Vasudha G.S. , N. Sowmya , H.C. Manjunatha , D. Prakash Babu , Nagaiah N. , Mayeen Khandekar , Krishnakanth E. , R. Soundar
{"title":"库仑裂变时标和逆运动学截面的研究","authors":"Vasudha G.S. , N. Sowmya , H.C. Manjunatha , D. Prakash Babu , Nagaiah N. , Mayeen Khandekar , Krishnakanth E. , R. Soundar","doi":"10.1016/j.physo.2023.100180","DOIUrl":null,"url":null,"abstract":"<div><p>In inverse kinematics, we explored Coulomb fission cross-sections and time scales. Heavier projectiles such as <sup>238</sup>U, <sup>132</sup>Xe, and <sup>208</sup>Pb on lighter targets such as <sup>16</sup>O <sup>26</sup>Mg, <sup>27</sup>Al, <sup>32</sup>S, <sup>35</sup>Cl, <span><math><msup><mrow></mrow><mrow><mn>40</mn><mo>,</mo><mn>48</mn></mrow></msup></math></span>Ca, <sup>45</sup>Sc, <span><math><msup><mrow></mrow><mrow><mn>48</mn><mo>,</mo><mn>50</mn></mrow></msup></math></span>Ti, <span><math><msup><mrow></mrow><mrow><mn>56</mn><mo>,</mo><mn>58</mn></mrow></msup></math></span>Fe, <sup>64</sup>Ni, <sup>89</sup>Y, <sup>30</sup>Si and <sup>65</sup>Zn were looked into. The photofission cross-sections and the number of equivalent photons impinge on the target nuclei are important parameters in cross-section assessment. The anticipated cross-sections increases with increase in atomic number of target nuclei. We also explored the time scale of projectile nuclei at various transition levels. The estimated time scales accord well with the available experimental value, which is in the order of picoseconds. In addition, we predicted time scales of <sup>165</sup>Ho nuclei in the transition state from <span><math><mrow><mn>19</mn><mo>/</mo><msup><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msup><mo>→</mo><mn>15</mn><mo>/</mo><msup><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msup></mrow></math></span> to <span><math><mrow><mn>29</mn><mo>/</mo><msup><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msup><mo>→</mo><mn>25</mn><mo>/</mo><msup><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msup></mrow></math></span> for which experimental time scales are not available in literature. As a result, Coulomb fission is one of the causes that has severely hampered in the formation of compound nuclei. Prediction of time scales, in particular, would aid in understanding the structure of various energy levels.</p></div>","PeriodicalId":36067,"journal":{"name":"Physics Open","volume":"17 ","pages":"Article 100180"},"PeriodicalIF":0.0000,"publicationDate":"2023-09-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Investigations on Coulomb fission time scales and cross sections in inverse kinematics\",\"authors\":\"Vasudha G.S. , N. Sowmya , H.C. Manjunatha , D. Prakash Babu , Nagaiah N. , Mayeen Khandekar , Krishnakanth E. , R. Soundar\",\"doi\":\"10.1016/j.physo.2023.100180\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>In inverse kinematics, we explored Coulomb fission cross-sections and time scales. Heavier projectiles such as <sup>238</sup>U, <sup>132</sup>Xe, and <sup>208</sup>Pb on lighter targets such as <sup>16</sup>O <sup>26</sup>Mg, <sup>27</sup>Al, <sup>32</sup>S, <sup>35</sup>Cl, <span><math><msup><mrow></mrow><mrow><mn>40</mn><mo>,</mo><mn>48</mn></mrow></msup></math></span>Ca, <sup>45</sup>Sc, <span><math><msup><mrow></mrow><mrow><mn>48</mn><mo>,</mo><mn>50</mn></mrow></msup></math></span>Ti, <span><math><msup><mrow></mrow><mrow><mn>56</mn><mo>,</mo><mn>58</mn></mrow></msup></math></span>Fe, <sup>64</sup>Ni, <sup>89</sup>Y, <sup>30</sup>Si and <sup>65</sup>Zn were looked into. The photofission cross-sections and the number of equivalent photons impinge on the target nuclei are important parameters in cross-section assessment. The anticipated cross-sections increases with increase in atomic number of target nuclei. We also explored the time scale of projectile nuclei at various transition levels. The estimated time scales accord well with the available experimental value, which is in the order of picoseconds. In addition, we predicted time scales of <sup>165</sup>Ho nuclei in the transition state from <span><math><mrow><mn>19</mn><mo>/</mo><msup><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msup><mo>→</mo><mn>15</mn><mo>/</mo><msup><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msup></mrow></math></span> to <span><math><mrow><mn>29</mn><mo>/</mo><msup><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msup><mo>→</mo><mn>25</mn><mo>/</mo><msup><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msup></mrow></math></span> for which experimental time scales are not available in literature. As a result, Coulomb fission is one of the causes that has severely hampered in the formation of compound nuclei. Prediction of time scales, in particular, would aid in understanding the structure of various energy levels.</p></div>\",\"PeriodicalId\":36067,\"journal\":{\"name\":\"Physics Open\",\"volume\":\"17 \",\"pages\":\"Article 100180\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-09-14\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physics Open\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S2666032623000455\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"Physics and Astronomy\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics Open","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S2666032623000455","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"Physics and Astronomy","Score":null,"Total":0}
Investigations on Coulomb fission time scales and cross sections in inverse kinematics
In inverse kinematics, we explored Coulomb fission cross-sections and time scales. Heavier projectiles such as 238U, 132Xe, and 208Pb on lighter targets such as 16O 26Mg, 27Al, 32S, 35Cl, Ca, 45Sc, Ti, Fe, 64Ni, 89Y, 30Si and 65Zn were looked into. The photofission cross-sections and the number of equivalent photons impinge on the target nuclei are important parameters in cross-section assessment. The anticipated cross-sections increases with increase in atomic number of target nuclei. We also explored the time scale of projectile nuclei at various transition levels. The estimated time scales accord well with the available experimental value, which is in the order of picoseconds. In addition, we predicted time scales of 165Ho nuclei in the transition state from to for which experimental time scales are not available in literature. As a result, Coulomb fission is one of the causes that has severely hampered in the formation of compound nuclei. Prediction of time scales, in particular, would aid in understanding the structure of various energy levels.