From optical spectra to phase diagrams — the binary mixture N2–CO
We investigated the T–c% phase diagram of the binary system N2–CO. From changes in IR spectra of all kinds of mode excitations (phonons, vibrons) we were able to determine the temperature of phase transitions (solid–solid, solid–liquid). The improvements in comparison to structural investigations by...
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| Дата: | 2007 |
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| Автори: | , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
2007
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| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/7773 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | From optical spectra to phase diagrams — the binary mixture N2–CO / M. Vetter, A.Brodyanski, H.-J. Jodl // Физика низких температур. — 2007. — Т. 33, № 2. — С. 1383-1392. — Бібліогр.: 18 назв. — англ. |
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Vetter, M. Brodyanski, A. Jodl, H.-J. 2010-04-12T13:14:28Z 2010-04-12T13:14:28Z 2007 From optical spectra to phase diagrams — the binary mixture N2–CO / M. Vetter, A.Brodyanski, H.-J. Jodl // Физика низких температур. — 2007. — Т. 33, № 2. — С. 1383-1392. — Бібліогр.: 18 назв. — англ. 0132-6414 https://nasplib.isofts.kiev.ua/handle/123456789/7773 We investigated the T–c% phase diagram of the binary system N2–CO. From changes in IR spectra of all kinds of mode excitations (phonons, vibrons) we were able to determine the temperature of phase transitions (solid–solid, solid–liquid). The improvements in comparison to structural investigations by x-rays or electrons are the following: sample growing and handling with perfect optical and thermodynamic quality; determination of actual concentration (N2)x(CO)y from optical spectra; reduction of thermal hysteresis by careful cooling–heating cycles of the samples. en Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України Динамика кристаллической решетки From optical spectra to phase diagrams — the binary mixture N2–CO Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
From optical spectra to phase diagrams — the binary mixture N2–CO |
| spellingShingle |
From optical spectra to phase diagrams — the binary mixture N2–CO Vetter, M. Brodyanski, A. Jodl, H.-J. Динамика кристаллической решетки |
| title_short |
From optical spectra to phase diagrams — the binary mixture N2–CO |
| title_full |
From optical spectra to phase diagrams — the binary mixture N2–CO |
| title_fullStr |
From optical spectra to phase diagrams — the binary mixture N2–CO |
| title_full_unstemmed |
From optical spectra to phase diagrams — the binary mixture N2–CO |
| title_sort |
from optical spectra to phase diagrams — the binary mixture n2–co |
| author |
Vetter, M. Brodyanski, A. Jodl, H.-J. |
| author_facet |
Vetter, M. Brodyanski, A. Jodl, H.-J. |
| topic |
Динамика кристаллической решетки |
| topic_facet |
Динамика кристаллической решетки |
| publishDate |
2007 |
| language |
English |
| publisher |
Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України |
| format |
Article |
| description |
We investigated the T–c% phase diagram of the binary system N2–CO. From changes in IR spectra of all kinds of mode excitations (phonons, vibrons) we were able to determine the temperature of phase transitions (solid–solid, solid–liquid). The improvements in comparison to structural investigations by x-rays or electrons are the following: sample growing and handling with perfect optical and thermodynamic quality; determination of actual concentration (N2)x(CO)y from optical spectra; reduction of thermal hysteresis by careful cooling–heating cycles of the samples.
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| issn |
0132-6414 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/7773 |
| citation_txt |
From optical spectra to phase diagrams — the binary mixture N2–CO / M. Vetter, A.Brodyanski, H.-J. Jodl // Физика низких температур. — 2007. — Т. 33, № 2. — С. 1383-1392. — Бібліогр.: 18 назв. — англ. |
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2025-12-07T18:48:22Z |
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