Matter radii of light halo nuclei
We reexamine the matter radii of diffuse halo nuclei, as deduced from reaction cross section measurements at high energy. Careful consideration is given to the intrinsic few-body structure of these projectiles and the adiabatic nature of the projectile-target interaction. Using {sup 11}Li, {sup 11}B...
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Veröffentlicht in: | Physical Review Letters 1996-05, Vol.76 (21), p.3903-3906 |
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description | We reexamine the matter radii of diffuse halo nuclei, as deduced from reaction cross section measurements at high energy. Careful consideration is given to the intrinsic few-body structure of these projectiles and the adiabatic nature of the projectile-target interaction. Using {sup 11}Li, {sup 11}Be, and {sup 8}B as examples we show that data require significantly larger matter radii than previously reported. The revised value for {sup 11}Li of 3.55fm is consistent with three-body models with significant 1{ital s}-intruder state components, which reproduce experimental {sup 9}Li momentum distributions following {sup 11}Li breakup, but were hitherto thought to be at variance with cross section data. {copyright} {ital 1996 The American Physical Society.} |
doi_str_mv | 10.1103/PhysRevLett.76.3903 |
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Careful consideration is given to the intrinsic few-body structure of these projectiles and the adiabatic nature of the projectile-target interaction. Using {sup 11}Li, {sup 11}Be, and {sup 8}B as examples we show that data require significantly larger matter radii than previously reported. The revised value for {sup 11}Li of 3.55fm is consistent with three-body models with significant 1{ital s}-intruder state components, which reproduce experimental {sup 9}Li momentum distributions following {sup 11}Li breakup, but were hitherto thought to be at variance with cross section data. {copyright} {ital 1996 The American Physical Society.}</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/PhysRevLett.76.3903</identifier><identifier>PMID: 10061142</identifier><language>eng</language><publisher>United States</publisher><subject>BERYLLIUM 11 ; BORON 8 ; CROSS SECTIONS ; LITHIUM 11 ; MATTER ; NUCLEAR HALOS ; NUCLEAR RADII ; PHYSICS ; PROJECTILES ; TARGETS</subject><ispartof>Physical Review Letters, 1996-05, Vol.76 (21), p.3903-3906</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c374t-9872303b7411e421ef900afb0d63ef5474b56811015567abbbdb8f8265c4fa0e3</citedby><cites>FETCH-LOGICAL-c374t-9872303b7411e421ef900afb0d63ef5474b56811015567abbbdb8f8265c4fa0e3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,881,2862,2863,27903,27904</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/10061142$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/285712$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Al-Khalili, JS</creatorcontrib><creatorcontrib>Tostevin, JA</creatorcontrib><title>Matter radii of light halo nuclei</title><title>Physical Review Letters</title><addtitle>Phys Rev Lett</addtitle><description>We reexamine the matter radii of diffuse halo nuclei, as deduced from reaction cross section measurements at high energy. Careful consideration is given to the intrinsic few-body structure of these projectiles and the adiabatic nature of the projectile-target interaction. Using {sup 11}Li, {sup 11}Be, and {sup 8}B as examples we show that data require significantly larger matter radii than previously reported. The revised value for {sup 11}Li of 3.55fm is consistent with three-body models with significant 1{ital s}-intruder state components, which reproduce experimental {sup 9}Li momentum distributions following {sup 11}Li breakup, but were hitherto thought to be at variance with cross section data. {copyright} {ital 1996 The American Physical Society.}</description><subject>BERYLLIUM 11</subject><subject>BORON 8</subject><subject>CROSS SECTIONS</subject><subject>LITHIUM 11</subject><subject>MATTER</subject><subject>NUCLEAR HALOS</subject><subject>NUCLEAR RADII</subject><subject>PHYSICS</subject><subject>PROJECTILES</subject><subject>TARGETS</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1996</creationdate><recordtype>article</recordtype><recordid>eNpNkMtOwzAQRS0EoqXwBUgo3bFJmbFjO1miipdUBEKwtmzHJkFpU2IHqX9PqnTR1WzOnXt1CLlGWCACu3uvduHD_a1cjAspFqwAdkKmCLJIJWJ2SqYADNMCQE7IRQg_AIBU5OdkggBiQOiUzF91jK5LOl3WddL6pKm_q5hUummTTW8bV1-SM6-b4K4Od0a-Hh8-l8_p6u3pZXm_Si2TWUyLXFIGzMgM0WUUnR-KtTdQCuY8z2RmuMiH4ci5kNoYU5rc51Rwm3kNjs3IfPzbhlirYOvobGXbzcbZqGjOJdKBuR2Zbdf-9i5Eta6DdU2jN67tg8KcF5TLYcOAshG1XRtC57zadvVadzuFoPb-1JE_JYXa-xtSN4eC3qxdeZQZhbF_ec5rsA</recordid><startdate>19960520</startdate><enddate>19960520</enddate><creator>Al-Khalili, JS</creator><creator>Tostevin, JA</creator><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>OTOTI</scope></search><sort><creationdate>19960520</creationdate><title>Matter radii of light halo nuclei</title><author>Al-Khalili, JS ; Tostevin, JA</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c374t-9872303b7411e421ef900afb0d63ef5474b56811015567abbbdb8f8265c4fa0e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1996</creationdate><topic>BERYLLIUM 11</topic><topic>BORON 8</topic><topic>CROSS SECTIONS</topic><topic>LITHIUM 11</topic><topic>MATTER</topic><topic>NUCLEAR HALOS</topic><topic>NUCLEAR RADII</topic><topic>PHYSICS</topic><topic>PROJECTILES</topic><topic>TARGETS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Al-Khalili, JS</creatorcontrib><creatorcontrib>Tostevin, JA</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Physical Review Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Al-Khalili, JS</au><au>Tostevin, JA</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Matter radii of light halo nuclei</atitle><jtitle>Physical Review Letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>1996-05-20</date><risdate>1996</risdate><volume>76</volume><issue>21</issue><spage>3903</spage><epage>3906</epage><pages>3903-3906</pages><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>We reexamine the matter radii of diffuse halo nuclei, as deduced from reaction cross section measurements at high energy. Careful consideration is given to the intrinsic few-body structure of these projectiles and the adiabatic nature of the projectile-target interaction. Using {sup 11}Li, {sup 11}Be, and {sup 8}B as examples we show that data require significantly larger matter radii than previously reported. The revised value for {sup 11}Li of 3.55fm is consistent with three-body models with significant 1{ital s}-intruder state components, which reproduce experimental {sup 9}Li momentum distributions following {sup 11}Li breakup, but were hitherto thought to be at variance with cross section data. {copyright} {ital 1996 The American Physical Society.}</abstract><cop>United States</cop><pmid>10061142</pmid><doi>10.1103/PhysRevLett.76.3903</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
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subjects | BERYLLIUM 11 BORON 8 CROSS SECTIONS LITHIUM 11 MATTER NUCLEAR HALOS NUCLEAR RADII PHYSICS PROJECTILES TARGETS |
title | Matter radii of light halo nuclei |
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