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宇宙正反物质不对称的起源
  • ISSN号:0023-074X
  • 期刊名称:《科学通报》
  • 时间:0
  • 分类:O4[理学—物理]
  • 作者机构:[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
  • 相关基金: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 and Outstanding Young Scientists Project of the Chinese Academy of Sciences
中文摘要:

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.

英文摘要:

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.

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期刊信息
  • 《科学通报》
  • 北大核心期刊(2011版)
  • 主管单位:中国科学院
  • 主办单位:中国科学院
  • 主编:周光召
  • 地址:北京东黄城根北街16号
  • 邮编:100717
  • 邮箱:csb@scichina.org
  • 电话:010-64036120 64012686
  • 国际标准刊号:ISSN:0023-074X
  • 国内统一刊号:ISSN:11-1784/N
  • 邮发代号:80-213
  • 获奖情况:
  • 首届国家期刊奖,中国期刊方阵“双高”期刊,第三届中国出版政府奖
  • 国内外数据库收录:
  • 美国化学文摘(网络版),美国数学评论(网络版),美国工程索引,日本日本科学技术振兴机构数据库,中国中国科技核心期刊,中国北大核心期刊(2004版),中国北大核心期刊(2008版),中国北大核心期刊(2011版),中国北大核心期刊(2014版),中国北大核心期刊(2000版)
  • 被引量:81792