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Solving the strong CP problem via aˉθ-characterized mirror symmetry
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作者 顾佩洪 《Chinese Physics C》 SCIE CAS CSCD 2024年第3期20-24,共5页
In the standard model QCD Lagrangian,a term of CP violating gluon density is theoretically expected to have a physical coefficientθ¯,which is typically on the order of unity.However,the upper bound on the electr... In the standard model QCD Lagrangian,a term of CP violating gluon density is theoretically expected to have a physical coefficientθ¯,which is typically on the order of unity.However,the upper bound on the electric dipole moment of the neutron enforces the value ofθ¯to be extremely small.The significant discrepancy between theoretical expectations and experimental results in this context is widely recognized as the strong CP problem.To solve this puzzle in an appealing context of two Higgs doublets,we propose aθ¯-characterized mirror symmetry between two Higgs singlets with respective discrete symmetries.In our scenario,the parameterθ¯can completely disappear from the full Lagrangian after the standard model fermions take a proper phase rotation as well as the Higgs doublets and singlets.Moreover,all of new physics for solving the strong CP problem can be allowed near the TeV scale. 展开更多
关键词 strong CP problem θ¯-characterized mirror symmetry two Higgs doublets
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宇宙正反物质不对称的起源 被引量:1
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作者 黄发朋 李明哲 +1 位作者 顾佩洪 张新民 《科学通报》 EI CAS CSCD 北大核心 2016年第11期1151-1156,共6页
宇宙中正反物质不对称性的起源是粒子物理和宇宙学中极具挑战性的问题,至今人们还不清楚该问题的本质.随着实验观测的日益精确,人们对这一未解之谜的研究日益深入.本文首先简要介绍宇宙正反物质不对称性之谜的背景,以及在理论上解释该... 宇宙中正反物质不对称性的起源是粒子物理和宇宙学中极具挑战性的问题,至今人们还不清楚该问题的本质.随着实验观测的日益精确,人们对这一未解之谜的研究日益深入.本文首先简要介绍宇宙正反物质不对称性之谜的背景,以及在理论上解释该问题所要满足的基本条件.然后结合最新的理论和实验进展,重点介绍了3种能自洽地解释正反物质不对称性并且能够在实验上进行验证的理论,包括电弱重子数产生机制、轻子数不对称产生机制以及引力重子数产生机制.期望未来更精确的实验能够验证究竟哪种机制才是宇宙正反物质不对称性的起源. 展开更多
关键词 正反物质不对称性 电弱相变 电弱重子数产生机制 轻子数不对称产生机制
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Detecting dark energy in long baseline neutrino oscillations
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作者 顾佩洪 毕效军 +2 位作者 冯波 杨炳麟 张新民 《Chinese Physics C》 SCIE CAS CSCD 北大核心 2008年第7期530-535,共6页
In this paper, we discuss a possibility of studying properties of dark energy in long baseline neutrino oscillation experiments. We consider two types of models of neutrino dark energy. For one type of models the scal... In this paper, we discuss a possibility of studying properties of dark energy in long baseline neutrino oscillation experiments. We consider two types of models of neutrino dark energy. For one type of models the scalar field is taken to be quintessence-like and for the other phantom-like. In these models the scalar fields couple to the neutrinos to give rise to spatially varying neutrino masses. We will show that the two types of models predict different behaviors of the spatial variation of the neutrino masses inside the Earth and consequently result in different signals in long baseline neutrino oscillation experiments. 展开更多
关键词 dark energy neutrino oscillation
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