Carrier behavior in the vicinity of pit defects in GaN characterized by ultraviolet light-assisted Kelvin probe force microscopy
Surface potentials in the vicinity of V-pits (cone bottom) and U-pits (blunt bottom) on epitaxial GaN surface have been systematically studied using ultraviolet (UV) light-assisted Kelvin probe force microscopy (KPFM). The band structure models are established to understand variation of the surface...
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Veröffentlicht in: | Science China. Physics, mechanics & astronomy mechanics & astronomy, 2019-06, Vol.62 (6), p.67311, Article 67311 |
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container_title | Science China. Physics, mechanics & astronomy |
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creator | Kai, CuiHong Sun, XiaoJuan Jia, YuPing Shi, ZhiMing Jiang, Ke Ben, JianWei Wu, You Wang, Yong Liu, HeNan Li, XiaoHang Li, DaBing |
description | Surface potentials in the vicinity of V-pits (cone bottom) and U-pits (blunt bottom) on epitaxial GaN surface have been systematically studied using ultraviolet (UV) light-assisted Kelvin probe force microscopy (KPFM). The band structure models are established to understand variation of the surface potentials at the pits and planar surface with and without UV light. The photo-generated carrier behavior at the pit defects is studied. According to the surface potential results, it can be deduced that the carrier distributions around the V- and U-pits are uneven. In dark, the electron concentration at the bottom of V-pit (30
n
0
) and Upit (15
n
0
) are higher than that at planar surface (
n
0
). Under UV light, for V-pit, the electron concentration at the cone bottom (4.93×10
11
n
0
) is lower than that at the surrounding planar surface (5.68×10
13
n
0
). For U-pit, the electron concentration at the blunt bottom is 1.35×10
12
n
0
, which is lower than that at the surrounding planar surface (6.13×10
13
n
0
). The non-equilibrium electron concentrations at different locations are calculated. Based on the non-equilibrium electron concentration, it can be concluded that the carrier recombination rate at pit defects is higher than that at planar surface. |
doi_str_mv | 10.1007/s11433-018-9320-x |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2918580189</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2918580189</sourcerecordid><originalsourceid>FETCH-LOGICAL-c316t-c238a8121ff263f698abb8411348595bc22474d49b1f36bd6a2df57c11ad961d3</originalsourceid><addsrcrecordid>eNp1UDtPwzAQjhBIVKU_gM0SsyFn52GPqIKCqGCB2XIcu3GVJsF2q5aJn46jIDFxy530Pe7uS5JrSG8hTcs7D5BRilNgmFOS4uNZMgNWcAyclOdxLsoMlzRjl8nC-20ai_I0K7NZ8r2UzlntUKUbebC9Q7ZDodHoYJXtbDih3qDBBlRro1XwI7ySr0g10kkVtLNfukbVCe3b4EaDVgfU2k0TsPTe-hDRF90eomxwfaWR6Z3SaGeV673qh9NVcmFk6_Xit8-Tj8eH9-UTXr-tnpf3a6woFAErQplkQMAYUlBTcCarimUA8auc55UiJP5TZ7wCQ4uqLiSpTV4qAFnzAmo6T24m33jG5177ILb93nVxpSAcWM5iejyyYGKN53mnjRic3Ul3EpCKMWsxZS0iW4xZi2PUkEnjI7fbaPfn_L_oB0lng5I</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2918580189</pqid></control><display><type>article</type><title>Carrier behavior in the vicinity of pit defects in GaN characterized by ultraviolet light-assisted Kelvin probe force microscopy</title><source>Alma/SFX Local Collection</source><source>SpringerLink Journals - AutoHoldings</source><creator>Kai, CuiHong ; Sun, XiaoJuan ; Jia, YuPing ; Shi, ZhiMing ; Jiang, Ke ; Ben, JianWei ; Wu, You ; Wang, Yong ; Liu, HeNan ; Li, XiaoHang ; Li, DaBing</creator><creatorcontrib>Kai, CuiHong ; Sun, XiaoJuan ; Jia, YuPing ; Shi, ZhiMing ; Jiang, Ke ; Ben, JianWei ; Wu, You ; Wang, Yong ; Liu, HeNan ; Li, XiaoHang ; Li, DaBing</creatorcontrib><description>Surface potentials in the vicinity of V-pits (cone bottom) and U-pits (blunt bottom) on epitaxial GaN surface have been systematically studied using ultraviolet (UV) light-assisted Kelvin probe force microscopy (KPFM). The band structure models are established to understand variation of the surface potentials at the pits and planar surface with and without UV light. The photo-generated carrier behavior at the pit defects is studied. According to the surface potential results, it can be deduced that the carrier distributions around the V- and U-pits are uneven. In dark, the electron concentration at the bottom of V-pit (30
n
0
) and Upit (15
n
0
) are higher than that at planar surface (
n
0
). Under UV light, for V-pit, the electron concentration at the cone bottom (4.93×10
11
n
0
) is lower than that at the surrounding planar surface (5.68×10
13
n
