Secondary Nuclei from Peripheral and Ultraperipheral Collisions of Relativistic Heavy Ions
The production of heavy secondary nuclei in 197 Au– 197 Au collisions at NICA and in 129 Xe– 129 Xe and 208 Pb– 208 Pb collisions at the LHC is calculated by means of Glauber Monte Carlo model connected with nuclear de-excitation models from Geant4 toolkit. The production of secondary nuclei in ultr...
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| Veröffentlicht in: | Bulletin of the Russian Academy of Sciences. Physics 2020-08, Vol.84 (8), p.1007-1011 |
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| container_title | Bulletin of the Russian Academy of Sciences. Physics |
| container_volume | 84 |
| creator | Pshenichnov, I. A. Dmitrieva, U. A. Svetlichnyi, A. O. |
| description | The production of heavy secondary nuclei in
197
Au–
197
Au collisions at NICA and in
129
Xe–
129
Xe and
208
Pb–
208
Pb collisions at the LHC is calculated by means of Glauber Monte Carlo model connected with nuclear de-excitation models from Geant4 toolkit. The production of secondary nuclei in ultraperipheral heavy-ion collisions is additionally simulated with the RELDIS model, which predicts the dominance of neutron emission in the electromagnetic interactions of the considered nuclei. As found, Te, I and Au, Hg, Tl nuclei are frequently produced, respectively, in decays of
129
Xe and
208
Pb excited electromagnetically at the LHC. In contrast, mostly gold isotopes are produced in ultraperipheral collisions at NICA. A possible impact of secondary nuclei on collider components is discussed. |
| doi_str_mv | 10.3103/S1062873820080249 |
| format | Article |
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197
Au–
197
Au collisions at NICA and in
129
Xe–
129
Xe and
208
Pb–
208
Pb collisions at the LHC is calculated by means of Glauber Monte Carlo model connected with nuclear de-excitation models from Geant4 toolkit. The production of secondary nuclei in ultraperipheral heavy-ion collisions is additionally simulated with the RELDIS model, which predicts the dominance of neutron emission in the electromagnetic interactions of the considered nuclei. As found, Te, I and Au, Hg, Tl nuclei are frequently produced, respectively, in decays of
129
Xe and
208
Pb excited electromagnetically at the LHC. In contrast, mostly gold isotopes are produced in ultraperipheral collisions at NICA. A possible impact of secondary nuclei on collider components is discussed.</description><identifier>ISSN: 1062-8738</identifier><identifier>EISSN: 1934-9432</identifier><identifier>DOI: 10.3103/S1062873820080249</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Atomic collisions ; Electromagnetic interactions ; Gold isotopes ; Hadrons ; Heavy Ions ; Ionic collisions ; Large Hadron Collider ; Lead isotopes ; Neutron emission ; Nuclear Physics ; Physics ; Physics and Astronomy ; Toolkits ; Xenon 129</subject><ispartof>Bulletin of the Russian Academy of Sciences. Physics, 2020-08, Vol.84 (8), p.1007-1011</ispartof><rights>Allerton Press, Inc. 2020</rights><rights>Allerton Press, Inc. 2020.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c2319-fdd550aa2a761e60118b9342d993f922428b819073f7e25b931113e35011cafb3</citedby><cites>FETCH-LOGICAL-c2319-fdd550aa2a761e60118b9342d993f922428b819073f7e25b931113e35011cafb3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.3103/S1062873820080249$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.3103/S1062873820080249$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Pshenichnov, I. A.</creatorcontrib><creatorcontrib>Dmitrieva, U. A.</creatorcontrib><creatorcontrib>Svetlichnyi, A. O.</creatorcontrib><title>Secondary Nuclei from Peripheral and Ultraperipheral Collisions of Relativistic Heavy Ions</title><title>Bulletin of the Russian Academy of Sciences. Physics</title><addtitle>Bull. Russ. Acad. Sci. Phys</addtitle><description>The production of heavy secondary nuclei in
197
Au–
197
Au collisions at NICA and in
129
Xe–
129
Xe and
208
Pb–
208
Pb collisions at the LHC is calculated by means of Glauber Monte Carlo model connected with nuclear de-excitation models from Geant4 toolkit. The production of secondary nuclei in ultraperipheral heavy-ion collisions is additionally simulated with the RELDIS model, which predicts the dominance of neutron emission in the electromagnetic interactions of the considered nuclei. As found, Te, I and Au, Hg, Tl nuclei are frequently produced, respectively, in decays of
129
Xe and
208
