistance of diamonds,
rigorous cleaning techniques involving strong acids and oxidizing
agents can be used The following procedure was used before, and in
most cases also after, neutron irradiation (1) hot hydrofluoric and
sulphuric acids ( 1 to 1 ) for 2 hours (to remove adhering silicate
matter). (2) hot mine acid for 3() minutes, repeated twice, (3) hot
distilled water for 5 minutes, repeated twite, (4) two washes in
acetone, (5) air-drying. All the reagents employed were of
analytical grade and were used without further purification.
Procedures involving hydrofluoric acid were carried out in new
Teflon-ware previously cleancM with the acid mixture used. The
other cleaning procedures were carried out in horosilicate
glassware that had been cleaned in hot nitri: acid before
use.
After being rlntvd, the samples were weighed and scaled in
high-purity polyethylene vials for the short irradiation. The
cleaning and weighing were done in a laboratory specially
constructed for this purpose, whuh had a filtercd-air supply and
contained only fiosc chemicals required for the cleaning.
The cleaning appeared to be satisfactory for the high quality
diamonds, since the results after rccleaning and re-analysis were
identical to the earlier results. In the boart samples there was
some evidence, after the repeated cleaning and analysis, that the
impurities had been leached.
2.J. IRRA»)AIIOS COSMTIOSS AM) H.VX MOSITORISV All the irradiations
were carried out in the Oak Ridge Research Reactor, Safari I, at
the South
African Atomic I nergy Hoard, Pclindaba, short irradiations of up
to 30 minutes being done in the pneumatic facility. High-purity
polyethylene 'rabbits' could be used in this facility, the diamonds
being sealed in smaller polyethylene vials inside them. The long
irradiations were carried out in the poolside facility, the
diamonds being scaled in quartz vials. Six of these quart/ vials
were sealed in a single high-purity aluminium rabbit. The neutron
flux*" and cadmium ratios in these two positions were as shown in
Table 1.
The total neutron flux received by each sample was measured by use
of a neutron-flux monitor. For the pneumatic irradiations, a 0,5
per cent gold platinum alloy was used for this purpose, the 411 keV
peak of the gold-198 isotope (half-life 2,7 days) being used for
flux correction. Mux monitoring wa» necessary, although the reactor
power (and therefore the total neutron output of the reactor) was
held constant to better than 1 per cent, since continual changes
were made to the
2
IKAC!' H ! MrVINIS l ) | \MHM)s
loiitigurari -1 <..' the reactor core I hi se resulted in
changes i,- .'u utiui nriirron i'uxo i! rhe t.'Xed irradiati» i
positions I hr flux monitor used for the poolstdc ir'adiatmns, « is
iror toil'", wnich was rolled into ,i sleeve complete!* surrounding
the uuart,- tube , ."it a'.-'-g rhr si-.pU !'':- enable.!
corrections to be rria.ie !.>r the overall variations in neutron
this ir ' tor the fiux era-'i-.-nt across each rabbit 1 his
gradient vas found to exceed 5 per cent tor the thermal neutron
flux, a;.: i" percent for the fast neutron '' , i \ ' (he iron «oil
had the additional i-lvant.u* that txith tr.r . nc—na! neutron arut
the fast neutron fluxes .nil.I be monitored simultaneously \ia the
reactions
' I e • -) i "* I >• i r"<T-M.. i
and , 4 | t i., f.i " \ | i ! Ifast-
In addition from tlv measured -.itm ot thermal t.. '.ic: nen'ronx.
3 •,ur!\ _'oo.t estimate of the epithcrmal tiux . ould be made'",
«hicn reduced lux > orrei <.•<•< c r . i - UK 'hose
elements having High epifhermal neutron troys actions
14 cm \11\1. KJIII'XUM luo * orripirfel* separarr . ountinir sv
stems were us--<! :n this Mori, one ar rl-e \f,>rn;«. I ner
y
Hoard ! \ l (H I'eltndaba. used tor the detection ot short lived
isotopes, and the other in the counting laboratories ,n the \iulear
I'hvsus Kesrarcb I'nit M ' H l' •• |ohat,-iesburg. «here the long
lived isotopes were dttcrmincd
2 4.1. AHi SyUem TN- sv >trm used t«.r the short lived work *
onsisted of a III t -n f.e'l.i» lerector. havinj.' .a
resolution ot „>.s ke\ t..r the 1 ' t2 ki \' peak ot coba't
••»> and M efficiency of ~.l ---r cent relative to that of a
T5by?5 mm Nal detector This was connected thri 'igh a Canberra
14D8C preamplifier *nA an Hscwt C W - V 4 amphtier to a Packard'»70
series 4tH>0-crianncl analyser Dati ;j;put was to a Kenncdrv
tnagiietic tape unit, and the data were processed on an IKM37H14S
computer using a modified version of .1 programme by Yule" I be
!•'•> Mil' an.ilog-jv to-digital converter of the Hacka'd
analyser had the capability ot being operated in the zero dead-time
mode described hv Haims I his eliminated any corrections due to
varying dead times during the counting period an important source
of error when counting times are of the same order as the half lite
The problems of pulse pile-up still remained and were reduced to
some extent bv the use of a pulser and the application of a
pulser-prak correction factor
The detector was shielded bv S cm of lead in the form of an
open-ended cylinder 30 cm in length and 15 cm in internal diameter.
A sample rotator was constructed that could approach the detector
through the open end of the cylinder The rotator was found to be
essentia! for tl'is work since the activities of the purest samples
were sv, low that they had to he counted I cm from afw' face of the
defector; vet they were so iinhotnogcncous tha' countrates could
vary In 5" per cent ut that distance2''. Rotation was found to
rc.luie the counting errors to a level at which they Were
insignificant compared with the errors in the determination ot peak
area. The rotator was constructed mainly from I'erspex. /nd was
mo.mted on an optical bench ha.ing click-stops at set distances for
rapid change', in detector sample distance.
2.4.2. \.P.H.I'. Syti'm
The counting system at the S I* K.l'. laboratories was similar,
consisting of a 45 cm 3 Ce(|.i> detector having a resolution of
2,4 per cent for the 13 32 keV peak of cobalr-60, and an efficiency
of 9.4 per cent relative to a 75-by-75 mm Nal(TI) detector This was
connected through a Canberra 1408C preamplifier and a Canberra 1417
amplifier, which incorporated a baseline restorer, to an
Interterhnique Didar 4000 channel analyser with a 100 MM/
analoguc-to-digital converter. Data output was onto an Ampcx
magnetic-tape unit. The system ilead time was corrected by use of a
pulser leak for the measurement of the total dead time 2*. This
reference peak was generated bv a Canberra 1501 stabilization
pulser, which was also used in conjunction with Intertechmque
digital stabilization circuits in the correction for gair, shifts.
Pulse pile-up was avoided bv a system dead time of less than 15 ^er
cent, so that pile-up was negligible.
This system waj shielded by a 5 cm cave of old lead, built to
contain the countn.g head of an automatic sample changer 3*'' 1 0
at distances of up to .3 cm from the detector face. The counting
head incorporated sample rotation for the reasons described above.
This rotator was mounted on an optical bench, and, to ensure
reproducible positions, a system of verniers and measuring blocks
was used to set detector sample distances to better than 0,005
cm.
2.5. QIAI.IIAIIM »ORK Preliminary work was undertaken to determine
how many elements could be iletermined by
instrumental neutron actuation analvs» in natural diamonds' and by
means of what isotopes Two samples were used tor thiN work. One was
a collective sample weighing 1.5 g and consisting ot approximately
200 small chips '.Aen from the Premier and rmsch Diamond Mines. IV
Beers Pool (Kimberlcyl. and the Consolidated Diamond Mines tie.,
the tour major diamond-producing regions of South Africa). The
chips were ot different colours, and were both inclusion-containing
and inclusion free. This was considered to be a good representative
diamond sample. The second sample, ten gem-q-alitv diamonds ot
different colours, was taken trom Consolidated Diamond Mines
The short-lived isotopes produced from these «amplcs were
investigated hv irradiation for 10 minutes and counting for 5
minutes at decay times from 1 to 60 minutes. The long-lived
isotopes were investigated in a similar manner. After an
irradiation period of 1?0 hours, the samples were repeatedly
counted with decav times frim 7 hours to 80 days the counting times
varying from 30 minutes to 2 hours-.
