{"title":"$U(1)_\\chi$与Seesaw Dirac中微子","authors":"E. Ma","doi":"10.31526/LHEP.1.2019.109","DOIUrl":null,"url":null,"abstract":"In the context of $SO(10) \\to SU(5)\\times U(1)\\chi$, it is shown how seesaw Dirac neutrinos \nmay be obtained. In this framework, $U(1)$ lepton number is conserved, with which self-interacting dark matter with a light scalar dilepton mediator may be implemented. In \naddition, $U(1)$ baryon number may be broken to (−1)3B, thereby generating a baryonasymmetry of the Universe. The axionic solution to the strong CP problem may alsobe incorporated.","PeriodicalId":36085,"journal":{"name":"Letters in High Energy Physics","volume":" ","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2018-11-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"6","resultStr":"{\"title\":\"$U(1)_\\\\chi$ and Seesaw Dirac Neutrinos\",\"authors\":\"E. Ma\",\"doi\":\"10.31526/LHEP.1.2019.109\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In the context of $SO(10) \\\\to SU(5)\\\\times U(1)\\\\chi$, it is shown how seesaw Dirac neutrinos \\nmay be obtained. In this framework, $U(1)$ lepton number is conserved, with which self-interacting dark matter with a light scalar dilepton mediator may be implemented. In \\naddition, $U(1)$ baryon number may be broken to (−1)3B, thereby generating a baryonasymmetry of the Universe. The axionic solution to the strong CP problem may alsobe incorporated.\",\"PeriodicalId\":36085,\"journal\":{\"name\":\"Letters in High Energy Physics\",\"volume\":\" \",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2018-11-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"6\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Letters in High Energy Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.31526/LHEP.1.2019.109\",\"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":"Letters in High Energy Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.31526/LHEP.1.2019.109","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"Physics and Astronomy","Score":null,"Total":0}
In the context of $SO(10) \to SU(5)\times U(1)\chi$, it is shown how seesaw Dirac neutrinos
may be obtained. In this framework, $U(1)$ lepton number is conserved, with which self-interacting dark matter with a light scalar dilepton mediator may be implemented. In
addition, $U(1)$ baryon number may be broken to (−1)3B, thereby generating a baryonasymmetry of the Universe. The axionic solution to the strong CP problem may alsobe incorporated.