author_facet Behn, U.
Thamm, A.
Brandt, O.
Grahn, H. T.
Behn, U.
Thamm, A.
Brandt, O.
Grahn, H. T.
author Behn, U.
Thamm, A.
Brandt, O.
Grahn, H. T.
spellingShingle Behn, U.
Thamm, A.
Brandt, O.
Grahn, H. T.
Journal of Applied Physics
Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
General Physics and Astronomy
author_sort behn, u.
spelling Behn, U. Thamm, A. Brandt, O. Grahn, H. T. 0021-8979 1089-7550 AIP Publishing General Physics and Astronomy http://dx.doi.org/10.1063/1.1412828 <jats:p>The amplitude and the signal-to-noise ratio of photoreflectance (PR) spectra are experimentally and theoretically investigated as a function of the pump and probe intensity. The model calculations of the PR amplitude and the signal-to-noise ratio based on a simple transport model taking the shot noise of the photodetector as the only noise source confirm the experimentally observed dependencies. Increasing the probe light intensity leads to a decrease of the absolute PR background noise. At the same time, the PR amplitude decreases. This may, in particular for comparable probe and pump intensities, result in a decrease of the signal-to-noise ratio.</jats:p> Optimization of the signal-to-noise ratio for photoreflectance spectroscopy Journal of Applied Physics
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title Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_unstemmed Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_full Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_fullStr Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_full_unstemmed Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_short Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_sort optimization of the signal-to-noise ratio for photoreflectance spectroscopy
topic General Physics and Astronomy
url http://dx.doi.org/10.1063/1.1412828
publishDate 2001
physical 5081-5085
description <jats:p>The amplitude and the signal-to-noise ratio of photoreflectance (PR) spectra are experimentally and theoretically investigated as a function of the pump and probe intensity. The model calculations of the PR amplitude and the signal-to-noise ratio based on a simple transport model taking the shot noise of the photodetector as the only noise source confirm the experimentally observed dependencies. Increasing the probe light intensity leads to a decrease of the absolute PR background noise. At the same time, the PR amplitude decreases. This may, in particular for comparable probe and pump intensities, result in a decrease of the signal-to-noise ratio.</jats:p>
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author Behn, U., Thamm, A., Brandt, O., Grahn, H. T.
author_facet Behn, U., Thamm, A., Brandt, O., Grahn, H. T., Behn, U., Thamm, A., Brandt, O., Grahn, H. T.
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container_issue 10
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description <jats:p>The amplitude and the signal-to-noise ratio of photoreflectance (PR) spectra are experimentally and theoretically investigated as a function of the pump and probe intensity. The model calculations of the PR amplitude and the signal-to-noise ratio based on a simple transport model taking the shot noise of the photodetector as the only noise source confirm the experimentally observed dependencies. Increasing the probe light intensity leads to a decrease of the absolute PR background noise. At the same time, the PR amplitude decreases. This may, in particular for comparable probe and pump intensities, result in a decrease of the signal-to-noise ratio.</jats:p>
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spelling Behn, U. Thamm, A. Brandt, O. Grahn, H. T. 0021-8979 1089-7550 AIP Publishing General Physics and Astronomy http://dx.doi.org/10.1063/1.1412828 <jats:p>The amplitude and the signal-to-noise ratio of photoreflectance (PR) spectra are experimentally and theoretically investigated as a function of the pump and probe intensity. The model calculations of the PR amplitude and the signal-to-noise ratio based on a simple transport model taking the shot noise of the photodetector as the only noise source confirm the experimentally observed dependencies. Increasing the probe light intensity leads to a decrease of the absolute PR background noise. At the same time, the PR amplitude decreases. This may, in particular for comparable probe and pump intensities, result in a decrease of the signal-to-noise ratio.</jats:p> Optimization of the signal-to-noise ratio for photoreflectance spectroscopy Journal of Applied Physics
spellingShingle Behn, U., Thamm, A., Brandt, O., Grahn, H. T., Journal of Applied Physics, Optimization of the signal-to-noise ratio for photoreflectance spectroscopy, General Physics and Astronomy
title Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_full Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_fullStr Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_full_unstemmed Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_short Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_sort optimization of the signal-to-noise ratio for photoreflectance spectroscopy
title_unstemmed Optimization of the signal-to-noise ratio for photoreflectance spectroscopy
topic General Physics and Astronomy
url http://dx.doi.org/10.1063/1.1412828