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LASER ABLATION COUPLED TO MASS QUADRUPOLE SPECTROMETRY (LAMQS) APPLIED TO ANCIENT COINS

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L. Torrisi1, G.Mondio2, A.M. Mezzasalma2, F. Caridi3, L. Giuffrida1, T. Serafino2, M. Cutroneo1, A. Baglione1 and A. Torrisi1

1Dipartimento di Fisica, Università di Messina, 2Dipartimento di Fisica della Materia e Ingegneria Elettronica

3Facoltà di Scienze MM. FF. NN., Università di Messina, V.le F. S. D’alcontres 31, 98166 S. Agata, Messina

LASER ABLATION COUPLED TO MASS QUADRUPOLE

SPECTROMETRY (LAMQS) APPLIED TO

ANCIENT COINS

Abstract

A Nd:Yag laser operating in second harmonic (532 nm), 3 ns pulse duration, 1-150 mJ pulse energy and 1-10 Hz repetition rate is employed to irradiate different coins placed in high vacuum chamber. The ablated material, in vapor phase, is analyzed by a mass quadrupole spectrome-ter in the range 1-300 amu with sensitivity up to 1 ppm. The “on line” analysis permits to investigate on the ele-ments, chemical compounds and isotopic ratios character-izing the coin composition.

Focused and unfocused laser beams can be employed to irradiate sub-millimetric or tens millimetric areas, respec-tively. The first method is employed to determine the ele-mental depth profiles from surface up to about 0.1 mm. The second method is employed to analyze the average composition of the superficial patina layers. This micro-invasive technique, associated to the characteristic X-ray fluorescence emission due to 20 keV electron impact, was employed to analyze different coins, based on bronze and silver, from VI up to XX sec.

INTRODUCTION

The Laser Ablation coupled to Mass Quadrupole Spec-trometry (LAMQS) is becoming an interesting analysis technique useful to investigate on the surface composition of different materials comprised ancient metallic coins [1]. The laser-target interactions give rise to a localized surface vaporization with formation of a crater which dimensions depends on the laser spot, laser energy and number of laser shots [2]. The high energy stability, repetitive beam profile and flexibility permit a controlled material removal from solid surface, layer by layer, till the wished depth.

The choice of the best laser irradiation parameters and the relative rapidity of analysis are the main advantages of the method, which make this technique attractive for elemental depth profile analysis, surface cleaning and non-disruptive surface processes. The ablation yield, given in terms of removed depth per laser pulse, can be measured in a

con-trollable manner by using suitable calibration samples irra-diated at different laser intensities [3]. The surface analysis is limited by the laser spot, controllable from the optical focusing lens. The penetration depth of the single laser shot depends on the laser and target properties. Thermal effects, mainly induced by infrared and visible lasers, enlarge the penetration depth in conductive targets, due to their high thermal conductivity. Photochemical effects, mainly due to ultraviolet lasers, limit the ablation depth only to the penetration absorption light and can be em-ployed for analysis in insulator samples [4].

The atomic and molecular emissions from the laser irradi-ated target can be analyzed by using a mass spectrometer, which permits to measure the masses with high sensitivity and high mass resolution, permitting to detect ppm level element and compound concentrations and to distinguish isotopic masses.

By increasing the irradiation time it is possible to remove atoms from depth layers and, by knowing the ablation rate, the mass spectrometry analysis may give the depth profile of the detected masses in the investigated surface. By using micrometric laser spots it is possible to investigate on the sample depth in a micro-invasive mode.

In this work LAMQS and characteristic X-ray fluorescence (XRF) are applied to some coins in order to determine their elemental composition, chemical compounds and isotopic ratios, both in surface and in depth, in order to give inter-esting information to numismatic field.

MATERIALS AND METHODS

The laser ablation was performed with a pulsed Nd:Yag working at 532 nm, 3 ns pulse duration, 1-10 Hz repetition rate and 1-150 mJ pulse energy. The laser beam was di-rected on the target placed in high vacuum (10-6 mbar)

through a thin glass window. The spot diameter is 1 mm2

and the incidence angle is 45°. The target can be moved vertically with the vacuum feedthrough, so that each laser shot can hit a fresh flat surface. Fig. 1 shows a photo of the experimental setup.

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of 8.3x108 W/cm2 corresponding to 25 mJ pulse energy,

and at 10 Hz repetition rate mode for times of the order of 20 seconds or less. In such conditions only the most super-ficial atomic monolayers can be removed, without damage of the surface and the ablation rate on a Cu and Ag calibra-tion samples demonstrated that the removing depth is about 10 nm/s [6]. During depth analysis the laser energy generally is increased to 150 mJ at which the removing depth increases to about 1 mm/s.

