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Radiative neutron capture by 2H, 7Li, 14C, and 14N nuclei at astrophysical energies
The possibility of describing experimental data on the total cross sections for the n 2 H, n 7 Li, n 14 C, and n 14 N radiative-capture processes within the potential cluster model involving forbidden states and their classification according to Young’s tableaux is considered. It is shown that this...
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Published in: | Physics of atomic nuclei 2013-07, Vol.76 (7), p.841-861 |
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cites | cdi_FETCH-LOGICAL-c284t-3ab3bcc0c096a896808d72416c6d79569859a07aca29a36e926afdd33631a28b3 |
container_end_page | 861 |
container_issue | 7 |
container_start_page | 841 |
container_title | Physics of atomic nuclei |
container_volume | 76 |
creator | Dubovichenko, S. B. |
description | The possibility of describing experimental data on the total cross sections for the
n
2
H,
n
7
Li,
n
14
C, and
n
14
N radiative-capture processes within the potential cluster model involving forbidden states and their classification according to Young’s tableaux is considered. It is shown that this model and the methods used here to construct potentials make it possible to describe correctly the behavior of the experimental cross sections at energies between 5 to 10 meV (5 × 10
−3
–10 × 10
−3
eV) and 1 to 15MeV. |
doi_str_mv | 10.1134/S106377881307003X |
format | article |
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H,
n
7
Li,
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C, and
n
14
N radiative-capture processes within the potential cluster model involving forbidden states and their classification according to Young’s tableaux is considered. It is shown that this model and the methods used here to construct potentials make it possible to describe correctly the behavior of the experimental cross sections at energies between 5 to 10 meV (5 × 10
−3
–10 × 10
−3
eV) and 1 to 15MeV.</description><identifier>ISSN: 1063-7788</identifier><identifier>EISSN: 1562-692X</identifier><identifier>DOI: 10.1134/S106377881307003X</identifier><language>eng</language><publisher>Boston: Springer US</publisher><subject>Nuclei ; Particle and Nuclear Physics ; Physics ; Physics and Astronomy</subject><ispartof>Physics of atomic nuclei, 2013-07, Vol.76 (7), p.841-861</ispartof><rights>Pleiades Publishing, Ltd. 2013</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c284t-3ab3bcc0c096a896808d72416c6d79569859a07aca29a36e926afdd33631a28b3</citedby><cites>FETCH-LOGICAL-c284t-3ab3bcc0c096a896808d72416c6d79569859a07aca29a36e926afdd33631a28b3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Dubovichenko, S. B.</creatorcontrib><title>Radiative neutron capture by 2H, 7Li, 14C, and 14N nuclei at astrophysical energies</title><title>Physics of atomic nuclei</title><addtitle>Phys. Atom. Nuclei</addtitle><description>The possibility of describing experimental data on the total cross sections for the
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2
H,
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Li,
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14
N radiative-capture processes within the potential cluster model involving forbidden states and their classification according to Young’s tableaux is considered. It is shown that this model and the methods used here to construct potentials make it possible to describe correctly the behavior of the experimental cross sections at energies between 5 to 10 meV (5 × 10
−3
–10 × 10
−3
eV) and 1 to 15MeV.</description><subject>Nuclei</subject><subject>Particle and Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><issn>1063-7788</issn><issn>1562-692X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNp9kM1KAzEUhYMoWKsP4C4P0NGbZCY_SylqhaJgFbob7mTSmjKmJZkR-vZNqTvB1Tlw7nc5HEJuGdwxJsr7BQMplNKaCVAAYnlGRqySvJCGL8-zz3FxzC_JVUobAMZ0BSOyeMfWY-9_HA1u6OM2UIu7foiONnvKZxOq5n5CWTmdUAxtNq80DLZznmJPMWVi97VP3mJHXXBx7V26Jhcr7JK7-dUx-Xx6_JjOivnb88v0YV5Yrsu-ENiIxlqwYCRqIzXoVvGSSStbZSppdGUQFFrkBoV0hktcta0QUjDkuhFjwk5_bdymFN2q3kX_jXFfM6iPq9R_VskMPzEp34a1i_VmO8SQa_4DHQDMV2JB</recordid><startdate>20130701</startdate><enddate>20130701</enddate><creator>Dubovichenko, S. B.</creator><general>Springer US</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20130701</creationdate><title>Radiative neutron capture by 2H, 7Li, 14C, and 14N nuclei at astrophysical energies</title><author>Dubovichenko, S. B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c284t-3ab3bcc0c096a896808d72416c6d79569859a07aca29a36e926afdd33631a28b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Nuclei</topic><topic>Particle and Nuclear Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dubovichenko, S. B.</creatorcontrib><collection>CrossRef</collection><jtitle>Physics of atomic nuclei</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dubovichenko, S. B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Radiative neutron capture by 2H, 7Li, 14C, and 14N nuclei at astrophysical energies</atitle><jtitle>Physics of atomic nuclei</jtitle><stitle>Phys. Atom. Nuclei</stitle><date>2013-07-01</date><risdate>2013</risdate><volume>76</volume><issue>7</issue><spage>841</spage><epage>861</epage><pages>841-861</pages><issn>1063-7788</issn><eissn>1562-692X</eissn><abstract>The possibility of describing experimental data on the total cross sections for the
n
2
H,
n
7
Li,
n
14
C, and
n
14
N radiative-capture processes within the potential cluster model involving forbidden states and their classification according to Young’s tableaux is considered. It is shown that this model and the methods used here to construct potentials make it possible to describe correctly the behavior of the experimental cross sections at energies between 5 to 10 meV (5 × 10
−3
–10 × 10
−3
eV) and 1 to 15MeV.</abstract><cop>Boston</cop><pub>Springer US</pub><doi>10.1134/S106377881307003X</doi><tpages>21</tpages></addata></record> |
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issn | 1063-7788 1562-692X |
language | eng |
recordid | cdi_crossref_primary_10_1134_S106377881307003X |
source | Springer Nature |
subjects | Nuclei Particle and Nuclear Physics Physics Physics and Astronomy |
title | Radiative neutron capture by 2H, 7Li, 14C, and 14N nuclei at astrophysical energies |
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