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Neutron Capture on 11B and 12B at Astrophysical Energies
The possibility of describing the experimental data for the total cross sections of radiative n 11 B capture to the ground state of the 12 B nucleus at thermal and astrophysical energies is considered within the framework of the modified potential cluster model with classification of orbital states...
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| Published in: | Russian physics journal 2017-08, Vol.60 (4), p.666-677 |
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| Main Authors: | , , , |
| Format: | Article |
| Language: | English |
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| cites | cdi_FETCH-LOGICAL-c246t-3aaeefe5f84ccec3c74cafd798d0f56caa04b4f92794c64f9ebc64db9f20c0153 |
| container_end_page | 677 |
| container_issue | 4 |
| container_start_page | 666 |
| container_title | Russian physics journal |
| container_volume | 60 |
| creator | Dubovichenko, S. B. Burkova, N. A. Dzhazairov-Kakhramanov, A. V. Tkachenko, A. S. |
| description | The possibility of describing the experimental data for the total cross sections of radiative n
11
B capture to the ground state of the
12
B nucleus at thermal and astrophysical energies is considered within the framework of the modified potential cluster model with classification of orbital states according to Young tableaux. It is shown that it is possible to explain the magnitude of the experimental cross sections at energies from 25.3 meV to 100 keV on the basis of just the E1 transition from the S state of n
11
B scattering to the ground state of the
12
B nucleus in the n
11
B channel. New theoretical results have been obtained for the total cross sections of n
12
B capture to the ground state of the
13
B nucleus. The rates of both reactions are calculated in the temperature range from 0.01 to 5.0 Т
9
. |
| doi_str_mv | 10.1007/s11182-017-1122-7 |
| format | article |
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11
B capture to the ground state of the
12
B nucleus at thermal and astrophysical energies is considered within the framework of the modified potential cluster model with classification of orbital states according to Young tableaux. It is shown that it is possible to explain the magnitude of the experimental cross sections at energies from 25.3 meV to 100 keV on the basis of just the E1 transition from the S state of n
11
B scattering to the ground state of the
12
B nucleus in the n
11
B channel. New theoretical results have been obtained for the total cross sections of n
12
B capture to the ground state of the
13
B nucleus. The rates of both reactions are calculated in the temperature range from 0.01 to 5.0 Т
9
.</description><identifier>ISSN: 1064-8887</identifier><identifier>EISSN: 1573-9228</identifier><identifier>DOI: 10.1007/s11182-017-1122-7</identifier><language>eng</language><publisher>New York: Springer US</publisher><subject>Absorption cross sections ; Condensed Matter Physics ; Ground state ; Hadrons ; Heavy Ions ; Helium ; Lasers ; Mathematical and Computational Physics ; Nuclear capture ; Nuclear Physics ; Nuclei (nuclear physics) ; Optical Devices ; Optics ; Photonics ; Physics ; Physics and Astronomy ; Scattering ; Theoretical</subject><ispartof>Russian physics journal, 2017-08, Vol.60 (4), p.666-677</ispartof><rights>Springer Science+Business Media, LLC 2017</rights><rights>Copyright Springer Science & Business Media 2017</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c246t-3aaeefe5f84ccec3c74cafd798d0f56caa04b4f92794c64f9ebc64db9f20c0153</citedby><cites>FETCH-LOGICAL-c246t-3aaeefe5f84ccec3c74cafd798d0f56caa04b4f92794c64f9ebc64db9f20c0153</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27903,27904</link.rule.ids></links><search><creatorcontrib>Dubovichenko, S. B.</creatorcontrib><creatorcontrib>Burkova, N. A.</creatorcontrib><creatorcontrib>Dzhazairov-Kakhramanov, A. V.</creatorcontrib><creatorcontrib>Tkachenko, A. S.</creatorcontrib><title>Neutron Capture on 11B and 12B at Astrophysical Energies</title><title>Russian physics journal</title><addtitle>Russ Phys J</addtitle><description>The possibility of describing the experimental data for the total cross sections of radiative n
11
B capture to the ground state of the
12
B nucleus at thermal and astrophysical energies is considered within the framework of the modified potential cluster model with classification of orbital states according to Young tableaux. It is shown that it is possible to explain the magnitude of the experimental cross sections at energies from 25.3 meV to 100 keV on the basis of just the E1 transition from the S state of n
11
B scattering to the ground state of the
12
B nucleus in the n
11
