1
S. Böttger a,b , C. Pipke b , D. Rosenberg b , W. Jansen b , U. E. A. Fittschen a,c a Chemistry Departement, Washington State University, Pullman, WA 99163 b Departement of Chemistry and its teaching methods, Europa-Universität Flensburg, Flensburg, Germany, 24943 c Technische Universität Clausthal, Institut für Anorganische und Analytische Chemie, Clausthal-Zellerfeld, Germany, 38678 Introduction Determination of gas phase mercury – Evaluation of internal standards and external calibration Sebastian Böttger [email protected] Prof. Dr. Ursula Fittschen [email protected] Objective and Experimental Results from AgNP method optimization Results from External Calibration The aim was to develop a reliable, precise, and accurate analysis of gas phase Hg by using TXRF. Chemicals and instrumentation needed are generally already available in laboratories using TXRF for elemental analysis, and a special setup is therefore not necessary. Enrichment of the gas phase Hg on AgNPs was performed and Hg concentrations were determined using a S2 Picofox TXRF (Bruker, Germany). A custom built micro-X-ray fluorescence spectrometer (μ-XRF) was used [10] for the optimization of sample preparation procedures, as well as provide reliable and accurate Hg determination. AgNPs are produced using AgNO 3 and NaBH 4 . Different procedures of preparation and determination were tested: rinsing of deposits after the drying process; absolute determination; internal standards and external calibration curves. Mercury and arsenic compounds were often used to prevent damage to cultural heritage specimens, e.g. herbaria and paintings [1]. Over time, Hg 0 air borne is formed. The pathway comprises bacterial activity and redox processes and is still subject of discussion. Mercury has previously been determined by REXES directly on specimens [1]. Portable mercury vapor indicator (MVI) [3,4], SEM, XRD, XPS and ICP-MS [3], and a portable analyzer using AAS [6] have also been used on a variety of samples. By using Total Reflection X-Ray Fluorescence (TXRF), workgroups have determined Hg in other samples like wastewater [6], seawater [7], and other liquid samples using Au-nanoparticles [8], and in seafood samples by using Ag- nanoparticles (AgNPs) [9]. To the best of our knowledge no data is published for the determination of gas phase Hg by using the AgNP-TXRF approach. Optimization of the Ag-NP preparation method μ-XRF evaluation of internal standards and conclusions about homogeneity Figure 3: μ-XRF images of elemental distribution. Color intensity of RGB images is scaled between 5 and 80 % of the maximum number of counts. 1 st row Ag and Cr (not washed), 2 nd row Ag and Mo (not washed), 3 rd row Ag washed and Mo. A B C D Figure 2: Different angles for the X-ray beam (Table 1). Ag/IS and amount of Ag [mg/L] Total deposit Ag/IS and Ag [mg/L] Area A Ag/IS and Ag [mg/L] Area B Ag/IS and Ag [mg/L] Area C Ag/IS and Ag [mg/L] Area D Max. Deviation from total [%] Ag and Cr (not washed) 7.92; 113.7 12.2; 73.8 6.27; 143.6 7.88; 114.3 7.88; 114.2 35 Ag and Mo (not washed) 0.033; 962 0.033; 976 0.035; 924 0.035; 926 0.032; 987 4 Ag washed and Mo 0.041; 776 0.047; 683 0.03; 926 0.053; 607 0.035; 908 22 Table 2: Results relating Ag to two internal standards, Cr & Mo, and the resulting deviation for different areas. The Cr-IS is not homogeneously distributed on the AgNPs and therefore gives highly variable results depending on the angle of irradiation (Table 2, Fig. 2, Fig. 3). The Mo-IS is more homogeneous and gives better results than the Cr-IS (Table 2, Fig. 3). The AgNPs were dropped on a Quartz- carrier and placed in a Hg saturated atmosphere and allowed to equilibrate for 24 h (Fig. 1). Efficiency