Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process

We report in this study the nuclear properties of proton-rich isotopes located along the rp-process path. The experiments have recently been performed at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University. The level properties above the proton separation energy of...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Galaviz, D, Amthor, A M, Bazin, D, Becerril, A D, Brown, B A, Chen, A A, Cole, A, Cook, J M, Elliot, T, Estrade, A, Fülöp, Z S, Gade, A, Glasmacher, T, Heger, A, Howard, M E, Kessler, R, Lorusso, G, Matos, M, Montes, F, Müller, W, Pereira, J, Schatz, H, Sherrill, B, Schertz, F, Shimbara, Y, Smith, E, Smith, K, Tamii, A, Stolz, A, Weisshaar, D, Wallace, M, Wiescher, M, Zegers, R G T
Format: Tagungsbericht
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 1
container_start_page 012009
container_title
container_volume 202
creator Galaviz, D
Amthor, A M
Bazin, D
Becerril, A D
Brown, B A
Chen, A A
Cole, A
Cook, J M
Elliot, T
Estrade, A
Fülöp, Z S
Gade, A
Glasmacher, T
Heger, A
Howard, M E
Kessler, R
Lorusso, G
Matos, M
Montes, F
Müller, W
Pereira, J
Schatz, H
Sherrill, B
Schertz, F
Shimbara, Y
Smith, E
Smith, K
Tamii, A
Stolz, A
Weisshaar, D
Wallace, M
Wiescher, M
Zegers, R G T
description We report in this study the nuclear properties of proton-rich isotopes located along the rp-process path. The experiments have recently been performed at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University. The level properties above the proton separation energy of the nuclei 30S, 36K and 37Ca were measured with precision of < 10 keV. This will allow a reduction in the determination of the astrophysical (p,γ) reaction rate under rp-process conditions.
doi_str_mv 10.1088/1742-6596/202/1/012009
format Conference Proceeding
fullrecord <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_journals_2579910118</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2579910118</sourcerecordid><originalsourceid>FETCH-LOGICAL-c399t-c7151b1e97485f9d2c51fb4b0e45aba80804661ff8f077aca156c85b063869cd3</originalsourceid><addsrcrecordid>eNqNkEFLwzAUx4MoOKdfQQoepdt7bZMmxzGmE6Ze9BzSLGEdta1JK-7bm1IZHnYwlxd4v9_jz5-QW4QZAudzzLMkZlSweQLJHOeACYA4I5Pj4vzP_5Jceb8HSMPLJ-T5pdeVafyh7nbGlz5qbNS6pmvq2JV6F9XDupxFq-_WuPLD1J2qImd8X3WBraNgRa6Ng6KN99fkwqrKm5vfOSXvD6u35TrevD4-LRebWKdCdLHOkWKBRuQZp1ZsE03RFlkBJqOqUBw4ZIyhtdxCniutkDLNaQEs5UzobTol9-PdnapkG3Ipd5CNKuV6sZFlnbSpBMhylmb0CwN9N9Ih5WdvfCf3Te_qEFAmNBcCAZEHio2Udo33ztjjYQQ5FC2HDuXQoQxFS5Rj0UHEUSyb9v9OfMI5ycp2a9MfplmLrQ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>conference_proceeding</recordtype><pqid>2579910118</pqid></control><display><type>conference_proceeding</type><title>Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process</title><source>Institute of Physics Open Access Journal Titles</source><creator>Galaviz, D ; Amthor, A M ; Bazin, D ; Becerril, A D ; Brown, B A ; Chen, A A ; Cole, A ; Cook, J M ; Elliot, T ; Estrade, A ; Fülöp, Z S ; Gade, A ; Glasmacher, T ; Heger, A ; Howard, M E ; Kessler, R ; Lorusso, G ; Matos, M ; Montes, F ; Müller, W ; Pereira, J ; Schatz, H ; Sherrill, B ; Schertz, F ; Shimbara, Y ; Smith, E ; Smith, K ; Tamii, A ; Stolz, A ; Weisshaar, D ; Wallace, M ; Wiescher, M ; Zegers, R G T</creator><creatorcontrib>Galaviz, D ; Amthor, A M ; Bazin, D ; Becerril, A D ; Brown, B A ; Chen, A A ; Cole, A ; Cook, J M ; Elliot, T ; Estrade, A ; Fülöp, Z S ; Gade, A ; Glasmacher, T ; Heger, A ; Howard, M E ; Kessler, R ; Lorusso, G ; Matos, M ; Montes, F ; Müller, W ; Pereira, J ; Schatz, H ; Sherrill, B ; Schertz, F ; Shimbara, Y ; Smith, E ; Smith, K ; Tamii, A ; Stolz, A ; Weisshaar, D ; Wallace, M ; Wiescher, M ; Zegers, R G T</creatorcontrib><description>We report in this study the nuclear properties of proton-rich isotopes located along the rp-process path. The experiments have recently been performed at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University. The level properties above the proton separation energy of the nuclei 30S, 36K and 37Ca were measured with precision of &lt; 10 keV. This will allow a reduction in the determination of the astrophysical (p,γ) reaction rate under rp-process conditions.