New results for radiative proton capture on 16O at astrophysical energies
The possibility of description of the experimental data for the astrophysical S -factor of the proton radiative capture on 16 O to the ground and first excited states of 17 F was considered in the frame of the modified potential cluster model with forbidden states and classification of the states ac...
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| Veröffentlicht in: | Indian journal of physics 2018-08, Vol.92 (8), p.947-953 |
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| container_title | Indian journal of physics |
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| creator | Dubovichenko, Sergey Dzhazairov-Kakhramanov, Albert |
| description | The possibility of description of the experimental data for the astrophysical
S
-factor of the proton radiative capture on
16
O to the ground and first excited states of
17
F was considered in the frame of the modified potential cluster model with forbidden states and classification of the states according to Young tableaux. It was shown that on the basis of the
E
1 transitions from the
P
states of p
16
O scattering to the bound states of
17
F in the p
16
O channel, it generally succeeded in explaining the values of total cross sections, astrophysical
S
-factor from 10 keV and reaction rate at temperatures from 0.01 to 5 T
9
. |
| doi_str_mv | 10.1007/s12648-018-1190-8 |
| format | Article |
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S
-factor of the proton radiative capture on
16
O to the ground and first excited states of
17
F was considered in the frame of the modified potential cluster model with forbidden states and classification of the states according to Young tableaux. It was shown that on the basis of the
E
1 transitions from the
P
states of p
16
O scattering to the bound states of
17
F in the p
16
O channel, it generally succeeded in explaining the values of total cross sections, astrophysical
S
-factor from 10 keV and reaction rate at temperatures from 0.01 to 5 T
9
.</description><identifier>ISSN: 0973-1458</identifier><identifier>EISSN: 0974-9845</identifier><identifier>DOI: 10.1007/s12648-018-1190-8</identifier><language>eng</language><publisher>New Delhi: Springer India</publisher><subject>Astrophysics ; Astrophysics and Astroparticles ; Nuclear physics ; Original Paper ; Physics ; Physics and Astronomy ; Protons ; Radiation</subject><ispartof>Indian journal of physics, 2018-08, Vol.92 (8), p.947-953</ispartof><rights>Indian Association for the Cultivation of Science 2018</rights><rights>Indian Journal of Physics is a copyright of Springer, (2018). All Rights Reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c1618-7ac68964d4922314028996614a4cc58122cdecbfbd4ded7195b59414b09e5f1a3</citedby><cites>FETCH-LOGICAL-c1618-7ac68964d4922314028996614a4cc58122cdecbfbd4ded7195b59414b09e5f1a3</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/s12648-018-1190-8$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s12648-018-1190-8$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Dubovichenko, Sergey</creatorcontrib><creatorcontrib>Dzhazairov-Kakhramanov, Albert</creatorcontrib><title>New results for radiative proton capture on 16O at astrophysical energies</title><title>Indian journal of physics</title><addtitle>Indian J Phys</addtitle><description>The possibility of description of the experimental data for the astrophysical
S
-factor of the proton radiative capture on
16
O to the ground and first excited states of
17
F was considered in the frame of the modified potential cluster model with forbidden states and classification of the states according to Young tableaux. It was shown that on the basis of the
E
1 transitions from the
P
states of p
16
O scattering to the bound states of
17
F in the p
16
O channel, it generally succeeded in explaining the values of total cross sections, astrophysical
S
-factor from 10 keV and reaction rate at temperatures from 0.01 to 5 T
9
.</description><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Nuclear physics</subject><subject>Original Paper</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Protons</subject><subject>Radiation</subject><issn>0973-1458</issn><issn>0974-9845</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>8G5</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNp1kDFPwzAUhC0EEqXwA9gsMRv8HNuxR1QBrVTRBWbLcZySqiTBdkD997gEiYnp3XB37_QhdA30Figt7yIwyRWhoAiApkSdoBnVJSdacXH6owsCXKhzdBHjjlKpoRQztHr2Xzj4OO5TxE0fcLB1a1P76fEQ-tR32NkhjcHjLEFusE3YxhT64e0QW2f32Hc-bFsfL9FZY_fRX_3eOXp9fHhZLMl687Ra3K-JA5nXldZJpSWvuWasAE6Z0lpK4JY7JxQw5mrvqqaqee3rErSohObAK6q9aMAWc3Qz9eZ9H6OPyez6MXT5pWG5rBAZh8wumFwu9DEG35ghtO82HAxQcyRmJmImEzNHYkblDJsyMXu7rQ9_zf-HvgHNiG0u</recordid><startdate>20180801</startdate><enddate>20180801</enddate><creator>Dubovichenko, Sergey</creator><creator>Dzhazairov-Kakhramanov, Albert</creator><general>Springer India</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>04Q</scope><scope>04W</scope><scope>3V.</scope><scope>7U5</scope><scope>7XB</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>8G5</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>M2O</scope><scope>MBDVC</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>Q9U</scope></search><sort><creationdate>20180801</creationdate><title>New results for radiative proton capture on 16O at astrophysical energies</title><author>Dubovichenko, Sergey ; Dzhazairov-Kakhramanov, Albert</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1618-7ac68964d4922314028996614a4cc58122cdecbfbd4ded7195b59414b09e5f1a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Astrophysics</topic><topic>Astrophysics and Astroparticles</topic><topic>Nuclear physics</topic><topic>Original Paper</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Protons</topic><topic>Radiation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dubovichenko, Sergey</creatorcontrib><creatorcontrib>Dzhazairov-Kakhramanov, Albert</creatorcontrib><collection>CrossRef</collection><collection>India Database</collection><collection>India Database: Science & Technology</collection><collection>ProQuest Central (Corporate)</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>Research Library (Alumni Edition)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Research Library Prep</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Research Library</collection><collection>Research Library (Corporate)</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>ProQuest Central Basic</collection><jtitle>Indian journal of physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dubovichenko, Sergey</au><au>Dzhazairov-Kakhramanov, Albert</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>New results for radiative proton capture on 16O at astrophysical energies</atitle><jtitle>Indian journal of physics</jtitle><stitle>Indian J Phys</stitle><date>2018-08-01</date><risdate>2018</risdate><volume>92</volume><issue>8</issue><spage>947</spage><epage>953</epage><pages>947-953</pages><issn>0973-1458</issn><eissn>0974-9845</eissn><abstract>The possibility of description of the experimental data for the astrophysical
S
-factor of the proton radiative capture on
16
O to the ground and first excited states of
17
F was considered in the frame of the modified potential cluster model with forbidden states and classification of the states according to Young tableaux. It was shown that on the basis of the
E
1 transitions from the
P
states of p
16
O scattering to the bound states of
17
F in the p
16
O channel, it generally succeeded in explaining the values of total cross sections, astrophysical
S
-factor from 10 keV and reaction rate at temperatures from 0.01 to 5 T
9
.</abstract><cop>New Delhi</cop><pub>Springer India</pub><doi>10.1007/s12648-018-1190-8</doi><tpages>7</tpages></addata></record> |
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| ispartof | Indian journal of physics, 2018-08, Vol.92 (8), p.947-953 |
| issn | 0973-1458 0974-9845 |
| language | eng |
| recordid | cdi_proquest_journals_2028350076 |
| source | SpringerNature Journals |
| subjects | Astrophysics Astrophysics and Astroparticles Nuclear physics Original Paper Physics Physics and Astronomy Protons Radiation |
| title | New results for radiative proton capture on 16O at astrophysical energies |
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