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Main Authors: An, Ok Song, Kang, Jin U, Kim, Yong Jin, Mun, Ui Ri, Ri, Un Gyong
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2501.09985
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author An, Ok Song
Kang, Jin U
Kim, Yong Jin
Mun, Ui Ri
Ri, Un Gyong
author_facet An, Ok Song
Kang, Jin U
Kim, Yong Jin
Mun, Ui Ri
Ri, Un Gyong
contents In this paper we construct a class of Degenerate Higher-Order Scalar-Tensor (DHOST) theories with an extra scalar field, which admits viable solutions of bouncing universe satisfying the following requirements: (i) absence of Belinski-Khalatnikov-Lifshitz (BKL) instability, ghost and gradient instability, (ii) absence of superluminality, (iii) generation of nearly scale-invariant curvature perturbations and very small tensor-to-scalar ratio, and (iv) conventional asymptotics in the distant past and future, where gravity sector is described by General Relativity and the DHOST scalar has a canonical form of Lagrangian. We also expect our models to have sufficiently small non-Gaussianities of primordial curvature perturbations to be compatible with observations. As such, this work exemplifies for the first time the fully viable two-field DHOST bouncing cosmology, which is free of instability and superluminality problems as well as compatible with observations.
format Preprint
id arxiv_https___arxiv_org_abs_2501_09985
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Fully viable DHOST bounce with extra scalar
An, Ok Song
Kang, Jin U
Kim, Yong Jin
Mun, Ui Ri
Ri, Un Gyong
High Energy Physics - Theory
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
In this paper we construct a class of Degenerate Higher-Order Scalar-Tensor (DHOST) theories with an extra scalar field, which admits viable solutions of bouncing universe satisfying the following requirements: (i) absence of Belinski-Khalatnikov-Lifshitz (BKL) instability, ghost and gradient instability, (ii) absence of superluminality, (iii) generation of nearly scale-invariant curvature perturbations and very small tensor-to-scalar ratio, and (iv) conventional asymptotics in the distant past and future, where gravity sector is described by General Relativity and the DHOST scalar has a canonical form of Lagrangian. We also expect our models to have sufficiently small non-Gaussianities of primordial curvature perturbations to be compatible with observations. As such, this work exemplifies for the first time the fully viable two-field DHOST bouncing cosmology, which is free of instability and superluminality problems as well as compatible with observations.
title Fully viable DHOST bounce with extra scalar
topic High Energy Physics - Theory
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2501.09985