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...
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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 |
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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 < 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 < 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 & 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 & Aerospace Database</collection><collection>ProQuest Advanced Technologies & 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 < 10 keV. 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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 |
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