Loading…

Investigation of Alpha-Induced Reactions on 107Ag at Astrophysical Energies

Cross sections of the 107Ag(α, γ)111In and 107Ag(α,n)110In reactions have been measured with the activation method at effective center-of-mass energies between 7.79 MeV and 12.00 MeV close to the astrophysical energy range. The irradiation and counting of the 107Ag targets was carried out at ATOMKI...

Full description

Saved in:
Bibliographic Details
Published in:Journal of physics. Conference series 2016-01, Vol.665 (1)
Main Authors: Yalçin, C, Özkan, N, Güray, R T, Gyürky, Gy, Kiss, G G, Szücs, T, Haiász, Z, Fülöp, Zs, Farkas, J, Somorjai, E, Korkulu, Z, Rauscher, T
Format: Article
Language:English
Subjects:
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 1
container_start_page
container_title Journal of physics. Conference series
container_volume 665
creator Yalçin, C
Özkan, N
Güray, R T
Gyürky, Gy
Kiss, G G
Szücs, T
Haiász, Z
Fülöp, Zs
Farkas, J
Somorjai, E
Korkulu, Z
Rauscher, T
description Cross sections of the 107Ag(α, γ)111In and 107Ag(α,n)110In reactions have been measured with the activation method at effective center-of-mass energies between 7.79 MeV and 12.00 MeV close to the astrophysical energy range. The irradiation and counting of the 107Ag targets was carried out at ATOMKI using the cyclotron accelerator and the low background counting facility, respectively. Cross section results are presented and compared with the predictions of Hauser-Feshbach statistical model calculations using the NON-SMOKER and TALYS-1.4 codes. In general, above 10 MeV, the model calculation are able to reproduce reasonably well the experimental data, but below 10 MeV, depending on some input parameters strong deviations are also found.
doi_str_mv 10.1088/1742-6596/665/1/012043
format article
fullrecord <record><control><sourceid>proquest_iop_j</sourceid><recordid>TN_cdi_proquest_journals_2574945790</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2574945790</sourcerecordid><originalsourceid>FETCH-LOGICAL-i710-48cfcbae0a0129d8521b8c99a05f6fe149539191b3a40e7aa8b8121f231e170c3</originalsourceid><addsrcrecordid>eNpFkF9LwzAUxYMoOKdfQQI-196bP03yWMbU4UCQvYc0S7eO0damE_z2pkzmfTkXzuHew4-QR4RnBK1zVIJlhTRFXhQyxxyQgeBXZHYxri-71rfkLsYDAE-jZuR91X6HODY7NzZdS7ualsd-77JVuz35sKWfwfnJiTS5CKrcUTfSMo5D1-9_YuPdkS7bMOyaEO_JTe2OMTz86ZxsXpabxVu2_nhdLcp11iiETGhf-8oFcKmo2WrJsNLeGAeyLuqAwkhu0GDFnYCgnNOVRoY14xhQgedz8nQ-2w_d1ymVt4fuNLTpo2VSCSOkMpBS7Jxquv4_gGAnZnbCYSc0NjGzaM_M-C8O6F1h</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2574945790</pqid></control><display><type>article</type><title>Investigation of Alpha-Induced Reactions on 107Ag at Astrophysical Energies</title><source>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</source><source>Full-Text Journals in Chemistry (Open access)</source><creator>Yalçin, C ; Özkan, N ; Güray, R T ; Gyürky, Gy ; Kiss, G G ; Szücs, T ; Haiász, Z ; Fülöp, Zs ; Farkas, J ; Somorjai, E ; Korkulu, Z ; Rauscher, T</creator><creatorcontrib>Yalçin, C ; Özkan, N ; Güray, R T ; Gyürky, Gy ; Kiss, G G ; Szücs, T ; Haiász, Z ; Fülöp, Zs ; Farkas, J ; Somorjai, E ; Korkulu, Z ; Rauscher, T</creatorcontrib><description>Cross sections of the 107Ag(α, γ)111In and 107Ag(α,n)110In reactions have been measured with the activation method at effective center-of-mass energies between 7.79 MeV and 12.00 MeV close to the astrophysical energy range. The irradiation and counting of the 107Ag targets was carried out at ATOMKI using the cyclotron accelerator and the low background counting facility, respectively. Cross section results are presented and compared with the predictions of Hauser-Feshbach statistical model calculations using the NON-SMOKER and TALYS-1.4 codes. In general, above 10 MeV, the model calculation are able to reproduce reasonably well the experimental data, but below 10 MeV, depending on some input parameters strong deviations are also found.