Scalar contributions to the S, T, U parameters in a 3-3-1 model

Abstract

Electroweak precision tests, expressed through the oblique parameters $S$, $T$, and $U$, impose stringent constraints on physics beyond the Standard Model. Gauge extensions of the Standard Model based on the $SU(3)_L \times U(1)_N$ symmetry predict a rich scalar and gauge spectrum that contribute to these parameters. Previous studies have shown that 3-3-1 gauge bosons give negligible contributions to the oblique parameters, while the contributions of the scalar sector to these parameters have received comparatively little attention. In particular, for the version of the $SU(3)_L \times U(1)_N$ model with right-handed neutrinos, the impact of the scalar sector on $S$, $T$ , and $U$ has not yet been addressed. In this work, we fill this gap and address sistematically the scalar contributions to the $S$, $T$ and $U$ within this version. As main result, we show that the parameter $T$ put stringent constraints on the masses and energy scales associated to the spectrum of scalars of the model.

Figures (7)

• Figure 1: Feynman diagrams at one-loop contributing for the vacuum polarization functions defined in Eqs.(\ref{['pol11c']}) and (\ref{['pol11cb']}).
• Figure 2: Predictions of the $331RHN$ model for the oblique parameter $T$ in the $(f, v_{\chi^{\prime}},..\lambda_9)$ plane. The left panel show the results to $T$ as function of $(f, v_{\chi^{\prime}},..\lambda_9)$. In the right panel we show $m_H$ and $m_{h_1^\pm}$ behavior, where the white distribution corresponds to the region where the oblique parameter reaches its experimental upper limit.
• Figure 3: Left panel: behavior of $T$ in the $(f, v_{\chi^{\prime}}, \ldots, \lambda_9)$ space after imposing the experimental constraint; right panel: maximum allowed $v_{\chi^{\prime}}(T)$ from the full scan, assuming $\lambda_7=\lambda_8=10^{-3}$ (upper) and $\lambda_7=\lambda_8\sim\lambda_{2,6,9}$ (lower).
• Figure 4: Predictions of the $331RHN$ model for the oblique parameter $T$ in the $(f, v_{\chi^{\prime}},..\lambda_9)$ plane to $m_{H^{\prime\prime}}$ and $m_{h_2^\pm}$. The left panel show the results to $T$ as function of $(f, v_{\chi^{\prime}},..\lambda_9)$. In the right panel the white distribution corresponds to the region where the oblique parameter reaches its experimental upper limit.
• Figure 5: Predictions of the $331RHN$ model for the oblique parameter $T$ in the $(f, v_{\chi^{\prime}},..\lambda_9)$ plane to $m_{A}$ . The left panel show the results to $T$ as function of $(f, v_{\chi^{\prime}},..\lambda_9)$. In the right panel the white distribution corresponds to the region where the oblique parameter reaches its experimental upper limit.