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相关论文: Modified gravity a la Galileon: Late time cosmic a…

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We consider the covariant galileon gravity taking into account the third order and fourth order scalar field Lagrangians L_3(\pi) and L_4(\pi) consisting of three and four $\pi$'s with four and five derivatives acting on them respectively.…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Radouane Gannouji , M. Sami

In this paper, we investigate the first and second order cosmological perturbations in the light mass Galileon (LMG) scenario. LMG action includes cubic Galileon term along with the standard kinetic term and a potential which is added…

广义相对论与量子宇宙学 · 物理学 2017-07-12 Md. Wali Hossain

A scalar-tensor theory of gravity can be made not only to account for the current cosmic acceleration, but also to satisfy solar-system and laboratory constraints, by introducing a non-linear derivative interaction for the scalar field.…

宇宙学与河外天体物理 · 物理学 2015-03-13 Tsutomu Kobayashi , Hiroyuki Tashiro , Daichi Suzuki

We study the cosmology of Galileon modified gravity models in the linear perturbation regime. We derive the fully covariant and gauge invariant perturbed field equations using two different methods, which give consistent results, and solve…

宇宙学与河外天体物理 · 物理学 2013-01-22 Alexandre Barreira , Baojiu Li , Carlton Baugh , Silvia Pascoli

The Galileon model is a modified gravity theory that may provide an explanation for the accelerated expansion of the Universe. This model does not suffer from instabilities or ghost problems (normally associated with higher-order derivative…

广义相对论与量子宇宙学 · 物理学 2013-07-02 J. Neveu , V. Ruhlmann-Kleider , A. Conley , N. Palanque-Delabrouille , P. Astier , J. Guy , E. Babichev

We studied the cosmological constraints on the Galileon gravity obtained from observational data of the growth rate of matter density perturbations, the supernovae Ia (SN Ia), the cosmic microwave background (CMB), and baryon acoustic…

宇宙学与河外天体物理 · 物理学 2012-07-03 Koichi Hirano , Zen Komiya , Hisato Shirai

In 'modified' gravity the observed acceleration of the universe is explained by changing the gravitational force law or the number of degrees of freedom in the gravitational sector. Both possibilities can be tested by measurements of…

宇宙学与河外天体物理 · 物理学 2017-12-27 Clare Burrage , David Parkinson , David Seery

We present the first constraints on the full parameter space of the Galileon modified gravity model, considering both the cosmological parameters and the coefficients which specify the additional terms in the Lagrangian due to the Galileon…

宇宙学与河外天体物理 · 物理学 2013-10-21 Alexandre Barreira , Baojiu Li , Ariel Sanchez , Carlton M. Baugh , Silvia Pascoli

In this paper, we have investigated the phase space analysis in modified Galileon cosmology, where the Galileon term is considered a coupled scalar field, $F(\phi)$. We focus on the exponential type function of $F(\phi)$ and the three…

广义相对论与量子宇宙学 · 物理学 2024-11-11 L. K. Duchaniya , B. Mishra , I. V. Fomin , S. V. Chervon

A Galileon field is one which obeys a spacetime generalization of the non-relativistic Galilean invariance. Such a field may possess non-canonical kinetic terms, but ghost-free theories with a well-defined Cauchy problem exist, constructed…

宇宙学与河外天体物理 · 物理学 2014-11-21 Clare Burrage , David Seery

We study the cosmology of a covariant Galileon field with five covariant Lagrangians and confront this theory with the most recent cosmological probes: the type Ia supernovae data (Constitution and Union2 sets), cosmic microwave background…

宇宙学与河外天体物理 · 物理学 2011-01-17 Savvas Nesseris , Antonio De Felice , Shinji Tsujikawa

The extended Galileon models possess tracker solutions with de Sitter attractors along which the dark energy equation of state is constant during the matter-dominated epoch, i.e. w_DE = -1-s, where s is a positive constant. Even with this…

宇宙学与河外天体物理 · 物理学 2012-03-19 Antonio De Felice , Shinji Tsujikawa

This paper analyses the cosmological consequences of a modified theory of gravity whose action integral is built from a linear combination of the Ricci scalar $R$ and a quadratic term in the covariant derivative of $R$. The resulting…

广义相对论与量子宇宙学 · 物理学 2015-12-31 R. R. Cuzinatto , C. A. M. de Melo , L. G. Medeiros , P. J. Pompeia

We study the cosmological effects of a Galileon term in scalar-tensor theories of gravity. The subset of scalar-tensor theories considered are characterized by a non-minimal coupling $F(\sigma) R$, a kinetic term with arbitrary sign $Z…

宇宙学与河外天体物理 · 物理学 2023-09-26 A. G. Ferrari , M. Ballardini , F. Finelli , D. Paoletti , N. Mauri

We investigate the generalized cubic covariant Galileon model, a kinetically driven dark energy model within the Horndeski class of theories. The model extends the cubic covariant Galileon by including power laws of the field derivatives in…

宇宙学与河外天体物理 · 物理学 2020-07-01 Noemi Frusciante , Simone Peirone , Luis Atayde , Antonio De Felice

Galileon gravity offers a robust gravitational theory for explaining cosmic acceleration, having a rich phenomenology of testable behaviors. We explore three classes of Galileon models -- standard uncoupled, and linearly or derivatively…

宇宙学与河外天体物理 · 物理学 2015-06-03 Stephen A. Appleby , Eric V. Linder

We develop a numerical algorithm to solve the high-order nonlinear derivative-coupling equation associated with the quartic Galileon model, and implement it in a modified version of the RAMSES N-body code to study the effect of the Galileon…

宇宙学与河外天体物理 · 物理学 2013-11-08 Baojiu Li , Alexandre Barreira , Carlton M. Baugh , Wojciech A. Hellwing , Kazuya Koyama , Silvia Pascoli , Gong-Bo Zhao

The Galileon theory belongs to the class of modified gravity models that can explain the late-time accelerated expansion of the Universe. In previous works, cosmological constraints on the Galileon model were derived, both in the uncoupled…

广义相对论与量子宇宙学 · 物理学 2017-03-29 J. Neveu , V. Ruhlmann-Kleider , P. Astier , M. Besançon , J. Guy , A. Möller , E. Babichev

The Galileon model is a tensor-scalar theory of gravity which explains the late acceleration of the Universe expansion with no instabilities and recovers General Relativity in the strong field limit. Most constraints obtained so far on…

宇宙学与河外天体物理 · 物理学 2020-06-16 Clément Leloup , Vanina Ruhlmann-Kleider , Jeremy Neveu , Arnaud de Mattia

Most of the information on our cosmos stems from either late-time observations or the imprint of early-time inhomogeneities on the cosmic microwave background. We explore to what extent early modifications of gravity, which become…

宇宙学与河外天体物理 · 物理学 2016-10-10 Nelson A. Lima , Vanessa Smer-Barreto , Lucas Lombriser
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