and reproducibility of the Hg- capture of washed and non-washed AgNP- specimens were studied (Table 1). The average standard deviation of Ag was ca. 10 % within a batch. Washed carriers contained ~60% less Ag than non-washed carriers. In addition to lower Ag levels, method optimization also resulted in increased Hg capture on washed carriers. References: [1] SIROIS, Collection Forum, 16 (1-2) (2001), 65-75. [2] V AUPEL, Deutsches Museum Wiss. Jahrbuch (1989), 189-226. [3] FELLOWES et al., J. Haz. Mat., 189 (2011), 660-669. [4] BRIGGS et al., New Phytol., 94 (1983), 453-457. [5] OYARZUN et al., Science Tot. Environ., 387 (2007), 346-352. [6] MARGUÍ et al., Talanta, 82 (2010), 821-827. [7] KOULOURIDAKIS et al., Instr. Science & Techn., 34:4 (2006), 425-433. [8] BENNUN, GOMEZ, Spetrochimica Acta Part B, 52 (1997), 1195-1200. [9] ROMERO et al., J. Anal. Spectrom., 29 (2014), 696-706. [10] FITTSCHEN et al. XRS (2017), sccepted manusscript. Neither IS gave completely satisfactory results. A five-point calibration curve was used for external calibration. Since AgNP weights on the carriers fell in the range of 100 - 200 ng, two calibration ranges were selected for Ag: 100 – 500 ng and 60 – 250 ng. A linear regression analysis was performed following the calculation of the residuum and elimination of outliers (Fig. 4). Higher Ag masses (> 300 ng) resulted in higher variability between replicates. Fig. 4: External calibration of Ag. A five-point calibration range of 60 – 200 ng was used for Hg. A linear regression analysis was performed following the calculation of the residuum and elimination of outliers (Fig. 5). The results deviate from the absolute values measured by the program Spectra. The maximal allowable work-place concentration for Hg is 0.020 mg/m 3 , which corresponds to ca. 850 pg absolute on the carrier. Since the actual concentrations in the museums Lower limits of detection (LLD) for Ag and Hg were found to be 129 pg and 4 pg, respectively. The calibration of Hg needs to be performed in a significantly lower concentration range. Since the maximum allowable work-place Hg concentration is 0.020 mg/m 3 , and concentrations found in the Flensburg museum, as well as other museums, a calibration range from 50 pg to 1 ng would be favorable. This would also significantly reduce matrix effects. y = 310.1x + 6598.4 R² = 0.8121 0 50000 100000 150000 200000 250000 0 100 200 300 400 500 600 Net Counts Ag (L1) Mass Ag (ng) External Calibration (Ag) Linear (External Calibration (Ag)) y = 1777.9x + 135789 R² = 0.5649 0 100000 200000 300000 400000 500000 600000 700000 0 50 100 150 200 250 Net Counts Hg (L1) Mass Hg (ng) External Calibration (Hg) Linear (External Calibration (Hg)) Fig. 5: External calibration of Hg. Treatment Ave. Absolute Ag [ng] Ave. Absolute Hg [ng] Ave. Hg/ Ag Non-washed AgNPs 67 0.5354 0.00085 Washed AgNPs 45 6.09396 0.01379 Table 1: Results relating absolute weights of Hg and Ag for washed and non-washed AgNPs. Fig. 1: Quartz-carrier with 10 μL of the AgNP allowed to equilibrate for 24 h in an Hg-saturated atmosphere. Ag L IS Kα RGB image Conclusions were found to be around 0.002 mg/m 3 (ca. 100 pg on the carrier), a calibration curve range of 0.05 1 ng would be more suitable for quantification purposes. A lower calibration curve range is also expected to be less prone to errors due to absorption effects. Acknowledgements: The authors would like to thank the Fittschen Group and Zentraler Ausschuss für Europa und Internationales der Europa-Universität Flensburg for a travel grant to do research at Washington State University, as well as the Ausschuss für Forschung und Entwicklung and the Abteilung Chemie und Ihre Didaktik der EUF.

