{"title":"Empirical model for fusion cross sections of Ca-induced reactions.","authors":"R. L., N. Sowmya, Sridhar K.N, Manjunatha Hc","doi":"10.1088/1674-1137/ad1a97","DOIUrl":null,"url":null,"abstract":"\n A new empirical formula for the astronomical S-factor has been suggested as a function of the Coulomb interaction parameter, center of mass energy, and barrier height. About 22 fusion reactions with 40,48Ca as projectiles were considered for different targets leading to compound nuclei with the atomic and mass numbers varying between 40 ≤ Z ≤112 and 88 ≤ A ≤278 respectively. The fusion cross-sections have been estimated using the Geometric factor, Gamow-Sommerfield factor and empirical formula for the S-factor. A better agreement has been obtained for the present work with that of available experiments when compared to Wong’s formula. The present work leads to a smaller standard deviation value when compared to Wong’s formula when used to correlate with the experimental data of Calcium-induced fusion reactions. Wong’s formula provides a good approximation of fusion cross-sections when center of mass energy is below the fusion barrier when compared to above the fusion barrier.","PeriodicalId":504778,"journal":{"name":"Chinese Physics C","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2024-01-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Physics C","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1088/1674-1137/ad1a97","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
A new empirical formula for the astronomical S-factor has been suggested as a function of the Coulomb interaction parameter, center of mass energy, and barrier height. About 22 fusion reactions with 40,48Ca as projectiles were considered for different targets leading to compound nuclei with the atomic and mass numbers varying between 40 ≤ Z ≤112 and 88 ≤ A ≤278 respectively. The fusion cross-sections have been estimated using the Geometric factor, Gamow-Sommerfield factor and empirical formula for the S-factor. A better agreement has been obtained for the present work with that of available experiments when compared to Wong’s formula. The present work leads to a smaller standard deviation value when compared to Wong’s formula when used to correlate with the experimental data of Calcium-induced fusion reactions. Wong’s formula provides a good approximation of fusion cross-sections when center of mass energy is below the fusion barrier when compared to above the fusion barrier.
提出了一个新的天文 S 因子经验公式,它是库仑相互作用参数、质心能量和屏障高度的函数。考虑了以 40,48Ca 为射弹的约 22 个不同目标的聚变反应,这些聚变反应导致原子序数和质量数分别在 40 ≤ Z ≤112 和 88 ≤ A ≤278 之间变化的化合物核。聚变截面是利用几何因子、伽莫-索默菲尔德因子和 S 因子的经验公式估算出来的。与黄氏公式相比,目前的工作与现有的实验获得了更好的一致性。在与钙诱导核聚变反应的实验数据相关联时,与 Wong 公式相比,本研究的标准偏差值较小。当质心能量低于聚变势垒与高于聚变势垒时,Wong 公式提供了聚变截面的良好近似值。