Electroweak-like baryogenesis with new chiral matter

被引:0
|
作者
Kohei Fujikura
Keisuke Harigaya
Yuichiro Nakai
Ruoquan Wang
机构
[1] Tokyo Institute of Technology,Department of Physics
[2] Institute for Advanced Study,School of Natural Sciences
[3] Shanghai Jiao Tong University,Tsung
[4] Rutgers University,Dao Lee Institute and School of Physics and Astronomy
关键词
Beyond Standard Model; Cosmology of Theories beyond the SM;
D O I
暂无
中图分类号
学科分类号
摘要
We propose a framework where a phase transition associated with a gauge symmetry breaking that occurs (not far) above the electroweak scale sets a stage for baryogenesis similar to the electroweak baryogenesis in the Standard Model. A concrete realization utilizes the breaking of SU(2)R× U(1)X→ U(1)Y. New chiral fermions charged under the extended gauge symmetry have nonzero lepton numbers, which makes the B − L symmetry anomalous. The new lepton sector contains a large flavor-dependent CP violation, similar to the Cabibbo-Kobayashi-Maskawa phase, without inducing sizable electric dipole moments of the Standard Model particles. A bubble wall dynamics associated with the first-order phase transition and SU(2)R sphaleron processes generate a lepton asymmetry, which is transferred into a baryon asymmetry via the ordinary electroweak sphaleron process. Unlike the Standard Model electroweak baryogenesis, the new phase transition can be of the strong first order and the new CP violation is not significantly suppressed by Yukawa couplings, so that the observed asymmetry can be produced. The model can be probed by collider searches for new particles and the observation of gravitational waves. One of the new leptons becomes a dark matter candidate. The model can be also embedded into a left-right symmetric theory to solve the strong CP problem.
引用
收藏
相关论文
共 50 条
  • [1] Electroweak-like baryogenesis with new chiral matter
    Fujikura, Kohei
    Harigaya, Keisuke
    Nakai, Yuichiro
    Wang, Ruoquan
    JOURNAL OF HIGH ENERGY PHYSICS, 2021, 2021 (07)
  • [2] Erratum to: Electroweak-like baryogenesis with new chiral matter
    Kohei Fujikura
    Keisuke Harigaya
    Yuichiro Nakai
    Isaac R. Wang
    Journal of High Energy Physics, 2021
  • [3] Erratum to: Electroweak-like baryogenesis with new chiral matter
    Kohei Fujikura
    Keisuke Harigaya
    Yuichiro Nakai
    Isaac R. Wang
    Journal of High Energy Physics, 2022
  • [4] Electroweak-like baryogenesis with new chiral matter (vol 7, 224, 2021)
    Fujikura, Kohei
    Harigaya, Keisuke
    Nakai, Yuichiro
    Wang, Isaac R.
    JOURNAL OF HIGH ENERGY PHYSICS, 2021, 2021 (12)
  • [5] Electroweak-like baryogenesis with new chiral matter (vol 7, 224, 2021)
    Fujikura, Kohei
    Harigaya, Keisuke
    Nakai, Yuichiro
    Wang, Isaac R.
    JOURNAL OF HIGH ENERGY PHYSICS, 2022, 2022 (01)
  • [6] CHIRAL CHARGE FLUX AND ELECTROWEAK BARYOGENESIS
    FUNAKUBO, K
    KAKUTO, A
    OTSUKI, S
    TAKENAGA, K
    TOYODA, F
    PROGRESS OF THEORETICAL PHYSICS, 1995, 93 (06): : 1067 - 1074
  • [7] Electroweak baryogenesis by axionlike dark matter
    Im, Sang Hui
    Jeong, Kwang Sik
    Lee, Yeseong
    PHYSICAL REVIEW D, 2022, 105 (03)
  • [8] Electroweak baryogenesis via chiral gravitational waves
    Abedi, H.
    Ahmadvand, M.
    Gousheh, S. S.
    PHYSICS LETTERS B, 2018, 786 : 35 - 38
  • [9] Electroweak baryogenesis, large Yukawas and dark matter
    Provenza, A
    Quiros, M
    Ullio, P
    JOURNAL OF HIGH ENERGY PHYSICS, 2005, (10):
  • [10] Enabling electroweak baryogenesis through dark matter
    Lewicki, Marek
    Rindler-Daller, Tanja
    Wells, James D.
    JOURNAL OF HIGH ENERGY PHYSICS, 2016, (06):