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Dark matter, electroweak phase transition, and gravitational waves in the type II two-Higgs-doublet model with a singlet scalar field

机译:用单向标量字段,II型二千港双峰模型中的暗物质,电牛相变和引力波

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In the framework of the type II two-Higgs-doublet model with a singlet scalar dark matter S , we study the dark matter observables, the electroweak phase transition, and the gravitational wave signals by such strongly first order phase transition after imposing the constraints of the LHC Higgs data. We take the heavy C P -even Higgs boson H as the only portal between the dark matter and standard model (SM) sectors, and find that the LHC Higgs data and dark matter observables require m S and m H to be larger than 130?GeV and 360?GeV for m A = 600 ? ? GeV in the case of the 125?GeV Higgs boson with the SM-like coupling. Next, we carve out some parameter space where a strongly first order electroweak phase transition can be achieved, and find benchmark points for which the amplitudes of gravitational wave spectra reach the sensitivities of the future gravitational wave detectors.
机译:在II型二峰值双盘模型的框架中,通过单向标量暗物质S,我们在施加约束之后通过如此强烈的一阶相转换来研究暗物质可观察到,电牛相转变和重力波信号 LHC HIGGS数据。 我们将沉重的CP -Even Higgs Boson H作为唯一的门户网站,并发现LHC HIGGS数据和暗物质可观察物需要M S和M H大于130?GEV 和360?gev for m a = 600? 还 GEV在125的情况下?GEV HIGGS BOSON具有SM样联轴器。 接下来,我们雕刻出一些参数空间,其中可以实现强烈的第一订单电导率相转变,并找到重力波谱的幅度达到未来引力波检测器的敏感性的基准点。

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