Term energies and radiative atomic data of carbon-like ions Na VI and Al VIII
Excitation energies belonging to the (1 s 2 )2 s 2 2 p 2 , 2 s 2 2 p 3 p , 2 s 2 p 3 , 2 s 2 2 p 3 s , and 2 s 2 2 p 3 d configurations of carbon-like Na VI and Al VIII have been calculated with the multi-configuration Rayleigh–Ritz variation method and restricted variation method, as well as wavele...
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Veröffentlicht in: | Indian journal of physics 2024-05, Vol.98 (5), p.1561-1572 |
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container_title | Indian journal of physics |
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creator | Sun, Yan Hu, Feng Chen, Qing Chen, Yunlong Liu, Dongdong Chen, Xuanshi Shi, Zhe Liu, Xi Liu, Yan Du, Wenyuan Sang, Cuicui |
description | Excitation energies belonging to the (1
s
2
)2
s
2
2
p
2
, 2
s
2
2
p
3
p
, 2
s
2
p
3
, 2
s
2
2
p
3
s
, and 2
s
2
2
p
3
d
configurations of carbon-like Na VI and Al VIII have been calculated with the multi-configuration Rayleigh–Ritz variation method and restricted variation method, as well as wavelengths, line strengths, oscillator strengths, transition rates for electric dipole transitions among these terms. High-accuracy calculations have been performed using a moderate scale of Slater basis function and accurate treatments of relativity, electron correlation, and quantum electrodynamic (QED) effects. The line strengths, transition oscillator strengths, and transition probabilities for the electric dipole transitions are determined. Deviations of line strengths between the length and velocity gauges are discussed, as well as with the experimentally compiled values from the National Institute for Standards and Technology (NIST) and other theoretical data wherever available. Furthermore, the accuracy of each electric dipole transition is assessed. The present results are accurate enough for identification of emission lines involving these terms and are also useful for precise spectral modeling and diagnosing in astrophysical and laboratory plasmas. |
doi_str_mv | 10.1007/s12648-023-02944-0 |
format | Article |
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p
2
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p
, 2
s
2
p
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, and 2
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3
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configurations of carbon-like Na VI and Al VIII have been calculated with the multi-configuration Rayleigh–Ritz variation method and restricted variation method, as well as wavelengths, line strengths, oscillator strengths, transition rates for electric dipole transitions among these terms. High-accuracy calculations have been performed using a moderate scale of Slater basis function and accurate treatments of relativity, electron correlation, and quantum electrodynamic (QED) effects. The line strengths, transition oscillator strengths, and transition probabilities for the electric dipole transitions are determined. Deviations of line strengths between the length and velocity gauges are discussed, as well as with the experimentally compiled values from the National Institute for Standards and Technology (NIST) and other theoretical data wherever available. Furthermore, the accuracy of each electric dipole transition is assessed. The present results are accurate enough for identification of emission lines involving these terms and are also useful for precise spectral modeling and diagnosing in astrophysical and laboratory plasmas.