</description><identifier>ISSN: 1742-6596</identifier><identifier>ISSN: 1742-6588</identifier><identifier>EISSN: 1742-6596</identifier><identifier>DOI: 10.1088/1742-6596/202/1/012009</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Astrophysics ; Cyclotrons ; Nuclear fusion ; Nuclear properties ; Nuclei ; Physics ; Protons ; Sciences of the Universe ; Solar and Stellar Astrophysics</subject><ispartof>Journal of physics. Conference series, 2010, Vol.202 (1), p.012009</ispartof><rights>Copyright IOP Publishing Jan 2010</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c399t-c7151b1e97485f9d2c51fb4b0e45aba80804661ff8f077aca156c85b063869cd3</citedby><cites>FETCH-LOGICAL-c399t-c7151b1e97485f9d2c51fb4b0e45aba80804661ff8f077aca156c85b063869cd3</cites><orcidid>0000-0001-8825-0976 ; 0000-0003-0303-3855 ; 0000-0002-9190-3971</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/1742-6596/202/1/012009/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>309,314,780,784,885,1553,4050,27628,27924,27925,53904,53931</link.rule.ids><linktorsrc>$$Uhttp://iopscience.iop.org/1742-6596/202/1/012009$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://in2p3.hal.science/in2p3-00476345$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Galaviz, D</creatorcontrib><creatorcontrib>Amthor, A M</creatorcontrib><creatorcontrib>Bazin, D</creatorcontrib><creatorcontrib>Becerril, A D</creatorcontrib><creatorcontrib>Brown, B A</creatorcontrib><creatorcontrib>Chen, A A</creatorcontrib><creatorcontrib>Cole, A</creatorcontrib><creatorcontrib>Cook, J M</creatorcontrib><creatorcontrib>Elliot, T</creatorcontrib><creatorcontrib>Estrade, A</creatorcontrib><creatorcontrib>Fülöp, Z S</creatorcontrib><creatorcontrib>Gade, A</creatorcontrib><creatorcontrib>Glasmacher, T</creatorcontrib><creatorcontrib>Heger, A</creatorcontrib><creatorcontrib>Howard, M E</creatorcontrib><creatorcontrib>Kessler, R</creatorcontrib><creatorcontrib>Lorusso, G</creatorcontrib><creatorcontrib>Matos, M</creatorcontrib><creatorcontrib>Montes, F</creatorcontrib><creatorcontrib>Müller, W</creatorcontrib><creatorcontrib>Pereira, J</creatorcontrib><creatorcontrib>Schatz, H</creatorcontrib><creatorcontrib>Sherrill, B</creatorcontrib><creatorcontrib>Schertz, F</creatorcontrib><creatorcontrib>Shimbara, Y</creatorcontrib><creatorcontrib>Smith, E</creatorcontrib><creatorcontrib>Smith, K</creatorcontrib><creatorcontrib>Tamii, A</creatorcontrib><creatorcontrib>Stolz, A</creatorcontrib><creatorcontrib>Weisshaar, D</creatorcontrib><creatorcontrib>Wallace, M</creatorcontrib><creatorcontrib>Wiescher, M</creatorcontrib><creatorcontrib>Zegers, R G T</creatorcontrib><title>Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process</title><title>Journal of physics. Conference series</title><description>We report in this study the nuclear properties of proton-rich isotopes located along the rp-process path. The experiments have recently been performed at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University. The level properties above the proton separation energy of the nuclei 30S, 36K and 37Ca were measured with precision of &lt; 10 keV. This will allow a reduction in the determination of the astrophysical (p,γ) reaction rate under rp-process conditions.