The measurements of the Higgs mass and top Yukawa coupling indicate that welive in a very special Universe, at the edge of the absolute stability of theelectroweak vacuum. If fully stable, the Standard Model (SM) can be extendedall the way up to the inflationary scale and the Higgs field, non-minimallycoupled to gravity with strength $\xi$, can be responsible for inflation. Weshow that the successful Higgs inflation scenario can also take place if the SMvacuum is not absolutely stable. This conclusion is based on two effects thatwere overlooked previously. The first one is associated with the effectiverenormalization of the SM couplings at the energy scale $M_P/\xi$, where $M_P$is the Planck scale. The second one is a symmetry restoration after inflationdue to high temperature effects that leads to the (temporary) disappearance ofthe vacuum at Planck values of the Higgs field.
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机译:希格斯质量和顶部汤川耦合的测量表明,我们生活在一个非常特殊的宇宙中,处于电弱真空绝对稳定的边缘。如果完全稳定,则可以将标准模型(SM)一直扩展到通货膨胀规模,并且非最小耦合强度为\\ xi $的希格斯场可导致通货膨胀。我们显示,如果SMvacuum并非绝对稳定,那么成功的希格斯通胀情景也可能发生。该结论基于先前被忽略的两个影响。第一个与在能量尺度$ M_P / \ xi $处SM耦合的有效重新归一化相关,其中$ M_P $是普朗克尺度。第二个是由于高温效应导致的膨胀后的对称恢复,导致希格斯场的普朗克值下真空(暂时)消失。
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