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相关论文: Friedmann Robertson Walker models with Conformally…

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In this manuscript, we show that three fundamental building blocks are supporting the Cosmological Principle. The first of them states that there is a special frame in the universe where the spatial geometry is intrinsically homogeneous and…

广义相对论与量子宇宙学 · 物理学 2024-01-05 Leandro G. Gomes

We consider a $D$-dimensional cosmological model with a dilaton field and two $(D-d-1)$-form field strengths which have nonvanishing fluxes in extra dimensions. Exact solutions for the model with a certain set of couplings are obtained by…

高能物理 - 理论 · 物理学 2018-09-24 Nahomi Kan , Masashi Kuniyasu , Kiyoshi Shiraishi , Kohjiroh Takimoto

We consider the appearance of multiple scalar fields in SFT inspired non-local models with a single scalar field at late times. In this regime all the scalar fields are free. This system minimally coupled to gravity can be analyzed…

高能物理 - 理论 · 物理学 2011-01-24 Federico Galli , Alexey S. Koshelev

We show how a nearly massless scalar field conformally and disformally coupled to matter can affect the dynamics of two bodies in their inspiralling phase before merging. We discuss both the conservative dynamics, e.g. how the energy of the…

广义相对论与量子宇宙学 · 物理学 2019-07-03 Philippe Brax , Anne-Christine Davis , Adrien Kuntz

In this paper we study the dynamical behaviour of a simple cosmological model defined by a spatially flat Robertson-Walker geometry, conformally coupled with a massive scalar field. We determine a Lyapunov-like function for the non-linear…

广义相对论与量子宇宙学 · 物理学 2009-10-31 M. A. Castagnino H. Giacomini , L. Lara

We propose and construct a two-parameter perturbative expansion around a Friedmann-Lema\^{i}tre-Robertson-Walker geometry that can be used to model high-order gravitational effects in the presence of non-linear structure. This framework…

宇宙学与河外天体物理 · 物理学 2017-02-15 Sophia R. Goldberg , Timothy Clifton , Karim A. Malik

We derive non-relativistic equations of motion for the formation of cosmological structure in a Scalar Field Dark Matter (SFDM) model corresponding to a complex scalar field endowed with a quadratic scalar potential. Starting with the full…

宇宙学与河外天体物理 · 物理学 2014-07-29 L. Arturo Urena-Lopez

In recent papers by the authors (S.~Motonaga and K.~Yagasaki, Obstructions to integrability of nearly integrable dynamical systems near regular level sets, submitted for publication, and K.~Yagasaki, Nonintegrability of nearly integrable…

动力系统 · 数学 2022-01-17 Shoya Motonaga , Kazuyuki Yagasaki

We reconsider the cosmological model discussed by Sung-Won Kim [Phys. Rev D 53, 6889 (1996)] in the context of Friedmann-Robertson-Walker cosmologies with a traversable wormhole, where it is assumed that the matter content is divided into…

广义相对论与量子宇宙学 · 物理学 2015-06-16 Mauricio Cataldo , Fernanda Arostica , Sebastian Bahamonde

We discuss massive scalar field with conformal coupling in Friedmann-Robertson-Walker (FRW) Universe of special type with constant electromagnetic field. Treating an external gravitational-electromagnetic background exactly, at first time…

高能物理 - 理论 · 物理学 2009-09-17 S. P. Gavrilov , D. M. Gitman , S. D. Odintsov

We study scaling symmetry in a class of non-minimally coupled scalar field in a background of Friedmann-Robertson-Walker (FRW) spacetime. We use a non-minimally coupling $R L^{(\varphi)}$. We find the corresponding conserved charge of that…

综合物理 · 物理学 2023-12-25 Malik Al Matwi

We derive a set of equations monitoring the evolution of covariant and gauge-invariant linear scalar perturbations of Friedman-Lema\^itre-Robertson-Walker models with multiple interacting non-linear scalar fields. We use a dynamical…

广义相对论与量子宇宙学 · 物理学 2014-08-06 Artur Alho , Filipe C. Mena

Despite impressive phenomenological successes, cosmological models are incomplete without an understanding of what happened at the big bang singularity. Maxwell electrodynamics, considered as a source of the classical Einstein field…

广义相对论与量子宇宙学 · 物理学 2017-02-17 A. Övgün

We construct a cosmological model from the inception of the Friedmann-Lem\^aitre-Robertson-Walker metric into the field equations of the f(R,L_m) gravity theory, with R being the Ricci scalar and L_m being the matter lagrangian density. The…

广义相对论与量子宇宙学 · 物理学 2024-03-21 B. S. Gonçalves , P. H. R. S. Moraes , B. Mishra

A Friedmann-Robertson-Walker cosmology with dark energy can be modelled using a quintessence field. That system is equivalent to a relativistic particle moving on a two-dimensional conformal spacetime. When the quintessence behaves as a…

广义相对论与量子宇宙学 · 物理学 2019-10-02 Felipe A. Asenjo , Sergio A. Hojman

We discuss the evolution of linear perturbations about a Friedmann-Robertson-Walker background metric, using only the local conservation of energy-momentum. We show that on sufficiently large scales the curvature perturbation on spatial…

天体物理学 · 物理学 2009-10-31 David Wands , Karim A. Malik , David H. Lyth , Andrew R. Liddle

We study the implications of a noncommutative geometry of the minisuperspace variables for the FRW universe with a conformally coupled scalar field. The investigation is carried out by means of a comparative study of the universe evolution…

高能物理 - 理论 · 物理学 2009-11-10 G. D. Barbosa

Radiaitve mechanism of conformal symmetry breaking in a comformal-invariant version of the Standard Model is considered. The Coleman-Weinberg mechanism of dimensional transmutation in this system gives rise to finite vacuum expectation…

高能物理 - 唯象学 · 物理学 2017-02-06 A. B. Arbuzov , R. G. Nazmitdinov , A. E. Pavlov , V. N. Pervushin , A. F. Zakharov

Recently, inhomogeneous generalisations of the Friedmann-Lemaitre-Robertson-Walker cosmological models have gained interest in the astrophysical community and are more often employed to study cosmological phenomena. However, in many papers…

宇宙学与河外天体物理 · 物理学 2011-10-17 Krzysztof Bolejko , Marie-Noëlle Célérier , Andrzej Krasiński

We give a complete description of the asymptotic behavior of a Friedmann-Robertson-Walker Universe with ``normal'' matter and a minimally coupled scalar field. We classify the conditions under which the Universe is or is not accelerating.…

广义相对论与量子宇宙学 · 物理学 2009-10-31 David I. Santiago Alexander S. Silbergleit