Confronting cosmic ray electron and positron excesses with hybrid triplet Higgs portal dark matter  

作　　者：Shao-Long Chen Amit Dutta Banik Ze-Kun Liu 陈绍龙;Amit Dutta Banik;刘泽坤(Key Laboratory of Quark and Lepton Physics(MoE)and Institute of Particle Physics,Central China Normal University,Wuhan 430079,China;Center for High Energy Physics,Peking University,Beijing 100871,China)

机构地区：[1]Key Laboratory of Quark and Lepton Physics(MoE)and Institute of Particle Physics,Central China Normal University,Wuhan 430079,China [2]Center for High Energy Physics,Peking University,Beijing 100871,China

出　　处：《Chinese Physics C》2022年第6期9-21,共13页中国物理C（英文版）

基　　金：Supported in part by the National Science Foundation of China(11775093,12175082)。

摘　　要：We perform a detailed study of scalar dark matter with triplet Higgs extensions of the Standard Model in order to explain the cosmic ray electron and positron excesses reported by AMS-02 and DAMPE.A detailed analysis of the AMS-02 positron excess reveals that for different orderings(normal,inverted,and quasi-degenerate)of neutrino mass,the hybrid triplet Higgs portal framework is more favored with respect to the single triplet Higgs portal for TeV scale dark matter.We also show that the resonant peak and continuous excess in DAMPE cosmic ray data can be well explained with the hybrid triplet Higgs portal dark matter when a dark matter sub-halo nearby is taken into account.

关 键 词：dark matter triplet Higgs neutrino mass electron and positron excesses 

分 类 号：P172.4[天文地球—天文学]