Canodian Mineralogist Yol. 27, pp. 219-224(1989)

EPRINVESTIGATION OF CARBONACEOUSNATURAL OUARTZ SINGLE CRYSTALS

PILLUTLA S. RAO, JOHN A. WEIL AND JOHN A.S. WILIAMS Departmentof Chemistry,University of Saskatchewan,Saskatoon, Saskatchewan S7N 0W0

ABSTRACT Nos donn€esne rdvblent aucune 6vidence de centresi liai- sonscarbone-oryglne daus lesquels le C pourrait substi- As part of an investigation of whether carbon can sub- tuer au Si. stitute for silicon in ming1sfu, electron paramagnetic resonancestudies were carried out on natural crystals of Clraduit par la Rddaction) a4;laftz from carbonaceous surroutrding.s, i.e., a cat- bonized log found in Utah, For these, as obtained, the Mots

A typical EPR spectrum of a UBQ crystal at RT' taken with ilte (= Z,r, is shown in Figure 2. Here B is the applied external magnetic field, and d is the ^ g.lqEs crystal optic axis (superscript indicates a unit vec- sddE tor). Figure 2 clearly shows a broad line and a sin- eilesharp line, plus much weaker lines at 341.185, 341.U7, 341.342, 341.410, 342.115and 342.42.0mT Ftc. 1. Two typical crystals of black quartz, as found at (z = 9.58089GHz). The broad line has a g-factor of the Utah location. Bar scale I mm. 2.0J2f,Q)and a width of 0.75 mT, defined asthd dis- EPR OF CARBONACEOUS OUARTZ CRYSTALS 221 tance between the two extrema of the fust deriva- tive. The sharp line has a g factor of 2.0060(l) and a width of 0.030mT. Crystal rotations with,8 in the XZ and XIl planes (,t is along a two-fold axis; see Nuttall & Weil 1981)disclosed that whereasthe broad line is isotropic, the narrow line is not and shows site splittings on rotation. From the rotation data, the sharp line was unequivocally identifred (from its g and 2eSihyperfine values) as arising from the E,' centre (Silsbee 196l). The other weak lines were found to be anisotropic. When we cooled the UBQ crystal to ca. 35 K in the Varian spectrometer, we observed the sameX- band EPR spectrum as at RT. No new lines were seen.As temperature was changed from RT to LT, the width of the broad line decreasedfrom 0.75 to 0.61 mT,'whereas the width of the E1' line appeared to increase very slightly, from 0.030 to Frc. 2. A typical 9.6 GHz EPR first-derivativespectrum 0.036 mT. The areasof the absorptionsfollow the of a UBQ crystalat room temperaturewhen 8//e. Boltzrnann temFerature dependence. One Utah crystal was X-irradiated at RT for 40 minutes. Irradiation causedno changein the widths ing this process. and g-factors of either the broad or the Es' line at The RT EPR spectrum of UBQ at 4.3 GHz RT, whereasthe relative intensity of the latter center differs somewhat from that at 9.6 GHz described increased(approximately 2.5 times) comparedto the above. We again found the isotropic broad line intensity of tle former one. The crystal was then (nidth 0.72 mT) and the Et' line. In addition to cooledto ca. 35 K in the X-band Varian spectrome- these,we noted a sextetcentered near the broad line. ter. To our surprise,no signal from [AlOn]oor any lWeassiened these six lines to Mn2+ (nuclear spin = other aluminum-based hole centers(Nuttatt & Weil 5/2) n the UBQ crystal. These six Mn2* lines are 1981)was observable.This is unusualin crystalsof isotropic, with a g-factor of 2.@11(l) with 55Mn natural quartz. No lines from Ge3+ centers (Weil hyperfine splitting of 9,42 mT. This splitting is 1984)were seeneither. The spectra do exhibit some reasonable for Mn2* bonded to oxygen in sixfold additional features at LT, including two relatively coordination (Simanek& Mueller 190). The absence strong anisotropic lines (approximately one-fourth of all but the sentral fine-strusture sextet suggests the intensity of E1' line) of nearly equal intensity, high static disorder for the ocqurence of the (pre- at362.129and362.358 mT (v = l0.lM cHa E//A. sumed) MnO5 clusters. We tried to remove surface We also noticed a single anisotropic weak line when impurities in the UBQ crystal by warming it gently B is parallel to e at362.857mT (v = l0.l4l0 GHz) in various solvents(CS2, conc. HNO3, conc. HrSOo, with a width of 0.024 mT. We could not detect any conc. HCI). This treatment did not remove the uuclear hyperline lines (such as from 25i or l3C1for Mn2+ signal. these above-mentionedadditional features (except- The black mantle material also gives a broad line ing Er'). The same crystal was subsequentlyheated at RT, with characteristicsidentical to those observed rnur at ca.520 K for about 12hours. The spectrum in UBQ. An ENDOR study, at 9.59 GW and ca. then recorded at LT showedvery little changein the l@ K, of this material (in air) showed a strong sin- intensity of the E1' line in comparison to its inten- ple line at 14.5MH4 plus someadditional very weak sity measured before tle X-ray treatment, but the featuresjust abovethis RF frequdncy.Thus the EPR above-mentioned lines disappeared. width appears to be caused by unresolved proton The broad line is stjll observablein UBQ (at RT hyperfine structtre.TheVl GHz EPR spectraof the and LT) after the crystal had beenheatedlo ca.720 mantle material reveal the presenceof the isotropic K for nearly 15 hours in air, whereas the E1' line broad line and the Mn2+ lines, plus some additional almost disappeared.Experience has shown that vir- weak features. The g factor and 55Mn hyperfine tually all paramagnetic centers (except transition- value are the samein the UBQ crystals and the sur- metal ions such as Fe3*) disappear when quartz is rounding mantle material. The additional features heatedto this temperature. After X-raying the crys- simultaneously present in the UBQ crystals and in tal at RT for nearly 45 minutes, the E1' line reap- tle mantle material were not identified. peared with almost the same intensity as before The mantle material was subjected to the follow- bleaching. We did not notice auy change in either ing treatments: a) exposure to X rays at RT for 40 the intensity or the linewidth of tle broad line dur- minutes, b) then heating in air for nearly 15 hours 222 THE CANADIAN MINERALOGIST at