Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films
Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. Th...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Kalygina, V. M. [verfasserIn] Almaev, A. V. [verfasserIn] Novikov, V. A. [verfasserIn] Petrova, Yu. S. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020 |
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| Übergeordnetes Werk: |
Enthalten in: Semiconductors - Berlin : Springer Science + Business Media, 1997, 54(2020), 6 vom: Juni, Seite 682-686 |
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| Übergeordnetes Werk: |
volume:54 ; year:2020 ; number:6 ; month:06 ; pages:682-686 |
| Links: |
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| DOI / URN: |
10.1134/S1063782620060093 |
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| Katalog-ID: |
SPR039927679 |
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| 520 | |a Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. | ||
| 700 | 1 | |a Almaev, A. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Novikov, V. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Petrova, Yu. S. |e verfasserin |4 aut | |
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10.1134/S1063782620060093 doi (DE-627)SPR039927679 (SPR)S1063782620060093-e DE-627 ger DE-627 rakwb eng 530 ASE 53.00 bkl 33.00 bkl Kalygina, V. M. verfasserin aut Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. Almaev, A. V. verfasserin aut Novikov, V. A. verfasserin aut Petrova, Yu. S. verfasserin aut Enthalten in Semiconductors Berlin : Springer Science + Business Media, 1997 54(2020), 6 vom: Juni, Seite 682-686 (DE-627)269019103 (DE-600)1473824-7 1090-6479 nnns volume:54 year:2020 number:6 month:06 pages:682-686 https://dx.doi.org/10.1134/S1063782620060093 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 53.00 ASE 33.00 ASE AR 54 2020 6 06 682-686 |
| spelling |
10.1134/S1063782620060093 doi (DE-627)SPR039927679 (SPR)S1063782620060093-e DE-627 ger DE-627 rakwb eng 530 ASE 53.00 bkl 33.00 bkl Kalygina, V. M. verfasserin aut Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. Almaev, A. V. verfasserin aut Novikov, V. A. verfasserin aut Petrova, Yu. S. verfasserin aut Enthalten in Semiconductors Berlin : Springer Science + Business Media, 1997 54(2020), 6 vom: Juni, Seite 682-686 (DE-627)269019103 (DE-600)1473824-7 1090-6479 nnns volume:54 year:2020 number:6 month:06 pages:682-686 https://dx.doi.org/10.1134/S1063782620060093 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 53.00 ASE 33.00 ASE AR 54 2020 6 06 682-686 |
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10.1134/S1063782620060093 doi (DE-627)SPR039927679 (SPR)S1063782620060093-e DE-627 ger DE-627 rakwb eng 530 ASE 53.00 bkl 33.00 bkl Kalygina, V. M. verfasserin aut Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. Almaev, A. V. verfasserin aut Novikov, V. A. verfasserin aut Petrova, Yu. S. verfasserin aut Enthalten in Semiconductors Berlin : Springer Science + Business Media, 1997 54(2020), 6 vom: Juni, Seite 682-686 (DE-627)269019103 (DE-600)1473824-7 1090-6479 nnns volume:54 year:2020 number:6 month:06 pages:682-686 https://dx.doi.org/10.1134/S1063782620060093 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 53.00 ASE 33.00 ASE AR 54 2020 6 06 682-686 |
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10.1134/S1063782620060093 doi (DE-627)SPR039927679 (SPR)S1063782620060093-e DE-627 ger DE-627 rakwb eng 530 ASE 53.00 bkl 33.00 bkl Kalygina, V. M. verfasserin aut Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. Almaev, A. V. verfasserin aut Novikov, V. A. verfasserin aut Petrova, Yu. S. verfasserin aut Enthalten in Semiconductors Berlin : Springer Science + Business Media, 1997 54(2020), 6 vom: Juni, Seite 682-686 (DE-627)269019103 (DE-600)1473824-7 1090-6479 nnns volume:54 year:2020 number:6 month:06 pages:682-686 https://dx.doi.org/10.1134/S1063782620060093 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 53.00 ASE 33.00 ASE AR 54 2020 6 06 682-686 |
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10.1134/S1063782620060093 doi (DE-627)SPR039927679 (SPR)S1063782620060093-e DE-627 ger DE-627 rakwb eng 530 ASE 53.00 bkl 33.00 bkl Kalygina, V. M. verfasserin aut Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. Almaev, A. V. verfasserin aut Novikov, V. A. verfasserin aut Petrova, Yu. S. verfasserin aut Enthalten in Semiconductors Berlin : Springer Science + Business Media, 1997 54(2020), 6 vom: Juni, Seite 682-686 (DE-627)269019103 (DE-600)1473824-7 1090-6479 nnns volume:54 year:2020 number:6 month:06 pages:682-686 https://dx.doi.org/10.1134/S1063782620060093 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 53.00 ASE 33.00 ASE AR 54 2020 6 06 682-686 |
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Kalygina, V. M. |
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Kalygina, V. M. ddc 530 bkl 53.00 bkl 33.00 Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films |
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530 ASE 53.00 bkl 33.00 bkl Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films |
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ddc 530 bkl 53.00 bkl 33.00 |
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Elektronische Aufsätze Aufsätze Elektronische Ressource |
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Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films |
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(DE-627)SPR039927679 (SPR)S1063782620060093-e |
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Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films |
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Kalygina, V. M. |
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Kalygina, V. M. Almaev, A. V. Novikov, V. A. Petrova, Yu. S. |
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Elektronische Aufsätze |
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Kalygina, V. M. |
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10.1134/S1063782620060093 |
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530 |
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verfasserin |
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solar-blind uv detectors based on β-$ ga_{2} %$ o_{3} $ films |
| title_auth |
Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films |
| abstract |
Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. |
| abstractGer |
Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. |
| abstract_unstemmed |
Abstract Resistive-type structures based on gallium-oxide films are studied. The $ Ga_{2} %$ O_{3} $ films are produced by radio-frequency magnetron-assisted sputtering of a β-$ Ga_{2} %$ O_{3} $ (99.9999%) target onto unheated sapphire substrates with preliminarily deposited platinum electrodes. The data on the structure and phase composition of the films are obtained immediately after sputtering and after annealing in argon at 900°C for 30 min. The current–voltage characteristics are recorded in the dark and upon exposure to radiation at the wavelength λ = 254 nm. It is shown that, after annealing, the photocurrent increases by an order of magnitude. The lack of sensitivity of the structures to radiation in the visible wavelength region (λ = 400 nm) is verified experimentally. |
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Solar-Blind UV Detectors Based on β-$ Ga_{2} %$ O_{3} $ Films |
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Almaev, A. V. Novikov, V. A. Petrova, Yu. S. |
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10.1134/S1063782620060093 |
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2024-07-04T02:10:43.829Z |
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