Loading…

Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV

The cross section of the ^{13}C(α,n)^{16}O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of ≈15%. Using a state-of-the-art neutron detection array, we have perf...

Full description

Saved in:
Bibliographic Details
Published in:Physical review letters 2024-02, Vol.132 (6), p.062702
Main Authors: deBoer, R J, Febbraro, M, Bardayan, D W, Boomershine, C, Brandenburg, K, Brune, C, Coil, S, Couder, M, Derkin, J, Dede, S, Fang, R, Fritsch, A, Gula, A, Gyürky, Gy, Hackett, B, Hamad, G, Jones-Alberty, Y, Kelmar, R, Manukyan, K, Matney, M, McDonaugh, J, Meisel, Z, Moylan, S, Nattress, J, Odell, D, O'Malley, P, Paris, M W, Robertson, D, Shahina, Singh, N, Smith, K, Smith, M S, Stech, E, Tan, W, Wiescher, M
Format: Article
Language:English
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue 6
container_start_page 062702
container_title Physical review letters
container_volume 132
creator deBoer, R J
Febbraro, M
Bardayan, D W
Boomershine, C
Brandenburg, K
Brune, C
Coil, S
Couder, M
Derkin, J
Dede, S
Fang, R
Fritsch, A
Gula, A
Gyürky, Gy
Hackett, B
Hamad, G
Jones-Alberty, Y
Kelmar, R
Manukyan, K
Matney, M
McDonaugh, J
Meisel, Z
Moylan, S
Nattress, J
Odell, D
O'Malley, P
Paris, M W
Robertson, D
Shahina
Singh, N
Smith, K
Smith, M S
Stech, E
Tan, W
Wiescher, M
description The cross section of the ^{13}C(α,n)^{16}O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of ≈15%. Using a state-of-the-art neutron detection array, we have performed a high resolution differential cross section study covering a broad energy range. These measurements result in a dramatic improvement in the extrapolation of the cross section to stellar energies potentially reducing the uncertainty to ≈5% and resolving long standing discrepancies in higher energy data.
doi_str_mv 10.1103/PhysRevLett.132.062702
format article
fullrecord <record><control><sourceid>pubmed</sourceid><recordid>TN_cdi_pubmed_primary_38394565</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>38394565</sourcerecordid><originalsourceid>FETCH-pubmed_primary_383945653</originalsourceid><addsrcrecordid>eNpjYJAzNNAzNDQw1g_IqCwOSi3zSS0p0TM0NtIzMDMyNzBiYuA0NDC31DU3NDThYOAqLs4yMDAwNDKzYGfgMLYwtjQxNTPlZIjxTU0sLi1KzU3NK1HIT1MoyUhViKs2NK511ji3UedRQ2defLVBrSZQyKzWX8ElMy0ttQioNDMxR8G5KL-4WCE4NbkkMz9PIa0oP1fBQM9CoSRfwUzP9NAC39QwHgbWtMSc4lReKM3NIOfmGuLsoVtQmpSbmhJfUJSZm1hUGQ9zjjFBBQA1CEh3</addsrcrecordid><sourcetype>Index Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV</title><source>American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)</source><creator>deBoer, R J ; Febbraro, M ; Bardayan, D W ; Boomershine, C ; Brandenburg, K ; Brune, C ; Coil, S ; Couder, M ; Derkin, J ; Dede, S ; Fang, R ; Fritsch, A ; Gula, A ; Gyürky, Gy ; Hackett, B ; Hamad, G ; Jones-Alberty, Y ; Kelmar, R ; Manukyan, K ; Matney, M ; McDonaugh, J ; Meisel, Z ; Moylan, S ; Nattress, J ; Odell, D ; O'Malley, P ; Paris, M W ; Robertson, D ; Shahina ; Singh, N ; Smith, K ; Smith, M S ; Stech, E ; Tan, W ; Wiescher, M</creator><creatorcontrib>deBoer, R J ; Febbraro, M ; Bardayan, D W ; Boomershine, C ; Brandenburg, K ; Brune, C ; Coil, S ; Couder, M ; Derkin, J ; Dede, S ; Fang, R ; Fritsch, A ; Gula, A ; Gyürky, Gy ; Hackett, B ; Hamad, G ; Jones-Alberty, Y ; Kelmar, R ; Manukyan, K ; Matney, M ; McDonaugh, J ; Meisel, Z ; Moylan, S ; Nattress, J ; Odell, D ; O'Malley, P ; Paris, M W ; Robertson, D ; Shahina ; Singh, N ; Smith, K ; Smith, M S ; Stech, E ; Tan, W ; Wiescher, M</creatorcontrib><description>The cross section of the ^{13}C(α,n)^{16}O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of ≈15%. Using a state-of-the-art neutron detection array, we have performed a high resolution differential cross section study covering a broad energy range. These measurements result in a dramatic improvement in the extrapolation of the cross section to stellar energies potentially reducing the uncertainty to ≈5% and resolving long standing discrepancies in higher energy data.