Mass-spectrometric investigations of gas evolution

Method of mass-spectrometry with time-of-flight recording of the desorbed products was used to study the gas evolution of impurities from the subsurface layer of Si crystals molten by the electron beam (of ~2 mm² area) in the vacuum of 10⁻⁵ – 10⁻⁷ Pa. It is shown that irrespective of vacuum level, o...

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Дата:2006
Автори: Asnis, Yu.A., Baranskii, P.I., Babich, V.M., Zabolotin, S.P., Ptushinskii, Yu.G., Sukretnyi, V.G.
Формат: Стаття
Мова:English
Опубліковано: Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України 2006
Назва видання:Semiconductor Physics Quantum Electronics & Optoelectronics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/121441
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Mass-spectrometric investigations of gas evolution / Yu.A. Asnis, P.I. Baranskii, V.M. Babich, S.P. Zabolotin, Yu.G. Ptushinskii, V.G. Sukretnyi // Semiconductor Physics Quantum Electronics & Optoelectronics. — 2006. — Т. 9, № 2. — С. 4-7. — Бібліогр.: 6 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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spelling irk-123456789-1214412017-06-15T03:05:43Z Mass-spectrometric investigations of gas evolution Asnis, Yu.A. Baranskii, P.I. Babich, V.M. Zabolotin, S.P. Ptushinskii, Yu.G. Sukretnyi, V.G. Method of mass-spectrometry with time-of-flight recording of the desorbed products was used to study the gas evolution of impurities from the subsurface layer of Si crystals molten by the electron beam (of ~2 mm² area) in the vacuum of 10⁻⁵ – 10⁻⁷ Pa. It is shown that irrespective of vacuum level, oxygen (m = 32) and hydrogen (m = 2) in the molecular state as well as Si atoms (m = 28) are registered as the main components of gas evolution in the mass-spectrum in melting. With longer time of the subsurface layer exposure in the molten state, an indication of CO evolution (fragment peak m = 12) appears in the mass-spectrum. There is, however, a ground to believe that this is the consequence of gas evolution from the fixtures, and not from the Si sample. Features of gas evolution were revealed at the initial stage of heating and melting of Si sample, depending on the previous heat-treatment of the sample. If melting the subsurface zone proceeds after contact with the atmosphere, initial peaks of evolution of oxygen and hydrogen molecules and Si atoms are observed. These are partially weakened with further keeping the sample in the molten state. In our opinion, such a peak is due to contamination of the surface at such a contact. A long-term exposure in vacuum of a sample cooled after melting does not lead to appearance of the above peak at subsequent melting. 2006 Article Mass-spectrometric investigations of gas evolution / Yu.A. Asnis, P.I. Baranskii, V.M. Babich, S.P. Zabolotin, Yu.G. Ptushinskii, V.G. Sukretnyi // Semiconductor Physics Quantum Electronics & Optoelectronics. — 2006. — Т. 9, № 2. — С. 4-7. — Бібліогр.: 6 назв. — англ. 1560-8034 PACS 81.05.Cy http://dspace.nbuv.gov.ua/handle/123456789/121441 en Semiconductor Physics Quantum Electronics & Optoelectronics Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description Method of mass-spectrometry with time-of-flight recording of the desorbed products was used to study the gas evolution of impurities from the subsurface layer of Si crystals molten by the electron beam (of ~2 mm² area) in the vacuum of 10⁻⁵ – 10⁻⁷ Pa. It is shown that irrespective of vacuum level, oxygen (m = 32) and hydrogen (m = 2) in the molecular state as well as Si atoms (m = 28) are registered as the main components of gas evolution in the mass-spectrum in melting. With longer time of the subsurface layer exposure in the molten state, an indication of CO evolution (fragment peak m = 12) appears in the mass-spectrum. There is, however, a ground to believe that this is the consequence of gas evolution from the fixtures, and not from the Si sample. Features of gas evolution were revealed at the initial stage of heating and melting of Si sample, depending on the previous heat-treatment of the sample. If melting the subsurface zone proceeds after contact with the atmosphere, initial peaks of evolution of oxygen and hydrogen molecules and Si atoms are observed. These are partially weakened with further keeping the sample in the molten state. In our opinion, such a peak is due to contamination of the surface at such a contact. A long-term exposure in vacuum of a sample cooled after melting does not lead to appearance of the above peak at subsequent melting.
format Article
author Asnis, Yu.A.
Baranskii, P.I.
Babich, V.M.
Zabolotin, S.P.
Ptushinskii, Yu.G.
Sukretnyi, V.G.
spellingShingle Asnis, Yu.A.
Baranskii, P.I.
Babich, V.M.
Zabolotin, S.P.
Ptushinskii, Yu.G.
Sukretnyi, V.G.
Mass-spectrometric investigations of gas evolution
Semiconductor Physics Quantum Electronics & Optoelectronics
author_facet Asnis, Yu.A.
Baranskii, P.I.
Babich, V.M.
Zabolotin, S.P.
Ptushinskii, Yu.G.
Sukretnyi, V.G.
author_sort Asnis, Yu.A.
title Mass-spectrometric investigations of gas evolution
title_short Mass-spectrometric investigations of gas evolution
title_full Mass-spectrometric investigations of gas evolution
title_fullStr Mass-spectrometric investigations of gas evolution
title_full_unstemmed Mass-spectrometric investigations of gas evolution
title_sort mass-spectrometric investigations of gas evolution
publisher Інститут фізики напівпровідників імені В.Є. Лашкарьова НАН України
publishDate 2006
url http://dspace.nbuv.gov.ua/handle/123456789/121441
citation_txt Mass-spectrometric investigations of gas evolution / Yu.A. Asnis, P.I. Baranskii, V.M. Babich, S.P. Zabolotin, Yu.G. Ptushinskii, V.G. Sukretnyi // Semiconductor Physics Quantum Electronics & Optoelectronics. — 2006. — Т. 9, № 2. — С. 4-7. — Бібліогр.: 6 назв. — англ.
series Semiconductor Physics Quantum Electronics & Optoelectronics
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first_indexed 2023-10-18T20:39:27Z
last_indexed 2023-10-18T20:39:27Z
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