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Dive into the research topics where Mario Burger is active.

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Featured researches published by Mario Burger.


Radiochimica Acta | 2005

Radiochemical separation of actinides from environmental samples for determination with DF-ICP-MS and alpha spectrometry

Marin Ayranov; Urs Krähenbühl; Hans Sahli; Stefan Röllin; Mario Burger

Summary The purpose of this study was to develop an optimised sample preparation method for the determination of Pu, Am, and Cm in environmental samples, soils, and sediments, and to compare the sensitivities of DF-ICP-MS, alpha spectrometry, and liquid scintillation alpha spectrometry. Borate fusion was used for sample material digestion. Two methods based on TOPO liquid–liquid extraction and combination of TEVA and TRU extraction chromatography showed highest yields of 92.7% for Pu, 86.8% for Am, and 87.6% for Cm. The detection limits were between 0.014–0.034 Bq/kg for 239Pu, 0.014–0.093 Bq/kg for 240Pu, and 0.011–1.20 Bq/kg for 241Am. Analytical results for 238Pu, 239Pu, 240Pu, 241Pu and 241Am and their isotope ratios in certified reference materials (IAEA-135 and IAEA-300) indicated very good accuracy of the methods proposed.


Radiochimica Acta | 2005

Determination of neptunium in soil by ICP-MS

Marin Ayranov; Urs Krähenbühl; Hans Sahli; Stefan Röllin; Mario Burger

Summary A fast and simple method for the determination of 237Np in soil is presented. The borate fusion decreases the sample pre-treatment time and a TEVA extraction chromatography separates neptunium from uranium and the interfering matrix components. A comparison of the sensitivities of alpha spectrometry and sector field ICP-MS for determination of 237Np is presented.


Analytica Chimica Acta | 1991

Critical evaluation of the determination of zirconium and hafnium in meteorites by instrumental and radiochemical neutron activation analysis

Mario Burger; Urs Krähenbühl

Abstract Neutron activation analysis (instrumental or radiochemical) is suitable for the determination of zirconium and hafnium in samples of geochemical origin only when sufficient attention is paid to interfering nuclides. The size of the necessary correction for INAA depends on the composition of the sample; this problem is discussed. The radiochemical technique which is recommended involves separation of the samples, precipitations and anion-exchange separation. Results are given for various standard reference materials and for meteorites.


Radiochimica Acta | 1989

Determination of Refractory Trace Elements in Chinese Meteorites by RNAA

Urs Krähenbühl; Mario Burger

Some refractory trace elements are important target elements for Spallation reactions in meteorites. These elements also serve to characterize the investigated meteorites. The elements Ti, Y, Zr, Hf, W and Ta were measured after radiochemical separation in chondrites from China. After acid digestion of the irradiated samples, the group separations were obtained by precipitation reactions. The necessary radiochemical purification of the pure β emitter Y was realized on a Lewatite OC 1026 column. For all the other elements discrete gamma radiation was measured.


Journal of Radioanalytical and Nuclear Chemistry | 2017

A procedure for the sequential determination of radionuclides in soil and sediment samples

Hans Sahli; Stefan Röllin; Viktoria Putyrskaya; Eckhard Klemt; Béatrice Balsiger; Mario Burger; José A. Corcho Alvarado

We present a new radiochemical procedure for the sequential determination of Sr, Am, Pu, Th and U radionuclides. For the validation, seven IAEA certified reference materials were analyzed for 239Pu, 240Pu, 241Pu, 238U and 232Th isotopes by ICP-MS, 243Am by alpha spectrometry and 90Sr by low level gas proportional counting. The sequential method was then used for determining the radionuclide profiles in one sediment core collected in the River Rhine, near Augst, downstream of the Swiss nuclear power plants.


Meteoritics & Planetary Science | 1998

Noble gases and chemical composition of Shergotty mineral fractions, Chassigny, and Yamato 793605: The trapped argon‐40/argon‐36 ratio and ejection times of Martian meteorites

D. Terribilini; Otto Eugster; Mario Burger; Alfred Jakob; Urs Krähenbühl


Proceedings of the NIPR Symposium on Antarctic Meteorites | 1989

Preliminary report on the Yamato-86032 lunar meteorite: III. Ages, noble gas isotopes, oxygen isotopes and chemical abundances

Otto Eugster; Samuel Niedermann; Mario Burger; Urs Krähenbühl; H. W. Weber; Robert N. Clayton; Toshiko K. Mayeda


Archive | 1989

Refractory trace elements in different classes of achondrites by RNAA and INAA and some noble gas data

Mario Burger; Otto Eugster; Urs Krähenbühl


Journal of Radioanalytical and Nuclear Chemistry | 2009

Sensitivity of DF-ICP-MS, PERALS and alpha-spectrometry for the determination of actinides: A comparison

Marin Ayranov; Urs Krähenbühl; Stefan Röllin; Mario Burger


Archive | 1990

Refractory trace elements in lunar meteorites MAC88104 and MAC88105

Urs Krähenbühl; Mario Burger; Otto Eugster

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