0
). For U-pit, the electron concentration at the blunt bottom is 1.35×10
12
n
0
, which is lower than that at the surrounding planar surface (6.13×10
13
n
0
). The non-equilibrium electron concentrations at different locations are calculated. Based on the non-equilibrium electron concentration, it can be concluded that the carrier recombination rate at pit defects is higher than that at planar surface.</description><identifier>ISSN: 1674-7348</identifier><identifier>EISSN: 1869-1927</identifier><identifier>DOI: 10.1007/s11433-018-9320-x</identifier><language>eng</language><publisher>Beijing: Science China Press</publisher><subject>Astronomy ; Carrier recombination ; Classical and Continuum Physics ; Defects ; Microscopy ; Observations and Techniques ; Physics ; Physics and Astronomy ; Pits ; Ultraviolet radiation</subject><ispartof>Science China. Physics, mechanics & astronomy, 2019-06, Vol.62 (6), p.67311, Article 67311</ispartof><rights>Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2019</rights><rights>Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2019.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-c238a8121ff263f698abb8411348595bc22474d49b1f36bd6a2df57c11ad961d3</citedby><cites>FETCH-LOGICAL-c316t-c238a8121ff263f698abb8411348595bc22474d49b1f36bd6a2df57c11ad961d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11433-018-9320-x$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11433-018-9320-x$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Kai, CuiHong</creatorcontrib><creatorcontrib>Sun, XiaoJuan</creatorcontrib><creatorcontrib>Jia, YuPing</creatorcontrib><creatorcontrib>Shi, ZhiMing</creatorcontrib><creatorcontrib>Jiang, Ke</creatorcontrib><creatorcontrib>Ben, JianWei</creatorcontrib><creatorcontrib>Wu, You</creatorcontrib><creatorcontrib>Wang, Yong</creatorcontrib><creatorcontrib>Liu, HeNan</creatorcontrib><creatorcontrib>Li, XiaoHang</creatorcontrib><creatorcontrib>Li, DaBing</creatorcontrib><title>Carrier behavior in the vicinity of pit defects in GaN characterized by ultraviolet light-assisted Kelvin probe force microscopy</title><title>Science China. Physics, mechanics & astronomy</title><addtitle>Sci. China Phys. Mech. Astron</addtitle><description>Surface potentials in the vicinity of V-pits (cone bottom) and U-pits (blunt bottom) on epitaxial GaN surface have been systematically studied using ultraviolet (UV) light-assisted Kelvin probe force microscopy (KPFM). The band structure models are established to understand variation of the surface potentials at the pits and planar surface with and without UV light. The photo-generated carrier behavior at the pit defects is studied. According to the surface potential results, it can be deduced that the carrier distributions around the V- and U-pits are uneven. In dark, the electron concentration at the bottom of V-pit (30
n
0
) and Upit (15
n
0
) are higher than that at planar surface (
n
0
). Under UV light, for V-pit, the electron concentration at the cone bottom (4.93×10
11
n
0
) is lower than that at the surrounding planar surface (5.68×10
13
n
0
). For U-pit, the electron concentration at the blunt bottom is 1.35×10
12
n
0
, which is lower than that at the surrounding planar surface (6.13×10
13
n
0
). The non-equilibrium electron concentrations at different locations are calculated. Based on the non-equilibrium electron concentration, it can be concluded that the carrier recombination rate at pit defects is higher than that at planar surface.</description><subject>Astronomy</subject><subject>Carrier recombination</subject><subject>Classical and Continuum Physics</subject><subject>Defects</subject><subject>Microscopy</subject><subject>Observations and Techniques</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Pits</subject><subject>Ultraviolet radiation</subject><issn>1674-7348</issn><issn>1869-1927</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>AFKRA</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp1UDtPwzAQjhBIVKU_gM0SsyFn52GPqIKCqGCB2XIcu3GVJsF2q5aJn46jIDFxy530Pe7uS5JrSG8hTcs7D5BRilNgmFOS4uNZMgNWcAyclOdxLsoMlzRjl8nC-20ai_I0K7NZ8r2UzlntUKUbebC9Q7ZDodHoYJXtbDih3qDBBlRro1XwI7ySr0g10kkVtLNfukbVCe3b4EaDVgfU2k0TsPTe-hDRF90eomxwfaWR6Z3SaGeV673qh9NVcmFk6_Xit8-Tj8eH9-UTXr-tnpf3a6woFAErQplkQMAYUlBTcCarimUA8auc55UiJP5TZ7wCQ4uqLiSpTV4qAFnzAmo6T24m33jG5177ILb93nVxpSAcWM5iejyyYGKN53mnjRic3Ul3EpCKMWsxZS0iW4xZi2PUkEnjI7fbaPfn_L_oB0lng5I</recordid><startdate>20190601</startdate><enddate>20190601</enddate><creator>Kai, CuiHong</creator><creator>Sun, XiaoJuan</creator><creator>Jia, YuPing</creator><creator>Shi, ZhiMing</creator><creator>Jiang, Ke</creator><creator>Ben, JianWei</creator><creator>Wu, You</creator><creator>Wang, Yong</creator><creator>Liu, HeNan</creator><creator>Li, XiaoHang</creator><creator>Li, DaBing</creator><general>Science