机构地区:[1]Theoretical Physics Division,Institute of High Energy Physics,Chinese Academy of Sciences,P.O.Box 918-4,Beijing 100049,China [2]CAS Key Laboratory for Researches in Galaxies and Cosmology,Department of Astronomy,University of Science and Technology of China,Chinese Academy of Sciences,Hefei 230026,China [3]Key Laboratory of Particle Astrophysicsl Institute of Higl Energy Physics,Chinese Academy of Science,P.O.Box 918-3,Beijing 100049,China
出 处:《Chinese Physics C》2016年第11期49-54,共6页中国物理C(英文版)
基 金:Supported by NSFC(11121092,11033005,11375220,11421303);CAS PilotB Program,the China Postdoctoral Science Foundation(2016M590133);Chinese National Youth Thousand Talents Program,the USTC start-up funding(KY2030000049);Youth Innovation Promotion Association Project;Outstanding Young Scientists Project of the Chinese Academy of Sciences
摘 要:Recently, a novel idea [1] has been proposed to relax the electroweak hierarchy problem through the cosmological inflation and the axion periotic potential. Here, we further assume that only the attractive inflation is needed to explain the light mass of the Higgs boson, where we do not need a specified periodic potential of the axion field. Attractive inflation during the early universe drives the Higgs boson mass from the large value in the early universe to the small value at present, where the Higgs mass is an evolving parameter of the Universe. Thus, the small Higgs mass can technically originate from the cosmological evolution rather than dynamical symmetry or anthropics. Further, we study the possible collider signals or constraints at a future lepton collier and the possible constraints from the muon anomalous magnetic moment. A concrete attractive relaxion model is also discussed, which is consistent with the data of Planck 2015.Recently, a novel idea [1] has been proposed to relax the electroweak hierarchy problem through the cosmological inflation and the axion periotic potential. Here, we further assume that only the attractive inflation is needed to explain the light mass of the Higgs boson, where we do not need a specified periodic potential of the axion field. Attractive inflation during the early universe drives the Higgs boson mass from the large value in the early universe to the small value at present, where the Higgs mass is an evolving parameter of the Universe. Thus, the small Higgs mass can technically originate from the cosmological evolution rather than dynamical symmetry or anthropics. Further, we study the possible collider signals or constraints at a future lepton collier and the possible constraints from the muon anomalous magnetic moment. A concrete attractive relaxion model is also discussed, which is consistent with the data of Planck 2015.
关 键 词:HIGGS INFLATION electroweak hierarchy
分 类 号:O572.2[理学—粒子物理与原子核物理]
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