1,417 research outputs found

    Leptogenesis with supersymmetric Higgs triplets in TeV region

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    The leptogenesis with supersymmetric Higgs triplets is studied in the light of experimental verification in the TeV region. The lepton number asymmetry appears just after the inflation via multiscalar coherent evolution of Higgs triplets and antislepton on a flat manifold. If the Higgs triplet mass terms dominate over the negative thermal-log term for the Hubble parameter H comparable to the Higgs triplet mass M_\Delta, the asymmetry is fixed readily to some significant value by the redshift and rotation of these scalar fields, providing the sufficient lepton-to-entropy ratio n_L / s \sim 10^-10. This can be the case even with M_\Delta \sim 1 TeV for the reheating temperature T_R \sim 10^6 GeV and the mass parameter M / \lambda \sim 10^22 GeV of the nonrenormalizable superpotential terms relevant for leptogenesis.Comment: 8 Pages, 2 figures. The discussion about the stability of the VEV's of the Higgs triplets is adde

    Affleck-Dine leptogenesis with triplet Higgs

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    We study an extension of the supersymmetric standard model including a pair of electroweak triplet Higgs Δ\Delta and Δˉ{\bar \Delta}. The neutrinos acquire Majorana masses mediated by these triplet Higgs fields rather than the right-handed neutrinos. The successful leptogenesis for baryogenesis can be realized after the inflation through the Affleck-Dine mechanism on a flat manifold consisting of Δ\Delta, Δˉ{\bar \Delta}, e~c{\tilde e}^c (anti-slepton), even if the triplet Higgs mass MΔM_\Delta is much larger than the gravitino mass m3/2103GeVm_{3/2} \sim 10^3 {\rm GeV}. Specifically, due to the effects of the potential terms provided with the superpotential terms MΔΔˉΔM_\Delta {\bar \Delta} \Delta, (λL//2M)ΔˉΔˉecec(\lambda_{L /} / 2M) {\bar \Delta} {\bar \Delta} e^c e^c, (λΔ/2M)ΔˉΔΔˉΔ(\lambda_\Delta / 2M) {\bar \Delta} \Delta {\bar \Delta} \Delta (λL//λΔ0.33\lambda_{L /} / \lambda_\Delta \sim 0.3 - 3), the phases of Δ\Delta, Δˉ{\bar \Delta}, e~c{\tilde e}^c are rotated at the time with the Hubble parameter HMΔH \sim M_\Delta, producing generally the asymmetry with fraction ϵL0.1\epsilon_L \sim 0.1. If MΔM_\Delta is large enough, this early leptogenesis can be completed before the thermal effects take place.Comment: 11 pages, 2 figure

    Using Conservative Estimation for Conditional Probability instead of Ignoring Infrequent Case

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    There are several estimators of conditional probability from observed frequencies of features. In this paper, we propose using the lower limit of confidence interval on posterior distribution determined by the observed frequencies to ascertain conditional probability. In our experiments, this method outperformed other popular estimators.Comment: The 2016 International Conference on Advanced Informatics: Concepts, Theory and Application (ICAICTA2016
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