ca.7?.0K, and c) then exposureto X rays again carbon-oxygen divacancy radicals present in irradi- at RT. The spectra were recorded after each treat- ated silicon (Lee et al, 1977). All the above- meut. There was no noticeable change eitler in the mentioned carbon-oxygen radicals were measured g-factor or linewidth of the broad line during the with EPR at 77 K. above experiments.No new lines were found. As was mentioned in the results section, we Treameft of tle mantle material at RT with conc. observed four weaker lines in UBQ at fields below H2SOn(aq),conc. HNO3(aq), conc. HCI (aq) and the strong broad line and two more weaker lines CS2 showed it to be almost completely soluble in above the broad line. We tried to measure angular tlese solvents. The black-colored solutions thus dependencesfor thesesix lines at X band, but unfor- obtained gave symmetrical broad EPR signals with tunately the lines were too weak (and the strong lines identical g-factors Q.W28\, but with decreased interfered) to do this quantitatively. We can say tlat linewidths, semparedto the width obtained from the tle range of g factors for the lower-field four lines solid mantle material. The broad line is still present is roughly 2.ffi57 to 2.N75, whereas for the other (both atRT and at LT) intheUBQ crystalswen after two lines it is 1.9987b 2.N?2. None of the above treating the crystalswith thesedifferent solvents;the radicals cited in the literature can be responsiblefor color of both the crystal and the solvent remained these six lines, since the range ofg factors for these unchanged. carbon radicals (except perhaps CO+) is incompat- Our experimentsto find carbon as a substitutional ible with our results. impurity for silicon in quartz were extended with We can concludethat tle color of tle black quartz studiesof Herkimer "" quartz srystals.The crystals investigated herein is due to macroscopic RT EPR spectra of these (four) crystals, containing organic impurities presentin the crystal, and not due small visible black inclusions, gavea broad line with to substitutional "point" impurities'in the quartz a g factor of 2.N22(l) and a width of 0.42 mT, at strusture. It has been suggested from the low- botl frequenciesof measurement(9.4 and24 GHz). temperature EPR spectra of coal ash, which do not We found the samebroad line, at9.4 GHz, in "black contain a broad line at g = 2,that the latter in coal chunks" removed from the Herkimer crystals, witl arises from organic matter @etcofsky et al. l98l). a g factor ot 2.M?5(l) and a width of 0.53 mT. At Sincethe width of the broad line in BQ remains the A GHz, we noticed some weak additional features sameboth at 9.6 and 2/+.3G}Iz, we consludethat (not Mnz+ lines), in addition to the isotropic broad the breadth is causedby unresolved hyperfine lines, line. Someof theseHerkimer crystalswere subjected presumably from protons, and not by overlap of to 45 minutes of X-irradiation. We did not find any different g-fastor spectra (hyperfine values are laorlo centers (Nuttall & weil 19sl) in the LT independent of frequency). The width of ttre broad EPR spectraof thesegrysrals, but somedo show lines lines in soals usually depends on the percentageof due to Ge * 6a impurif (Weil 1984). carbon present.For coals with carbon contentsrang- A Herkiner quartz crystal containing no visible ing from 55 to 9090, the corresponding linewidths black inclusions gaveno BPR lines. Specifically, the vary"from 0.52 to 0.86 nT @etcofsky et al. l98l). broad line is absent. The crystal was then X- Our mantle material has a carbon composition of irradiated at RT, whereupon the RT EPR spestrum 8090and a linewidth of 0.75 mT, in good agreement showedweak lines due to Ge and the LT EPR spec- with the above general trend. trum showed fAlo4lo, in addition to the Ge centers. As was mentioned in the resultssection, Herkimer Unlike the UBQ crystals, nong of the Herkimer quartz crystals with blask inclusions do give the quartz crystals (with and without black inclusions) broad line, whereas crystals without these do not. showedthe E1' spestrum. Thus it is indeed the black "anthraxolite" particles that give rise to the free radical EPR signal. D$cussroN eNo Sunmrenv The absenceof the six Mn2+ lines in our X-band spectra of the UBQ and mantle material, and their A few oxygeniccarbon-containing free radicalsare presenceat K band, may be due to greater line- known, but not in crystallins qvartz. No carbon broadening at the lower frequency (caused by the tetroxide free radical species seemsto have been relatively greater anisotropy effects of the fine- reported in any material. However, CO3 and CO! structureterms in the spin Hamiltonian). Sucheffects radicals were observedafter grinding quartz sand in were observed(Lehmann 1987)for Mn2+ in AIPO4. a CO2 atmosphere (Ebert & Hennig 1974) and Manganese in coals (Retcofsky et al. l98L), rn presumably are surface species. Other known in oil sands(Malhotra & Buckmaster 1985) carbon-orygen radicals potentially relevant to our and in petrified wood from Bristol, England (Ikeya study are COt, COl- (Serway & Marshall 1967), 1982) has been reported, and at least in some CO! (Marshallet al. 19il), HCO3- (C.asset al. 1974) instances occurs in CaCO, inclusions (Malhotra & (all the above observed in calcite), CO+ on a H- Graham 1985). type zeolite (Vedrine & Naccache 1973), and In summary, we have discovered that coal-like EPR OF CARBONACEOUS QUARTZ CRYSTALS 223 materials containing free radicals can be intimately Lrr, Y.-H., Comrrr, J.W. & Bnowrn, K.L, (1977): associatedlqith quartz crystals. Our attempt by EPR EPR of a carbon-orygen-divacancycomplex in to identify carbon atoms occurring substitutionally irradiated silicon. Phys. Stotus Solidi (A) 41, for silicon in thesesamples of a-quartz, in which tle 637-@7. opportunity for carbon substitution appearedto be high, gave negative results. This finding is consis- LEuuarN,G. (1987):Defects in minerals.Cryst. Lat- tent $/ith our theoretical predictions. ticeDefects Amorphous Mater. (U.K.) t4, 307-317 .