The spectra collected were processed, and the peak energies, peak
areas, error in peak-area calculation, and decay times were stored
on magnetic tape These data were then processed b\ a prognmmc that
applied a least-squares fit to a log-linear plot of peak area
versus time for each of the gamm. ray peaks found 3''. The
half-life was calculated from the best-fu line, which, together
with the gamma-ray energy, could be used to obtain an unambiguous
identification of the isotope producing that gamma ray. f-rom the
same plot, interferences from isotopes having different half lives
couid be found. The best decay time (before counting) could be
obtained for rjrh, isotope from the minimum shown in a plot of the
error in peak-area calculation versus Prr.... I ypical half-life
plots are shown in Figures 1 to 4.
From this and later work. 61 isotopes produced by 44 elements were
found (Table 2). The gamma-ray peaks used for quantitative analysis
were also determined from these results, together with the
potentially interfering gamma-rav peaks.
2.6. QUANTITATIVE DETERMINATION OV SHORTLIVED ISOTOPES The work
involving the determination of short-lived isotopes was carried out
at the reactor in a
small counting laboratory dedicated to this work. The irradiation
and counting procedure was as follows. After the diamond samples
had been '«radiated for 30 minutes in the pneumatic facility, they
were transferred from their container to a clean, unirradiated vial
and counted. Two count-, were made: one after a decay time of 90
seconds for 20«) seconds, and the other after 420 seconds for 2000
seconds. The purpose of the first count was to measure the isotopes
with half-lives between 60 and 600 seconds with the minimum
interference from the longer-lived isotopes, and the second count
was to measure these longer-lived isotopes, which had half-lives
longer than 600 seconds, after most of the activity from the
short-lived isotopes had decayed. The second count could be made
closer to the detector owing to the fall in sample activity. This
increased the sensitivity of detection for the less active,
longer-lived isotopes
The counting system was standardized by the use of
analytical-rcagcnt-gradc compounds, either as weighed *• 'ounts of
the solid, w 'icrc low specific activities were produced, or as
dilute solutions. The solutions we.' made up with a lower limit of
1 fig/ml to avo'd problems of ion adsorption onto the walls of
containers, and were micro-pipetted into clean, high-puriy
polyethylene vials. The irradiated standards were counted in
duplicate at various positions on the optical bench, and distance
calibrations were made to calibrate the other pre-set counting
positions.
2.1. QUANTITATIVE DETERMINATION OF I.ONGI.IVED ISOTOPES Because
these isotopes had longer half-lives, there was time for these
samples to i.<r transferred
from the reactor to the counting facilities housed away from the
reactor at the N.P.R.U. As previously discussed, the samples were
sealed in quartz tubing. These samples were irradiated in batches
of 24 for approximately 100 hours in a Predominantly thermal flux
of 8 X 10 1 3 n cm" 1 s~' and returned after a 2-day cooling
period. The exteriors of the quartz vials were cleaned with
hydrochloric acid, water, and acetone for the removal of external
contamination. After the tubes had been broken in the Clean Room
and the diamonds removed, the diamonds were repeatedly washed in
hot nitric acid until no gamma-ray activity was detected in the
washings. They were then dried, weighed, and packed into
polyethylene vials before being loaded into the magazine of the
automatic sample changer. The counting schedule ensured that the
maximum amount of data was collected under the best possible
conditions. The optimum decay time before counting for each isotope
was determined from the qualitative work. From this work, decay
timet of 3, 7, 14, 21, 50, and 150 days were selected. The
4
TRACE ELEMENTS IN DIAMONDS
first tount. after ' daw' decav. was for 30 minutes, and the rest
of the counts were tor I hour All the samples were counted in
duplicate at each decay time, with frequent instrumental checks to
avoid unnecessary data loss due to malfunctioning of the
equipment.
Standardization was achieved bv the use of the international rock
standards prepared bv the United States Ceoiogical Survey ll'SGS)
These rock standards were irradiated under the same conditions as
the samples, and. after such a long irradiation, they were
extremely active and had to be counted at long distances from the
detector The accurate dist.-icc calibration previously obtained"*
was applied to the data for the standards so thjt the counting
positions used for the diamonds could be calibrated. Some elements
tor which no data were available from the rock standards, eg.
iridium, were standardized bv pipetting of dilute solutions of
known concentrations onto graphite, drying, and irradiating under
the above conditions. The USdS standards used, the elements
standardized, and the values chosen are given in Tables 3 and
4
2.R. IIMITS O'' DETECTION For the following reasons, the limits of
detection found in this work approach the theoretical
limits calculated for instrumental neutron-activanon analysis (a)
lack of matrix interference from carbon. (b) the high purity of the
bettrr-qualirv diamonds, (c) the long irradiation time used, Id)
the high fluxes aiailablc. <e) thr low matrix interference from
the major elements of the silicate inclusions
All of the above made it possible to determine the trace elements
present in the inclusions, which were themselves present at trace
levels. For the most-sensitive elements, e.g. vanadium scandium,
arsenic, lanthanum, samarium, europium, dysprosium, holmium,
lutctium, indium, gold, and thorium, concentrations of about 1 part
in HJ1 2 were detectable. At the other extreme, the limits of
detection for some of the least sensitive elements determined by
instrumental neutron-activation analysis ranged from the 20 ng
level for nickel and calcium to the 10 /ig level for sulphui. It
should be emphasized that manv of these elements arc not normally
regarded as candidates for activation analysis unless they arc
present at relatively high concentrations.
2.9. DATA REDUCTION The gamma ray spectra produced in this work
were stored on magnetic tape and were processed
on the IBM 360/50 or IBM 370/145 computer at the University of the
Witwatersrand. The main computer programme used was a modified
version" of 'HEVESEY'. written by Yule 2". This calcalated peak
energies and areas, and gave possible isotope identifications.
Corrections were made for variations in neutron flux, and for
isotope decay. As well as being supplied on hard copy, these data
were stored on magnetic tape and were used as the input, together
with concentration factors, to a further programme that calculated
the concentrations of the various elements.
Obviously, this simple scheme of analysis could be used only where
interference-free peaks were found. Initially, interferences were
corrected manually until a computer programme was available to
apply suitable corrections.
The large amount of data produced (some 2000 gamma-ray spectra)
will necessitate sophisticated treatment if maximum information is
to be extracted trom them, and modifications and improvements are
being made to the data-reduction facilities to enable more detailed
results to be obtained.
J. RESULTS The quantitative data obtained in this work are given in
Tables 5 to 8. The wide range of levels
found for different elements results in large variations in
precision and accuracy; errors arise from the counting statistics
for the peak area and from the size of the Complon background
beneath the peaks. In general, errors of 40 per ctnt were the
maximum found, primarily at the lowest concentrations of the
elements. At higher levels of activity, this error decreases
rapidly, and errors of 5 to 15 per cent are typical for most
results. Where necessary, detection limits were calculated from
three standard deviations of the background count in the peak
channels.
The data are given to a maximum of three significant figures, which
reflects the best estimated precision of this work, viz, about 5
per cent.
Comparison of the data in Table 6 with previously published
results1 * shows a generally good agreement except at the lower
concentrations of the element*. This discrepancy may be due to
improvements in the equipment ot the experimental procedure, which
resulted in enhanced sensitive - and precision at lower
concentrations. There is also some evidence for the leaching of
impurities from
5
TRACE ELEMENTS IN DIAMONDS
some of the inclusion-containing and boart diamonds. Kinally. many
of the diamonds clove during the long irradiation, and it is to he
expected that inclusions would he exposed on the fresh surfaces I
hesc inclusions would be removed or leached bv the hot acids used
for cleaning the diamonds, thus resulting in lower concentrations
for the elements on the second analysis
The decay times at which the different isotopes were counted,
together with the detection limits found and the standards used,
arc given in Table 9.
The following elements could be determined from the analysis lines
given in Fable 4 without significant interference sodium,
magnesium, aluminium, sulphur, chlorine, potassium, calcium,
scandium, titanium, vanadium, iron, cobalt, nickel, arsenic,
rubidium, stroi.tium. antimony, caesium. barium, lanthanum,
samarium, europium, dysprosium, holmium. lutetium. tantalum,
indium, and gold. Oxygen was determined by fast neutron-activation
analysis !
The dementi for which a significant interference was found on one
isotope were chromium, manganese, copper, antimony, barium, cerium,
ytterbium, and thorium. The interferences and the precautions taken
in obtaining these concentrations arc given below.
3.1. CHROUIIH The 3I(> keV peak of chromium-51 overlapped the
317 keV peak of iridium-1°2. The combined
peak area was correct d bv determination of the iridium 1°2
contribution from the ratio of the 317 keV peak to the
interference-free 468 keV peak.