Results from AgNP method optimization · 2017. 9. 26. · Hg [ng] Ave. Hg/Ag Non-washed AgNPs 67 0.5354 0.00085 Washed AgNPs 45 6.09396 0.01379 Table 1: Results relating absolute

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Page 1: Results from AgNP method optimization · 2017. 9. 26. · Hg [ng] Ave. Hg/Ag Non-washed AgNPs 67 0.5354 0.00085 Washed AgNPs 45 6.09396 0.01379 Table 1: Results relating absolute

S. Böttgera,b, C. Pipkeb, D. Rosenbergb, W. Jansenb, U. E. A. Fittschena,c

aChemistry Departement, Washington State University, Pullman, WA 99163bDepartement of Chemistry and its teaching methods, Europa-Universität Flensburg, Flensburg, Germany, 24943

cTechnische Universität Clausthal, Institut für Anorganische und Analytische Chemie, Clausthal-Zellerfeld, Germany, 38678

Introduction

Determination of gas phase mercury –Evaluation of internal standards and external calibration

Sebastian Böttger

[email protected]

Prof. Dr. Ursula [email protected]

Objective and Experimental

Results from AgNP method optimization

Results from External Calibration

The aim was to develop a reliable, precise, and accurate analysis of gas phaseHg by using TXRF.➢ Chemicals and instrumentation needed are generally already available in

laboratories using TXRF for elemental analysis, and a special setup is thereforenot necessary.

➢ Enrichment of the gas phase Hg on AgNPs was performed and Hg concentrationswere determined using a S2 Picofox TXRF (Bruker, Germany).

➢ A custom built micro-X-ray fluorescence spectrometer (µ-XRF) was used [10] forthe optimization of sample preparation procedures, as well as provide reliableand accurate Hg determination.

➢ AgNPs are produced using AgNO3 and NaBH4. Different procedures ofpreparation and determination were tested: rinsing of deposits after the dryingprocess; absolute determination; internal standards and external calibrationcurves.

Mercury and arsenic compounds were often used to prevent damage tocultural heritage specimens, e.g. herbaria and paintings [1]. Over time, Hg0 airborne is formed. The pathway comprises bacterial activity and redox processesand is still subject of discussion.

Mercury has previously been determined by REXES directly on specimens [1].Portable mercury vapor indicator (MVI) [3,4], SEM, XRD, XPS and ICP-MS [3],and a portable analyzer using AAS [6] have also been used on a variety ofsamples.

By using Total Reflection X-Ray Fluorescence (TXRF), workgroups havedetermined Hg in other samples like wastewater [6], seawater [7], and otherliquid samples using Au-nanoparticles [8], and in seafood samples by using Ag-nanoparticles (AgNPs) [9]. To the best of our knowledge no data is publishedfor the determination of gas phase Hg by using the AgNP-TXRF approach.

Optimization of the Ag-NP preparation method µ-XRF evaluation of internal standards and conclusions about homogeneity

Figure 3: µ-XRF images of elemental distribution. Color intensity ofRGB images is scaled between 5 and 80 % of the maximumnumber of counts. 1st row Ag and Cr (not washed), 2nd row Ag andMo (not washed), 3rd row Ag washed and Mo.

A B

C

D

Figure 2: Different angles for the X-ray beam(Table 1).

Ag/IS and amount of Ag [mg/L]

Total deposit

Ag/IS and Ag [mg/L] Area A

Ag/IS and Ag [mg/L] Area B

Ag/ISand Ag [mg/L] Area C

Ag/IS and Ag [mg/L] Area D

Max. Deviation

from total [%]

Ag and Cr (not washed)

7.92; 113.712.2; 73.8

6.27; 143.6

7.88; 114.3

7.88; 114.2

35

Ag and Mo (not washed)

0.033; 9620.033;

9760.035;

9240.035;

9260.032;

9874

Ag washedand Mo 0.041; 776

0.047;683

0.03;926

0.053;607

0.035;908

22

Table 2: Results relating Ag to two internal standards, Cr & Mo, andthe resulting deviation for different areas.

The Cr-IS is not homogeneouslydistributed on the AgNPs and thereforegives highly variable results dependingon the angle of irradiation (Table 2, Fig. 2,Fig. 3). The Mo-IS is more homogeneousand gives better results than the Cr-IS(Table 2, Fig. 3).

The AgNPs were dropped on a Quartz-carrier and placed in a Hg saturatedatmosphere and allowed to equilibrate for24 h (Fig. 1).

