Technical note: On the reliability of laboratory beta-source calibration for luminescence dating
<p>The dose rate of the <span class="inline-formula"><sup>90</sup></span>Sr <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspm...
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doaj-9ef68ce3aa374ebebdeffcb9a3343daf2021-06-23T06:48:10ZengCopernicus PublicationsGeochronology2628-37192021-06-01337138110.5194/gchron-3-371-2021Technical note: On the reliability of laboratory beta-source calibration for luminescence datingB. Mauz0L. Martin1M. Discher2C. Tribolo3S. Kreutzer4S. Kreutzer5C. Bahl6A. Lang7N. Mercier8Department of Geography and Geology, University of Salzburg, 5020 Salzburg, AustriaIRAMAT-CRP2A, UMR 5060, CNRS-Université Bordeaux Montaigne, 33600 Pessac, FranceDepartment of Geography and Geology, University of Salzburg, 5020 Salzburg, AustriaIRAMAT-CRP2A, UMR 5060, CNRS-Université Bordeaux Montaigne, 33600 Pessac, FranceIRAMAT-CRP2A, UMR 5060, CNRS-Université Bordeaux Montaigne, 33600 Pessac, FranceGeography & Earth Sciences, Aberystwyth University, Aberystwyth SY23 3FL, UKDepartment of Geography and Geology, University of Salzburg, 5020 Salzburg, AustriaDepartment of Geography and Geology, University of Salzburg, 5020 Salzburg, AustriaIRAMAT-CRP2A, UMR 5060, CNRS-Université Bordeaux Montaigne, 33600 Pessac, France<p>The dose rate of the <span class="inline-formula"><sup>90</sup></span>Sr <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="527256ea34e0af356380afd605ccefc0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-3-371-2021-ie00001.svg" width="8pt" height="14pt" src="gchron-3-371-2021-ie00001.png"/></svg:svg></span></span> <span class="inline-formula"><sup>90</sup></span>Y beta source used in most luminescence readers is a laboratory key parameter. There is a well-established body of knowledge about parameters controlling accuracy and precision of the calibration value but some hard-to-explain inconsistencies still exist. Here, we have investigated the impact of grain size, aliquot size and irradiation geometry on the resulting calibration value through experiments and simulations. The resulting data indicate that the dose rate of an individual beta source results from the interplay of a number of parameters, most of which are well established by previous studies. Our study provides evidence for the impact of aliquot size on the absorbed dose in particular for grain sizes of 50–200 <span class="inline-formula">µ</span>m. For this grain-size fraction, the absorbed dose is enhanced by <span class="inline-formula">∼</span> 10 %–20 % as aliquot size decreases due to the radial increase of dose rate towards the centre of the aliquot. The enhancement is most variable for 50–100 <span class="inline-formula">µ</span>m grains mounted as aliquots of <span class="inline-formula"><</span> 8 mm size. The enhancement is reversed when large grains are mounted as small aliquots due to the edge effect by which the dose induced by backscattered electrons is reduced. While the build-up of charge dictates the increase of absorbed dose with the increase of grain size, this principle becomes more variable with changing irradiation geometry. We conclude that future calibration samples should consist of subsamples composed of small, medium, large and very large quartz grains, each obtaining several gamma doses. The calibration value measured with small, medium and large aliquots is then obtained from the inverse slope of the fitted line, not from a single data point. In this way, all possible irradiation geometries of an individual beta source are covered, and the precision of the calibration is improved.</p>https://gchron.copernicus.org/articles/3/371/2021/gchron-3-371-2021.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
B. Mauz L. Martin M. Discher C. Tribolo S. Kreutzer S. Kreutzer C. Bahl A. Lang N. Mercier |
spellingShingle |
B. Mauz L. Martin M. Discher C. Tribolo S. Kreutzer S. Kreutzer C. Bahl A. Lang N. Mercier Technical note: On the reliability of laboratory beta-source calibration for luminescence dating Geochronology |
author_facet |
B. Mauz L. Martin M. Discher C. Tribolo S. Kreutzer S. Kreutzer C. Bahl A. Lang N. Mercier |
author_sort |
B. Mauz |
title |
Technical note: On the reliability of laboratory beta-source calibration for luminescence dating |
title_short |
Technical note: On the reliability of laboratory beta-source calibration for luminescence dating |
title_full |
Technical note: On the reliability of laboratory beta-source calibration for luminescence dating |
title_fullStr |
Technical note: On the reliability of laboratory beta-source calibration for luminescence dating |
title_full_unstemmed |
Technical note: On the reliability of laboratory beta-source calibration for luminescence dating |
title_sort |
technical note: on the reliability of laboratory beta-source calibration for luminescence dating |
publisher |
Copernicus Publications |
series |
Geochronology |
issn |
2628-3719 |
publishDate |
2021-06-01 |
description |
<p>The dose rate of the <span class="inline-formula"><sup>90</sup></span>Sr <span class="inline-formula"><math xmlns="http://www.w3.org/1998/Math/MathML" id="M2" display="inline" overflow="scroll" dspmath="mathml"><mo>/</mo></math><span><svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="8pt" height="14pt" class="svg-formula" dspmath="mathimg" md5hash="527256ea34e0af356380afd605ccefc0"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="gchron-3-371-2021-ie00001.svg" width="8pt" height="14pt" src="gchron-3-371-2021-ie00001.png"/></svg:svg></span></span> <span class="inline-formula"><sup>90</sup></span>Y beta source used in most
luminescence readers is a laboratory key parameter. There is a
well-established body of knowledge about parameters controlling accuracy and
precision of the calibration value but some hard-to-explain inconsistencies
still exist. Here, we have investigated the impact of grain size, aliquot
size and irradiation geometry on the resulting calibration value through
experiments and simulations. The resulting data indicate that the dose rate
of an individual beta source results from the interplay of a number of
parameters, most of which are well established by previous studies. Our
study provides evidence for the impact of aliquot size on the absorbed dose
in particular for grain sizes of 50–200 <span class="inline-formula">µ</span>m. For this grain-size
fraction, the absorbed dose is enhanced by <span class="inline-formula">∼</span> 10 %–20 % as
aliquot size decreases due to the radial increase of dose rate towards
the centre of the aliquot. The enhancement is most variable for 50–100 <span class="inline-formula">µ</span>m
grains mounted as aliquots of <span class="inline-formula"><</span> 8 mm size. The enhancement is
reversed when large grains are mounted as small aliquots due to the edge
effect by which the dose induced by backscattered electrons is reduced.
While the build-up of charge dictates the increase of absorbed dose with the
increase of grain size, this principle becomes more variable with changing
irradiation geometry. We conclude that future calibration samples should
consist of subsamples composed of small, medium, large and very large quartz
grains, each obtaining several gamma doses. The calibration value measured
with small, medium and large aliquots is then obtained from the inverse
slope of the fitted line, not from a single data point. In this way, all
possible irradiation geometries of an individual beta source are covered,
and the precision of the calibration is improved.</p> |
url |
https://gchron.copernicus.org/articles/3/371/2021/gchron-3-371-2021.pdf |
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