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Sensitivity of the halo nuclei-12C elastic scattering at incident nucleon energy 800 MeV to the halo density distribution
In the framework of Glauber optical limit approximation where Coulomb effect is taken into account, the elastic scattering differential cross section for halo nuclei with 12 C at 800 MeV/N has been calculated. Its sensitivity to the halo densities and the root mean square of the core and halo is the...
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Published in: | Indian journal of physics 2017-10, Vol.91 (10), p.1245-1258 |
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container_end_page | 1258 |
container_issue | 10 |
container_start_page | 1245 |
container_title | Indian journal of physics |
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creator | Hassan, M A M Nour El-Din, M S M Ellithi, A Hosny, H Salama, T N E |
description | In the framework of Glauber optical limit approximation where Coulomb effect is taken into account, the elastic scattering differential cross section for halo nuclei with
12
C
at 800 MeV/N has been calculated. Its sensitivity to the halo densities and the root mean square of the core and halo is the main goal of the current study. The projectile nuclei are taken to be one-neutron and two-neutron halo. The calculations are carried out for Gaussian–Gaussian, Gaussian–Oscillator and Gaussian-2 s phenomenological densities for each considered projectile in the mass number range 6–29. Also included a comparison between the obtained results of phenomenological densities and the results within the microscopic densities LSSM of
6
He
and
11
Li
and microscopic densities GCM of
11
Be
where the density of the target nucleus
12
C
obtained from electron-
12
C
scattering is used. The zero range approximation is considered in the calculations. We found that the sensitivity of elastic scattering differential cross section to the halo density is clear if the nucleus appears as two clear different clusters, core and halo. |
doi_str_mv | 10.1007/s12648-017-1018-y |
format | article |
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12
C
at 800 MeV/N has been calculated. Its sensitivity to the halo densities and the root mean square of the core and halo is the main goal of the current study. The projectile nuclei are taken to be one-neutron and two-neutron halo. The calculations are carried out for Gaussian–Gaussian, Gaussian–Oscillator and Gaussian-2 s phenomenological densities for each considered projectile in the mass number range 6–29. Also included a comparison between the obtained results of phenomenological densities and the results within the microscopic densities LSSM of
6
He
and
11
Li
and microscopic densities GCM of
11
Be
where the density of the target nucleus
12
C
obtained from electron-
12
C
scattering is used. The zero range approximation is considered in the calculations. We found that the sensitivity of elastic scattering differential cross section to the halo density is clear if the nucleus appears as two clear different clusters, core and halo.</description><identifier>ISSN: 0973-1458</identifier><identifier>EISSN: 0974-9845</identifier><identifier>DOI: 10.1007/s12648-017-1018-y</identifier><language>eng</language><publisher>New Delhi: Springer India</publisher><subject>Approximation ; Astrophysics and Astroparticles ; Atomic properties ; Clusters ; Density distribution ; Elastic limit ; Elastic scattering ; Energy distribution ; Mathematical analysis ; Nuclear cross sections ; Nuclear physics ; Nuclei (nuclear physics) ; Original Paper ; Physics ; Physics and Astronomy ; Scattering ; Sensitivity</subject><ispartof>Indian journal of physics, 2017-10, Vol.91 (10), p.1245-1258</ispartof><rights>Indian Association for the Cultivation of Science 2017</rights><rights>Indian Journal of Physics is a copyright of Springer, 2017.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c161y-2f7b213d0b712f01d710ae6c7b380faed62a4dc92c04143c3212277db1bf37a43</citedby><cites>FETCH-LOGICAL-c161y-2f7b213d0b712f01d710ae6c7b380faed62a4dc92c04143c3212277db1bf37a43</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>Hassan, M A M</creatorcontrib><creatorcontrib>Nour El-Din, M S M</creatorcontrib><creatorcontrib>Ellithi, A</creatorcontrib><creatorcontrib>Hosny, H</creatorcontrib><creatorcontrib>Salama, T N E</creatorcontrib><title>Sensitivity of the halo nuclei-12C elastic scattering at incident nucleon energy 800 MeV to the halo density distribution</title><title>Indian journal of physics</title><addtitle>Indian J Phys</addtitle><description>In the framework of Glauber optical limit approximation where Coulomb effect is taken into account, the elastic scattering differential cross section for halo nuclei with
12
C
at 800 MeV/N has been calculated. Its sensitivity to the halo densities and the root mean square of the core and halo is the main goal of the current study. The projectile nuclei are taken to be one-neutron and two-neutron halo. The calculations are carried out for Gaussian–Gaussian, Gaussian–Oscillator and Gaussian-2 s phenomenological densities for each considered projectile in the mass number range 6–29. Also included a comparison between the obtained results of phenomenological densities and the results within the microscopic densities LSSM of
6
He
and
11
Li
and microscopic densities GCM of
11
Be