3.2. MAXtiASf.St. The interference-free 1811 keV peak of
mangancsc-56 could be used when relatively high levels
of manganese were found. At lower levels, the more sensitive 845
keV peak was used. This interfered with the 844 keV peak of
magnesium-27, which could be corrected by the ratio from the 1014
keV peak of magnesium-27.
3.3. COPPER The 1039 keV peak of copper-66 was interfered with by
the KHO keV peak of gallium-70. No
correction could be applied for this interference since the other
main peak of gallium-70 at 173 keV also had an interference this
time from the 172 keV peak of tantilum-182m. Data for copper were
therefore calculated on the first count when the 1340 keV peak of
coppct-64 was also found, or when the interference from gallium was
assumed to be minor because of the absence of other peak? r.g., :'
2201 keV and 2507 keV.
3.4. ASTIMOSY Although data for antimony were calculated from the
interference-free 1691 keV peak of
antimony-124, the shorter-lived isotope antimony-122 was also used
as a check. However, the 564 keV peak of antimony-122 had an
interference from the 564 keV peak of caesium-1 34, and, in samples
having high levels of caesium, only the antimony-124 isotope was
used.
3.5. BARIl'M The levels for barium were determined from the
banum-131 and barium-139 isotopes. The
166 keV peak of barium-139 had a small interference from the 170keV
peak of magnesium-27. The ratio of the 170keV peak to the 1014 keV
peak of magnesium-27 was used to correct for the contribution to
the barium peak.
3.6. CERIUM Two interferences were found on the 145 keV peak of
ccnum-141 first, a direct interference
from the 143 keV peak of iron-59, which could be corrected for by
subtraction of the iron contribution calculated from the ratio of
the 143 keV peak to the interference-free 1099 keV peak of iron-59;
second, the 145 keV peak fell on the Compton edge of peaks in the
300 to 320 keV region (predominantly chrcmium-51). which had the
effect of broadening the peak boundaries, as determined by the
computer programme, and thus increasing the ccnum-141 peak area by
large and variable amounts. Corrections for this second error were
applied manually to the raw data.
3.1 YTTERBIUM The 198 keV gamma-ray peak of ytterbium-169 had an
interference from the 197 keV peak of
terbium-160. A correction was applied based on the ratio of the 197
keV peak to the 887 keV peak of terbium-160. Alternatively, the
area of the 197 keV peak was determined after the ytterbium-169
isotope had completely decayed, and was corrected for decay and
subtracted from the data obtained after a shore decay. The 396 keV
peak of ytterbium-175 had an interference from the 398 keV peak of
protactinium-233. A correction was applied bated on the ratio of
the 198 keV peak to the 312 keV peak of protactinium-233; or the
area of the 398 keV peak of protactinium-233 was determined after a
long decay, aid was then corrected and subtracted from the
short-decay data.
6
!
i.H IHOKIl 11 Ific 312 keV peak ot protactimum-2 33 'used tor the
thorium dctcrn mationi h.i.! an interference
from the 3<»8kcV peak of ir.di'im 1 0 2 \ currco. >n was
determined from the ratio of the- 308 keV peak to the interference
tree *68 keV peak of indium-192
4 DISCUSSION AND CONCLUSION ihr data presented here have been
statistically and gcochcmically "* ' * interpreted I he high
impurm !evcls found ir. the green and brown samples were found to
be significantly correlated with thr colours It is therefore
possible that the presence of suhmicroscopu mineral inclusions ma\
!>c resr onsible for the colours Alternative or additional
reasons for the correlations ma- be that the coloured stones grew
under conditions favouring the incorporation of minute inclusions,
or that the darker colours prevented some small inclusions from
being observed when the stones were categorized.
A significant difference was found in the trace-clement levels of
the purer diamonds from Premier, compared with those from l-insch
and Jagcrsfontcin I his mas indicate a difference in the growth
environment ot diamonds from different sources'*'"
When results of this woi1* arc compared with previous results i
Appendix I. there is general agreement tor the higher levels of the
elements determined Differences occur ar the lower ievcls,
some
' these values being 10 or 1(H» times lower than previous reported
values The present report and a paper' * on the same work represent
the first published quantitative
determinations, bv ncutron-activatin analysis^ of oxygen, sulphur,
chlorine, vanadium, arsenic, rubidium, strontium, terbium, hoimium
and tantalum, and the first published qualitative determinations bv
the same technique, of germanium, bromine, ncodymium, eadolinium,
erbium, and platinum, in diamond.
I he results show that some of these samples are the purest
diamonds analysed to date, which reflects favourably on the careful
selection procedure used The discovery and determination of many-
new elements show the extreme sensitivity of the instrumental
neutron-activation technique used here in conjunction with the
ideal matrix of carbon
5. ACKNOWLEDGEMENT; fins study was matte (ussiblc through the
financial support and co-operation of a number of
organizations and individuals. Thanks arc due to the Anglo American
Corporation of South Africa and l>c Beers Industrial Diamonds of
South Africa Limited for sponsorship and for the supply of the
diamonds used in this study, the University of the Witwatersrand
and the South African. Atomic Energy Board for their assistance; Mr
J.B. Hawthorne ot the Anglo American Corporation and Drs K.A. Kaal
and R.J. Cavcnev of the Diamond Research Laboratory for their
encouragement and interest, and Professor DM. Hawkins for his
advice and assistance in the statistical treatment of the
data.
6. REFERENCES 1. MARX, PC. Hi», sLig . I.onj.. vol 38. 1972. p.
636. 2. KENNEDY, C-.C, and NOROI.IE. BE. I ,,m firnl. vol. 63.
1968, p. 495- 3. '"MGNER, P.A. The diamond fields of Southern
Africa. Cape Town, C. Struik Ltd. 1971. 4. WILLIAMS, A.F. The
genesis of the diamond. London. E. Benn Ltd, 1932. 5. KOCCO.
(i.C... CARSON, O.L., and CALL J P hit J. Jppl, HiUÍiat Isotope,
vol. 17. 1966.
p. 433. 6. COLLINS, A.T., and WILLIAMS, A.W.S. / Phyy < . vol.
4. 1971. p. 1789. 7. CHRENKO, R.M. Phyy H,v li, vol. 7. 1973. p. 4
,60 8. CHESLF.Y, E.G. Am. .awtrjlogist, vol. 27. 1942. p. 20. 9.
RAAL, E.A. Am. Mwrralogist. vol. 42. 1957. p. 354.
10. EVANS, T. Diamond research 1973. London, Industrial Diamond
Distributors, 1973. p. 2. 11. MELTON, C.E., SALOTTI, C.A., and
GIARDINI. A.A. Am. MinmhfiM, vol. 57. 1972. p. 1518. 12. CHRENKO,
R.M., McDONALD, R.S., and DARROW. K.A. Saturr. l.onJ., vol.213.
1967.
p. 474. 13. SEAL, M.Nature, l.ond., vol. 212. 1966. p. 1528. 14.
MEYER, H.O.A., and BOYD, E.R. Ceochm. Cosmochim. Acta, vol. 36.
1972. p. 1255. 15. MEYER, H.O.A., and SVISER0, D.P. International
Conference on Kimberlites, Cape Town,
1973. 16. MOORE, M„ and LANG, A.R. Phil. Mac . vol. 25. 1973. p.
219.
7
FKAt.F ELEMENTS IN DIAMONDS
17. TAKAÍ.I. M . and l.ANO. A R r*-., K"> .V«> \ voi 281.
1964. p HO 18. FFSO_ H.W.. BIBBY. D M . SH ISO HOP. J.P.F., and
WAITF.RSON. j IW. ( rjjwanaht i h,m
vol. 17. l»>74 p 1«S 19. I.K.HTOWI.FRS, F.C.. l«.i,yr I M I I I
, vol. 3«. 1962 p 1398 20. LKiHTOWl.FKS r ( l « i w < hem. vol.
15. 1963. p. 1283. 21. l.KiHTOWLF.RS. K : M l l V i l \\l) IHHSOl
t>l,Y Of l\lnsiKIM IV\\IO\[)S Hwh J
U',1 London. Industrial Diamond information Bure.u, 1967. p. 27 22.
RANDA. / . . BFNADA. 1 . KVNUR. I . and KOl'VIMSKY, J J.
raJ,ojnjiyt I hrni.. vol 14
1973 p 437 23. VANCE. E.R., HARRIS. J.W., and MILLEDO-E. H.J. Mm
\Ug.. I on J vol 39 19:3 p 349 24. LANG. A.R \jrurr l.on.t . voi.
