Modeling the Radiolysis of Supercritical Water by Fast Neutrons: Density Dependence of the Yields of Primary Species at 400°C
A reliable understanding of radiolysis processes in supercritical water (SCW)-cooled reactors is crucial to developing chemistry control strategies that minimize the corrosion and degradation of materials. However, directly measuring the chemistry in reactor cores is difficult due to the extreme con...
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description | A reliable understanding of radiolysis processes in supercritical water (SCW)-cooled reactors is crucial to developing chemistry control strategies that minimize the corrosion and degradation of materials. However, directly measuring the chemistry in reactor cores is difficult due to the extreme conditions of high temperature and pressure and mixed neutron and gamma-radiation fields, which are incompatible with normal chemical instrumentation. Thus, chemical models and computer simulations are an important route of investigation for predicting the detailed radiation chemistry of the coolant in a SCW reactor and the consequences for materials. Surprisingly, information on the fast neutron radiolysis of water at high temperatures is limited, and even more so for fast neutron irradiation of SCW. In this work, Monte Carlo simulations were used to predict the G values for the primary species e–aq, H•, H2, •OH and H2O2 formed from the radiolysis of pure, deaerated SCW (H2O) by 2 MeV monoenergetic neutrons at 400°C as a function of water density in the range of ∼0.15–0.6 g/cm3. The 2 MeV neutron was taken as representative of a fast neutron flux in a reactor. For light water, the moderation of these neutrons after knock-on collisions with water molecules generated mostly recoil protons of 1.264, 0.465, 0.171 and 0.063 MeV. Neglecting oxygen ion recoils and assuming that the most significant contribution to the radiolysis came from these first four recoil protons, the fast neutron yields were estimated as the sum of the G values for these protons after appropriate weightings were applied according to their energy. Calculated yields were compared with available experimental data and with data obtained for low-LET radiation. Most interestingly, the reaction of H• atoms with water was found to play a critical role in the formation yields of H2 and •OH at 400°C. Recent work has underscored the potential importance of this reaction above 200°C, but its rate constant is still controversial. |
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However, directly measuring the chemistry in reactor cores is difficult due to the extreme conditions of high temperature and pressure and mixed neutron and gamma-radiation fields, which are incompatible with normal chemical instrumentation. Thus, chemical models and computer simulations are an important route of investigation for predicting the detailed radiation chemistry of the coolant in a SCW reactor and the consequences for materials. Surprisingly, information on the fast neutron radiolysis of water at high temperatures is limited, and even more so for fast neutron irradiation of SCW. In this work, Monte Carlo simulations were used to predict the G values for the primary species e–aq, H•, H2, •OH and H2O2 formed from the radiolysis of pure, deaerated SCW (H2O) by 2 MeV monoenergetic neutrons at 400°C as a function of water density in the range of ∼0.15–0.6 g/cm3. The 2 MeV neutron was taken as representative of a fast neutron flux in a reactor. For light water, the moderation of these neutrons after knock-on collisions with water molecules generated mostly recoil protons of 1.264, 0.465, 0.171 and 0.063 MeV. Neglecting oxygen ion recoils and assuming that the most significant contribution to the radiolysis came from these first four recoil protons, the fast neutron yields were estimated as the sum of the G values for these protons after appropriate weightings were applied according to their energy. Calculated yields were compared with available experimental data and with data obtained for low-LET radiation. Most interestingly, the reaction of H• atoms with water was found to play a critical role in the formation yields of H2 and •OH at 400°C. Recent work has underscored the potential importance of this reaction above 200°C, but its rate constant is still controversial.