</description><identifier>ISSN: 0973-1458</identifier><identifier>EISSN: 0974-9845</identifier><identifier>DOI: 10.1007/s12648-023-02944-0</identifier><language>eng</language><publisher>New Delhi: Springer India</publisher><subject>Astrophysics and Astroparticles ; Basis functions ; Carbon ; Configurations ; Electric dipoles ; Emission analysis ; Original Paper ; Oscillator strengths ; Oscillators ; Physics ; Physics and Astronomy ; Quantum electrodynamics ; Relativity ; Transition probabilities</subject><ispartof>Indian journal of physics, 2024-05, Vol.98 (5), p.1561-1572</ispartof><rights>Indian Association for the Cultivation of Science 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c319t-40655f436bb82c73809a663d4f1894b316d5a289ecbdf2d7ed3fd1ba2bdcbdcb3</citedby><cites>FETCH-LOGICAL-c319t-40655f436bb82c73809a663d4f1894b316d5a289ecbdf2d7ed3fd1ba2bdcbdcb3</cites><orcidid>0000-0001-8546-4370</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s12648-023-02944-0$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s12648-023-02944-0$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Sun, Yan</creatorcontrib><creatorcontrib>Hu, Feng</creatorcontrib><creatorcontrib>Chen, Qing</creatorcontrib><creatorcontrib>Chen, Yunlong</creatorcontrib><creatorcontrib>Liu, Dongdong</creatorcontrib><creatorcontrib>Chen, Xuanshi</creatorcontrib><creatorcontrib>Shi, Zhe</creatorcontrib><creatorcontrib>Liu, Xi</creatorcontrib><creatorcontrib>Liu, Yan</creatorcontrib><creatorcontrib>Du, Wenyuan</creatorcontrib><creatorcontrib>Sang, Cuicui</creatorcontrib><title>Term energies and radiative atomic data of carbon-like ions Na VI and Al VIII</title><title>Indian journal of physics</title><addtitle>Indian J Phys</addtitle><description>Excitation energies belonging to the (1
s
2
)2
s
2
2
p
2
, 2
s
2
2
p
3
p
, 2
s
2
p
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p
3
s
, and 2
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configurations of carbon-like Na VI and Al VIII have been calculated with the multi-configuration Rayleigh–Ritz variation method and restricted variation method, as well as wavelengths, line strengths, oscillator strengths, transition rates for electric dipole transitions among these terms. High-accuracy calculations have been performed using a moderate scale of Slater basis function and accurate treatments of relativity, electron correlation, and quantum electrodynamic (QED) effects. The line strengths, transition oscillator strengths, and transition probabilities for the electric dipole transitions are determined. Deviations of line strengths between the length and velocity gauges are discussed, as well as with the experimentally compiled values from the National Institute for Standards and Technology (NIST) and other theoretical data wherever available. Furthermore, the accuracy of each electric dipole transition is assessed. The present results are accurate enough for identification of emission lines involving these terms and are also useful for precise spectral modeling and diagnosing in astrophysical and laboratory plasmas.</description><subject>Astrophysics and Astroparticles</subject><subject>Basis functions</subject><subject>Carbon</subject><subject>Configurations</subject><subject>Electric dipoles</subject><subject>Emission analysis</subject><subject>Original Paper</subject><subject>Oscillator strengths</subject><subject>Oscillators</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum electrodynamics</subject><subject>Relativity</subject><subject>Transition probabilities</subject><issn>0973-1458</issn><issn>0974-9845</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNp9kEtLAzEUhYMoWKt_wFXAdTTvSZal-BiouqluQzJJSmo7U5Op4L932hHcCfdyz-Kcc-ED4JrgW4JxdVcIlVwhTNmwmnOET8AE64ojrbg4PWqGCBfqHFyUssZYalKJCXhehryFoQ15lUKBtvUwW59sn74CtH23TQ30trewi7Cx2XUt2qSPAFPXFvhi4Xt9zMw2g6rrS3AW7aaEq987BW8P98v5E1q8Ptbz2QI1jOgecSyFiJxJ5xRtKqawtlIyzyNRmjtGpBeWKh0a5yP1VfAseuIsdb45DJuCm7F3l7vPfSi9WXf73A4vDdWyIoJpxQYXHV1N7krJIZpdTlubvw3B5oDNjNjMgM0csRk8hNgYKoO5XYX8V_1P6gfoaW7B</recordid><startdate>20240501</startdate><enddate>20240501</enddate><creator>Sun, Yan</creator><creator>Hu, Feng</creator><creator>Chen, Qing</creator><creator>Chen, Yunlong</creator><creator>Liu, Dongdong</creator><creator>Chen, Xuanshi</creator><creator>Shi, Zhe</creator><creator>Liu, Xi</creator><creator>Liu, Yan</creator><creator>Du, Wenyuan</creator><creator>Sang, Cuicui</creator><general>Springer