213. 1974. p. 195 25. BIBBY. D M . and RASMLSSEN. S.H. RAÍvnhem.
rjJiojnjtyt iff... vol 9 1972. p 1. 26. RASMUSSEN, S.F.. FESQ,
11.W., SELLSOHOP, J.P.F.. and STFFLF. r.W. Johannesburg.
National Institute for Metallurgy. Report ni> If 6.1. 1973 27.
YULE. HP. Washington, National Bureau of Standards, Sp,\ l'ub. M2
1969 p. 1108 28. HARMS. J VttW lustrum. Meth., vol 53 1967. p 192
29. BIBBY. DM., and RASMUSSEN. S.E. RjJunbem rj.i„>jnjlyi Lett.,
vol. 14. 1973 p. 9. 30. ZANDERS. J.A.J., BIBBY. D.M . and
RASMUSSEN. S.E J I'hys t., vol. 6. 1973. p. 973 31. WATTF.RSON.
1... WATTERSON. J.I.W., RASMUSSEN. S.F... SELLSOHOP. J P F . . and
STEELE.
T.W. Johannesburg. National Institute for Metallurgy, Report no
1476. 1972. 32. BiBBY, DM., SELLSOHOP. J.P.F.. and STEELE. T.W.
Johannesburg. National Institute for
Metallurgy. Report no. 16.19. 1974. 33. ERASMUS. OS.. HAWKINS, DM..
KABLE, F J D. FESQ. H.W, BIBBY. DM., SF.LLSOHOP.
J.P.K., and STEELE, T.W. Johannesburg, National Institute for
Metallurgy, Report no /652. (To be published).
34. FF.SQ, H.W.. BIBBY, DM., ERASMUS. O S . KABLF., F.J D.. and
SEl.LSCHOP, J P F International O-nferencc on Kimberlites, Cape
Town. 1973.
35. FESQ, HW., BIBBY, D M , FRASMUS. OS.. KABLF.. F..J.D..
SEL1-S0HOP. J P F . and STEELE, T.W. Johannesburg, National
Institute for Metallurgy, Reynrt no 16.16. (To be published).
36. DYER, H.B., RAAL, FA., DU PREEZ, I... and LOUBSER, J.H.N. I'hil
VIJ* , vol II. 1965. p. 763.
8
/4J»/.f. /
\eutrnm flmxet and cadmium ratios
Position Neutron flux Od ratio in cm " s i (for cobalt I
Pneumatic facility 2 -•" I 0 1 32 PooKulc facility 8 X U)' ' ' i
i
1.4.81/ 2
1 lemenf K, . | :„
niKlkir
Half -hlr i j m m i - r i ; ^ealo-* dr t r t t r t. kcV
AnalvM-.
peak. kcV
Sa Ni-24 15 «I h 1 «f.H I 7 3 2 U H i 1368
M» M r 2 7 9.45 mm 11)14 844 1014
Al. Si AI-28 2,31 min 1779 12681 S I ) 757(1)1 > 1770
S S-37 5.05 mm 20H«K|)I ) 208OIDI1
(1 «.I-3R 37,3 mm 2167 1642 2167
1642
K K 4 2 12.5 h 1525 1525
<a « j -49 8.8 mm 20o2( l ) l 1 2062(l )F)
V Sc-46 83.9 «1 112(1 889 889
t a . Ti S*-47 3.43 .1 160 161)
l> Or 51 27.8 d 320 320
I I T i SI 5.8 mm 321» 929 61)8 320
V V 5 2 3.76 mm 1434 1434
Mn Mn-56 2.56 h 2113 7891 D M
1811 16021SK
I T Mn-54 303 d 835 835
I T I T - 3 9 45.7 d 1292 1099 193 141 1099
1292
(A; C.W.O 5.27» 1332 1173 1332
1173
<u Cu-64 12.8 h 1346 a- 1346
( u C u d * 5.1 mm 103« 1039
C.a { . » 7 0 21,1 mm 104H 1048
G» C,a72 14.1 h 2202 2 Í 0 8 2202
( k Cc-75 79 mm 26S 199 26$
As Av76 26,3 h $59 657 1216 6$7
Hr Br-80 17.6 min 617 0* 617
Br Br-82 35.9 b 777 J 34 619 6 9 8 777
828 1044 1317 147$ 1044
Kb Kb-86 18,7 d 1077 1077
Sr S f -87m 2,84 h 389 389
St> Sb 122 2.75 d 564 693 $64
Sb Sb-124 «0,9.1 603
TABLt. 2 ItomtJ)
Element Kadio- Hall lite l iunnu- r iy peak» * detected. keV
Anatywa
nuvlide
peak. krV
a 1>134 2.07 v 605 7«6 7«6
Ba B i l M 11.3 J 496
124
Ba Ba 1)9 S3 mm !o6 l * >
La l.a-140 40.3 J 1595 816 487 329 15*5
172 242 267 432 876
751 950
Nd NJ-147 11.1 d 91 31V 531 91
531
Sm Sm-153 47,1 h 70 103 103
Sm Sm-155 21.9 mm 104 104
Ey Eu-152 m 9.35 h 122
1315
Eu F.u-152 12.2 y 122 245 344 411 I 408
444 779 964 1086 1086
1408 367 1112 1299 779
344
122
1595
103
Tb Tb-160 73 d 87 197 216 299 879
879 966 1178 1200 299
1272 1312 309 393 1272
765 362 1003 111 ) 87
Of Dy-165 2,36 h 95
715
296
Yb Yb-169 30.6 d 64 9 4 110 1 ) 1 198
177 198 308 177
Lu Lu-177 6,75 d 208 113 208
T« Ti -182 115,1 d 68 100 152 222 1222
229
1189
W W-187 24,0 h 686 479 134 7 Í 6 8 *
k lr-192 74,4 d 296 308 J17 46« 4o0
S M 604 612 206 296
374 416 484 7 8 Í
U lr-194 19,7 h 328 » 4 645 32«
6 4 }
peak. kcV
ft Au-198
i ! 2
312
228
KM
278
106
TABU. 3
Value
Na
Standard
USGS GSP i 2,08 "., K USGS GSP-1 4,59 % Sc USGS BCR 1 32,0 p.p.m.
Ti USGS BCR 1 12750.0 p.p.m. O USCS DTS 1 4160,0 p.p.m. Ee USC.S
BCR 1 9,36 p.p.m. Co USGS BCR 1 38.0 p.p.m. Ni USC.S DTS 1 2440.0
p.p.m. Rb uses C;SP i 261,0 p.p.m. Sb USGS GSP 1 3,1 p.p.m. Cs
Internal std OK227 2,05 p.p.m. Ba USGS GSP 1 1335,0 p.p.m. La USG5
GSP 1 175,0 p.p.m. Cc USGS GSP 1 320,0 p.p.m. Eu USGS GSP 1 2,24
p.p.m. T * USGS GSP 1 1,06 p.p.m. 1 m USGS GSP 1
.. ., 106,0 p.p.m. 1
TABIt 4
KJJH aurttJri of jijfiw/it•»»•<- fur tfiunuutwe atudysa
!
\ . i Vi 2-i 15 h 1 .(.8 5 Al A; :s 2..M min ; 1779
S Mc 2 7 S-57
9.5 mm \ 844.U 1UU.1 5.(»5 min ! 5 h»2.4. 208O <DF >
CI n 58 37,5 mm ] 1642.7 K K 42 12.4 h 129J .6 Cj ( .1-49 8.8 mm 3
0 8 5 . 2572 'M- i. 2062t » 1 )
Sk 4 o 85 .9 J 8 8 9 . 2 , 1120.4 Ti
V is
5.8 mm 520 3.7o min 1454 27.8 a 520,1
Mn Mn 56 2.6 h 8 4 6 . 9 . 1810,8 l e Ft 59 45,2 d 1099,2 . 1291,5
Co Co-60 m 10.5 :mn 58.5
G>-60 5.27 v 1175 ,2 . 1552,5 N'l Ni-<S5 2,6 h 1115 .4 .
1401,7
C J
Co-58 Cu-66
71.5 d J l l . O , 810 .5 5,1 mm 1059
As As-7 6 26.5 h 559.2 , 657 ,4 Rb Kb-86 18.7 d 1076,8 Sr Sb
Sr-87 m Sb-122
2,8 h 388,2 2,7 d 564,1
St.-] 24 60 ,0 d 6 0 2 . 8 . 1690,8 Cs O i l 34 2,0 y ! 6 0 4 , 6 .