</description><identifier>ISSN: 0033-7587</identifier><identifier>EISSN: 1938-5404</identifier><identifier>DOI: 10.1667/RR13715.1</identifier><identifier>PMID: 25409127</identifier><language>eng</language><publisher>United States: The Radiation Research Society</publisher><subject>Chemicals ; Density dependence ; Fast Neutrons ; High temperature ; Hot Temperature ; Hydrogen peroxide ; Kinetics ; Monte Carlo Method ; Monte Carlo methods ; Monte Carlo simulation ; Neutrons ; Protons ; Radiochemistry ; Radiolysis ; Recoil protons ; Scavenging ; SHORT COMMUNICATION ; Space life sciences ; Water - chemistry</subject><ispartof>Radiation research, 2014-12, Vol.182 (6), p.695-704</ispartof><rights>Copyright © 2014 Radiation Research Society</rights><rights>Copyright Allen Press Publishing Services Dec 2014</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-b282t-3385f7da7c1f7e7f85e4ac59c46f85998a8e84958e6b15d33a84f226a8cc31f23</citedby><cites>FETCH-LOGICAL-b282t-3385f7da7c1f7e7f85e4ac59c46f85998a8e84958e6b15d33a84f226a8cc31f23</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/24545414$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/24545414$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,776,780,799,27903,27904,57995,58228</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/25409127$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Butarbutar, Sofia Loren</creatorcontrib><creatorcontrib>Meesungnoen, Jintana</creatorcontrib><creatorcontrib>Guzonas, David A.</creatorcontrib><creatorcontrib>Stuart, Craig R.</creatorcontrib><creatorcontrib>Jay-Gerin, Jean-Paul</creatorcontrib><title>Modeling the Radiolysis of Supercritical Water by Fast Neutrons: Density Dependence of the Yields of Primary Species at 400°C</title><title>Radiation research</title><addtitle>Radiat Res</addtitle><description>A reliable understanding of radiolysis processes in supercritical water (SCW)-cooled reactors is crucial to developing chemistry control strategies that minimize the corrosion and degradation of materials. However, directly measuring the chemistry in reactor cores is difficult due to the extreme conditions of high temperature and pressure and mixed neutron and gamma-radiation fields, which are incompatible with normal chemical instrumentation. Thus, chemical models and computer simulations are an important route of investigation for predicting the detailed radiation chemistry of the coolant in a SCW reactor and the consequences for materials. Surprisingly, information on the fast neutron radiolysis of water at high temperatures is limited, and even more so for fast neutron irradiation of SCW. In this work, Monte Carlo simulations were used to predict the G values for the primary species e–aq, H•, H2, •OH and H2O2 formed from the radiolysis of pure, deaerated SCW (H2O) by 2 MeV monoenergetic neutrons at 400°C as a function of water density in the range of ∼0.15–0.6 g/cm3. The 2 MeV neutron was taken as representative of a fast neutron flux in a reactor. For light water, the moderation of these neutrons after knock-on collisions with water molecules generated mostly recoil protons of 1.264, 0.465, 0.171 and 0.063 MeV. Neglecting oxygen ion recoils and assuming that the most significant contribution to the radiolysis came from these first four recoil protons, the fast neutron yields were estimated as the sum of the G values for these protons after appropriate weightings were applied according to their energy. Calculated yields were compared with available experimental data and with data obtained for low-LET radiation. Most interestingly, the reaction of H• atoms with water was found to play a critical role in the formation yields of H2 and •OH at 400°C. Recent work has underscored the potential importance of this reaction above 200°C, but its rate constant is still controversial.</description><subject>Chemicals</subject><subject>Density dependence</subject><subject>Fast Neutrons</subject><subject>High temperature</subject><subject>Hot Temperature</subject><subject>Hydrogen peroxide</subject><subject>Kinetics</subject><subject>Monte Carlo Method</subject><subject>Monte Carlo methods</subject><subject>Monte Carlo simulation</subject><subject>Neutrons</subject><subject>Protons</subject><subject>Radiochemistry</subject><subject>Radiolysis</subject><subject>Recoil protons</subject><subject>Scavenging</subject><subject>SHORT COMMUNICATION</subject><subject>Space life sciences</subject><subject>Water - chemistry</subject><issn>0033-7587</issn><issn>1938-5404</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>EIF</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp9kcFu1DAQhq0K1C6FAw8AstQDcEixYzu2e0MLBaQW0LYIcYocZwJeZePUdg574Zl4Bp4Mb7OA1APyYWz93_zj0Y_QY0pOaVXJl6sVZZKKU3qAFlQzVQhO-D20IISxQgolj9CDGNckv2mlD9FRmQFNS7lAPy59C70bvuH0HfDKtM732-gi9h2-mkYINrjkrOnxF5Mg4GaLz01M-ANMKfghnuHXMESXtrmOMLQwWNj17ty-OujbW6dPwW1M2OKrEayDiE3CnJBfP5cP0f3O9BEe7esx-nz-5nr5rrj4-Pb98tVF0ZSqTAVjSnSyNdLSToLslABurNCWV_mutTIKFNdCQdVQ0TJmFO_KsjLKWka7kh2j57PvGPzNBDHVGxct9L0ZwE-xphWTQmhJZEZP7qBrP4Uh_y5TXBNVUrIzfDFTNvgYA3T1OO9YU1LvQqn3odQ0s0_3jlOzgfYv-SeFDDyZgXVMPvzTuciH8qw_m_XGeT_Af0b9BhJdnGo</recordid><startdate>201412</startdate><enddate>201412</enddate><creator>Butarbutar, Sofia Loren</creator><creator>Meesungnoen, Jintana</creator><creator>Guzonas, David A.</creator><creator>Stuart, Craig R.</creator><creator>Jay-Gerin, Jean-Paul</creator><general>The Radiation Research Society</general><general>Radiation Research Society</general><general>Allen Press Inc</general><scope>CGR</scope><scope>CUY</scope><scope>CVF</scope><scope>ECM</scope><scope>EIF</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7QF</scope><scope>7QP</scope><scope>7QQ</scope><scope>7QR</scope><scope>7RV</scope><scope>7SC</scope><scope>7SE</scope><scope>7SP</scope><scope>7SR</scope><scope>7TA</scope><scope>7TB</scope><scope>7TK</scope><scope>7U5</scope><scope>7U7</scope><scope>7X7</scope><scope>7XB</scope><scope>88E</scope><scope>8BQ</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F28</scope><scope>FR3</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>H8G</scope><scope>HCIFZ</scope><scope>JG9</scope><scope>JQ2</scope><scope>K9.