Quantum corrections to Higgs inflation in Einstein-Cartan gravity

被引:5
作者
He, Minxi [1 ,2 ]
Kamada, Kohei [3 ,4 ,5 ]
Mukaida, Kyohei [1 ,6 ]
机构
[1] Theory Ctr, IPNS, KEK, 1-1 Oho, Tsukuba, Ibaraki 3050801, Japan
[2] Inst Basic Sci IBS, Ctr Theoret Phys Univ, Particle Theory & Cosmol Grp, 55 Expo-ro, Daejeon 34126, South Korea
[3] Univ Chinese Acad Sci HIAS UCAS, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
[4] Univ Tokyo, Res Ctr Early Universe RESCEU, Grad Sch Sci, Hongo 7-3-1,Bunkyo-ku, Tokyo 1130033, Japan
[5] Int Ctr Theoret Phys Asia Pacific ICTP AP, Hangzhou, Peoples R China
[6] Grad Inst Adv Studies Sokendai, 1-1 Oho, Tsukuba, Ibaraki 3050801, Japan
关键词
Cosmological models; Early Universe Particle Physics; Effective Field Theories; Scattering Amplitudes; SYMMETRY-BREAKING; PHASE-TRANSITION; DYNAMICAL MODEL; STANDARD MODEL; UNIVERSE; FIELD; COSMOLOGY; SCALARON; FLATNESS; HORIZON;
D O I
10.1007/JHEP01(2024)014
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
This paper studies the quantum corrections to the Higgs inflation model in the context of the Einstein-Cartan (E-C) gravity in the large-N limit with N being the number of real scalar components in Higgs. Recently, it is realized that the Higgs inflation in the E-C formalism smoothly connects those in the metric and the Palatini formalisms in the presence of a non-minimal coupling between the Higgs fields and the Nieh-Yan term. This motivates us to investigate the quantum corrections in large-N limit to the E-C Higgs inflation and to clarify how the Ricci curvature squared R2 induced by the quantum corrections succeeds in Ultraviolet (UV)-extending the Higgs inflation in metric formalism while it fails in the Palatini case. We show that a generalized R2-term required for the renormalization in the E-C formalism induces a new scalar degree of freedom (DoF), the scalaron, which gradually decouples with the system due to its increasing mass as approaching the Palatini limit. The presence of the scalaron extends the UV cutoff at vacuum of the original model except for the parameter space close to the Palatini limit. This UV-extension is expected to solve the strong coupling problem that may exist during (p)reheating in the absence of the scalaron.
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页数:34
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