Two different bronze coins of archaeological interest coined in the Mediterranean basin, coming from Anti-nopoulis (Egypt) and coined in the VI-VII century a.D. and Syracuse (Sicily, Italy), coined in the same historical pe-riod, were analyzed. The Egyptian and Syracuse coins are reported in the photo of Fig. 2a and Fig. 2b, respectively. Moreover, two different silver coins, consisting in a Greek tetradrachm from Messana (Messina-Italy) dated to 470–

466 B.C. and coined under the ruling of Anassila, and from Italy of 1937, coined under the Vittorio Emanuele III re d‟Italia, were also analyzed.

The Greek and Italian coins are reported in the photo of Fig. 2c and Fig. 2d, respectively.

A Balzer-Pfeifer MQS spectrometer, 300 amu full scale, less than 1 amu mass resolution and less than 1 ppm sensi-tivity, was interfaced to the vacuum chamber in order to detect the masses emitted from the laser ablation process. The MQS mass selection occurs thank to a selective ra-diofrequency applied to four parallel rods, while the high sensitivity is obtained by the use of a secondary electron multiplier. The quadrupole operates by plotting the mass yield vs. the mass value or, by fixing the masses of inter-est, by plotting the masses vs. the irradiation time. Charac-teristic X-ray fluorescence (XRF) analysis, induced by 20 keV electron beam, was performed with a high vacuum SEM microscope and a X-ray Si(Li) detector. XRF permit-ted to analyze the elemental composition of the investi-gated samples and to furnish the input masses parameters for the MQS spectrometer. XRF analysis is limited to the electron range depth in the metal which is about 600 nm for Ag and 800 nm for Cu. LAMQS analysis depends on the ablation yield and on the number of the laser pulses employed to ablate the metal surface. A surface profiler, Tencor P-10, with high horizontal and vertical resolution, has been employed to measure the surface roughness on the surface of the two coins. It uses 1 mg tip force sweep-ing on the selected zones of the sample, especially in cor-respondence of the craters produced by the laser ablation on the coins. The crater profile permits to measure the ab-lation yield in terms of ablated depth/pulse and to correlate the MQS profile with the real sample depth.

RESULTS

The preliminary analyses performed through XRF permit-ted to evince the elemental composition of the patina lay-ers of the different coins. As an example, Fig. 3 shows typical XRF spectra coming from the surface analysis of the Egypt bronze (a) and Greek silver (b) coins.

The first indicates the typical bronze content in Cu, Pb, Fe and Al with trace elements of Si, Cl, K and Ca, probably present as oxides in the ancient patina. The second shows a high Ag characteristic peak indicating that the silver was employed as pure in the phase of coin. Also in this case the patina layer contains many trace elements, such as C, Cu, Zn, Mg, Al, Si, S and Cl and oxygen probably present as oxide compounds.

A confirm of these elements was given by MQS analysis. As an example Fig. 4 shows two typical MQS spectra ob-tained detecting the removed species from the Syracuse ablated coin. The first is relative to the mass range 60-100 amu (a) and the second to the mass range 100-300 amu (b). In both cases many chemical compounds are indicated as

Fig. 1: Photo of the experimental set up.

Vacuum chamber

Laser system

EQP 300

Fig. 2: Photo of the four investigated old coins: The Alexandria bronze

coin of VII-VII sec. a.D. (a); the Syracuse bronze coin of VII-VIII sec a.D. (b); the Greek silver coin tetradrachm of IV sec B.C. (c) and the recent Italy silver coin of XX sec. (d).

a) b)

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content of the patina surface which appears rich in oxides, carbides and chlorides of the main bronze elements Cu, Fe, Sn and Pb.

A particular attention was given to the measurements of the isotopic ratios of the lead in the bronze samples. Lead has four isotopes and their relative ratios are suitable of little variations, characteristic of the mineral used for the coin.

Fig. 5 shows two typical MQS spectra relative to the char-acteristic lead isotopic masses measured in Alexandria (Egypt) (a) and Syracuse (b) bronze coins. The measured isotopic ratios are reported in Tab. I and compared with the expected ratio values coming from the global measurement on the terrestrial crust [5].

The little difference values of the isotopic ratios are very important because they are typical of the used minerals employed during the coin phase. Thus, from the point of view of archeology, numismatic and historic, the compari-son between different coins and coins and mineral contents permit to deduct important information for the scientific and cultural communities.

In order to have more information of the depth composi-tion of the coin, depth profile investigacomposi-tions were con-ducted by using the laser ablation at 1 Hz repetition rate. The measurements, correlated with the ablation yield, per-mit to know the patina thickness, the presence of segrega-tion effects and, in general, to have informasegrega-tion of the

depth profile of elements, chemical compounds and iso-tope ratios. As an example, Fig. 6 reports two MQS plots relative to the masses 16 (a) and 107 amu (b), representa-tive of the O16 and Ag107, respectively, for the Italian silver

coin (Fig. 2d).

