Temperature-tuned Maxwell-Boltzmann neutron spectra for kT ranging from 30 up to 50 keV for nuclear astrophysics studies

The need of neutron capture cross section measurements for astrophysics motivates present work, where calculations to generate stellar neutron spectra at different temperatures are performed. The accelerator-based (7)Li(p,n)(7)Be reaction is used. Shaping the proton beam energy and the sample coveri...

Full description

Saved in:
Bibliographic Details
Published in:Applied radiation and isotopes 2012-08, Vol.70 (8), p.1583-1589
Main Authors: Martín-Hernández, G, Mastinu, P F, Praena, J, Dzysiuk, N, Capote Noy, R, Pignatari, 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 1589
container_issue 8
container_start_page 1583
container_title Applied radiation and isotopes
container_volume 70
creator Martín-Hernández, G
Mastinu, P F
Praena, J
Dzysiuk, N
Capote Noy, R
Pignatari, M
description The need of neutron capture cross section measurements for astrophysics motivates present work, where calculations to generate stellar neutron spectra at different temperatures are performed. The accelerator-based (7)Li(p,n)(7)Be reaction is used. Shaping the proton beam energy and the sample covering a specific solid angle, neutron activation for measuring stellar-averaged capture cross section can be done. High-quality Maxwell-Boltzmann neutron spectra are predicted. Assuming a general behavior of the neutron capture cross section a weighted fit of the spectrum to Maxwell-Boltzmann distributions is successfully introduced.
doi_str_mv 10.1016/j.apradiso.2012.05.004
format article
fullrecord <record><control><sourceid>proquest_pubme</sourceid><recordid>TN_cdi_proquest_miscellaneous_1024479318</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1024479318</sourcerecordid><originalsourceid>FETCH-LOGICAL-p141t-1eca15e09c667fc0960fe54d33c50e37f31b6209631f5ed6dd8a0ec9fffd46f83</originalsourceid><addsrcrecordid>eNo1kMtOwzAURC0kREvhFyov2SRc23kuoeIlFbEpbCvXvi5pEyf4IVq-ngJlNdLozEgzhEwZpAxYcb1J5eCkbnyfcmA8hTwFyE7ImFUlT-oKYETOvd_Awa1qfkZGnJeCizobk90CuwGdDNFhEqJFTZ_l7hPbNrnt2_DVSWupxRhcb6kfUAUnqekd3S6ok3bd2DU1ru-oABoHGnqaA93i2y9jo2pROir9IT68732jPPUh6gb9BTk1svV4edQJeb2_W8wek_nLw9PsZp4MLGMhYagkyxFqVRSlUVAXYDDPtBAqBxSlEWxV8IMtmMlRF1pXElDVxhidFaYSE3L11zu4_iOiD8uu8eqwT1rso18y4FlW1oL9oNMjGlcd6uXgmk66_fL_LfENubVu0w</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1024479318</pqid></control><display><type>article</type><title>Temperature-tuned Maxwell-Boltzmann neutron spectra for kT ranging from 30 up to 50 keV for nuclear astrophysics studies</title><source>Elsevier:Jisc Collections:Elsevier Read and Publish Agreement 2022-2024:Freedom Collection (Reading list)</source><creator>Martín-Hernández, G ; Mastinu, P F ; Praena, J ; Dzysiuk, N ; Capote Noy, R ; Pignatari, M</creator><creatorcontrib>Martín-Hernández, G ; Mastinu, P F ; Praena, J ; Dzysiuk, N ; Capote Noy, R ; Pignatari, M</creatorcontrib><description>The need of neutron capture cross section measurements for astrophysics motivates present work, where calculations to generate stellar neutron spectra at different temperatures are performed. The accelerator-based (7)Li(p,n)(7)Be reaction is used. Shaping the proton beam energy and the sample covering a specific solid angle, neutron activation for measuring stellar-averaged capture cross section can be done. High-quality Maxwell-Boltzmann neutron spectra are predicted. Assuming a general behavior of the neutron capture cross section a weighted fit of the spectrum to Maxwell-Boltzmann distributions is successfully introduced.</description><identifier>EISSN: 1872-9800</identifier><identifier>DOI: 10.1016/j.apradiso.2012.05.004</identifier><identifier>PMID: 22732394</identifier><language>eng</language><publisher>England</publisher><ispartof>Applied radiation and isotopes, 2012-08, Vol.70 (8), p.1583-1589</ispartof><rights>Copyright © 2012 Elsevier Ltd. All rights reserved.</rights><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/22732394$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Martín-Hernández, G</creatorcontrib><creatorcontrib>Mastinu, P F</creatorcontrib><creatorcontrib>Praena, J</creatorcontrib><creatorcontrib>Dzysiuk, N</creatorcontrib><creatorcontrib>Capote Noy, R</creatorcontrib><creatorcontrib>Pignatari, M</creatorcontrib><title>Temperature-tuned Maxwell-Boltzmann neutron spectra for kT ranging from 30 up to 50 keV for nuclear astrophysics studies</title><title>Applied radiation and isotopes</title><addtitle>Appl Radiat Isot</addtitle><description>The need of neutron capture cross section measurements for astrophysics motivates present work, where calculations to generate stellar neutron spectra at different temperatures are performed. The accelerator-based (7)Li(p,n)(7)Be reaction is used. Shaping the proton beam energy and the sample covering a specific solid angle, neutron activation for measuring stellar-averaged capture cross section can be done. High-quality Maxwell-Boltzmann neutron spectra are predicted. Assuming a general behavior of the neutron capture cross section a weighted fit of the spectrum to Maxwell-Boltzmann distributions is successfully introduced.