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Spectroscopic features of ultrahigh-pressure impact glasses of the Kara astrobleme
The state of substances under ultrahigh pressures and temperatures (UHPHT) now raises a special interest as a matter existing under extreme conditions and as potential new material. Under laboratory conditions only small amounts of micrometer-sized matter are produced at a pressure up to 100 GPa and...
Autores principales: | , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2018
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5932052/ https://www.ncbi.nlm.nih.gov/pubmed/29720696 http://dx.doi.org/10.1038/s41598-018-25037-z |
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author | Shumilova, T. G. Lutoev, V. P. Isaenko, S. I. Kovalchuk, N. S. Makeev, B. A. Lysiuk, A. Yu. Zubov, A. A. Ernstson, K. |
author_facet | Shumilova, T. G. Lutoev, V. P. Isaenko, S. I. Kovalchuk, N. S. Makeev, B. A. Lysiuk, A. Yu. Zubov, A. A. Ernstson, K. |
author_sort | Shumilova, T. G. |
collection | PubMed |
description | The state of substances under ultrahigh pressures and temperatures (UHPHT) now raises a special interest as a matter existing under extreme conditions and as potential new material. Under laboratory conditions only small amounts of micrometer-sized matter are produced at a pressure up to 100 GPa and at room temperature. Simultaneous combination of ultrahigh pressures and temperatures in a lab still requires serious technological effort. Here we describe the composition and structure of the UHPHT vein-like impact glass discovered by us in 2015 on the territory of the Kara astrobleme (Russia) and compare its properties with impact glass from the Ries crater (Germany). A complex of structural and spectroscopic methods presents unusual high pressure marks of structural elements in 8-fold co-ordination that had been described earlier neither in synthetic nor natural glasses. The Kara natural UHPHT glasses being about 70 Ma old have well preserved initial structure, presenting some heterogeneity as a result of partial liquation and crystallization differentiation where an amorphous component is proposed to originate from low level polymerization. Homogeneous parts of the UHPHT glasses can be used to deepened fundamental investigation of a substance under extreme PT conditions and to technological studies for novel material creations. |
format | Online Article Text |
id | pubmed-5932052 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2018 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-59320522018-05-09 Spectroscopic features of ultrahigh-pressure impact glasses of the Kara astrobleme Shumilova, T. G. Lutoev, V. P. Isaenko, S. I. Kovalchuk, N. S. Makeev, B. A. Lysiuk, A. Yu. Zubov, A. A. Ernstson, K. Sci Rep Article The state of substances under ultrahigh pressures and temperatures (UHPHT) now raises a special interest as a matter existing under extreme conditions and as potential new material. Under laboratory conditions only small amounts of micrometer-sized matter are produced at a pressure up to 100 GPa and at room temperature. Simultaneous combination of ultrahigh pressures and temperatures in a lab still requires serious technological effort. Here we describe the composition and structure of the UHPHT vein-like impact glass discovered by us in 2015 on the territory of the Kara astrobleme (Russia) and compare its properties with impact glass from the Ries crater (Germany). A complex of structural and spectroscopic methods presents unusual high pressure marks of structural elements in 8-fold co-ordination that had been described earlier neither in synthetic nor natural glasses. The Kara natural UHPHT glasses being about 70 Ma old have well preserved initial structure, presenting some heterogeneity as a result of partial liquation and crystallization differentiation where an amorphous component is proposed to originate from low level polymerization. Homogeneous parts of the UHPHT glasses can be used to deepened fundamental investigation of a substance under extreme PT conditions and to technological studies for novel material creations. Nature Publishing Group UK 2018-05-02 /pmc/articles/PMC5932052/ /pubmed/29720696 http://dx.doi.org/10.1038/s41598-018-25037-z Text en © The Author(s) 2018 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/. |
spellingShingle | Article Shumilova, T. G. Lutoev, V. P. Isaenko, S. I. Kovalchuk, N. S. Makeev, B. A. Lysiuk, A. Yu. Zubov, A. A. Ernstson, K. Spectroscopic features of ultrahigh-pressure impact glasses of the Kara astrobleme |
title | Spectroscopic features of ultrahigh-pressure impact glasses of the Kara astrobleme |
title_full | Spectroscopic features of ultrahigh-pressure impact glasses of the Kara astrobleme |
title_fullStr | Spectroscopic features of ultrahigh-pressure impact glasses of the Kara astrobleme |
title_full_unstemmed | Spectroscopic features of ultrahigh-pressure impact glasses of the Kara astrobleme |
title_short | Spectroscopic features of ultrahigh-pressure impact glasses of the Kara astrobleme |
title_sort | spectroscopic features of ultrahigh-pressure impact glasses of the kara astrobleme |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5932052/ https://www.ncbi.nlm.nih.gov/pubmed/29720696 http://dx.doi.org/10.1038/s41598-018-25037-z |
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