B channel. New theoretical results have been obtained for the total cross sections of n
12
B capture to the ground state of the
13
B nucleus. The rates of both reactions are calculated in the temperature range from 0.01 to 5.0 Т
9
.</description><subject>Absorption cross sections</subject><subject>Condensed Matter Physics</subject><subject>Ground state</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Helium</subject><subject>Lasers</subject><subject>Mathematical and Computational Physics</subject><subject>Nuclear capture</subject><subject>Nuclear Physics</subject><subject>Nuclei (nuclear physics)</subject><subject>Optical Devices</subject><subject>Optics</subject><subject>Photonics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Scattering</subject><subject>Theoretical</subject><issn>1064-8887</issn><issn>1573-9228</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp1kD1PwzAURS0EEqXwA9giMRvec5zYHkvFl1TBArPlOs-lVUmCnQz997gKAwvTvcM570mXsWuEWwRQdwkRteCAiiMKwdUJm2GlSm6E0Ke5Qy251lqds4uUdgDZqtWM6Vcah9i1xdL1wxipyBXxvnBtU6DIORSLlIH-85C23u2Lh5biZkvpkp0Ft0909Ztz9vH48L585qu3p5flYsW9kPXAS-eIAlVBS-_Jl15J70KjjG4gVLV3DuRaBiOUkb7OhdY5mrUJAjxgVc7ZzXS3j933SGmwu26MbX5p0QiDqEAdKZwoH7uUIgXbx-2XiweLYI8D2Wkgmweyx4Gsyo6YnJTZdkPxz-V_pR8bpGc8</recordid><startdate>20170801</startdate><enddate>20170801</enddate><creator>Dubovichenko, S. B.</creator><creator>Burkova, N. A.</creator><creator>Dzhazairov-Kakhramanov, A. V.</creator><creator>Tkachenko, A. S.</creator><general>Springer US</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20170801</creationdate><title>Neutron Capture on 11B and 12B at Astrophysical Energies</title><author>Dubovichenko, S. B. ; Burkova, N. A. ; Dzhazairov-Kakhramanov, A. V. ; Tkachenko, A. S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c246t-3aaeefe5f84ccec3c74cafd798d0f56caa04b4f92794c64f9ebc64db9f20c0153</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Absorption cross sections</topic><topic>Condensed Matter Physics</topic><topic>Ground state</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Helium</topic><topic>Lasers</topic><topic>Mathematical and Computational Physics</topic><topic>Nuclear capture</topic><topic>Nuclear Physics</topic><topic>Nuclei (nuclear physics)</topic><topic>Optical Devices</topic><topic>Optics</topic><topic>Photonics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Scattering</topic><topic>Theoretical</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dubovichenko, S. B.</creatorcontrib><creatorcontrib>Burkova, N. A.</creatorcontrib><creatorcontrib>Dzhazairov-Kakhramanov, A. V.</creatorcontrib><creatorcontrib>Tkachenko, A. S.</creatorcontrib><collection>CrossRef</collection><jtitle>Russian physics journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dubovichenko, S. B.</au><au>Burkova, N. A.</au><au>Dzhazairov-Kakhramanov, A. V.</au><au>Tkachenko, A. S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Neutron Capture on 11B and 12B at Astrophysical Energies</atitle><jtitle>Russian physics journal</jtitle><stitle>Russ Phys J</stitle><date>2017-08-01</date><risdate>2017</risdate><volume>60</volume><issue>4</issue><spage>666</spage><epage>677</epage><pages>666-677</pages><issn>1064-8887</issn><eissn>1573-9228</eissn><abstract>The possibility of describing the experimental data for the total cross sections of radiative n
11
B capture to the ground state of the
12
B nucleus at thermal and astrophysical energies is considered within the framework of the modified potential cluster model with classification of orbital states according to Young tableaux. It is shown that it is possible to explain the magnitude of the experimental cross sections at energies from 25.3 meV to 100 keV on the basis of just the E1 transition from the S state of n
11
B scattering to the ground state of the
12
B nucleus in the n
11
B channel. New theoretical results have been obtained for the total cross sections of n
12
B capture to the ground state of the
13
B nucleus. The rates of both reactions are calculated in the temperature range from 0.01 to 5.0 Т
9
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| fulltext | fulltext |
| identifier | ISSN: 1064-8887 |
| ispartof | Russian physics journal, 2017-08, Vol.60 (4), p.666-677 |
| issn | 1064-8887 1573-9228 |
| language | eng |
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| source | Springer Link |
| subjects | Absorption cross sections Condensed Matter Physics Ground state Hadrons Heavy Ions Helium Lasers Mathematical and Computational Physics Nuclear capture Nuclear Physics Nuclei (nuclear physics) Optical Devices Optics Photonics Physics Physics and Astronomy Scattering Theoretical |
| title | Neutron Capture on 11B and 12B at Astrophysical Energies |
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