2,509 research outputs found

    Detecting interactions between dark matter and photons at high energy e+e−e^+e^- colliders

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    We investigate the sensitivity to the effective operators describing interactions between dark matter particles and photons at future high energy e+e−e^+e^- colliders via the \gamma+ \slashed{E} channel. Such operators could be useful to interpret the potential gamma-ray line signature observed by the Fermi-LAT. We find that these operators can be further tested at e+e−e^+ e^- colliders by using either unpolarized or polarized beams. We also derive a general unitarity condition for 2→n2 \to n processes and apply it to the dark matter production process e+e−→χχγe^+e^-\to\chi\chi\gamma.Comment: 13 pages, 8 figure

    SUSY SU(5) ×S4\times S_{4} GUT Flavor Model for Fermion Masses and Mixings with Adjoint, Large θ13PMNS\theta^{PMNS}_{13}

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    We propose an S4S_{4} flavor model based on supersymmetric (SUSY) SU(5) GUT. The first and third generations of \textbf{10} dimensional representations in SU(5) are all assigned to be 111_{1} of S4S_{4}. The second generation of \textbf{10} is to be 121_{2} of S4S_{4}. Right-handed neutrinos of singlet \textbf{1} and three generations of 5ˉ\bar{\textbf{5}} are all assigned to be 313_{1} of S4S_{4}. The VEVs of two sets of flavon fields are allowed a moderate hierarchy, that is ⟨Φν⟩∼λc⟨Φe⟩\langle\Phi^{\nu}\rangle \sim \lambda_{c}\langle\Phi^{e}\rangle. Tri-Bimaximal (TBM) mixing can be produced at both leading order (LO) and next to next to leading order (NNLO) in neutrino sector. All the masses of up-type quarks are obtained at LO. We also get the bottom-tau unification mτ=mbm_{\tau}=m_{b} and the popular Georgi-Jarlskog relation mμ=3msm_{\mu}=3m_{s} as well as a new mass relation me=827mdm_{e}=\frac{8}{27}m_{d} in which the novel Clebsch-Gordan (CG) factor arises from the adjoint field H24H_{24}. The GUT relation leads to a sizable mixing angle θ12e∼θc\theta^{e}_{12} \sim \theta_{c} and the correct quark mixing matrix VCKMV_{CKM} can also be realised in the model. The resulting CKM-like mixing matrix of charged leptons modifies the vanishing θ13ν\theta^{\nu}_{13} in TBM mixing to a large θ13PMNS≃θc/2\theta^{PMNS}_{13}\simeq\theta_{c}/\sqrt{2}, in excellent agreement with experimental results. A Dirac CP violation phase ϕ12≃±π/2\phi_{12}\simeq\pm\pi/2 is required to make the deviation from θ12ν\theta^{\nu}_{12} small. We also present some phenomenological numerical results predicted by the model.Comment: 36 pages, 12 figures, major revison to the previous editio

    Production of proton-rich nuclei around Z=84-90 in fusion-evaporation reactions

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    Within the framework of the dinuclear system model, production cross sections of proton-rich nuclei with charged numbers of Z=84-90 are investigated systematically. Possible combinations with the 28^{28}Si, 32^{32}S, 40^{40}Ar bombarding the target nuclides 165^{165}Ho, 169^{169}Tm, 170−174^{170-174}Yb, 175,176^{175,176}Lu, 174,176−180^{174,176-180}Hf and 181^{181}Ta are analyzed thoroughly. The optimal excitation energies and evaporation channels are proposed to produce the proton-rich nuclei. The systems are feasible to be constructed in experiments. It is found that the neutron shell closure of N=126 is of importance during the evaporation of neutrons. The experimental excitation functions in the 40^{40}Ar induced reactions can be nicely reproduced. The charged particle evaporation is comparable with neutrons in cooling the excited proton-rich nuclei, in particular for the channels with α\alpha and proton evaporation. The production cross section increases with the mass asymmetry of colliding systems because of the decrease of the inner fusion barrier. The channels with pure neutron evaporation depend on the isotopic targets. But it is different for the channels with charged particles and more sensitive to the odd-even effect.Comment: 15 pages, 10 figures. arXiv admin note: text overlap with arXiv:0803.1117, arXiv:0707.258
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