The pressure and temperature dependent fluorescence line-shift of strontium tetraborate has been measured concurrently with x-ray diffraction from the pressure standards sodium chloride or gold. Temperature was found to have a small effect on the fluorescence line-shift under pressure. We found a maximum pressure uncertainty of ±1.8 GPa at 25 GPa (7.2%) and 857 K when making no temperature correction. The fluorescence line-shifts for ruby, Alexandrite, and samarium-doped yttrium aluminum garnet were also determined, using our strontium tetraborate calibration to determine pressure and a thermocouple to measure temperature. Fluorescence measurements were extended up to 800 K for ruby and Alexandrite. Temperature was found to have a small effect on the fluorescence line-shift of samarium-doped yittrium aluminum garnet. We found a maximum uncertainty of ±2.7 GPa at 25 GPa (11.1%) and 857 K when no temperature correction was applied. We determined equations relating to the fluorescence line position from these data, which include a cross derivative term to account for the combined effect of pressure and temperature. We present a method to independently determine pressure and/or temperature from combined fluorescence line-shift measurements of a pair of optical sensors.
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15 July 2011
Research Article|
July 27 2011
Determination of the variation of the fluorescence line positions of ruby, strontium tetraborate, alexandrite, and samarium-doped yttrium aluminum garnet with pressure and temperature
Selva Vennila Raju;
Selva Vennila Raju
a)
1Earth and Planetary Science,
University of California
, Berkeley, California 94720-4767, USA
2Institute of Geophysics and Planetary Physics,
University of California
, Santa Cruz, California 95064, USA
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Joseph M. Zaug;
Joseph M. Zaug
3
Lawrence Livermore National Laboratory
, P.O. Box 808, L-350, Livermore, California 94551, USA
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Bin Chen;
Bin Chen
1Earth and Planetary Science,
University of California
, Berkeley, California 94720-4767, USA
2Institute of Geophysics and Planetary Physics,
University of California
, Santa Cruz, California 95064, USA
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Jinyuan Yan;
Jinyuan Yan
1Earth and Planetary Science,
University of California
, Berkeley, California 94720-4767, USA
2Institute of Geophysics and Planetary Physics,
University of California
, Santa Cruz, California 95064, USA
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Jason W. Knight;
Jason W. Knight
4
Advanced Light Source, Lawrence Berkeley National Laboratory
, Berkeley, California 94720, USA
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Raymond Jeanloz;
Raymond Jeanloz
1Earth and Planetary Science,
University of California
, Berkeley, California 94720-4767, USA
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Simon M. Clark
Simon M. Clark
1Earth and Planetary Science,
University of California
, Berkeley, California 94720-4767, USA
4
Advanced Light Source, Lawrence Berkeley National Laboratory
, Berkeley, California 94720, USA
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a)
Author to whom correspondence should be addressed. Electronic mail: [email protected]
J. Appl. Phys. 110, 023521 (2011)
Article history
Received:
April 06 2011
Accepted:
May 27 2011
Citation
Selva Vennila Raju, Joseph M. Zaug, Bin Chen, Jinyuan Yan, Jason W. Knight, Raymond Jeanloz, Simon M. Clark; Determination of the variation of the fluorescence line positions of ruby, strontium tetraborate, alexandrite, and samarium-doped yttrium aluminum garnet with pressure and temperature. J. Appl. Phys. 15 July 2011; 110 (2): 023521. https://doi.org/10.1063/1.3608167
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