795 ,7 Ba Ba-1 31 11,5 d ! 4 9 6 , 5 , 123,8. 215,•>
Ba-139 82,8 min j 165,6 U La-140 40.2 h i 1595.4 , 4 8 7 , 0 Ce
Ce-141 32.5 d j 145,4 Sm Sm-153 4,7 h , 103
Sm-155 21,9 min 104 F.u Eu-152 12,0 y 344 , 779 , 964 ,2
Dy Dy-165 2,36 h 1112 . 1 4 0 8
9 5 , 280, 362. 6 3 3 . 7 1 5
Ho Yb
Ho-166 Yb-169
Yb-175 4,2 d 198, 3 0 7
114, 282 , 396 Lu l .u-177 6,7 d 113 , 2 0 8 T J Ta-182 115,0 d
1121 ,4 , 1221,4 Ir Ir-192 74,2 d 316 .5 , 4 „ 7 , ? f
Au Th
Au-198 Pa-233
4 1 1 , 8 311 ,9
The gamma-ray energies used for quantitative determinations are
underlined.
12
tract tirmrnn m fttmm fcwuA
w ^ f l f '%! J « o n 1 AJ i«Ji
í 1 P m
P:A .' : J I
P2B ,1 : 15
P5B ,) > 39
J 1 5 2
ppm p p b. p p m : p p m
Í:
p p m P P f c
. t o ; * 1 I.M 0 . 2 4 17 0 O i l O.OM : o « »
0 . 2 4 1.4 0.5«) 3 2 . 0 1 « 0 2 1 i 0 . 0 4 i - 5
0 . 1 5 5 4 4 7 2 5 . o 1 2 1 9 0 . 0 9 ; 6 . o
I I I » * 0.2V 0 . 2 3 2 6 . 0 0 4 7 »> IÍB ! o . o j •' 2
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o n 0 4 1 0 37 2 4 . 0 0 . 4 O O.09 , 0 .O4 l . o
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0 . 7 » I I . ' i 11 • 4 7 3.» • o .25 \ 9 0
l « l 8 " 5 4 I S O 0 12 4 5 i n 0 .1 7 1 5 . 1
0 34 9 i lo.o t » . r . 3 9 6 . 4 O l ? • B O
0 . 6 4 1 . " 2.7 4 0 0 2 3 0 . 6 4 0 , 0 6 j 5 .0
( i i : 5 4 4 .5 2 0 . 0 I ' M 5 1 1.4 0 0 7 < 5 . 0
0 . 1 4 2 4 2 7 6 6 0 0 . 0 5 1.» 1 2 0 . 0 « i ''' 4 4 47 0 14 7 9
3 0 . 0 1 1 7 2 5 o '.» • 2 .0 ' 45 0
2 0 14 O 7 o 6 4 . 0 0 3 4 12 o 2.7 0 1« ' 46.11
J I 0
2 3 O 0
450 .0
0 , 9 7
0 , 4 2
0 , 5 0
2 6 9
0 4 4
0 . 4 1
N i l
21 o
290 0
« I I
117 O
i 2 0 « o
2 l o . o
» 2 < M >
12 o
2 5
7 30 0
2 B O O
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t*J> o , 4 )
2 2 0 0 O . I O t
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2200.0
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0 , 0 2
I 2.1 I 0.4) I | 1 . 2 7
I ) . 5
0 > Nn mrMr inclutiom
1 • V w l W f i rH' l i r l ton*
p .p .b . • p a r t * per b i l l i o n 110 1
1 ' C l r »
3 » i f o w n
4 •• f f f c t n
13
I K \ l I I l > M I N I S IN DIAMONDS
1
1
1
14
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; .s ? •: : ï •: : Í 2 5 S 2 •: -s s ; | % s •: •: s § | s 1111 ï
'
I 1111111i1111 I f ï i f ï s « m « i g g í s s s : »
= ïzsmH-ïlzííítïi «SSSËSif§ 1 I ï ' 1.0
0.04
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0.J9
0.40
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|
! I» S S i a i l I S? z l !Ê 1!
I s 5 s § = 2 2 s 5 ! s s g = : =: = g = s s Í = -| e § s | £ |
f
4.0
450.0
174.0
61,0
210O .0
ï* 1 11111 -S -I -= 11 -5 s 11 = 115 | i i ? « = ? s 2 | e s 2 s i
i
! ! Ï i •: •= i I«12 2 s 5 -! : 5 s s 5 5 5 S * " S 5 5 •= IS11 p 1
|§.= 5 ! 11 ï | i s c ï § s 511 ! •- •: 5 •=: § Í •- = Ï : ? ï l' -
- - - * . - 4 S » - Ï * ^ . - - I I Ï : - « - c e e i s - s s s o e
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( — s = c s = = = = s ï c s - - - r. ,-: c £ c c o e c o © .
•*
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= = 8 = = » = Sf 1 = * 1 £ | | - ! | J ï *
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:»
S •= = £ IS S •= S ÊÊ § 1 Ê - s g | i' 1 I I ! ! I | ï i | I I I I
^ i ! ! | U Í U 2s - r
S g S 2 5 > r : s 5 C 2 i S e § ; S S 5=585*55 H 1 1 2 i* f M -
! S l 2 5 g ï - = S 5 2 | - = 2 i ? §•= 2 S ^ c
Í 5 C 5 2 S | 2 2 | 2 2 =2-- gg | £ | g | 5 ,
0,002
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7
c c - c r = = c - " = - <z z z z z „ - :: - - - z - ~ z z - z
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.! I '- f
t S
r.4«l> 7
T T
1 ! " 'T —-' "' ., 1 K ! <- V „ r——
V .. * • • ,., s. ( I I A> Mb V •*> ( j •a U < r %m ,.
t>> II» \:, 1 u ! .. Ir A n rh
; r p.-n r p in p p -11 P ? m r ? m p.p *• p p .m ; p p m p p i '
... -.. p p m p p i , p p h
I I 14
p p l . ' p p m j P P h
1 1
P f » p p b p p b p p b p p m p p h p # l . p p j . p p i p p b P P
b p p i , p p l , p p t , p p i , p p i : P P b p p b P p b ,
pp.b
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T
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().«)» ( . H O I
1 ) 0 2 »
:;« : H Í I 1 4 H f. 4? 11 0 51 - .. 1 ft i l . ' l 1 6 1 . 4 4 11
I 0 7 K 7 •. ..... ... " 6 l lMl.O 0 0 4 ! 10.9 0 . 1 0 0 , 6 « 4 I
O 11.5» 1 2 0 . 1 1 7 0 O 5 6 o I il 14 0 12J 1 ) 1 1 1 ) 1
; i : • ; «vs < \)<*2* ' i ! •* . , , ,« * 25 1) uov I M U M
( M i l I . . 4 1 4 1 O 0 14 1 I I m m 0 0 0 5 O i l 0 0 5 O I I O
i W I i i ( * } ! i ) (»,2 O d l 7
í 4 1 i n . i i W 1 « '"' 2 f i » 4 0 . 1 ( 11 1 1 l . • 0,111 m i
: 4 1 . 2 t 1 5 . 1 i) ^ 4 11 ' i . 1 9 4 0 . 0 O 0 U 5 124 0 51 I-
17 2 1 H l l l O 1 4 5 2 7 i i 1 4 0.O49 11(16 , . 1ft i i 1 3
u,oo» 0 135
u i H : l ' . M i 7 i 2 * i f I * 11(1.') ( l 12 . . . If . O 15
O.l. l 1 11 2 4 4 H , 1 4 . 1 1 i ' 4 * : 5 .. ;t 0 . W 1 I 9 . 1 1
0 21 0.2O 21,11 1 1 . 4 1 ( 1 1 7 n i l » - , i t 1.11)4
!- i U ' i t O t t ir • * « i ) - • ! 51 >l I I 15 „ ,0 l ) t
> 4 » urn ( 1 5 I I I 5 " t r> » 4 • i ' S M O 11 O.IMMV
11.16 29 0 i * 2 ~ U 6 4 O K I ! H 11) , , , 1 4 4 ' , , m i l
l
1 S 1 , 0,1 It (ft ' M •*-»<*> >5.) . ' l '1.41 !> 1 I
„„-.• 0 111 O 4 I . . O 7 . . •1 > 4 ., Ï " ; : , . . , . 2 • J
O . I V o,2^ ; » i > i . i n (1.H15 ...»- ,1 W * , ' '(114
,' * \ í - < - < • / « » " ! ' í H .'! " * * 14D.H :« ]JU>
i * 1 '1 2 I . O » l . o 4 9 0 ( 1 I 4 « t t l 1 0 9 0 , 1 i n . K
4 0 4 . . 0 1 9 59,(1 I I . 4 0 ( l . » 9 2 2 2 0 4 M | 4 ) 0 » 5 n
9 | i i • 7 1 » 4 1 1 I , i ] i 1 1 1 4 1 •1 1 4 O.l 4 2 3 .