</description><issn>1872-9800</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNo1kMtOwzAURC0kREvhFyov2SRc23kuoeIlFbEpbCvXvi5pEyf4IVq-ngJlNdLozEgzhEwZpAxYcb1J5eCkbnyfcmA8hTwFyE7ImFUlT-oKYETOvd_Awa1qfkZGnJeCizobk90CuwGdDNFhEqJFTZ_l7hPbNrnt2_DVSWupxRhcb6kfUAUnqekd3S6ok3bd2DU1ru-oABoHGnqaA93i2y9jo2pROir9IT68732jPPUh6gb9BTk1svV4edQJeb2_W8wek_nLw9PsZp4MLGMhYagkyxFqVRSlUVAXYDDPtBAqBxSlEWxV8IMtmMlRF1pXElDVxhidFaYSE3L11zu4_iOiD8uu8eqwT1rso18y4FlW1oL9oNMjGlcd6uXgmk66_fL_LfENubVu0w</recordid><startdate>201208</startdate><enddate>201208</enddate><creator>Martín-Hernández, G</creator><creator>Mastinu, P F</creator><creator>Praena, J</creator><creator>Dzysiuk, N</creator><creator>Capote Noy, R</creator><creator>Pignatari, M</creator><scope>NPM</scope><scope>7X8</scope></search><sort><creationdate>201208</creationdate><title>Temperature-tuned Maxwell-Boltzmann neutron spectra for kT ranging from 30 up to 50 keV for nuclear astrophysics studies</title><author>Martín-Hernández, G ; Mastinu, P F ; Praena, J ; Dzysiuk, N ; Capote Noy, R ; Pignatari, M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p141t-1eca15e09c667fc0960fe54d33c50e37f31b6209631f5ed6dd8a0ec9fffd46f83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Martín-Hernández, G</creatorcontrib><creatorcontrib>Mastinu, P F</creatorcontrib><creatorcontrib>Praena, J</creatorcontrib><creatorcontrib>Dzysiuk, N</creatorcontrib><creatorcontrib>Capote Noy, R</creatorcontrib><creatorcontrib>Pignatari, M</creatorcontrib><collection>PubMed</collection><collection>MEDLINE - Academic</collection><jtitle>Applied radiation and isotopes</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Martín-Hernández, G</au><au>Mastinu, P F</au><au>Praena, J</au><au>Dzysiuk, N</au><au>Capote Noy, R</au><au>Pignatari, M</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Temperature-tuned Maxwell-Boltzmann neutron spectra for kT ranging from 30 up to 50 keV for nuclear astrophysics studies</atitle><jtitle>Applied radiation and isotopes</jtitle><addtitle>Appl Radiat Isot</addtitle><date>2012-08</date><risdate>2012</risdate><volume>70</volume><issue>8</issue><spage>1583</spage><epage>1589</epage><pages>1583-1589</pages><eissn>1872-9800</eissn><abstract>The need of neutron capture cross section measurements for astrophysics motivates present work, where calculations to generate stellar neutron spectra at different temperatures are performed. The accelerator-based (7)Li(p,n)(7)Be reaction is used. Shaping the proton beam energy and the sample covering a specific solid angle, neutron activation for measuring stellar-averaged capture cross section can be done. High-quality Maxwell-Boltzmann neutron spectra are predicted. Assuming a general behavior of the neutron capture cross section a weighted fit of the spectrum to Maxwell-Boltzmann distributions is successfully introduced.</abstract><cop>England</cop><pmid>22732394</pmid><doi>10.1016/j.apradiso.2012.05.004</doi><tpages>7</tpages></addata></record>
fulltext fulltext
identifier EISSN: 1872-9800
ispartof Applied radiation and isotopes, 2012-08, Vol.70 (8), p.1583-1589
issn 1872-9800
language eng
recordid cdi_proquest_miscellaneous_1024479318
source Elsevier:Jisc Collections:Elsevier Read and Publish Agreement 2022-2024:Freedom Collection (Reading list)
title Temperature-tuned Maxwell-Boltzmann neutron spectra for kT ranging from 30 up to 50 keV for nuclear astrophysics studies
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-27T21%3A49%3A21IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_pubme&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Temperature-tuned%20Maxwell-Boltzmann%20neutron%20spectra%20for%20kT%20ranging%20from%2030%20up%20to%2050%20keV%20for%20nuclear%20astrophysics%20studies&rft.jtitle=Applied%20radiation%20and%20isotopes&rft.au=Mart%C3%ADn-Hern%C3%A1ndez,%20G&rft.date=2012-08&rft.volume=70&rft.issue=8&rft.spage=1583&rft.epage=1589&rft.pages=1583-1589&rft.eissn=1872-9800&rft_id=info:doi/10.1016/j.apradiso.2012.05.004&rft_dat=%3Cproquest_pubme%3E1024479318%3C/proquest_pubme%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-p141t-1eca15e09c667fc0960fe54d33c50e37f31b6209631f5ed6dd8a0ec9fffd46f83%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1024479318&rft_id=info:pmid/22732394&rfr_iscdi=true