AcKTIowLEDGBNIENTS LFsrevrcr, I.E. (1959): Crystals of quartz in coals. Sov. Phys. Dokl. (EneI. Transl.) 4, U-26. This work was carried out under the auspicesof the Natural Sciences and Engineering Research Mamorre, & Buqonesrrn, H.A. (1985):The behavior Council of Canada. We are most grateful to Mr. F. of mineralsin Cold Lake oil sandsunder dry com- Fornelius (Centerville, Utah), Mr. & Mrs. C. Gro- bustionconditions. Appl. Clay Sci.l,225-236. man @ethlehem,Pennsylvania), Ms J. Kaylor @ed- path Museum, McGill University, Montreal, Que- & Gnenau, W.R.M. (1985): Origin of the bec), Mr. & Mrs. R. Mercer (Palmerton, Mn2+ ion e.p.r. spectrum in Pittsburgh No. 8 Pennsylvania) and Mr. N. Rochester (Morris bituminous coal. Fuel M, n0-n2. Museum, Morristown, New Jersey)for providing us with the crystals investigated. Thanks are due to Mansnan, S.A., Ren\rBeno,A.R., Snnwav,R.A. & SaskatchewanResearch Council for the neutron acti- Hoocns, J. A. (1964): Electron spin resonance vation analysis and radiocarbon dating, to our absorption spectrum of CO2 molecule-ions in Department of Chemistry Analytical Lab and espe- single-crystalelcite. Mol. Phys. 8,225-231. cially to Dr. L. W. Bader for the chemical analysis, and to Bruker Analytische Messtechnik (Rheinstet- McEecnrm, R.J., Wur, J.A. & MBznv,P.G. (1988): providing ten, FRG) for the ENDOR spectra. We Ab initio calculations on tetramethoxymethane. thank Prof. R. J. Kirkpatrick and an unknown Can. J. Chem. 66.2041-2044. referee for their helpful comments.

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