{"title":"$U(1)_{\\chi}$、Seesaw暗物质和希格斯衰变","authors":"E. Ma","doi":"10.31526/LHEP.1.2019.103","DOIUrl":null,"url":null,"abstract":"It has recently been pointed out that the underlying symmetry of dark matter may well be $U(1)_\\chi$ (coming from $SO(10) \\to SU(5) \\times U(1)_\\chi$) with the dark parity of any given particle determined by $(-1)^{Q_\\chi+2j}$, where $Q_\\chi$ is its $U(1)_\\chi$ charge and $j$ its spin angular momentum. Armed with this new insight, previous simple models of dark matter are reinterpreted, and a novel idea is proposed that light seesaw dark matter exists in analogy to light neutrinos and is produced by the rare decay of the standard-model Higgs boson.","PeriodicalId":36085,"journal":{"name":"Letters in High Energy Physics","volume":" ","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2018-10-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"6","resultStr":"{\"title\":\"$U(1)_{\\\\chi}$, Seesaw Dark Matter, and Higgs Decay\",\"authors\":\"E. Ma\",\"doi\":\"10.31526/LHEP.1.2019.103\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"It has recently been pointed out that the underlying symmetry of dark matter may well be $U(1)_\\\\chi$ (coming from $SO(10) \\\\to SU(5) \\\\times U(1)_\\\\chi$) with the dark parity of any given particle determined by $(-1)^{Q_\\\\chi+2j}$, where $Q_\\\\chi$ is its $U(1)_\\\\chi$ charge and $j$ its spin angular momentum. Armed with this new insight, previous simple models of dark matter are reinterpreted, and a novel idea is proposed that light seesaw dark matter exists in analogy to light neutrinos and is produced by the rare decay of the standard-model Higgs boson.\",\"PeriodicalId\":36085,\"journal\":{\"name\":\"Letters in High Energy Physics\",\"volume\":\" \",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2018-10-15\",\"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.1.2019.103\",\"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.1.2019.103","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"Physics and Astronomy","Score":null,"Total":0}
$U(1)_{\chi}$, Seesaw Dark Matter, and Higgs Decay
It has recently been pointed out that the underlying symmetry of dark matter may well be $U(1)_\chi$ (coming from $SO(10) \to SU(5) \times U(1)_\chi$) with the dark parity of any given particle determined by $(-1)^{Q_\chi+2j}$, where $Q_\chi$ is its $U(1)_\chi$ charge and $j$ its spin angular momentum. Armed with this new insight, previous simple models of dark matter are reinterpreted, and a novel idea is proposed that light seesaw dark matter exists in analogy to light neutrinos and is produced by the rare decay of the standard-model Higgs boson.