</scope><scope>KB0</scope><scope>KR7</scope><scope>L7M</scope><scope>LK8</scope><scope>L~C</scope><scope>L~D</scope><scope>M0S</scope><scope>M1P</scope><scope>M7P</scope><scope>NAPCQ</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>7X8</scope></search><sort><creationdate>201412</creationdate><title>Modeling the Radiolysis of Supercritical Water by Fast Neutrons: Density Dependence of the Yields of Primary Species at 400°C</title><author>Butarbutar, Sofia Loren ; Meesungnoen, Jintana ; Guzonas, David A. ; Stuart, Craig R. ; Jay-Gerin, Jean-Paul</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-b282t-3385f7da7c1f7e7f85e4ac59c46f85998a8e84958e6b15d33a84f226a8cc31f23</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Chemicals</topic><topic>Density dependence</topic><topic>Fast Neutrons</topic><topic>High temperature</topic><topic>Hot Temperature</topic><topic>Hydrogen peroxide</topic><topic>Kinetics</topic><topic>Monte Carlo Method</topic><topic>Monte Carlo methods</topic><topic>Monte Carlo simulation</topic><topic>Neutrons</topic><topic>Protons</topic><topic>Radiochemistry</topic><topic>Radiolysis</topic><topic>Recoil protons</topic><topic>Scavenging</topic><topic>SHORT COMMUNICATION</topic><topic>Space life sciences</topic><topic>Water - 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Academic</collection><jtitle>Radiation research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Butarbutar, Sofia Loren</au><au>Meesungnoen, Jintana</au><au>Guzonas, David A.</au><au>Stuart, Craig R.</au><au>Jay-Gerin, Jean-Paul</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Modeling the Radiolysis of Supercritical Water by Fast Neutrons: Density Dependence of the Yields of Primary Species at 400°C</atitle><jtitle>Radiation research</jtitle><addtitle>Radiat Res</addtitle><date>2014-12</date><risdate>2014</risdate><volume>182</volume><issue>6</issue><spage>695</spage><epage>704</epage><pages>695-704</pages><issn>0033-7587</issn><eissn>1938-5404</eissn><abstract>A reliable understanding of radiolysis processes in supercritical water (SCW)-cooled reactors is crucial to developing chemistry control strategies that minimize the corrosion and degradation of materials. However, directly measuring the chemistry in reactor cores is difficult due to the extreme conditions of high temperature and pressure and mixed neutron and gamma-radiation fields, which are incompatible with normal chemical instrumentation. Thus, chemical models and computer simulations are an important route of investigation for predicting the detailed radiation chemistry of the coolant in a SCW reactor and the consequences for materials. Surprisingly, information on the fast neutron radiolysis of water at high temperatures is limited, and even more so for fast neutron irradiation of SCW. In this work, Monte Carlo simulations were used to predict the G values for the primary species e–aq, H•, H2, •OH and H2O2 formed from the radiolysis of pure, deaerated SCW (H2O) by 2 MeV monoenergetic neutrons at 400°C as a function of water density in the range of ∼0.15–0.6 g/cm3. The 2 MeV neutron was taken as representative of a fast neutron flux in a reactor. For light water, the moderation of these neutrons after knock-on collisions with water molecules generated mostly recoil protons of 1.264, 0.465, 0.171 and 0.063 MeV. Neglecting oxygen ion recoils and assuming that the most significant contribution to the radiolysis came from these first four recoil protons, the fast neutron yields were estimated as the sum of the G values for these protons after appropriate weightings were applied according to their energy. Calculated yields were compared with available experimental data and with data obtained for low-LET radiation. Most interestingly, the reaction of H• atoms with water was found to play a critical role in the formation yields of H2 and •OH at 400°C. Recent work has underscored the potential importance of this reaction above 200°C, but its rate constant is still controversial.</abstract><cop>United States</cop><pub>The Radiation Research Society</pub><pmid>25409127</pmid><doi>10.1667/RR13715.1</doi><tpages>10</tpages></addata></record> |
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subjects | Chemicals Density dependence Fast Neutrons High temperature Hot Temperature Hydrogen peroxide Kinetics Monte Carlo Method Monte Carlo methods Monte Carlo simulation Neutrons Protons Radiochemistry Radiolysis Recoil protons Scavenging SHORT COMMUNICATION Space life sciences Water - chemistry |
title | Modeling the Radiolysis of Supercritical Water by Fast Neutrons: Density Dependence of the Yields of Primary Species at 400°C |
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