0
. ' H ; i n t . ' » . < H :*» l ' í l l I 7 i ) ( ( 2 M • M l i
" •! 1 6 1 441.11 »111 .11 7 9 0 0 4 4 » » • , 1 t ., 9 0 . . I . 2
» 16.11 4 1 29011 1 2 . » 22 11 2 2 o 15 t i " i i» 0 . 7 2 : r * ,
1 l t . 0 1 9 1 7
'*< ! 1?« t >.<» ; * I * ) ) ) 1 5 H I 1 f: 1 21 21 (1 1 1
0 I I 291 IO 05 " 4 6 4 1 ( 1 2 > , l 5 2 0 O . 0 4 2 16.11 1.2
2 » o j l 5 1 12 ft O 4 (1 1 * , 1 1 1 ( i 1 2 i, .1 ft D 0 »
7
i ) * \ ' 1 2 « ' • i is», ! 1 * : 4 I 2 i m . i l 1 4 14 ; I 2» 1
1 . 6 1 2 4 . 1 2 4 0 . ( 1 1 1 9 ( 1 2 9 11 , ' ' 9 1 5O.0 o IS 5
1 . 0 0 . O 7 9 i a 4 » 2 7 0 0 , 0 14 » 26,(1 2.2 0 . 4 9 « f t i
. 2 . 1 2 7 s : 1 e l D. I I39 1 II
> f t Í ? * H < 2 " H * I I i : ' 14 V I i l 4 i l 241) il ft
O 4 1 VH O ,7,„. I0441.0 2 Ï , » 4 6 (* i : 6 1 14 » 6 . 0 2 1 . l
l 5.1 1 2 0 0 . 1 . 9 » . ( l 1 7(1,(1 12,5 2 2 2 9 1 i i ,.- 1 , 4
9 H I 1 ' ft' I . . 007 2O.0
" i«< I H < r i ; 1 ft,+ U K I lonon : » 11 2 I I 5 V IIWH
7.5 14,1. 1 6 0 . 0 * y 2 9 11 1 o l 1 4 4 1 1 1 0.611 6 5 1 1 0 1»
0 . 1 » 4 .4 21O0.O I O 6 21,11 1 5 0 . I l l 0 ~ ' i . i h i O I 4
i , i , M 2 * O.0O9 2.f
; I ' M i • K K í . i 0 * 1 1 < l.í* 6 7 . 1 1 0 . 6 3 2 2 I I 9
4 I I 12 11 I I 1 1 2 . » 62.(1 1 » » 4 6 11 I I ' 4 loo.o 0 . 9 I
0 . 0 6 7 1 1 4 0 . 1 4 15 W o 1 » 1 9 0 . 1 0 .O66 0 , 0 2 0 .2 1
( 1 9 . . , 17 <M()ft O. I -06 0 . 2 3
1 "'H ! .1 P W I t l . W I I 7 . f i 2 Ift » 1 1 1 1 1 4 ) A l l 1
. 5 11.50 i n n 0 4 »1 2 1 0 . l l 2 0 » 1 4 1 I I '« »5(111 1 . 4
9 I I M 7 14 .6 (1.5ft 0 . 4 11.124 0 1 o I r . (1.64 ( t . 7 b
O.I-63
| ( ! " -> 1 * M'-'.i 5 : 7 S O I ' 7 7 9 1 ) . 1 » i i i m o
11.4 12 6 2 2 0 . l i I7IH).(> 1 7 0 0 ( 1 M i i 4 4 4 1 . 1 f '
» l loo.o '•' 45.11 0 . J 5 5 » 0 9 4 1 1 1 0 . 0 1 2 . . I 7 7 . ,
. » 4 1.7 2 5 1.5 1.5 1 5 l f t .2 * . f t 11,1(17 4 , 2
1 J,»H 1 H H . M l l t l l < > , M 1 6 » f ï f t l 1 4 5 0 "
4 * : '•'•" 0 .65 11.21 12 5 7 4 . » 2 2 0 o i n » 6 6 0 " I 0 0 O
. O O I 5 1 4 . 0 o.lo 0 . 4 7 4 4 O 0 1 7 1 • 0 . 1 7 0 . 0 » 0 (
1 1 ( I . I I 9 I I . .17 " . 5 4 O.OI 2
| J11 X 1 ! IV- .1 n I I 1 J .« «>.M 6 0 0 ( 1 1 4 ; 1 22 I l l
l R 0.(15 1 o y . i 24 11 Í . Ï 2».o 1 6 4 l o o 1 . 0 1 5 1 0 »
0.1(22 0 . 1 4 0 .17 » 5 . 0 2 . 0 1,9 0 .1 0 O 4 4 O.OI •1.9» ,1
37 (1.015
J i l » I » ' NJ i 0 ï » "-* 1 1 , 9 4 1 0 7 . 0 0 . 4 7 i n . "
11.12 0.11 2 5 1641.11 » 9 11 '" 2111 1 I k I W . O 1.1.54 0 . 0 »
1 0 . 2 0 0 . 7 2 72 .0 1 1 » 1 6 0 0 7 H .50 () M9 0 . 0 1 1
J I M 1 ' • * : " . ( i * ' ' 1 5 ' * I H O O I I ft 1 I )6,0 7."
5.6 9 4 0 2 * 0 . 0 I I » 0 . 1 . 2 R » 54 11 0 9 1 441.11 I . . 26
70.11 0 . 4 » 0 . 6 7 1.4 2 1 0 0 . 0 H O 6 3 . 0 5.7 1.42 2.0 0 .
4 0 . 7 ft.l 11,22 0.1X1» 4 . »
J12H I ) ; i 9 ) . i I , f t : 4ft,«J H I 144MÏ.O 7 2 j 4*1.(1 )»
1.6 11,11 »00.11 4 7 I I O 7 5 » I 4 » . l 5 ' 2T»»1,0 17 9 » » 2 .
0 1 » 3.1 7.7 J 4 0 0 . O inn 7 1 . 0 S.i' 0 » ! 3.1 o,7 0 , 7 6 ,6
3.7 o.o; 3 6 . 0
j i :< i I ! 4Sft,i 1
1 | 2 ' i 77.1» ft.» » 0 0 . 0 4 . 7 47.11 1.5 5.4 441.0 »9110 »711
( l 2ft.» • O i l 5 1 2 I N . O 5 . 9 ft* o 0 5 O »2.0 ).» 450O.O 1
6 . 0 7 1 0 ».7 1 6 1 2 5 o,4 11,7 « . I ! 4 .6 11,7» 0 . 0 3 » 5
9
I I I A 1 < ! » 4 . 1 1 1
; | » .15 ' 9 . » O.ft ï 4 1 0 . 0 1 1 1 ' 1 « 0.16 0 . 4 0 ft o
»611 M . O I f t . » 124 II 2 1 WWIO.O 0 . 5 0 1 5 . 0 0,0445 16
().»! 2 4 0 4 . i i ».! 1.1 0,115 0 . 0 4 o.l 0 . 6 4 11.29
O.I112
JI .B ; 1 1 1711...
-L I ; j», j 1711.0
I ft 5.n 3 A O 0 . 0 1 9 . 0 | 195.0 12,1 » 0 2641,11 1 H O . O 5 4
O 0 . 0 111.11 4WI . I I
• 1 1 2 » 154WO.I1 » 7 . 0 2.4 15O0 2.6 M 0 D . 0 1 2 4 . 0 230.0
25.0 1.6 3.4 2.1 1.3 33.11 2 5 0 . 1 2 2 29.(1
ImluMon O • No v inbk (ixluMon*
1 - VMihk i n d u H o m
ip.p b * part» per b iH»n < 10 >
< ftloUT 1 * ( I n .
