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Higgs Inflation with four-form couplings
Journal of Physics G: Nuclear and Particle Physics ( IF 3.4 ) Pub Date : 2021-04-08 , DOI: 10.1088/1361-6471/abefa4
C J Ouseph , Kingman Cheung

We consider a new inflationary model in which an antisymmetric tensor field A νρσ and its four-form field strength F μνρσ = 4∂[μ A νρσ] are coupled to the scalar sector of the standard model and to the Ricci scalar $\mathcal{R}$. The four-form field induces modifications to the Higgs self-coupling constant, the cosmological constant, and the non-minimal coupling constant, which results in the modification to the inflaton potential. We also show that there is no need for the Higgs-gravity coupling in the presence of four-form gravity interaction, but still can produce the right amount of density perturbation for inflation.



中文翻译:

具有四形式耦合的希格斯膨胀

我们考虑一个新的暴胀模型,其中反对称张量场A νρσ及其四形式场强F μνρσ = 4∂ [ μ A νρσ ]耦合到标准模型的标量扇区和 Ricci 标量。四形式场引起希格斯自耦合常数、宇宙学常数和非最小耦合常数的修改,从而导致对暴胀子势的修改。我们还表明,在存在四形式重力相互作用的情况下,不需要希格斯引力耦合,但仍然可以产生适量的密度扰动以进行膨胀。 $\mathcal{R}$

更新日期:2021-04-08
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