Peccei-Quinn mechanism and axion interactions in 3-3-1 model with Cosmological Inflation

Семинары

Семинар отдела «Теория фундаментальных взаимодействий»

Дата и время: четверг, 5 октября 2023 г., в 16:00

Место: аудитория им. Блохинцева (4-й этаж), Лаборатория теоретической физики им. Н.Н. Боголюбова; онлайн-семинар в Zoom

Тема семинара: «Peccei-Quinn mechanism and axion interactions in the 3-3-1 model with Cosmological Inflation»

Докладчик: Хоанг Нгок Лонг (Университет Ванланга, Вьетнам)

Аннотация:

Based on the Peccei-Quinn (PQ) assignment, the PQ charge operator in the 3-3-1 model with Cosmological Inflation is constructed in terms of diagonal operators T3 and T8 of the SU(3)L subgroup. The formula shows that difference of PQ charges of up and down quarks is 2, i.e., ΔQA = 2, while for electric charge, as usually ΔQ = 1. For right handed fermions, electric charges (Q) of left-handed and right-handed are assumed to be equal, while for (QA) is opposite. PQ charge of neutral scalars equal ±2, while for charged scalars, it vanishes. The couplings of axion with fermions are presented. To have correct kinetic term for the axion, the PQ scale fpq is to be VEV of the singlet scalar boson, namely, fpq = vϕ. The point is worth emphasized that the axion has doubly derivative coupling with scalar playing the role of inflaton. The new effects mainly happen in the energy region from 107GeV to 1011GeV. The chiral effective Lagrangian as usually provides axion mass consistent with model independent prediction.