China Press</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>P5Z</scope><scope>P62</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PTHSS</scope></search><sort><creationdate>20190601</creationdate><title>Carrier behavior in the vicinity of pit defects in GaN characterized by ultraviolet light-assisted Kelvin probe force microscopy</title><author>Kai, CuiHong ; Sun, XiaoJuan ; Jia, YuPing ; Shi, ZhiMing ; Jiang, Ke ; Ben, JianWei ; Wu, You ; Wang, Yong ; Liu, HeNan ; Li, XiaoHang ; Li, DaBing</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c316t-c238a8121ff263f698abb8411348595bc22474d49b1f36bd6a2df57c11ad961d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Astronomy</topic><topic>Carrier recombination</topic><topic>Classical and Continuum Physics</topic><topic>Defects</topic><topic>Microscopy</topic><topic>Observations and Techniques</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Pits</topic><topic>Ultraviolet radiation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kai, CuiHong</creatorcontrib><creatorcontrib>Sun, XiaoJuan</creatorcontrib><creatorcontrib>Jia, YuPing</creatorcontrib><creatorcontrib>Shi, ZhiMing</creatorcontrib><creatorcontrib>Jiang, Ke</creatorcontrib><creatorcontrib>Ben, JianWei</creatorcontrib><creatorcontrib>Wu, You</creatorcontrib><creatorcontrib>Wang, Yong</creatorcontrib><creatorcontrib>Liu, HeNan</creatorcontrib><creatorcontrib>Li, XiaoHang</creatorcontrib><creatorcontrib>Li, DaBing</creatorcontrib><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>Engineering Collection</collection><jtitle>Science China. Physics, mechanics & astronomy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kai, CuiHong</au><au>Sun, XiaoJuan</au><au>Jia, YuPing</au><au>Shi, ZhiMing</au><au>Jiang, Ke</au><au>Ben, JianWei</au><au>Wu, You</au><au>Wang, Yong</au><au>Liu, HeNan</au><au>Li, XiaoHang</au><au>Li, DaBing</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Carrier behavior in the vicinity of pit defects in GaN characterized by ultraviolet light-assisted Kelvin probe force microscopy</atitle><jtitle>Science China. Physics, mechanics & astronomy</jtitle><stitle>Sci. China Phys. Mech. Astron</stitle><date>2019-06-01</date><risdate>2019</risdate><volume>62</volume><issue>6</issue><spage>67311</spage><pages>67311-</pages><artnum>67311</artnum><issn>1674-7348</issn><eissn>1869-1927</eissn><abstract>Surface potentials in the vicinity of V-pits (cone bottom) and U-pits (blunt bottom) on epitaxial GaN surface have been systematically studied using ultraviolet (UV) light-assisted Kelvin probe force microscopy (KPFM). The band structure models are established to understand variation of the surface potentials at the pits and planar surface with and without UV light. The photo-generated carrier behavior at the pit defects is studied. According to the surface potential results, it can be deduced that the carrier distributions around the V- and U-pits are uneven. In dark, the electron concentration at the bottom of V-pit (30
n
0
) and Upit (15
n
0
) are higher than that at planar surface (
n
0
). Under UV light, for V-pit, the electron concentration at the cone bottom (4.93×10
11
n
0
) is lower than that at the surrounding planar surface (5.68×10
13
n
0
). For U-pit, the electron concentration at the blunt bottom is 1.35×10
12
n
0
, which is lower than that at the surrounding planar surface (6.13×10
13
n
0
). The non-equilibrium electron concentrations at different locations are calculated. Based on the non-equilibrium electron concentration, it can be concluded that the carrier recombination rate at pit defects is higher than that at planar surface.</abstract><cop>Beijing</cop><pub>Science China Press</pub><doi>10.1007/s11433-018-9320-x</doi></addata></record> |
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source | Alma/SFX Local Collection; SpringerLink Journals - AutoHoldings |
subjects | Astronomy Carrier recombination Classical and Continuum Physics Defects Microscopy Observations and Techniques Physics Physics and Astronomy Pits Ultraviolet radiation |
title | Carrier behavior in the vicinity of pit defects in GaN characterized by ultraviolet light-assisted Kelvin probe force microscopy |
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