Kh. Helensana Devi, K. Sashikanta Singh, N. Nimai Singh
{"title":"Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM","authors":"Kh. Helensana Devi, K. Sashikanta Singh, N. Nimai Singh","doi":"10.1155/2023/2365316","DOIUrl":null,"url":null,"abstract":"We analyze the radiative stability of the next-to-tribimaximal mixings (NTBM) with the variation of the SUSY breaking scale (<span><svg height=\"9.25202pt\" style=\"vertical-align:-3.29111pt\" version=\"1.1\" viewbox=\"-0.0498162 -5.96091 15.1941 9.25202\" width=\"15.1941pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"></path></g><g transform=\"matrix(.0091,0,0,-0.0091,10.192,3.132)\"></path></g></svg>)</span> in MSSM, for both normal ordering (NO) and inverted ordering (IO) at the fixed input value of the seesaw scale <span><svg height=\"14.8825pt\" style=\"vertical-align:-3.2911pt\" version=\"1.1\" viewbox=\"-0.0498162 -11.5914 29.79 14.8825\" width=\"29.79pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"></path></g><g transform=\"matrix(.0091,0,0,-0.0091,12.22,3.132)\"></path></g><g transform=\"matrix(.013,0,0,-0.013,22.159,0)\"></path></g></svg><span></span><svg height=\"14.8825pt\" style=\"vertical-align:-3.2911pt\" version=\"1.1\" viewbox=\"33.372183799999995 -11.5914 22.096 14.8825\" width=\"22.096pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,33.422,0)\"></path></g><g transform=\"matrix(.013,0,0,-0.013,39.662,0)\"></path></g><g transform=\"matrix(.0091,0,0,-0.0091,45.902,-5.741)\"></path></g><g transform=\"matrix(.0091,0,0,-0.0091,50.334,-5.741)\"></path></g></svg></span> GeV and two different values of <span><svg height=\"12.7178pt\" style=\"vertical-align:-3.42947pt\" version=\"1.1\" viewbox=\"-0.0498162 -9.28833 26.6668 12.7178\" width=\"26.6668pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"></path></g><g transform=\"matrix(.013,0,0,-0.013,4.043,0)\"></path></g><g transform=\"matrix(.013,0,0,-0.013,9.633,0)\"></path></g><g transform=\"matrix(.013,0,0,-0.013,18.986,0)\"></path></g></svg>.</span> All the neutrino oscillation parameters receive varying radiative corrections irrespective of the <svg height=\"9.25202pt\" style=\"vertical-align:-3.29111pt\" version=\"1.1\" viewbox=\"-0.0498162 -5.96091 15.1941 9.25202\" width=\"15.1941pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"><use xlink:href=\"#g113-110\"></use></g><g transform=\"matrix(.0091,0,0,-0.0091,10.192,3.132)\"><use xlink:href=\"#g50-84\"></use></g></svg> values at the electroweak scale, which are all within the <svg height=\"8.55521pt\" style=\"vertical-align:-0.2063904pt\" version=\"1.1\" viewbox=\"-0.0498162 -8.34882 13.7356 8.55521\" width=\"13.7356pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"></path></g><g transform=\"matrix(.013,0,0,-0.013,6.24,0)\"></path></g></svg> range of the latest global fit data at a low value of <span><svg height=\"12.7178pt\" style=\"vertical-align:-3.42947pt\" version=\"1.1\" viewbox=\"-0.0498162 -9.28833 26.6668 12.7178\" width=\"26.6668pt\" xmlns=\"http://www.w3.org/2000/svg\" xmlns:xlink=\"http://www.w3.org/1999/xlink\"><g transform=\"matrix(.013,0,0,-0.013,0,0)\"><use xlink:href=\"#g121-114\"></use></g><g transform=\"matrix(.013,0,0,-0.013,4.043,0)\"><use xlink:href=\"#g121-95\"></use></g><g transform=\"matrix(.013,0,0,-0.013,9.633,0)\"><use xlink:href=\"#g121-108\"></use></g><g transform=\"matrix(.013,0,0,-0.013,18.986,0)\"><use xlink:href=\"#g113-224\"></use></g></svg>.</span> NO is found to be more stable than IO for all four different NTBM mixing patterns.","PeriodicalId":7498,"journal":{"name":"Advances in High Energy Physics","volume":" 24","pages":""},"PeriodicalIF":1.5000,"publicationDate":"2023-11-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advances in High Energy Physics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1155/2023/2365316","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 0
Abstract
We analyze the radiative stability of the next-to-tribimaximal mixings (NTBM) with the variation of the SUSY breaking scale () in MSSM, for both normal ordering (NO) and inverted ordering (IO) at the fixed input value of the seesaw scale GeV and two different values of . All the neutrino oscillation parameters receive varying radiative corrections irrespective of the values at the electroweak scale, which are all within the range of the latest global fit data at a low value of . NO is found to be more stable than IO for all four different NTBM mixing patterns.
期刊介绍：
Advances in High Energy Physics publishes the results of theoretical and experimental research on the nature of, and interaction between, energy and matter. Considering both original research and focussed review articles, the journal welcomes submissions from small research groups and large consortia alike.
京公网安备 11010802042870号
京ICP备2023020795号-1
分享
求助内容：
应助结果提醒方式：
扫码关注我们