Both spectra, recorded irradiating with 150 mJ pulse en-ergy and 1 Hz repetition rate, show a yield decreasing with the irradiation time, due to the crater depth effect which reduces the laser focusing and the particle emission to-wards the MQS detector. It is the ratios between the two spectra yields, in terms of Ag107/O16, that shows an

inter-esting result in terms of elemental profile with the irradia-tion time, as reported in Fig. 6c. Finally, the data elabora-tion obtained by using a smoothing process cancels the background peaks due to the 1 Hz ablation repetition rate and it gives a clear profile with the irradiation time, as re-ported in Fig. 6d. This last plot contains also a depth scale which permits to correlate the element profile with the sample depth. This correlation between the irradiation time and the depth is obtained measuring the ablation yield in the coin, i.e. the crater depth per each laser shot.

Two typical crater shapes obtained by using the surface depth profiler in the Alexandria bronze (Fig. 2a) and Ital-ian silver coins (Fig. 2d) are reported in Fig. 7. By using 0 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000 0 1000 2000 3000 4000 5000 S K Ag L Ag L Ag L Ag L Cl K CK O K Al K Mg K Si K Cu L Zn L Zn K Cu K Cu K C on te gg i energia (eV) Selinunte Argento 0 2500 5000 7500 10000 12500 15000 0 500 1000 1500 2000 Fe Ca Ca K Cl Pb Pb Pb Cu Al Si O Cu Cu F lu o re sc en ce Y ie ld energy (eV) PAN2 Egyptian bronze coin Yie ld ( Coun ts )

X-ray Energy (eV)

Greek silver coin

a)

b)

Fig. 3: XRF spectra relative to the patina analysis of the Alexandria

bronze coin (a) and of the Greek silver coin (b).

60 65 70 75 80 85 90 95 100 0,0 0,2 0,4 0,6 0,8 1,0 1,2 1,4 FeCl CuH2 FeO CuCN CuH Cu Cu(OH)2 CuS CuO CuCl Syracuse coin, 30 mJ, 10 Hz, focus, det=90° a)

mass (amu) Ion curren t (x10 -9 A) 100 120 140 160 180 200 220 240 260 280 300 0 1 2 3 4 Cu4O2 PbO PbC2S PbClO PbCl CuClH2 CuCO2 Cu2 SnSO4 Pb SnO

Syracuse, 30 mJ, 10 Hz, focus, det=90° b)

Ion current (x10

-1

0 A)

mass (amu)

Fig. 4: MQS spectra analysis of the Syracuse bronze coin in the mass

range 60-100 amu (a) and 100-300 amu (b).

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pulse laser energy of 150 mJ, the first crater is due to 25 laser shots and the second crater to 50 laser shots, both have a diameter aperture of about 1 mm. In these condi-tions the measured ablation yield is of 3.2 m/pulse and 1 m/pulse, for the bronze and silver coin, respectively, which correspond to 3.2 m/s and 1 m/s of ablation rate, by using 1 Hz repetition rate, in the two cases, respec-tively.

Thus the Ag/O increment vs. depth indicates that the sur-face patina is rich of Ag oxides while the bulk is rich of pure Ag. The depth profile reported in Fig. 6d shows that the oxides layers of the patina have a thickness of the order of 100 mm, in good agreement with literature [6].

205 206 207 208 209 0.0 0.5 1.0 1.5 2.0 2.5 3.0

Alexandria, 30 mJ, 10 Hz, focus, det=90° a)

208 Pb/206 Pb = 2.75 207 Pb/206 Pb = 1.5 Ion current (x10 -1 2 A) mass (amu) 205 206 207 208 209 0.0 0.5 1.0 1.5 2.0 2.5

3.0 Syracuse coin, 30 mJ, 10 Hz, focus, det=90° b)

208 Pb/206 Pb = 1.87 207 Pb/206 Pb = 1.13 Ion current (x10 -1 2 A) mass (amu)

Fig. 5: Comparison of the MQS spectra relative to the isotope mass peak

detected in the bronze

Tab. I: Comparison of the measurements of the isotopic lead ratios in the

two bronze coins with the expected values based on the mean isotopic abundances.

