DOI: 10.1126/science.285.5430.983a. (Mg,Fe)SiO <sub>3</sub> -Perovskite Stability and Lower Mantle Conditions

(Mg,Fe)SiO 3 -Perovskite Stability and Lower Mantle Conditions

10.1126/science.285.5430.983a

Crossref journal-article

American Association for the Advancement of Science (AAAS)

Science (221)

Bibliography

Dubrovinsky, L. S., Saxena, S. K., & Rekhi, S. (1999). (Mg,Fe)SiO 3 -Perovskite Stability and Lower Mantle Conditions. Science, 285(5430), 983â983.

Authors 3

L. S. Dubrovinsky (first)
S. K. Saxena (additional)
S. Rekhi (additional)

References 48 Referenced 8

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A. Chopelas and R. Boehler in High Pressure Research: Application to Earth and Planetary Science Y. Syano and M. Manghnani Eds. (Terra Tokyo 1992) pp. 101–108; M. Eremets High Pressure Experimental Methods (Oxford Univ. Press Oxford 1996).
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In (13) it is stated “the only indication of the presence of perovskite is a broad band near 800 cm −1 which is frequently observed for (Mg Fe)SiO 3 -perovskites.” While this band does not correspond to any major Raman peaks of perovskite it is common for 6-coordinated silicon in silica.
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Dates

Type	When
Created	23 years ago (July 27, 2002, 5:42 a.m.)
Deposited	1 year, 7 months ago (Jan. 13, 2024, 3:59 a.m.)
Indexed	1 year, 6 months ago (Feb. 6, 2024, 10:23 a.m.)
Issued	26 years ago (Aug. 13, 1999)
Published	26 years ago (Aug. 13, 1999)
Published Print	26 years ago (Aug. 13, 1999)

Funders 0

None

BibTeX

@article{Dubrovinsky_1999, title={(Mg,Fe)SiO 3 -Perovskite Stability and Lower Mantle Conditions}, volume={285}, ISSN={1095-9203}, url={http://dx.doi.org/10.1126/science.285.5430.983a}, DOI={10.1126/science.285.5430.983a}, number={5430}, journal={Science}, publisher={American Association for the Advancement of Science (AAAS)}, author={Dubrovinsky, L. S. and Saxena, S. K. and Rekhi, S.}, year={1999}, month=aug, pages={983–983} }

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