Efficiency and reproducibility of the Hg-capture of washed and non-washed AgNP-specimens were studied (Table 1). Theaverage standard deviation of Ag was ca.10 % within a batch. Washed carrierscontained ~60% less Ag than non-washedcarriers. In addition to lower Ag levels,method optimization also resulted inincreased Hg capture on washed carriers.

References:

[1] SIROIS, Collection Forum, 16 (1-2) (2001), 65-75.

[2] VAUPEL, Deutsches Museum Wiss. Jahrbuch (1989), 189-226.

[3] FELLOWES et al., J. Haz. Mat., 189 (2011), 660-669.

[4] BRIGGS et al., New Phytol., 94 (1983), 453-457.

[5] OYARZUN et al., Science Tot. Environ., 387 (2007), 346-352.

[6] MARGUÍ et al., Talanta, 82 (2010), 821-827.

[7] KOULOURIDAKIS et al., Instr. Science & Techn., 34:4 (2006), 425-433.

[8] BENNUN, GOMEZ, Spetrochimica Acta Part B, 52 (1997), 1195-1200.

[9] ROMERO et al., J. Anal. Spectrom., 29 (2014), 696-706.

[10] FITTSCHEN et al. XRS (2017), sccepted manusscript.

Neither IS gave completely satisfactoryresults. A five-point calibration curve wasused for external calibration. Since AgNPweights on the carriers fell in the range of100 - 200 ng, two calibration ranges wereselected for Ag: 100 – 500 ng and 60 –250 ng.➢ A linear regression analysis was

performed following the calculation ofthe residuum and elimination ofoutliers (Fig. 4).

➢ Higher Ag masses (> 300 ng) resulted inhigher variability between replicates.

Fig. 4: External calibration of Ag.

➢ A five-point calibration range of 60 –200 ng was used for Hg.

➢ A linear regression analysis wasperformed following the calculation ofthe residuum and elimination ofoutliers (Fig. 5).

➢ The results deviate from the absolutevalues measured by the programSpectra.

➢ The maximal allowable work-placeconcentration for Hg is 0.020 mg/m3,which corresponds to ca. 850 pgabsolute on the carrier. Since theactual concentrations in the museums

➢ Lower limits of detection (LLD) for Ag and Hg were found to be 129 pg and 4pg, respectively.

➢ The calibration of Hg needs to be performed in a significantly lowerconcentration range. Since the maximum allowable work-place Hgconcentration is 0.020 mg/m3, and concentrations found in the Flensburgmuseum, as well as other museums, a calibration range from 50 pg to 1 ngwould be favorable. This would also significantly reduce matrix effects.

y = 310.1x + 6598.4R² = 0.8121

0

50000

100000

150000

200000

250000

0 100 200 300 400 500 600

Net

Co

un

ts A

g (L

1)

Mass Ag (ng)

External Calibration (Ag) Linear (External Calibration (Ag))

y = 1777.9x + 135789R² = 0.5649

0

100000

200000

300000

400000

500000

600000

700000

0 50 100 150 200 250

Net

Co

un

ts H

g (L

1)

Mass Hg (ng)External Calibration (Hg) Linear (External Calibration (Hg))

Fig. 5: External calibration of Hg.

TreatmentAve.

Absolute Ag [ng]

Ave. Absolute Hg [ng]

Ave. Hg/Ag

Non-washedAgNPs

67 0.5354 0.00085

WashedAgNPs

45 6.09396 0.01379

Table 1: Results relating absolute

weights of Hg and Ag for washed

and non-washed AgNPs.

Fig. 1: Quartz-carrier with 10 µL of the AgNP allowed to equilibrate for 24 h in an Hg-saturated atmosphere.

Ag L IS Kα RGB image

Conclusions were found to be around 0.002 mg/m3 (ca. 100 pg on the carrier), acalibration curve range of 0.05 – 1 ng would be more suitable forquantification purposes. A lower calibration curve range is also expected tobe less prone to errors due to absorption effects.

Acknowledgements: The authors would like to thank the Fittschen Group andZentraler Ausschuss für Europa und Internationales der Europa-UniversitätFlensburg for a travel grant to do research at Washington State University, as wellas the Ausschuss für Forschung und Entwicklung and the Abteilung Chemie undIhre Didaktik der EUF.