</description><subject>Astrophysics</subject><subject>Cyclotrons</subject><subject>Nuclear fusion</subject><subject>Nuclear properties</subject><subject>Nuclei</subject><subject>Physics</subject><subject>Protons</subject><subject>Sciences of the Universe</subject><subject>Solar and Stellar Astrophysics</subject><issn>1742-6596</issn><issn>1742-6588</issn><issn>1742-6596</issn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2010</creationdate><recordtype>conference_proceeding</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNkEFLwzAUx4MoOKdfQQoepdt7bZMmxzGmE6Ze9BzSLGEdta1JK-7bm1IZHnYwlxd4v9_jz5-QW4QZAudzzLMkZlSweQLJHOeACYA4I5Pj4vzP_5Jceb8HSMPLJ-T5pdeVafyh7nbGlz5qbNS6pmvq2JV6F9XDupxFq-_WuPLD1J2qImd8X3WBraNgRa6Ng6KN99fkwqrKm5vfOSXvD6u35TrevD4-LRebWKdCdLHOkWKBRuQZp1ZsE03RFlkBJqOqUBw4ZIyhtdxCniutkDLNaQEs5UzobTol9-PdnapkG3Ipd5CNKuV6sZFlnbSpBMhylmb0CwN9N9Ih5WdvfCf3Te_qEFAmNBcCAZEHio2Udo33ztjjYQQ5FC2HDuXQoQxFS5Rj0UHEUSyb9v9OfMI5ycp2a9MfplmLrQ</recordid><startdate>20100101</startdate><enddate>20100101</enddate><creator>Galaviz, D</creator><creator>Amthor, A M</creator><creator>Bazin, D</creator><creator>Becerril, A D</creator><creator>Brown, B A</creator><creator>Chen, A A</creator><creator>Cole, A</creator><creator>Cook, J M</creator><creator>Elliot, T</creator><creator>Estrade, A</creator><creator>Fülöp, Z S</creator><creator>Gade, A</creator><creator>Glasmacher, T</creator><creator>Heger, A</creator><creator>Howard, M E</creator><creator>Kessler, R</creator><creator>Lorusso, G</creator><creator>Matos, M</creator><creator>Montes, F</creator><creator>Müller, W</creator><creator>Pereira, J</creator><creator>Schatz, H</creator><creator>Sherrill, B</creator><creator>Schertz, F</creator><creator>Shimbara, Y</creator><creator>Smith, E</creator><creator>Smith, K</creator><creator>Tamii, A</creator><creator>Stolz, A</creator><creator>Weisshaar, D</creator><creator>Wallace, M</creator><creator>Wiescher, M</creator><creator>Zegers, R G T</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</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>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0001-8825-0976</orcidid><orcidid>https://orcid.org/0000-0003-0303-3855</orcidid><orcidid>https://orcid.org/0000-0002-9190-3971</orcidid></search><sort><creationdate>20100101</creationdate><title>Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process</title><author>Galaviz, D ; Amthor, A M ; Bazin, D ; Becerril, A D ; Brown, B A ; Chen, A A ; Cole, A ; Cook, J M ; Elliot, T ; Estrade, A ; Fülöp, Z S ; Gade, A ; Glasmacher, T ; Heger, A ; Howard, M E ; Kessler, R ; Lorusso, G ; Matos, M ; Montes, F ; Müller, W ; Pereira, J ; Schatz, H ; Sherrill, B ; Schertz, F ; Shimbara, Y ; Smith, E ; Smith, K ; Tamii, A ; Stolz, A ; Weisshaar, D ; Wallace, M ; Wiescher, M ; Zegers, R G T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c399t-c7151b1e97485f9d2c51fb4b0e45aba80804661ff8f077aca156c85b063869cd3</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Astrophysics</topic><topic>Cyclotrons</topic><topic>Nuclear fusion</topic><topic>Nuclear properties</topic><topic>Nuclei</topic><topic>Physics</topic><topic>Protons</topic><topic>Sciences of the Universe</topic><topic>Solar and Stellar Astrophysics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Galaviz, D</creatorcontrib><creatorcontrib>Amthor, A M</creatorcontrib><creatorcontrib>Bazin, D</creatorcontrib><creatorcontrib>Becerril, A D</creatorcontrib><creatorcontrib>Brown, B A</creatorcontrib><creatorcontrib>Chen, A A</creatorcontrib><creatorcontrib>Cole, A</creatorcontrib><creatorcontrib>Cook, J M</creatorcontrib><creatorcontrib>Elliot, T</creatorcontrib><creatorcontrib>Estrade, A</creatorcontrib><creatorcontrib>Fülöp, Z S</creatorcontrib><creatorcontrib>Gade, A</creatorcontrib><creatorcontrib>Glasmacher, T</creatorcontrib><creatorcontrib>Heger, A</creatorcontrib><creatorcontrib>Howard, M