</description><identifier>ISSN: 1742-6588</identifier><identifier>EISSN: 1742-6596</identifier><identifier>DOI: 10.1088/1742-6596/665/1/012043</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Cross-sections ; Cyclotrons ; Physics ; Statistical models</subject><ispartof>Journal of physics. Conference series, 2016-01, Vol.665 (1)</ispartof><rights>Published under licence by IOP Publishing Ltd</rights><rights>2016. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><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/2574945790?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25753,27924,27925,37012,44590</link.rule.ids></links><search><creatorcontrib>Yalçin, C</creatorcontrib><creatorcontrib>Özkan, N</creatorcontrib><creatorcontrib>Güray, R T</creatorcontrib><creatorcontrib>Gyürky, Gy</creatorcontrib><creatorcontrib>Kiss, G G</creatorcontrib><creatorcontrib>Szücs, T</creatorcontrib><creatorcontrib>Haiász, Z</creatorcontrib><creatorcontrib>Fülöp, Zs</creatorcontrib><creatorcontrib>Farkas, J</creatorcontrib><creatorcontrib>Somorjai, E</creatorcontrib><creatorcontrib>Korkulu, Z</creatorcontrib><creatorcontrib>Rauscher, T</creatorcontrib><title>Investigation of Alpha-Induced Reactions on 107Ag at Astrophysical Energies</title><title>Journal of physics. Conference series</title><addtitle>J. Phys.: Conf. Ser</addtitle><description>Cross sections of the 107Ag(α, γ)111In and 107Ag(α,n)110In reactions have been measured with the activation method at effective center-of-mass energies between 7.79 MeV and 12.00 MeV close to the astrophysical energy range. The irradiation and counting of the 107Ag targets was carried out at ATOMKI using the cyclotron accelerator and the low background counting facility, respectively. Cross section results are presented and compared with the predictions of Hauser-Feshbach statistical model calculations using the NON-SMOKER and TALYS-1.4 codes. In general, above 10 MeV, the model calculation are able to reproduce reasonably well the experimental data, but below 10 MeV, depending on some input parameters strong deviations are also found.</description><subject>Cross-sections</subject><subject>Cyclotrons</subject><subject>Physics</subject><subject>Statistical models</subject><issn>1742-6588</issn><issn>1742-6596</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNpFkF9LwzAUxYMoOKdfQQI-196bP03yWMbU4UCQvYc0S7eO0damE_z2pkzmfTkXzuHew4-QR4RnBK1zVIJlhTRFXhQyxxyQgeBXZHYxri-71rfkLsYDAE-jZuR91X6HODY7NzZdS7ualsd-77JVuz35sKWfwfnJiTS5CKrcUTfSMo5D1-9_YuPdkS7bMOyaEO_JTe2OMTz86ZxsXpabxVu2_nhdLcp11iiETGhf-8oFcKmo2WrJsNLeGAeyLuqAwkhu0GDFnYCgnNOVRoY14xhQgedz8nQ-2w_d1ymVt4fuNLTpo2VSCSOkMpBS7Jxquv4_gGAnZnbCYSc0NjGzaM_M-C8O6F1h</recordid><startdate>20160105</startdate><enddate>20160105</enddate><creator>Yalçin, C</creator><creator>Özkan, N</creator><creator>Güray, R T</creator><creator>Gyürky, Gy</creator><creator>Kiss, G G</creator><creator>Szücs, T</creator><creator>Haiász, Z</creator><creator>Fülöp, Zs</creator><creator>Farkas, J</creator><creator>Somorjai, E</creator><creator>Korkulu, Z</creator><creator>Rauscher, T</creator><general>IOP Publishing</general><scope>O3W</scope><scope>TSCCA</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></search><sort><creationdate>20160105</creationdate><title>Investigation of Alpha-Induced Reactions on 107Ag at Astrophysical Energies</title><author>Yalçin, C ; Özkan, N ; Güray, R T ; Gyürky, Gy ; Kiss, G G ; Szücs, T ; Haiász, Z ; Fülöp, Zs ; Farkas, J ; Somorjai, E ; Korkulu, Z ; Rauscher, T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-i710-48cfcbae0a0129d8521b8c99a05f6fe149539191b3a40e7aa8b8121f231e170c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Cross-sections</topic><topic>Cyclotrons</topic><topic>Physics</topic><topic>Statistical