16
I RAO ELEMENTS IN DIAMONDS
TABIt V
Drtjy time after uhich the isotopes were .left tr.l M,intUrJ\. .mJ
Jetrct urn hwiti
I >.-.. . '• t l l ' K - , .._ |
l ->"T« '«)- *>u « I | 7.1 u : :; ! 5 » ! l > . ' , . - .
, . - S i i m l i r l
' ' < ' <2(>0«l i ?t M H 1 . 1 »11 r., (60m> I C J l M-
• . f,* i - . i f t O r n i
- j
\ , . ' l • • .
- j
1 Í .M ' 1
> * • ;,, , s
- • ; . * . • »
• • I ) I H H M N i ; H( K 1
1 . 5 i • ...,': 1 I K ;
\ - 5 2 • ' o • M m : V - ( ) • M \ ( > , « . . i n
i « 1 ' • • . . , » > , , ; H h !
M i l * ' • • • I l l M i ' l Mn U N O . « . ' ' I I
1 . V < * • • H | l « HI K I
( . , o l l m U . I K I 5 ( n l M P i i « « . . i n
1 t> f * l • • ' I M N M 5 BCK ; ' . 6 « • ( > . 7 N i l N O
, i ; « J l i l i
( ,.-5Hl V I • • . I I U\ [> IS 1
( i i 6 6 ! • • I I . I K I * C u ( V I , i : «..In
\ « - - < . • n (MKMI02 \ < . : 0 , / H \ 0 | V i l n
Ml. HA • • * I t . l K l l f.M» 1
M 87m • 11.(11 S n N O , i .
M . 1 2 2 : • • 11 1H H I 1 (,SP 1
V ^ I 2 t • • O.O0O0I ( .SI ' 1
<« I .M • * • (I.IKHlI »<K 1
H i l W • (V(H B J O > I «iiln
K.i 1 < 1 • • * «.(KM ( , S V I
I i ! Hi ' • • ( ,000005 <.SP 1
<.<-Ml t f • • • t',(MMK)5 GSP 1
Nni-15 < ' • ( 000005 S m j i w i i h
Sm-I 55 ' I U H K X I 5 S m . i N O i ) ,
Hi-152 • • • 0.000002 (iSP I
Mo 166 ' 0.000005 H o , ( N O , ) ,
M i 169 • * 0.0001 V h j I N O j ) . ,
VI. 175 • <(.0OI)l V l i 2 ! N O . | ) ,
I n 177 • • 0.00000$ I . i i . l N O i l )
I i 1X2 • * • 0,0000$ GSP 1
Ir 102 • • • 0.0000005 <Nll4>jlrC:l A <oln
An 108 * 0.0000005 NH4A11CI4
• 0.0000005 GSP 1
Jf, - Counting lime.
'H , B*P*ï8fFW£PP* t"^íWa*iP" i&
Oamma-ray paah M9 k«V Actual harf-lifa «3,90011 Mcourad hatfltfa
86.000d
0,00 40,00 »0,00 110,00
OAVS
•JN l«,M 14,00 32,00 40,00 40,00 U.00 (4,00 72,00 DECAY T I M E ,
d
00,00 M,00 M,00 104,00
F I G U R E 1 Decay curves for scandium 46
7/,00 «0,00 (1,00 9*,00 104,00
F IGURE 2 Decay curve (or lanthanum 140 and iridium 192
to* Gamma-ray peak 406 k*V Actual hwMifa 11.300 d Maaturwl h.ilf
lif» 11.500 d
S
I
> W
Z
0,00 I I I I
1,00 «,00 ït,oo »,00 40,00 (»,00 s«,oo OCCAY TIME, d
«.,00 71,00 »0,00 • »,00 »(,00 104.,00
FIGURE 3 Decay curve for barium 131
•s
1000
TRACK ELEMENTS IN DIAMONDS
A SUMMARY OF THE PREVIOUS WORK ON NATURAL DIAMONDS
The literature survey carried out for this project collected much
of the previous analytical data obtained for diamonds, and Table II
gives a summary i.f this, together with the results obtained in
this work. It thus provides a useful comparison with the results of
the present work The rarlv work of Wagner1 and Williams* has teen
omitted because thev could anaksc only t ie ash obtained from the
combustion of Uurr stones containing extremely high concentrations
of impurities Mn» approach is understandable when the sensitivity
of the analytical methods avat. :t>le to them is realized It is
of interest to note the emphasis on neutron-activation analysis
both for qualitative measurements (approximately 60 per cent of ail
elements detected) and for quantitative determinations
(approximately 80 per cent of all the results). If only the data
obtained since 19o3 arc considered, these figures are both greater
than s»0 per cent This shows, probably more clearly than in any
other way, the acceptance of neutron-activation analysis as the
preferred technique for the analysis of diamonds Although the
values given for the various elements cover wide ranges, occasional
results are extremely high compared with the other values reported
These may be due to contamination, or to the use of unsophisticated
cqu.oment One example of this is the gold value of 20 p.p.m.
reported by Krccdman' This was the first /".ample of
neutron-ac'ivation analysis applied to diamonds, and the very high
result may have been due either :o the crude equipment available to
him, or to contamination (e.g.. as a result of cleaning in platinum
gold laboratory ware) In addition, the results given by only one
laboratory must he considered suspect until confirmed te.g . for
hafnium and mercury4), and the presence of relarivrly complex
organic compounds is surprising in view of the extreme conditions
in which diamonds form . However, it must be appreciated that in
the extreme all elements can be potentially found in diamond, that
all diamonds arc different, and that widely differing
concentrations of elements can be expected.
In the future it is certain that more elements will be found in
diamonds by the application of existing and new methods of
analysis. It can be expected that more effort will be applied to
the determination of the position and variation of impurities
within single diamor Is, and in the use of the results to gain an
understanding of diamond growth and the conditions existing in the
Earth's upper mantle.
22
ÊAHIt I •
1 Mimm.try nl \<nnr •liment\ JO./ ïiimpnuiith ,/fttv'i -.' .in.I
mr.nuir.i in .tijinnn.h
—"^—————— 1 íe*m*nr
Kef r r r m r M r i M - r r : •. j i n i " . I t - . - • • - ' i :
- ' - -
• " • • • p o u n d i 1 Vs t , , , « i . r k i •i'»-'.