E</creatorcontrib><creatorcontrib>Kessler, R</creatorcontrib><creatorcontrib>Lorusso, G</creatorcontrib><creatorcontrib>Matos, M</creatorcontrib><creatorcontrib>Montes, F</creatorcontrib><creatorcontrib>Müller, W</creatorcontrib><creatorcontrib>Pereira, J</creatorcontrib><creatorcontrib>Schatz, H</creatorcontrib><creatorcontrib>Sherrill, B</creatorcontrib><creatorcontrib>Schertz, F</creatorcontrib><creatorcontrib>Shimbara, Y</creatorcontrib><creatorcontrib>Smith, E</creatorcontrib><creatorcontrib>Smith, K</creatorcontrib><creatorcontrib>Tamii, A</creatorcontrib><creatorcontrib>Stolz, A</creatorcontrib><creatorcontrib>Weisshaar, D</creatorcontrib><creatorcontrib>Wallace, M</creatorcontrib><creatorcontrib>Wiescher, M</creatorcontrib><creatorcontrib>Zegers, R G T</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Access via ProQuest (Open Access)</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>Hyper Article en Ligne (HAL)</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Galaviz, D</au><au>Amthor, A M</au><au>Bazin, D</au><au>Becerril, A D</au><au>Brown, B A</au><au>Chen, A A</au><au>Cole, A</au><au>Cook, J M</au><au>Elliot, T</au><au>Estrade, A</au><au>Fülöp, Z S</au><au>Gade, A</au><au>Glasmacher, T</au><au>Heger, A</au><au>Howard, M E</au><au>Kessler, R</au><au>Lorusso, G</au><au>Matos, M</au><au>Montes, F</au><au>Müller, W</au><au>Pereira, J</au><au>Schatz, H</au><au>Sherrill, B</au><au>Schertz, F</au><au>Shimbara, Y</au><au>Smith, E</au><au>Smith, K</au><au>Tamii, A</au><au>Stolz, A</au><au>Weisshaar, D</au><au>Wallace, M</au><au>Wiescher, M</au><au>Zegers, R G T</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process</atitle><btitle>Journal of physics. Conference series</btitle><date>2010-01-01</date><risdate>2010</risdate><volume>202</volume><issue>1</issue><spage>012009</spage><pages>012009-</pages><issn>1742-6596</issn><issn>1742-6588</issn><eissn>1742-6596</eissn><abstract>We report in this study the nuclear properties of proton-rich isotopes located along the rp-process path. The experiments have recently been performed at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University. The level properties above the proton separation energy of the nuclei 30S, 36K and 37Ca were measured with precision of &lt; 10 keV. This will allow a reduction in the determination of the astrophysical (p,γ) reaction rate under rp-process conditions.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1742-6596/202/1/012009</doi><orcidid>https://orcid.org/0000-0001-8825-0976</orcidid><orcidid>https://orcid.org/0000-0003-0303-3855</orcidid><orcidid>https://orcid.org/0000-0002-9190-3971</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier ISSN: 1742-6596
ispartof Journal of physics. Conference series, 2010, Vol.202 (1), p.012009
issn 1742-6596
1742-6588
1742-6596
language eng
recordid cdi_proquest_journals_2579910118
source Institute of Physics Open Access Journal Titles
subjects Astrophysics
Cyclotrons
Nuclear fusion
Nuclear properties
Nuclei
Physics
Protons
Sciences of the Universe
Solar and Stellar Astrophysics
title Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-01T16%3A04%3A54IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=proceeding&rft.atitle=Nucleosynthesis%20of%20proton-rich%20nuclei.%20Experimental%20results%20on%20the%20rp-process&rft.btitle=Journal%20of%20physics.%20Conference%20series&rft.au=Galaviz,%20D&rft.date=2010-01-01&rft.volume=202&rft.issue=1&rft.spage=012009&rft.pages=012009-&rft.issn=1742-6596&rft.eissn=1742-6596&rft_id=info:doi/10.1088/1742-6596/202/1/012009&rft_dat=%3Cproquest_O3W%3E2579910118%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2579910118&rft_id=info:pmid/&rfr_iscdi=true