models</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Yalçin, C</creatorcontrib><creatorcontrib>Özkan, N</creatorcontrib><creatorcontrib>Güray, R T</creatorcontrib><creatorcontrib>Gyürky, Gy</creatorcontrib><creatorcontrib>Kiss, G G</creatorcontrib><creatorcontrib>Szücs, T</creatorcontrib><creatorcontrib>Haiász, Z</creatorcontrib><creatorcontrib>Fülöp, Zs</creatorcontrib><creatorcontrib>Farkas, J</creatorcontrib><creatorcontrib>Somorjai, E</creatorcontrib><creatorcontrib>Korkulu, Z</creatorcontrib><creatorcontrib>Rauscher, T</creatorcontrib><collection>IOP Publishing Free Content</collection><collection>IOPscience (Open Access)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</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 (Proquest) (PQ_SDU_P3)</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest advanced technologies &amp; aerospace journals</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</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><jtitle>Journal of physics. Conference series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Yalçin, C</au><au>Özkan, N</au><au>Güray, R T</au><au>Gyürky, Gy</au><au>Kiss, G G</au><au>Szücs, T</au><au>Haiász, Z</au><au>Fülöp, Zs</au><au>Farkas, J</au><au>Somorjai, E</au><au>Korkulu, Z</au><au>Rauscher, T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Investigation of Alpha-Induced Reactions on 107Ag at Astrophysical Energies</atitle><jtitle>Journal of physics. Conference series</jtitle><addtitle>J. Phys.: Conf. Ser</addtitle><date>2016-01-05</date><risdate>2016</risdate><volume>665</volume><issue>1</issue><issn>1742-6588</issn><eissn>1742-6596</eissn><abstract>Cross sections of the 107Ag(α, γ)111In and 107Ag(α,n)110In reactions have been measured with the activation method at effective center-of-mass energies between 7.79 MeV and 12.00 MeV close to the astrophysical energy range. The irradiation and counting of the 107Ag targets was carried out at ATOMKI using the cyclotron accelerator and the low background counting facility, respectively. Cross section results are presented and compared with the predictions of Hauser-Feshbach statistical model calculations using the NON-SMOKER and TALYS-1.4 codes. In general, above 10 MeV, the model calculation are able to reproduce reasonably well the experimental data, but below 10 MeV, depending on some input parameters strong deviations are also found.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1742-6596/665/1/012043</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1742-6588
ispartof Journal of physics. Conference series, 2016-01, Vol.665 (1)
issn 1742-6588
1742-6596
language eng
recordid cdi_proquest_journals_2574945790
source Publicly Available Content Database (Proquest) (PQ_SDU_P3); Full-Text Journals in Chemistry (Open access)
subjects Cross-sections
Cyclotrons
Physics
Statistical models
title Investigation of Alpha-Induced Reactions on 107Ag at Astrophysical Energies
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T19%3A27%3A51IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_iop_j&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Investigation%20of%20Alpha-Induced%20Reactions%20on%20107Ag%20at%20Astrophysical%20Energies&rft.jtitle=Journal%20of%20physics.%20Conference%20series&rft.au=Yal%C3%A7in,%20C&rft.date=2016-01-05&rft.volume=665&rft.issue=1&rft.issn=1742-6588&rft.eissn=1742-6596&rft_id=info:doi/10.1088/1742-6596/665/1/012043&rft_dat=%3Cproquest_iop_j%3E2574945790%3C/proquest_iop_j%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-i710-48cfcbae0a0129d8521b8c99a05f6fe149539191b3a40e7aa8b8121f231e170c3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2574945790&rft_id=info:pmid/&rfr_iscdi=true