Potential cluster calculations for the astrophysical S-factor and reaction rate of the radiative 3He(4He,γ)7Be capture
In the frame of a modified potential cluster model based on the classification of orbital states according to Young diagrams and revised interaction potential parameters for the bound states of 7 Be in the 3 He 4 He cluster model with forbidden states, the astrophysical S -factor for the radiative c...
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| Veröffentlicht in: | Indian journal of physics 2019-03, Vol.93 (3), p.279-283 |
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| container_title | Indian journal of physics |
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| creator | Dubovichenko, S. B. Burkova, N. A. Dzhazairov-Kakhramanov, A. V. |
| description | In the frame of a modified potential cluster model based on the classification of orbital states according to Young diagrams and revised interaction potential parameters for the bound states of
7
Be in the
3
He
4
He cluster model with forbidden states, the astrophysical
S
-factor for the radiative capture reaction
3
He(
4
He,γ)
7
Be has been calculated from 10 keV. The result obtained,
S
(23 keV) = 0.561 keV·b, reproduces the latest experimental data at 23 keV. The calculated and parametrized reaction rate is compared with some known results in the range of temperatures from 0.05 to 5
T
9
. |
| doi_str_mv | 10.1007/s12648-018-1287-0 |
| format | Article |
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7
Be in the
3
He
4
He cluster model with forbidden states, the astrophysical
S
-factor for the radiative capture reaction
3
He(
4
He,γ)
7
Be has been calculated from 10 keV. The result obtained,
S
(23 keV) = 0.561 keV·b, reproduces the latest experimental data at 23 keV. The calculated and parametrized reaction rate is compared with some known results in the range of temperatures from 0.05 to 5
T
9
.</description><identifier>ISSN: 0973-1458</identifier><identifier>EISSN: 0974-9845</identifier><identifier>DOI: 10.1007/s12648-018-1287-0</identifier><language>eng</language><publisher>New Delhi: Springer India</publisher><subject>Astrophysics and Astroparticles ; Clusters ; Interaction parameters ; Mathematical models ; Original Paper ; Physics ; Physics and Astronomy</subject><ispartof>Indian journal of physics, 2019-03, Vol.93 (3), p.279-283</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-c246t-d2cc6f3e6d1d27242ce5d7ca62ae39eccd2600a9918208bcdaaf95c1b46a511a3</citedby><cites>FETCH-LOGICAL-c246t-d2cc6f3e6d1d27242ce5d7ca62ae39eccd2600a9918208bcdaaf95c1b46a511a3</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/s12648-018-1287-0$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s12648-018-1287-0$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Dubovichenko, S. B.</creatorcontrib><creatorcontrib>Burkova, N. A.</creatorcontrib><creatorcontrib>Dzhazairov-Kakhramanov, A. V.</creatorcontrib><title>Potential cluster calculations for the astrophysical S-factor and reaction rate of the radiative 3He(4He,γ)7Be capture</title><title>Indian journal of physics</title><addtitle>Indian J Phys</addtitle><description>In the frame of a modified potential cluster model based on the classification of orbital states according to Young diagrams and revised interaction potential parameters for the bound states of
7
Be in the
3
He
4
He cluster model with forbidden states, the astrophysical
S
-factor for the radiative capture reaction
3
He(
4
He,γ)
7
Be has been calculated from 10 keV. The result obtained,
S
(23 keV) = 0.561 keV·b, reproduces the latest experimental data at 23 keV. The calculated and parametrized reaction rate is compared with some known results in the range of temperatures from 0.05 to 5
T
9
.</description><subject>Astrophysics and Astroparticles</subject><subject>Clusters</subject><subject>Interaction parameters</subject><subject>Mathematical models</subject><subject>Original Paper</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><issn>0973-1458</issn><issn>0974-9845</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</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>eNp1kFFLwzAUhYsoOKc_wLeALwpGk7RN00cd6oSBgvoc7pJb11HbmaTKfpf_w99ktgo--XQPnO-cCydJjjm74IwVl54LmSnKuKJcqIKynWTEyiKjpcry3a1OKc9ytZ8ceL9kTJa8yEfJ52MXsA01NMQ0vQ_oiIHG9A2Eums9qTpHwgIJ-OC61WLt62iTJ1qBCdGC1hKHUUeYOAhIumrLO7B1rPhAkk7xNJvi-ffXWXGNsX0VeoeHyV4Fjcej3ztOXm5vnidTOnu4u59czagRmQzUCmNklaK03IpCZMJgbgsDUgCmJRpjhWQMypIrwdTcWICqzA2fZxJyziEdJydD78p17z36oJdd79r4UgvOFBNFKlWk-EAZ13nvsNIrV7-BW2vO9GZfPeyr4756s69mMSOGjI9s-4rur_n_0A8oMn-O</recordid><startdate>20190301</startdate><enddate>20190301</enddate><creator>Dubovichenko, S. 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V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c246t-d2cc6f3e6d1d27242ce5d7ca62ae39eccd2600a9918208bcdaaf95c1b46a511a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Astrophysics and Astroparticles</topic><topic>Clusters</topic><topic>Interaction parameters</topic><topic>Mathematical models</topic><topic>Original Paper</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dubovichenko, S. B.</creatorcontrib><creatorcontrib>Burkova, N. A.</creatorcontrib><creatorcontrib>Dzhazairov-Kakhramanov, A. 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B.</au><au>Burkova, N. A.</au><au>Dzhazairov-Kakhramanov, A. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Potential cluster calculations for the astrophysical S-factor and reaction rate of the radiative 3He(4He,γ)7Be capture</atitle><jtitle>Indian journal of physics</jtitle><stitle>Indian J Phys</stitle><date>2019-03-01</date><risdate>2019</risdate><volume>93</volume><issue>3</issue><spage>279</spage><epage>283</epage><pages>279-283</pages><issn>0973-1458</issn><eissn>0974-9845</eissn><abstract>In the frame of a modified potential cluster model based on the classification of orbital states according to Young diagrams and revised interaction potential parameters for the bound states of
7
Be in the
3
He
4
He cluster model with forbidden states, the astrophysical
S
-factor for the radiative capture reaction
3
He(
4
He,γ)
7
Be has been calculated from 10 keV. The result obtained,
S
(23 keV) = 0.561 keV·b, reproduces the latest experimental data at 23 keV. The calculated and parametrized reaction rate is compared with some known results in the range of temperatures from 0.05 to 5
T
9
.</abstract><cop>New Delhi</cop><pub>Springer India</pub><doi>10.1007/s12648-018-1287-0</doi><tpages>5</tpages></addata></record> |
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| language | eng |
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| subjects | Astrophysics and Astroparticles Clusters Interaction parameters Mathematical models Original Paper Physics Physics and Astronomy |
| title | Potential cluster calculations for the astrophysical S-factor and reaction rate of the radiative 3He(4He,γ)7Be capture |
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