Elko as an inflaton candidate

Abstract Elko is a spin-half fermion with a two-fold Wigner degeneracy and Klein–Gordon dynamics. In this paper, we show that in a spatially flat FLRW space-time, slow-roll inflation can be initiated by the homogeneous Elko fields. The inflaton is a composite scalar field obtained by contracting the spinor field with its dual. This is possible because the background evolution as described by the Friedmann equation is completely determined by the scalar field. This approach has the advantage that we do not need to specify the initial conditions for every component of the spinor fields. We derive the equation of motion for the inflaton and also show that this solution is an attractor. Finally, we examine the slow-roll parameters and the power-spectrum, showing that obtaining a behavior in agreement with observational requirements is hard to be obtained, unless one uses more complicated potentials, which may act a limitation of Elko inflation.

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Publication Details

Journal
The European Physical Journal C
Published
2025-06-06
DOI
https://doi.org/10.1140/epjc/s10052-025-14361-0
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.00

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article

Elko as an inflaton candidate

Siyi Zhou, Haomin Rao, X. Chen, Cheng-Yang Lee et al.
The European Physical Journal C
Cosmology and Gravitation Theories
article

Elko as an inflaton candidate

Siyi Zhou, Haomin Rao, X. Chen, Cheng-Yang Lee, Wenqi Yu, Yanjiao Ma
article en

Abstract

Abstract Elko is a spin-half fermion with a two-fold Wigner degeneracy and Klein–Gordon dynamics. In this paper, we show that in a spatially flat FLRW space-time, slow-roll inflation can be initiated by the homogeneous Elko fields. The inflaton is a composite scalar field obtained by contracting the spinor field with its dual. This is possible because the background evolution as described by the Friedmann equation is completely determined by the scalar field. This approach has the advantage that we do not need to specify the initial conditions for every component of the spinor fields. We derive the equation of motion for the inflaton and also show that this solution is an attractor. Finally, we examine the slow-roll parameters and the power-spectrum, showing that obtaining a behavior in agreement with observational requirements is hard to be obtained, unless one uses more complicated potentials, which may act a limitation of Elko inflation.

The European Physical Journal CVol. 85(6)
Chongqing University (CN), Hong Kong University of Science and Technology (HK), Sichuan University (CN), Shaoguan University (CN), University of Hong Kong (HK)
National Natural Science Foundation of China, Shaoguan University
Openalex Percentile: Top 92%
Cosmology and Gravitation Theories
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