range1»
- -.. <pp HI un;r-\c of ..TUiNC \ h o w n >
I I - f. Ms
H H •! OS
( l l , l I f . O i l s Ms
\ 5 MS
I D ! 5 < H I Jo 2Not) I'A
1 ! i M i n i l » ( I ' \
1) 12 1 V V \
1 .V 1 W 11 in iron 1 N \ A
\ . i 8. 14 OS
15. 1«. N A
4 0.73 t<. : o . o \\\ i 7 NT) to 34 N A
If» 0.0O4 t o 4.2 N A
1« 11.05 to (1,4 N A
l \ \ 0.OOÍ t o K.I N A
MU H. >>. 14 os 7 4 i »
i n 7 ro iV> N A
I H 30 N A
2 0 N'l) t o 1 5 OS
21 0.1 t o 3 o (" rw 0 , 0 4 to 37(1 N A
A l H. « . 14 OS
15 , U N A
I f . O.Oo to 9,1 N A
18 0 ,4 t o 1 0 0 N A
?() N O t o 8 0 OS
21 21 0 ,04 to 3 OS
2 3 23 0,1 t o 2 0 N A
2 4 0 ,2 t o 8 0 N A
rw 0 , 0 2 t o 6 5 N A
lABIh 1-1 teont.ii
" Element Reference Measure»! values Technique c o m p o u n d ! TW
- this n a r k ) j m i ringn
(p p m unless otherwise shown)
Si 8 . 0 . 14 OS 7 80 OS
20 NT) t o 50 OS
21 0.05 to 40 OS
S In v\ TW 10 to *>0 NA
CI 16 NA
Ar 5 MS
K 16 NA
Cn «. 9, 14 OS
21 0,1 t o 0.8 OS
•rw 0,025 to 195 NA
Sc 4 0,32 to 2 8 0 p .p .b . NA
' 6 0.04 t o 8 ,96 p .p .b . NA
1H 0,54 to 52 p .p .b . NA
25 0,001 to 0 ,4 p .p .b . NA
TW 0 ,004 to 18,6 pp.1). NA
Ti 0, 14 OS
20 ND to 8 OS
26 0.06 OS
rw 0,005 to 29 NA
V 16 0,3 t o 64 ,3 p .p .b . NA
V 0,06 to 2 6 0 p .p .b . NA
Cr 14, 20 OS
7 20 OS
17 0,073 to 144 NA
18 0,08 to 1 0 0 0 NA
25 0 ,0004 to 0 ,09 NA
TW 0 ,0005 to 6,6 NA
24
IKA< r. I IE MEN IS I s |>| \.MONI>s
I AMI II <ïonl.l>
I lenient Keteren. •: Measure,! '.alues 1 c h n i q u c
u i m p o u m l ! I W trus « . , r k | <in<i r inses
i p p ni un.css otherwise shown >
Mn '» OS
15. 1'. NA 4 0.O43 to 3.* NA 7 1 OS
17 - 0.0OO1 !,. 3.2 NA IK o oo2 5 !,> 2.5 N \
19 i i . i ) 0 2 t , i i i . i i ' ) NA
IW o .ooo? t,, 5.4 NA
l< 8, " . |f, OS 7 200 OS \t> 0.2 r.> 20.7 NA
2o Nl) to" 30 OS
21 0.03 to 7 OS TW 0.07 to 141) N \
( i> 9 OS
4 0 .0034 to «..4 NA If. 0.DOD3 to D.254 NA 18 0 .054 to 11.77
NA
25 0 .0005 to 1,5 NA TW 0 . 0 0 0 3 to 1.5 NA
Nl Id NA 7 80 OS
25 0.02 to 4«) NA
rw O.o25 to 46 NA
Cu 8, 14 OS 16 NA 7 40 OS
17 0 ,0005 to 4 0 NA
18 O.O50 to 2 ,9 NA
19 0 ,0004 to 0 .9 NA
20 Nl) t o 8 OS
25 0 , 0 0 2 6 to 1,1 NA
rw 0.001 to 15 NA
/ n 9 OS
( , i 4 NA
TW 0,001 to I t , 9 p . p . b . NA
Br 16 NA
Kiement c o m p o u n d
! i i
Kb 1 r>
Zi
F:U 4 16 TW
Measured values Techn ique
and ranges i p p . m unless otherwise s h o w n )
| | NA
t
I
NA
NA
OS
30 1
NA
0,05 to 4 p , b . i NA 0.02 to 350 p .p .b i
NA
NA
0 ,041 to 5.6 p . p . b . NA
OS
0 ,0015 t o 0,94 NA
1,4 t o 3,o NA
0 ,00002 to 0 ,001 NA 0 ,00001 t o 0 , 1 2 4 NA
NA
0 ,014 to 16,8 NA
0 , 0 0 0 0 5 t o 0 , 2 3 0 NA
NA
0,01 to 25 p.p.b. NA
0 ,12 to 97 p . p . b . NA
0 , 0 4 to 5,48 p .p .b . NA
0,001 to 3,6 p.p.b. NA
26
IABLK II (comtdl
F.lement/ Reference Measured values Technique c o m p o u n d ITW
rh i i work l and ranges
1 (p .p .m unless o therwise shown)
K.U i 4 0,12 t o 97 p .p .b NA
l o 0 ,04 to 5.48 p .p .b . ! NA | TW 0 ,001 t o 3.6 p p .b .
NA
( .d Í 1 " NA
Tb 1 16 0 .06 to 0 ,98 p .p .b . NA
'>> 1
| TW 0 ,03 to 4.7 p.p.b. NA
l l o rw 0.01 t o 1,5 p p . " . NA
Fr 16 NA
Yb i- NA 1,5 t o 8 ,2 p . p . b . NA
, T W 0 , 1 6 to 3,0 p.p.b. NA
l.u ! «6 NA 4 0 ,76 to 3.0 p .p .b . NA TW 0,01 to 0 ,65 p p .b .
NA
l lf 9 OS 4 0,5 to 86 p . p .b . NA
Ta 4 NA 16 0 ,4 to 1,6 p.p.b. NA TW 0 , 0 6 6 to 33,0 p.p.b.
NA
W 4. 16 NA 25 0 , 0 0 9 to 0,6 p.p.b. NA
Ir 4, 1 6 NA 25 0 , 0 0 0 6 to 160 p.p.b. NA TW 0 ,0005 to 37 ,0
p.p.b. NA
Pt 9 _ OS TW NA
Au 16 NA 3 2 0 NA 4 0 ,05 t o 65 p.p.b. NA 18 0 , 0 7 2 t o 5,4
p.p.b. NA 25 0 ,001 to 0,1 p.p.b. NA TW 0,001 t o 0 ,37 p p.b.
NA
H» 4 0 , 0 0 4 t o 5,4 NA
to 9, 14 - OS
r ,4S l . f II (contJ)
Element Reference Measured values • echmqjc compound ITW = this
work! and ranges
(p.p.m. unless otherwise shown*
Th 4 0,77 to 70O p.p b \ \ r\\ O.f) to 29 p.p b. NA
t' 4 V \ TW NA
LEGEND
G Gravimetric
OS Optical spec t roscopy
PA Photon act ivat ion
CPA Charged-particle activation
Indicates qualitative de te rmina t ion only
ND Not de tec ted (optical spec t roscopy general ly)
p .p .b . Parts per billion ( l O 9 )
2«
R E F F K F M ES
1 W'AGNF.R. P \ |lu- di.mi.irul l i r ids of Southern \ t r i ca
Cap,- | , , . A r , ( s m i i k I ->!, I « " l
- Wll I IAMS \ I | ' i f ^cnt-si-. nt the d iamond London, I Benn I
t . : 19<>
-' I K F F D M A N N s / .(.,•..-:. « . . . s . voi 20 1952 p l"4(
l
•* K \ N D A . / , K I N A D V | M N C I R . | . and K O I A T M S
K V J ; , , , . . „ • , • , - . . .,' • + i*>7» p 4<r
5 M F L I l - N ( I arid ! . t \ K I ) l \ | . \ A. Personal
Conimunciatu , ! : 19"4
" KAIM K. \\ . ami BOND. W [.. / • , ' v «.•: . v.,- | | 5 1959 p
K,-
" \ N ( . l S. J ( . Wll I li A . and S I A N K O . W S . ./ j / .
; , / ' / • - , , . m . J 9 ! 9,,« r 1915
H Bl NI INf , . I M and VAN V A I . K E N B l ' R G . A I . , , , -
\lr-i vol 4 3. 195H p 1"2
9 S 1 R A I \ 1 \ N I S . M l and AKA. F / / \<;,-r , / , - „ .
s „ . . v,,! 73 1951 p 5^43
""• ROCCO. ( . ( . . ( . A R S O N O.I. . and C.M.I. ) \> h,- /
, , , , , ; « . , . , , , - Is. < , , „ - . u . < | -
I9r,r,
p 433
11 S H . I . S M I O I ' J.P.I- . HIBBV D M . FRASMCS, I V, and M I
V . A Y . I) » . D u m o n d R e w a r d
1974 Industrial Diamond Div tnbu to . s , London 1974 . p 43
12 KIBBY. I) M. and SI I I Si HOI'. J PI- I rjj„,j„jiv, , /,, „, U
) i 1 2 l<>74 p UK
13 BIBBV. D M . SFI .LSCHOP J.P.I . and S I F F L F , T W
Johannesburg . National Inst i tute tor Metallurgy. H-pi>n m, /
o f / . 1974.
!4 ( I I F S I I Y . I ( . \„„- II..,,-. vol 27 1942 p 2o
15 I.OOS. K , IAEA SYtiiinar Product ion and use ot short lived
ivtopcs in reactors . 5th to 9 th Nov
1962 vol 2. 1963 p 45 .
l o I I SQ, II W.. BIBBV. D M . SFI .LSCHOP J P I and WAÏ 11 KSON.
J I W / , ,.l,,.„;,,,, • , / • , , „
vol 17. 1974. p 195.
17 k O H O C H N U . O V , H.N, U A / U N O V . M P . ORI .OV. Vu.
I . , and SPIKVN, V I . . I>,k, U.,,i.
\juk. S.SSK.. vol 171 |9f>6 p. 107
IS < . | . . \S l NOV. M P , K O B O Í H N K . O V . P N , a n d
O R L O V . Vu I. Is •„,,,„ • „ , , , , , , . V l > ; ? | 9 n
7
p. 231 19 I .K .MTOWI. IRS . F..C. Wir/y/ t >;,» . vol 35 1963 p
12K5. 20 K A A I , I A I w r \U» ,. vol 42 1957 p 3 5 4
21 GNEVl . 'SI IFV. M A., and KRAVTSOV Va. M Ih.lk \k.U. Vir.*
SSAK.. vol 130. I 960 p . 154
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