Pb excited electromagnetically at the LHC. In contrast, mostly gold isotopes are produced in ultraperipheral collisions at NICA. A possible impact of secondary nuclei on collider components is discussed.</description><subject>Atomic collisions</subject><subject>Electromagnetic interactions</subject><subject>Gold isotopes</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Ionic collisions</subject><subject>Large Hadron Collider</subject><subject>Lead isotopes</subject><subject>Neutron emission</subject><subject>Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Toolkits</subject><subject>Xenon 129</subject><issn>1062-8738</issn><issn>1934-9432</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp1UN9LwzAQDqLgnP4BvgV8ruYuTds8ylA3GCrOvfhS0jbRjK6pSTfYf2_GhD2IT3fc9-PuPkKugd1yYPxuASzDIucFMlYwTOUJGYHkaSJTjqexj3Cyx8_JRQgrxoSQKEbkY6Fr1zXK7-jzpm61pca7NX3V3vZf2quWqq6hy3bwqj_OJq5tbbCuC9QZ-qZbNditDYOt6VSr7Y7OInRJzoxqg776rWOyfHx4n0yT-cvTbHI_T2rkIBPTNEIwpVDlGeiMARRVPBwbKbmRiCkWVQGS5dzkGkXEAIBrLiKzVqbiY3Jz8O29-97oMJQrt_FdXFliKliKacYhsuDAqr0LwWtT9t6u498lsHIfYfknwqjBgyZEbvep_dH5f9EPdGlxyw</recordid><startdate>20200801</startdate><enddate>20200801</enddate><creator>Pshenichnov, I. A.</creator><creator>Dmitrieva, U. A.</creator><creator>Svetlichnyi, A. O.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20200801</creationdate><title>Secondary Nuclei from Peripheral and Ultraperipheral Collisions of Relativistic Heavy Ions</title><author>Pshenichnov, I. A. ; Dmitrieva, U. A. ; Svetlichnyi, A. O.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2319-fdd550aa2a761e60118b9342d993f922428b819073f7e25b931113e35011cafb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Atomic collisions</topic><topic>Electromagnetic interactions</topic><topic>Gold isotopes</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Ionic collisions</topic><topic>Large Hadron Collider</topic><topic>Lead isotopes</topic><topic>Neutron emission</topic><topic>Nuclear Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Toolkits</topic><topic>Xenon 129</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pshenichnov, I. A.</creatorcontrib><creatorcontrib>Dmitrieva, U. A.</creatorcontrib><creatorcontrib>Svetlichnyi, A. O.</creatorcontrib><collection>CrossRef</collection><jtitle>Bulletin of the Russian Academy of Sciences. Physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pshenichnov, I. A.</au><au>Dmitrieva, U. A.</au><au>Svetlichnyi, A. O.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Secondary Nuclei from Peripheral and Ultraperipheral Collisions of Relativistic Heavy Ions</atitle><jtitle>Bulletin of the Russian Academy of Sciences. Physics</jtitle><stitle>Bull. Russ. Acad. Sci. Phys</stitle><date>2020-08-01</date><risdate>2020</risdate><volume>84</volume><issue>8</issue><spage>1007</spage><epage>1011</epage><pages>1007-1011</pages><issn>1062-8738</issn><eissn>1934-9432</eissn><abstract>The production of heavy secondary nuclei in
197
Au–
197
Au collisions at NICA and in
129
Xe–
129
Xe and
208
Pb–
208
Pb collisions at the LHC is calculated by means of Glauber Monte Carlo model connected with nuclear de-excitation models from Geant4 toolkit. The production of secondary nuclei in ultraperipheral heavy-ion collisions is additionally simulated with the RELDIS model, which predicts the dominance of neutron emission in the electromagnetic interactions of the considered nuclei. As found, Te, I and Au, Hg, Tl nuclei are frequently produced, respectively, in decays of
129
Xe and
208
Pb excited electromagnetically at the LHC. In contrast, mostly gold isotopes are produced in ultraperipheral collisions at NICA. A possible impact of secondary nuclei on collider components is discussed.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.3103/S1062873820080249</doi><tpages>5</tpages></addata></record> |
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| ispartof | Bulletin of the Russian Academy of Sciences. Physics, 2020-08, Vol.84 (8), p.1007-1011 |
| issn | 1062-8738 1934-9432 |
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| source | SpringerLink Journals - AutoHoldings |
| subjects | Atomic collisions Electromagnetic interactions Gold isotopes Hadrons Heavy Ions Ionic collisions Large Hadron Collider Lead isotopes Neutron emission Nuclear Physics Physics Physics and Astronomy Toolkits Xenon 129 |
| title | Secondary Nuclei from Peripheral and Ultraperipheral Collisions of Relativistic Heavy Ions |
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