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Please use this identifier to cite or link to this item: http://hdl.handle.net/11375/6479
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dc.contributor.advisorReid, J.en_US
dc.contributor.authorLabrie, Danielen_US
dc.date.accessioned2014-06-18T16:35:34Z-
dc.date.available2014-06-18T16:35:34Z-
dc.date.created2009-07-23en_US
dc.date.issued1980-10en_US
dc.identifier.otheropendissertations/179en_US
dc.identifier.other1435en_US
dc.identifier.other908376en_US
dc.identifier.urihttp://hdl.handle.net/11375/6479-
dc.description.abstract<p>This thesis examines the feasibility of using infrared spectroscopy to carry out radiocarbon dating. Conventional radiocarbon dating techniques are limited in sensitivity by the very small fraction of C¹⁴ atoms which disintegrate during the counting period. Our proposed infrared technique does not suffer from this limitation, but we must overcome the problem of interfering infrared spectra caused by stable isotopes, and develop methods for detecting extremely small infrared absorption coefficients.</p> <p>The apparatus employed consists of a tunable diode laser and a multipass optical cell. Radiocarbon is detected in the form of C¹⁴O₂, and it is shown that interference-free detection can be attained provided the gas sample is cooled to dry ice temperature. To achieve sufficient sensitivity we have developed a second harmonic detection scheme. As part of out optimisation procedure, the experimental and theoretical second harmonic lineshapes were compared over a wide range of experimental conditions. Good agreement was found in all cases.</p> <p>With the present apparatus, the minimum detectable infrared absorption coefficient was ~ 1x10ˉ⁷ mˉ¹. This compares with a sensitivity of ~ 1x10ˉ⁹ mˉ¹ which is required for practical radiocarbon dating. The noise mechanisms which limit the present sensitivity were investigated in some detail, and results obtained at short time constants in small optical cells are extrapolated to long optical cells and measurement times of several hours. Based on these extrapolations, radiocarbon dating by infrared spectroscopy appears feasible, and will require much smaller carbon samples than is required by conventional disintegration counting techniques.</p>en_US
dc.subjectPhysicsen_US
dc.subjectPhysicsen_US
dc.titleStudy of Radiocarbon Detection By laser spectroscopyen_US
dc.typethesisen_US
dc.contributor.departmentPhysicsen_US
dc.description.degreeMaster of Science (MS)en_US
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