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Inflation based on a classically scale invariant extended standard model
International Journal of Modern Physics A ( IF 1.4 ) Pub Date : 2021-09-02 , DOI: 10.1142/s0217751x21501694 Katsuki Tomita 1
International Journal of Modern Physics A ( IF 1.4 ) Pub Date : 2021-09-02 , DOI: 10.1142/s0217751x21501694 Katsuki Tomita 1
Affiliation
We extend a classically scale invariant model where the electroweak symmetry breaking is triggered by the dynamical chiral symmetry breaking in a hidden QCD sector, and a real singlet scalar S mediates these two sectors. Our model can explain cosmic inflation without unitarity violation in addition. Slow-roll inflation occurs along a valley in scalar potential. In the original model, the coupling − λ H S between the Higgs field H and S is always negative and therefore, the potential has its valleys in H -S mixed directions. For large value of the top Yukawa coupling y t , the potential along the valley becomes negative since the Higgs quartic coupling λ H becomes negative at inflationary scale. Then slow-roll inflation cannot occur. For inflation to definitely occur, we render the coupling − λ H S positive at inflationary scale and consider the S -inflation case. This is achieved by introducing a new singlet scalar η with the large coupling λ H η to H . By this extension, λ H can also always be positive, and we consider this case as the simplest case. We consider inflation with the nonminimal coupling ξ S between S and gravity. Although ξ S is large such as ξ S ≃ 𝒪 ( 1 0 3 ) , unitarity is not violated since couplings between S and other fields are sufficiently small. η is odd under a new symmetry Z 2 not to mix with H regardless of largeness of λ H η . Because of this symmetry, η may have its relic abundance Ω η ĥ 2 comparable with the observational value Ω obs ĥ 2 ≃ 0 . 1 2 of the dark matter relic abundance. However, the spin-independent elastic cross-section σ SI η of η exceeds the observational bound σ SI obs ∼ 𝒪 ( 1 0 − 4 7 ) cm2. Hence, we impose the resonance condition m η ≃ m S / 2 and reduce Ω η ĥ 2 to much smaller than Ω obs ĥ 2 . Constraints from the electroweak scale physics and inflationary scale physics are much strong, and the allowed parameter space is very narrow.
中文翻译:
基于经典尺度不变扩展标准模型的通货膨胀
我们扩展了一个经典尺度不变模型,其中电弱对称性破缺是由隐藏的 QCD 扇区中的动态手征对称破缺触发的,以及一个真正的单重态标量小号 调解这两个部门。我们的模型可以解释宇宙膨胀而不会另外违反统一性。缓慢滚动的通货膨胀沿着标量势的山谷发生。在原始模型中,联轴器 - λ H 小号 希格斯场之间H 和小号 总是负的,因此,潜力有它的谷底H -小号 混合方向。用于大值顶部汤川联轴器是的 吨 ,由于希格斯四次耦合,沿谷的势变为负λ H 在通货膨胀规模上变为负数。这样就不会发生慢速通胀。为了确定暴胀发生,我们渲染耦合 - λ H 小号 通胀规模为正,并考虑小号 -通货膨胀案例。这是通过引入一个新的单线态标量来实现的η 与大型联轴器λ H η 到H . 通过这个扩展,λ H 也可以总是为正的,我们认为这种情况是最简单的情况。我们考虑膨胀与非最小耦合ξ 小号 之间小号 和重力。虽然ξ 小号 很大比如ξ 小号 ≃ 𝒪 ( 1 0 3 ) ,不违反统一性,因为之间的耦合小号 和其他领域足够小。η 在新的对称性下是奇数Z 2 不要混合H 不论大小λ H η . 由于这种对称性,η 可能有它的遗迹丰富Ω η H 2 与观测值相当Ω 观测值 H 2 ≃ 0 . 1 2 暗物质遗迹丰度。然而,与自旋无关的弹性截面σ SI η 的η 超出观察范围σ SI 观测值 ~ 𝒪 ( 1 0 - 4 7 ) 厘米2。因此,我们强加了共振条件米 η ≃ 米 小号 / 2 并减少Ω η H 2 远小于Ω 观测值 H 2 . 来自电弱尺度物理和暴胀尺度物理的约束非常强,允许的参数空间非常狭窄。
更新日期:2021-09-02
中文翻译:
基于经典尺度不变扩展标准模型的通货膨胀
我们扩展了一个经典尺度不变模型,其中电弱对称性破缺是由隐藏的 QCD 扇区中的动态手征对称破缺触发的,以及一个真正的单重态标量