where the density of the target nucleus
12
C
obtained from electron-
12
C
scattering is used. The zero range approximation is considered in the calculations. We found that the sensitivity of elastic scattering differential cross section to the halo density is clear if the nucleus appears as two clear different clusters, core and halo.</description><subject>Approximation</subject><subject>Astrophysics and Astroparticles</subject><subject>Atomic properties</subject><subject>Clusters</subject><subject>Density distribution</subject><subject>Elastic limit</subject><subject>Elastic scattering</subject><subject>Energy distribution</subject><subject>Mathematical analysis</subject><subject>Nuclear cross sections</subject><subject>Nuclear physics</subject><subject>Nuclei (nuclear physics)</subject><subject>Original Paper</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Scattering</subject><subject>Sensitivity</subject><issn>0973-1458</issn><issn>0974-9845</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp1kEtOwzAURS0EEqWwAGaWGBv8bCdOhqjiJxUx4DO1HMdpXQWn2C5SWA1rYWWkDRJMGL03uOde6SB0CvQcKJUXEVguCkJBEqBQkH4PTWgpBSkLke3vfk5AZMUhOopxRWlegswm6OPR-uiSe3epx12D09LipW477DemtY4Am2Hb6picwdHolGxwfoF1ws4bV1ufxmTnsfU2LHpcUPr1eW9fcOp-2-rdSo9rF1Nw1Sa5zh-jg0a30Z783Cl6vr56mt2S-cPN3exyTgzk0BPWyIoBr2klgTUUaglU29zIihe00bbOmRa1KZmhAgQ3nAFjUtYVVA2XWvApOht716F729iY1KrbBD9MKig5ZBljZTGkYEyZ0MUYbKPWwb3q0CugaqtYjYrVoFhtFat-YNjIxPXWig1_mv-FvgGE4YCa</recordid><startdate>20171001</startdate><enddate>20171001</enddate><creator>Hassan, M A M</creator><creator>Nour El-Din, M S M</creator><creator>Ellithi, A</creator><creator>Hosny, H</creator><creator>Salama, T N E</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>20171001</creationdate><title>Sensitivity of the halo nuclei-12C elastic scattering at incident nucleon energy 800 MeV to the halo density distribution</title><author>Hassan, M A M ; Nour El-Din, M S M ; Ellithi, A ; Hosny, H ; Salama, T N E</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c161y-2f7b213d0b712f01d710ae6c7b380faed62a4dc92c04143c3212277db1bf37a43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Approximation</topic><topic>Astrophysics and Astroparticles</topic><topic>Atomic properties</topic><topic>Clusters</topic><topic>Density distribution</topic><topic>Elastic limit</topic><topic>Elastic scattering</topic><topic>Energy distribution</topic><topic>Mathematical analysis</topic><topic>Nuclear cross sections</topic><topic>Nuclear physics</topic><topic>Nuclei (nuclear physics)</topic><topic>Original Paper</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Scattering</topic><topic>Sensitivity</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hassan, M A M</creatorcontrib><creatorcontrib>Nour El-Din, M S M</creatorcontrib><creatorcontrib>Ellithi, A</creatorcontrib><creatorcontrib>Hosny, H</creatorcontrib><creatorcontrib>Salama, T N E</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)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</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>Hassan, M A M</au><au>Nour El-Din, M S M</au><au>Ellithi, A</au><au>Hosny, H</au><au>Salama, T N E</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Sensitivity of the halo nuclei-12C elastic scattering at incident nucleon energy 800 MeV to the halo density distribution</atitle><jtitle>Indian journal of physics</jtitle><stitle>Indian J Phys</stitle><date>2017-10-01</date><risdate>2017</risdate><volume>91</volume><issue>10</issue><spage>1245</spage><epage>1258</epage><pages>1245-1258</pages><issn>0973-1458</issn><eissn>0974-9845</eissn><abstract>In the framework of Glauber optical limit approximation where Coulomb effect is taken into account, the elastic scattering differential cross section for halo nuclei with
12
C
at 800 MeV/N has been calculated. Its sensitivity to the halo densities and the root mean square of the core and halo is the main goal of the current study. The projectile nuclei are taken to be one-neutron and two-neutron halo. The calculations are carried out for Gaussian–Gaussian, Gaussian–Oscillator and Gaussian-2 s phenomenological densities for each considered projectile in the mass number range 6–29. Also included a comparison between the obtained results of phenomenological densities and the results within the microscopic densities LSSM of
6
He
and
11
Li
and microscopic densities GCM of
11
Be
where the density of the target nucleus
12
C
obtained from electron-
12
C
scattering is used. The zero range approximation is considered in the calculations. We found that the sensitivity of elastic scattering differential cross section to the halo density is clear if the nucleus appears as two clear different clusters, core and halo.</abstract><cop>New Delhi</cop><pub>Springer India</pub><doi>10.1007/s12648-017-1018-y</doi><tpages>14</tpages></addata></record> |
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subjects | Approximation Astrophysics and Astroparticles Atomic properties Clusters Density distribution Elastic limit Elastic scattering Energy distribution Mathematical analysis Nuclear cross sections Nuclear physics Nuclei (nuclear physics) Original Paper Physics Physics and Astronomy Scattering Sensitivity |
title | Sensitivity of the halo nuclei-12C elastic scattering at incident nucleon energy 800 MeV to the halo density distribution |
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