Resolving the 11B(p, \({\alpha_0}\)) Cross Section Discrepancies between 0.5 and 3.5 MeV

The reaction 11B(p, 3\({\alpha}\)) is relevant for fields as diverse as material science, nuclear structure, nuclear astrophysics, and fusion science. However, for the channel proceeding via the ground state of 8Be, the available cross-section data shows large discrepancies of both normalization and...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2019-08
Main Authors: Munch, Michael, Kirsebom, Oliver Sølund, Swartz, Jacobus Andreas, Hans Otto Uldall Fynbo
Format: Article
Language:English
Subjects:
Astrophysics
Cross-sections
Nuclear astrophysics
Nuclear fusion
Nuclear structure
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
container_start_page
container_title arXiv.org
container_volume
creator Munch, Michael
Kirsebom, Oliver Sølund
Swartz, Jacobus Andreas
Hans Otto Uldall Fynbo
description The reaction 11B(p, 3\({\alpha}\)) is relevant for fields as diverse as material science, nuclear structure, nuclear astrophysics, and fusion science. However, for the channel proceeding via the ground state of 8Be, the available cross-section data shows large discrepancies of both normalization and energy scale. The present paper reports on a measurement of the 11B(p, \({\alpha_0}\)) cross section using an array of modern large area segmented silicon detectors and low beam current on an enriched thin target with the aim of resolving the discrepancies amongst previous measurements.
doi_str_mv 10.48550/arxiv.1908.04064
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2272608105</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2272608105</sourcerecordid><originalsourceid>FETCH-LOGICAL-a525-420a2eb1061ef23cfda02649aa7cb821fe5a9a0afda456c50ee50d76a29c7f483</originalsourceid><addsrcrecordid>eNotjktLw0AURgdBsNT-AHcDblow8c6dmTyWWusDKoIWcREIN9Mbm1KSmEmrIP53A7o68C3Od4Q4UxCaxFq4pO6rOoQqhSQEA5E5EiPUWgWJQTwRE--3AIBRjNbqkXh7Zt_sDlX9LvsNS6Wup-2FzKbfGe3aDeXwk81mct413ssXdn3V1PKm8q7jlmpXsZcF95_MtYTQSqrXUg985NdTcVzSzvPkn2Oxul2s5vfB8unuYX61DMiiDQwCIRcKIsUlaleuaWgzKVHsigRVyZZSAhp2YyNngdnCOo4IUxeXJtFjcf6nbbvmY8--z7fNvquHxxwxxggSBVb_As75UJY</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2272608105</pqid></control><display><type>article</type><title>Resolving the 11B(p, \({\alpha_0}\)) Cross Section Discrepancies between 0.5 and 3.5 MeV</title><source>ProQuest - Publicly Available Content Database</source><creator>Munch, Michael ; Kirsebom, Oliver Sølund ; Swartz, Jacobus Andreas ; Hans Otto Uldall Fynbo</creator><creatorcontrib>Munch, Michael ; Kirsebom, Oliver Sølund ; Swartz, Jacobus Andreas ; Hans Otto Uldall Fynbo</creatorcontrib><description>The reaction 11B(p, 3\({\alpha}\)) is relevant for fields as diverse as material science, nuclear structure, nuclear astrophysics, and fusion science. However, for the channel proceeding via the ground state of 8Be, the available cross-section data shows large discrepancies of both normalization and energy scale. The present paper reports on a measurement of the 11B(p, \({\alpha_0}\)) cross section using an array of modern large area segmented silicon detectors and low beam current on an enriched thin target with the aim of resolving the discrepancies amongst previous measurements.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1908.04064</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Astrophysics ; Cross-sections ; Nuclear astrophysics ; Nuclear fusion ; Nuclear structure</subject><ispartof>arXiv.org, 2019-08</ispartof><rights>2019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2272608105?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25751,27923,37010,44588</link.rule.ids></links><search><creatorcontrib>Munch, Michael</creatorcontrib><creatorcontrib>Kirsebom, Oliver Sølund</creatorcontrib><creatorcontrib>Swartz, Jacobus Andreas</creatorcontrib><creatorcontrib>Hans Otto Uldall Fynbo</creatorcontrib><title>Resolving the 11B(p, \({\alpha_0}\)) Cross Section Discrepancies between 0.5 and 3.5 MeV</title><title>arXiv.org</title><description>The reaction 11B(p, 3\({\alpha}\)) is relevant for fields as diverse as material science, nuclear structure, nuclear astrophysics, and fusion science. However, for the channel proceeding via the ground state of 8Be, the available cross-section data shows large discrepancies of both normalization and energy scale. The present paper reports on a measurement of the 11B(p, \({\alpha_0}\)) cross section using an array of modern large area segmented silicon detectors and low beam current on an enriched thin target with the aim of resolving the discrepancies amongst previous measurements.