India</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0001-8546-4370</orcidid></search><sort><creationdate>20240501</creationdate><title>Term energies and radiative atomic data of carbon-like ions Na VI and Al VIII</title><author>Sun, Yan ; Hu, Feng ; Chen, Qing ; Chen, Yunlong ; Liu, Dongdong ; Chen, Xuanshi ; Shi, Zhe ; Liu, Xi ; Liu, Yan ; Du, Wenyuan ; Sang, Cuicui</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c319t-40655f436bb82c73809a663d4f1894b316d5a289ecbdf2d7ed3fd1ba2bdcbdcb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Astrophysics and Astroparticles</topic><topic>Basis functions</topic><topic>Carbon</topic><topic>Configurations</topic><topic>Electric dipoles</topic><topic>Emission analysis</topic><topic>Original Paper</topic><topic>Oscillator strengths</topic><topic>Oscillators</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum electrodynamics</topic><topic>Relativity</topic><topic>Transition probabilities</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sun, Yan</creatorcontrib><creatorcontrib>Hu, Feng</creatorcontrib><creatorcontrib>Chen, Qing</creatorcontrib><creatorcontrib>Chen, Yunlong</creatorcontrib><creatorcontrib>Liu, Dongdong</creatorcontrib><creatorcontrib>Chen, Xuanshi</creatorcontrib><creatorcontrib>Shi, Zhe</creatorcontrib><creatorcontrib>Liu, Xi</creatorcontrib><creatorcontrib>Liu, Yan</creatorcontrib><creatorcontrib>Du, Wenyuan</creatorcontrib><creatorcontrib>Sang, Cuicui</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Indian journal of physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sun, Yan</au><au>Hu, Feng</au><au>Chen, Qing</au><au>Chen, Yunlong</au><au>Liu, Dongdong</au><au>Chen, Xuanshi</au><au>Shi, Zhe</au><au>Liu, Xi</au><au>Liu, Yan</au><au>Du, Wenyuan</au><au>Sang, Cuicui</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Term energies and radiative atomic data of carbon-like ions Na VI and Al VIII</atitle><jtitle>Indian journal of physics</jtitle><stitle>Indian J Phys</stitle><date>2024-05-01</date><risdate>2024</risdate><volume>98</volume><issue>5</issue><spage>1561</spage><epage>1572</epage><pages>1561-1572</pages><issn>0973-1458</issn><eissn>0974-9845</eissn><abstract>Excitation energies belonging to the (1
s
2
)2
s
2
2
p
2
, 2
s
2
2
p
3
p
, 2
s
2
p
3
, 2
s
2
2
p
3
s
, and 2
s
2
2
p
3
d
configurations of carbon-like Na VI and Al VIII have been calculated with the multi-configuration Rayleigh–Ritz variation method and restricted variation method, as well as wavelengths, line strengths, oscillator strengths, transition rates for electric dipole transitions among these terms. High-accuracy calculations have been performed using a moderate scale of Slater basis function and accurate treatments of relativity, electron correlation, and quantum electrodynamic (QED) effects. The line strengths, transition oscillator strengths, and transition probabilities for the electric dipole transitions are determined. Deviations of line strengths between the length and velocity gauges are discussed, as well as with the experimentally compiled values from the National Institute for Standards and Technology (NIST) and other theoretical data wherever available. Furthermore, the accuracy of each electric dipole transition is assessed. The present results are accurate enough for identification of emission lines involving these terms and are also useful for precise spectral modeling and diagnosing in astrophysical and laboratory plasmas.</abstract><cop>New Delhi</cop><pub>Springer India</pub><doi>10.1007/s12648-023-02944-0</doi><tpages>12</tpages><orcidid>https://orcid.org/0000-0001-8546-4370</orcidid></addata></record> |
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subjects | Astrophysics and Astroparticles Basis functions Carbon Configurations Electric dipoles Emission analysis Original Paper Oscillator strengths Oscillators Physics Physics and Astronomy Quantum electrodynamics Relativity Transition probabilities |
title | Term energies and radiative atomic data of carbon-like ions Na VI and Al VIII |
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