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arXiv · 2401.11794

Exploring the Impact of Dissipation Coefficient in Warm Higgs Inflation

Wei Cheng·Xue-Wen Chen·Ruiyu Zhou·Jiu-Jiang Jiang·Xin-Rui Dai·Zi-Han Zhang·Tong Qin
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Abstract

In this study, we conducted a detailed analysis of the core parameter of Warm Higgs Inflation (WHI) $-$ the dissipation coefficient ($Q$). As a crucial parameter in the warm inflation process, $Q$ exerts profound influences on the entire evolutionary process. By meticulously deriving the relationships between various quantities and $Q$, we successfully circumvented the common preconceptions regarding strong and weak dissipation, laying the foundation for a more accurate exploration of their interconnections. Taking into account the constraints imposed by Cosmic Microwave Background, we observed that the dissipation coefficient $Q$ remains at extremely low levels throughout the entire warm inflation process, i.e., $Q \ll 1$. This observation indicates that WHI falls under the category of weakly dissipative warm inflation. Despite being weakly dissipative, $Q$ still plays a crucial role in the evolution of temperature, energy, and other quantities, highlighting its significance and non-negligibility. We delved deeper into the impact of the primordial power spectrum on the dissipation coefficient $Q$ during the warm inflation process, discovering that the dependency is not significant. Consequently, this naturally leads to the unobtrusive dependence of the gravitational wave power spectrum on $Q$. Finally, we found that gravitational waves generated by WHI hold the potential for verification in future observational experiments, especially through the SKA100 experiment. These findings provide a theoretical support for a more profound understanding of the early evolution of the universe.

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Wei Cheng, Xue-Wen Chen, Ruiyu Zhou, Jiu-Jiang Jiang, Xin-Rui Dai, Zi-Han Zhang, Tong Qin. 2024-01-22. Exploring the Impact of Dissipation Coefficient in Warm Higgs Inflation. https://arxiv.org/abs/2401.11794

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