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相关论文: Late time cosmological evolution in DHOST models

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We study cosmic evolution based on the fixed points in the dynamical analysis of the Degenerate Higher-Order Scalar-Tensor (DHOST) theories. We consider the DHOST theory in which the propagation speed of gravitational waves is equal to the…

宇宙学与河外天体物理 · 物理学 2022-05-10 Wittaya Thipaksorn , Khamphee Karwan

This article reviews scalar-tensor theories characterized by a Lagrangian that, despite the presence of second order derivatives, contain a single scalar degree of freedom. These theories, known as Degenerate Higher-Order Scalar-Tensor…

广义相对论与量子宇宙学 · 物理学 2019-04-17 David Langlois

Degenerate Higher Order Scalar Tensor (DHOST) theories are the most general scalar-tensor theories whose Lagrangian depends on the metric tensor and a single scalar field and its derivatives up to second order. They propagate only one…

宇宙学与河外天体物理 · 物理学 2024-11-06 Andrei Lazanu

In the context of Degenerate Higher-Order Scalar-Tensor (DHOST) theories, we study cosmological solutions and their stability properties. In particular, we explicitly illustrate the crucial role of degeneracy by showing how the higher order…

高能物理 - 理论 · 物理学 2019-01-16 Marco Crisostomi , Kazuya Koyama , David Langlois , Karim Noui , Daniele A. Steer

This contribution reviews scalar-tensor theories whose Lagrangian contains second-order derivatives of a scalar field but nevertheless propagate only one scalar mode (in addition to the usual two tensor modes), and are thus not plagued with…

广义相对论与量子宇宙学 · 物理学 2018-03-05 David Langlois

We investigate the parameter distributions of the viable generalized scalar-tensor theory with conventional dust matter after GW170817 in a model-independent way. We numerically construct the models by computing the time evolution of a…

广义相对论与量子宇宙学 · 物理学 2020-10-22 Shun Arai , Purnendu Karmakar , Atsushi Nishizawa

We construct gravitational modifications that go beyond Horndeski, namely theories with extended nonminimal derivative couplings, in which the coefficient functions depend not only on the scalar field but also on its kinetic energy. Such…

广义相对论与量子宇宙学 · 物理学 2017-03-01 Tiberiu Harko , Francisco S. N. Lobo , Emmanuel N. Saridakis , Minas Tsoukalas

Most existing theories of dark energy and/or modified gravity, involving a scalar degree of freedom, can be conveniently described within the framework of the Effective Theory of Dark Energy, based on the unitary gauge where the scalar…

高能物理 - 理论 · 物理学 2017-05-24 David Langlois , Michele Mancarella , Karim Noui , Filippo Vernizzi

Since the discovery of the accelerated expansion of the present Universe, significant theoretical developments have been made in the area of modified gravity. In the meantime, cosmological observations have been providing more high-quality…

Invertible disformal transformations are a useful tool to investigate ghost-free scalar-tensor theories. By performing a higher-derivative generalization of the invertible disformal transformation on Horndeski theories, we construct a novel…

广义相对论与量子宇宙学 · 物理学 2023-01-16 Kazufumi Takahashi , Masato Minamitsuji , Hayato Motohashi

We present a new class of nonsingular bounce cosmology free from instabilities, using a single scalar field coupled to gravity within the framework of the Degenerate Higher-Order Scalar-Tensor (DHOST) theories. In this type of scenarios,…

广义相对论与量子宇宙学 · 物理学 2020-09-02 Amara Ilyas , Mian Zhu , Yunlong Zheng , Yi-Fu Cai , Emmanuel N. Saridakis

We investigate the late-time evolution of the Universe within a cosmological model in which dark matter and dark energy are identified with two interacting scalar fields. Using methods of qualitative analysis of dynamical systems, we…

广义相对论与量子宇宙学 · 物理学 2021-06-14 Paulo M. Sá

We investigate the potential of cosmological observations, such as galaxy surveys, for constraining degenerate higher-order scalar-tensor (DHOST) theories, focusing in particular on the linear growth of the matter density fluctuations. We…

宇宙学与河外天体物理 · 物理学 2019-05-29 Shin'ichi Hirano , Tsutomu Kobayashi , Daisuke Yamauchi , Shuichiro Yokoyama

Theories of dark energy and modified gravity can be strongly constrained by astrophysical or cosmological observations, as illustrated by the recent observation of the gravitational wave event GW170817 and of its electromagnetic counterpart…

广义相对论与量子宇宙学 · 物理学 2018-11-02 David Langlois , Ryo Saito , Daisuke Yamauchi , Karim Noui

Future observations of the large-scale structure have the potential to investigate cosmological models with a high degree of complexity, including the properties of gravity on large scales, the presence of a complicated dark energy…

宇宙学与河外天体物理 · 物理学 2019-02-26 Robert Reischke , Alessio Spurio Mancini , Björn Malte Schäfer , Philipp M. Merkel

We show that most classes of shift-symmetric degenerate higher-order scalar-tensor (DHOST) theories which satisfy certain degeneracy conditions are not compatible with the conditions for the existence of exact black hole solutions with a…

广义相对论与量子宇宙学 · 物理学 2019-09-04 Masato Minamitsuji , James Edholm

We study the cosmological evolution of a scalar field in Horndeski gravity, assuming that the scalar field is subdominant with respect to the cosmic fluid. We first analyse the most general shift-symmetric action that respects local Lorentz…

广义相对论与量子宇宙学 · 物理学 2020-04-08 Nicola Franchini , Thomas P. Sotiriou

We use the Equation of State (EoS) approach to study the evolution of the dark sector in Horndeski models, the most general scalar-tensor theories with second order equations of motion. By including the effects of the dark sector into our…

宇宙学与河外天体物理 · 物理学 2019-09-24 Francesco Pace , Richard A. Battye , Boris Bolliet , Damien Trinh

We show that theories of mimetic gravity can be viewed as degenerate higher-order scalar-tensor (DHOST) theories that admit an extra local (gauge) symmetry in addition to the usual diffeomorphism invariance. We reformulate and classify…

广义相对论与量子宇宙学 · 物理学 2019-03-19 David Langlois , Michele Mancarella , Karim Noui , Filippo Vernizzi

The ghost-free theory of massive gravity with two dynamical metrics has been shown to produce viable cosmological expansion, where the late-time acceleration of the Universe is due to the finite range of the gravitational interaction rather…

宇宙学与河外天体物理 · 物理学 2014-10-29 Adam R. Solomon , Yashar Akrami , Tomi S. Koivisto
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