</description><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/PhysRevLett.132.062702</identifier><identifier>PMID: 38394565</identifier><language>eng</language><publisher>United States</publisher><ispartof>Physical review letters, 2024-02, Vol.132 (6), p.062702</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/38394565$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>deBoer, R J</creatorcontrib><creatorcontrib>Febbraro, M</creatorcontrib><creatorcontrib>Bardayan, D W</creatorcontrib><creatorcontrib>Boomershine, C</creatorcontrib><creatorcontrib>Brandenburg, K</creatorcontrib><creatorcontrib>Brune, C</creatorcontrib><creatorcontrib>Coil, S</creatorcontrib><creatorcontrib>Couder, M</creatorcontrib><creatorcontrib>Derkin, J</creatorcontrib><creatorcontrib>Dede, S</creatorcontrib><creatorcontrib>Fang, R</creatorcontrib><creatorcontrib>Fritsch, A</creatorcontrib><creatorcontrib>Gula, A</creatorcontrib><creatorcontrib>Gyürky, Gy</creatorcontrib><creatorcontrib>Hackett, B</creatorcontrib><creatorcontrib>Hamad, G</creatorcontrib><creatorcontrib>Jones-Alberty, Y</creatorcontrib><creatorcontrib>Kelmar, R</creatorcontrib><creatorcontrib>Manukyan, K</creatorcontrib><creatorcontrib>Matney, M</creatorcontrib><creatorcontrib>McDonaugh, J</creatorcontrib><creatorcontrib>Meisel, Z</creatorcontrib><creatorcontrib>Moylan, S</creatorcontrib><creatorcontrib>Nattress, J</creatorcontrib><creatorcontrib>Odell, D</creatorcontrib><creatorcontrib>O'Malley, P</creatorcontrib><creatorcontrib>Paris, M W</creatorcontrib><creatorcontrib>Robertson, D</creatorcontrib><creatorcontrib>Shahina</creatorcontrib><creatorcontrib>Singh, N</creatorcontrib><creatorcontrib>Smith, K</creatorcontrib><creatorcontrib>Smith, M S</creatorcontrib><creatorcontrib>Stech, E</creatorcontrib><creatorcontrib>Tan, W</creatorcontrib><creatorcontrib>Wiescher, M</creatorcontrib><title>Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>The cross section of the ^{13}C(α,n)^{16}O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of ≈15%. Using a state-of-the-art neutron detection array, we have performed a high resolution differential cross section study covering a broad energy range. These measurements result in a dramatic improvement in the extrapolation of the cross section to stellar energies potentially reducing the uncertainty to ≈5% and resolving long standing discrepancies in higher energy data.</description><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNpjYJAzNNAzNDQw1g_IqCwOSi3zSS0p0TM0NtIzMDMyNzBiYuA0NDC31DU3NDThYOAqLs4yMDAwNDKzYGfgMLYwtjQxNTPlZIjxTU0sLi1KzU3NK1HIT1MoyUhViKs2NK511ji3UedRQ2defLVBrSZQyKzWX8ElMy0ttQioNDMxR8G5KL-4WCE4NbkkMz9PIa0oP1fBQM9CoSRfwUzP9NAC39QwHgbWtMSc4lReKM3NIOfmGuLsoVtQmpSbmhJfUJSZm1hUGQ9zjjFBBQA1CEh3</recordid><startdate>20240209</startdate><enddate>20240209</enddate><creator>deBoer, R J</creator><creator>Febbraro, M</creator><creator>Bardayan, D W</creator><creator>Boomershine, C</creator><creator>Brandenburg, K</creator><creator>Brune, C</creator><creator>Coil, S</creator><creator>Couder, M</creator><creator>Derkin, J</creator><creator>Dede, S</creator><creator>Fang, R</creator><creator>Fritsch, A</creator><creator>Gula, A</creator><creator>Gyürky, Gy</creator><creator>Hackett, B</creator><creator>Hamad, G</creator><creator>Jones-Alberty, Y</creator><creator>Kelmar, R</creator><creator>Manukyan, K</creator><creator>Matney, M</creator><creator>McDonaugh, J</creator><creator>Meisel, Z</creator><creator>Moylan, S</creator><creator>Nattress, J</creator><creator>Odell, D</creator><creator>O'Malley, P</creator><creator>Paris, M W</creator><creator>Robertson, D</creator><creator>Shahina</creator><creator>Singh, N</creator><creator>Smith, K</creator><creator>Smith, M S</creator><creator>Stech, E</creator><creator>Tan, W</creator><creator>Wiescher, M</creator><scope>NPM</scope></search><sort><creationdate>20240209</creationdate><title>Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV</title><author>deBoer, R J ; Febbraro, M ; Bardayan, D W ; Boomershine, C ; Brandenburg, K ; Brune, C ; Coil, S ; Couder, M ; Derkin, J ; Dede, S ; Fang, R ; Fritsch, A ; Gula, A ; Gyürky, Gy ; Hackett, B ; Hamad, G ; Jones-Alberty, Y ; Kelmar, R ; Manukyan, K ; Matney, M ; McDonaugh, J ; Meisel, Z ; Moylan, S ; Nattress, J ; Odell, D ; O'Malley, P ; Paris, M W ; Robertson, D ; Shahina ; Singh, N ; Smith, K ; Smith, M S ; Stech, E ; Tan, W ; Wiescher, M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-pubmed_primary_383945653</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>deBoer, R J</creatorcontrib><creatorcontrib>Febbraro, M</creatorcontrib><creatorcontrib>Bardayan, D W</creatorcontrib><creatorcontrib>Boomershine, C</creatorcontrib><creatorcontrib>Brandenburg, K</creatorcontrib><creatorcontrib>Brune, C</creatorcontrib><creatorcontrib>Coil, S</creatorcontrib><creatorcontrib>Couder, M</creatorcontrib><creatorcontrib>Derkin, J</creatorcontrib><creatorcontrib>Dede, S</creatorcontrib><creatorcontrib>Fang, R</creatorcontrib><creatorcontrib>Fritsch, A</creatorcontrib><creatorcontrib>Gula, A</creatorcontrib><creatorcontrib>Gyürky, Gy</creatorcontrib><creatorcontrib>Hackett, B</creatorcontrib><creatorcontrib>Hamad, G</creatorcontrib><creatorcontrib>Jones-Alberty, Y</creatorcontrib><creatorcontrib>Kelmar, R</creatorcontrib><creatorcontrib>Manukyan, K</creatorcontrib><creatorcontrib>Matney, M</creatorcontrib><creatorcontrib>McDonaugh, J</creatorcontrib><creatorcontrib>Meisel, Z</creatorcontrib><creatorcontrib>Moylan, S</creatorcontrib><creatorcontrib>Nattress, J</creatorcontrib><creatorcontrib>Odell, D</creatorcontrib><creatorcontrib>O'Malley, P</creatorcontrib><creatorcontrib>Paris, M W</creatorcontrib><creatorcontrib>Robertson, D</creatorcontrib><creatorcontrib>Shahina</creatorcontrib><creatorcontrib>Singh, N</creatorcontrib><creatorcontrib>Smith, K</creatorcontrib><creatorcontrib>Smith, M S</creatorcontrib><creatorcontrib>Stech, E</creatorcontrib><creatorcontrib>Tan, W</creatorcontrib><creatorcontrib>Wiescher, M</creatorcontrib><collection>PubMed</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>deBoer, R J</au><au>Febbraro, M</au><au>Bardayan, D W</au><au>Boomershine, C</au><au>Brandenburg, K</au><au>Brune, C</au><au>Coil, S</au><au>Couder, M</au><au>Derkin, J</au><au>Dede, S</au><au>Fang, R</au><au>Fritsch, A</au><au>Gula, A</au><au>Gyürky, Gy</au><au>Hackett, B</au><au>Hamad, G</au><au>Jones-Alberty, Y</au><au>Kelmar, R</au><au>Manukyan, K</au><au>Matney, M</au><au>McDonaugh, J</au><au>Meisel, Z</au><au>Moylan, S</au><au>Nattress, J</au><au>Odell, D</au><au>O'Malley, P</au><au>Paris, M W</au><au>Robertson, D</au><au>Shahina</au><au>Singh, N</au><au>Smith, K</au><au>Smith, M S</au><au>Stech, E</au><au>Tan, W</au><au>Wiescher, M</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2024-02-09</date><risdate>2024</risdate><volume>132</volume><issue>6</issue><spage>062702</spage><pages>062702-</pages><eissn>1079-7114</eissn><abstract>The cross section of the ^{13}C(α,n)^{16}O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of ≈15%. Using a state-of-the-art neutron detection array, we have performed a high resolution differential cross section study covering a broad energy range. These measurements result in a dramatic improvement in the extrapolation of the cross section to stellar energies potentially reducing the uncertainty to ≈5% and resolving long standing discrepancies in higher energy data.</abstract><cop>United States</cop><pmid>38394565</pmid><doi>10.1103/PhysRevLett.132.062702</doi></addata></record>
fulltext fulltext
identifier EISSN: 1079-7114
ispartof Physical review letters, 2024-02, Vol.132 (6), p.062702
issn 1079-7114
language eng
recordid cdi_pubmed_primary_38394565
source American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)
title Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-07T18%3A08%3A22IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-pubmed&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Measurement%20of%20the%20%5E%7B13%7DC(%CE%B1,%E2%80%89n_%7B0%7D)%5E%7B16%7DO%20Differential%20Cross%20Section%20from%200.8%20to%206.5%C2%A0MeV&rft.jtitle=Physical%20review%20letters&rft.au=deBoer,%20R%20J&rft.date=2024-02-09&rft.volume=132&rft.issue=6&rft.spage=062702&rft.pages=062702-&rft.eissn=1079-7114&rft_id=info:doi/10.1103/PhysRevLett.132.062702&rft_dat=%3Cpubmed%3E38394565%3C/pubmed%3E%3Cgrp_id%3Ecdi_FETCH-pubmed_primary_383945653%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/38394565&rfr_iscdi=true