Bronze Coin Period Pb208/Pb206 Pb207/

Pb206 Alexandria VI-VII sec. a.D. 2.75 1.5 Syracuse VII-VII sec. a.D. 1.87 1.13 Expected mean values 1.86-2.70 0.64-1.13 0 50 100 150 200 250 300 0.000 0.005 0.010 0.015 0.020 0.025 Time (s.) Ion current (x10 -8 A) 107Ag 0 50 100 150 200 250 300 0 1 2 3 4 5 6 7 Time (s.) Ion current (x10 -8 A) Oxygen (16 amu) 0 50 100 150 200 250 300 0.00 0.01 0.02 0.03 Time (s.) 107 Ag/O Yield Ratio 0 50 100 150 200 250 300 0,01 0,02 0,03 0 50 100 150 200 250 300 Depth (m) 107

Ag/O Yield Ratio,

smoothed

Time (s)

Fig. 6: LAMQS irradiation profiles in the Italian silver coin relative to the

Oxygen (a), Silver (b), Silver/Oxygen ratio (c), and data elaboration of the depth profile of Ag/O ratio (d) in the first superficial 300 micron depth.

(a)

(c) (b)

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L. Torrisi, G.Mondio, A.M. Mezzasalma, F. Caridi, L. Giuffrida, T. Serafino, F. Di Bartolo, A. Baglione and A. Torrisi

DISCUSSION AND CONCLUSIONS

LAMQS represents an useful technique to analyze the sur-face of metallic samples such as coins. Although the tech-nique is micro-invasive, the crater diameter is of the order of 1 mm and the depth of the order of 300 mm, the analysis can be applied to many samples of interest in archeology and numismatic.

A very important parameter of this analysis is represented by the control of the ablation yield in order to not damage the analyzed sample. To this low laser energy and number of laser shot should be employed. In this direction the liminary use of XRF technique has been used to have pre-liminary information about the elements, possible chemical compounds and isotopes that can be searched by using MQS.

Generally the analysis of one sample take a time of about 15 min but the data analysis and elaboration can take also 1 hour. However the investigation can be developed with

relative simple and economical instrumentations.

The analysis of bronze coin demonstrated that their com-position is different, that the chemical compounds of the patina are different and that the lead isotope ratios can be employed as characteristic property of the employed lead for the coin. Similarly, the two silver coins have different patina composition with different chemical compounds and different patina thicknesses.

However, in this work the potentiality of the analysis tech-nique is mainly discussed and not the obtained characteris-tic of the coin composition. At the moment the composi-tion results are less interesting because they are relative only to four samples coming from different country areas and to different historical periods. Only the application to many samples will permit to have a good statistical data analysis in order to deduct scientific interest conclusions because it will be possible to compare different coins from the same period, coin composition with mineral composi-tion and to distinguish true coins from false ones.

REFERENCES

[1] L. Torrisi, F. Caridi, L. Giuffrida, A. Torrisi, G. Mon-dio, T. Serafino, M. Caltabiano, E.D. Castrizio, E. Pa-niz, A. Salici, Nucl. Instr. and Methods B268,1657-1664, 2010

[2] D. Margarone, S. Gammino, J. Krása, E. Krouský, L. Láska, P. Parys, M. Pfeifer, M. Rosinski, K. Rohlena, J. Skála, L. Torrisi, J. Ullschmied, A. Velyhan, J. Wołowski, Czech J. of Physics, 56, B542-549, 2006 [3] A. Ilacqua, A.M. Mezzasalma, L. Torrisi and J.

Wolo-wski, Proc. PPLA2003, Messina, Sept. 03, Gammino-Mezzasalma-Neri-Torrisi Eds., World Sci. , Publ., Sin-gapore, 177-183, 2003

[4] L. Torrisi, A. Borrielli and D. Margarone, Nucl. Instr. And Meth. In Phys. Res. B 255, 373-379, 2007

[5] K.J.R. Rosman and P.D.P. Taylor “ISOTOPIC COM-POSITIONS OF THE ELEMENTS 1997”, Dep.nt of Appl. Physics, Curtin University of Technology, GPO Box U1987, Perth 6001, Australia. Web site: 2http:// old.iupac.org/reports/1998/7001rosman/iso.pdf [6] Società Italiana di Fisica “Proceeding of the

interna-tional school of Physics Enrico Fermi”, Course CLIV, Physics methods in Archeometry”, IOS Press, M. Missiroli Editor, 2004[32] H. Lai, N. P. Singh, Bioelectromagnetics 16, 207-210 (1995) 0 500 1000 1500 2000 -50 -40 -30 -20 -10 0 10 D e p th (  m) Scansion length (m) Depth profile of the Italian silver coin 25 mJ, 1 Hz repetition rate, 50 shots

Ablation yield Y = 1 m /pulse b) 0 200 400 600 800 -100 -80 -60 -40 -20 0 20 D e p th (  m) Scansion length (m) Depth profile of the Alexandria bronze coin 150 mJ, 1 Hz repetition rate, 25 shots

a)

Ablation yield Y = 3.2 m/pulse

Fig. 7: Crater depth profiles relative to the silver coins coming from

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