</description><subject>Astrophysics</subject><subject>Cross-sections</subject><subject>Nuclear astrophysics</subject><subject>Nuclear fusion</subject><subject>Nuclear structure</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotjktLw0AURgdBsNT-AHcDblow8c6dmTyWWusDKoIWcREIN9Mbm1KSmEmrIP53A7o68C3Od4Q4UxCaxFq4pO6rOoQqhSQEA5E5EiPUWgWJQTwRE--3AIBRjNbqkXh7Zt_sDlX9LvsNS6Wup-2FzKbfGe3aDeXwk81mct413ssXdn3V1PKm8q7jlmpXsZcF95_MtYTQSqrXUg985NdTcVzSzvPkn2Oxul2s5vfB8unuYX61DMiiDQwCIRcKIsUlaleuaWgzKVHsigRVyZZSAhp2YyNngdnCOo4IUxeXJtFjcf6nbbvmY8--z7fNvquHxxwxxggSBVb_As75UJY</recordid><startdate>20190812</startdate><enddate>20190812</enddate><creator>Munch, Michael</creator><creator>Kirsebom, Oliver Sølund</creator><creator>Swartz, Jacobus Andreas</creator><creator>Hans Otto Uldall Fynbo</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20190812</creationdate><title>Resolving the 11B(p, \({\alpha_0}\)) Cross Section Discrepancies between 0.5 and 3.5 MeV</title><author>Munch, Michael ; Kirsebom, Oliver Sølund ; Swartz, Jacobus Andreas ; Hans Otto Uldall Fynbo</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a525-420a2eb1061ef23cfda02649aa7cb821fe5a9a0afda456c50ee50d76a29c7f483</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Astrophysics</topic><topic>Cross-sections</topic><topic>Nuclear astrophysics</topic><topic>Nuclear fusion</topic><topic>Nuclear structure</topic><toplevel>online_resources</toplevel><creatorcontrib>Munch, Michael</creatorcontrib><creatorcontrib>Kirsebom, Oliver Sølund</creatorcontrib><creatorcontrib>Swartz, Jacobus Andreas</creatorcontrib><creatorcontrib>Hans Otto Uldall Fynbo</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</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 Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>ProQuest - Publicly Available Content Database</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>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Munch, Michael</au><au>Kirsebom, Oliver Sølund</au><au>Swartz, Jacobus Andreas</au><au>Hans Otto Uldall Fynbo</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Resolving the 11B(p, \({\alpha_0}\)) Cross Section Discrepancies between 0.5 and 3.5 MeV</atitle><jtitle>arXiv.org</jtitle><date>2019-08-12</date><risdate>2019</risdate><eissn>2331-8422</eissn><abstract>The reaction 11B(p, 3\({\alpha}\)) is relevant for fields as diverse as material science, nuclear structure, nuclear astrophysics, and fusion science. However, for the channel proceeding via the ground state of 8Be, the available cross-section data shows large discrepancies of both normalization and energy scale. The present paper reports on a measurement of the 11B(p, \({\alpha_0}\)) cross section using an array of modern large area segmented silicon detectors and low beam current on an enriched thin target with the aim of resolving the discrepancies amongst previous measurements.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1908.04064</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2019-08
issn 2331-8422
language eng
recordid cdi_proquest_journals_2272608105
source ProQuest - Publicly Available Content Database
subjects Astrophysics
Cross-sections
Nuclear astrophysics
Nuclear fusion
Nuclear structure
title Resolving the 11B(p, \({\alpha_0}\)) Cross Section Discrepancies between 0.5 and 3.5 MeV
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-14T13%3A14%3A49IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Resolving%20the%2011B(p,%20%5C(%7B%5Calpha_0%7D%5C))%20Cross%20Section%20Discrepancies%20between%200.5%20and%203.5%20MeV&rft.jtitle=arXiv.org&rft.au=Munch,%20Michael&rft.date=2019-08-12&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1908.04064&rft_dat=%3Cproquest%3E2272608105%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a525-420a2eb1061ef23cfda02649aa7cb821fe5a9a0afda456c50ee50d76a29c7f483%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2272608105&rft_id=info:pmid/&rfr_iscdi=true