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Combining the equivalence between cosmological particle creation and an effective viscous fluid pressure with the fact that the latter represents a dynamical degree of freedom within the second-order Israel-Stewart theory for imperfect…

天体物理学 · 物理学 2009-10-31 Winfried Zimdahl

We develop a formulation of particle mechanics in which the functional relation between force and kinetic energy is derived directly from local conservation mechanical energy $E$, rather than postulated through Newton's second law or a…

经典物理 · 物理学 2026-02-10 Thomas Oikonomou

A huge value of cosmological constant characteristic for the particle physics and the inflation of early Universe are inherently related to each other: one can construct a fine-tuned superpotential, which produces a flat potential of…

广义相对论与量子宇宙学 · 物理学 2015-06-03 V. V. Kiselev , S. A. Timofeev

We study the evolution of the universe in the presence of inflaton, matter, radiation, and holographic dark energy. The time evolution of the scale factor is obtained by solving the Friedmann equation of the universe with a good…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Hyeong-Chan Kim , Jae-Weon Lee , Jungjai Lee

We study evolution of a flat Friedmann-Robertson Walker universe filled with a bulk viscous cosmological fluid in a higher derivative theory of gravity in the presence of time varying gravitational and cosmological constant. Cosmological…

广义相对论与量子宇宙学 · 物理学 2015-03-13 B. C. Paul , P. S. Debnath

In this paper, we have studied a 5-dimensional warped product space-time with a time-dependent warp factor. This warp factor plays an important role in localizing matter to the 4-dimensional hypersurface constituting the observed universe…

广义相对论与量子宇宙学 · 物理学 2011-07-14 Sarbari Guha , Subenoy Chakraborty

In the standard FRW formalism, the scale factor is assumed to describe the expansion of the universe. However, by examining empty space with a positive cosmological constant (i.e., a de Sitter space), we find that this assumption is…

综合物理 · 物理学 2025-08-05 J. M. Greben

The fundamental nature and origin of dark energy are one of the premier mysteries of theoretical physics. In General Relativity Theory, the cosmological constant $\Lambda$ is the simplest explanation for dark energy. On the other hand, the…

广义相对论与量子宇宙学 · 物理学 2022-05-27 Raja Solanki , Avik De , Sanjay Mandal , P. K. Sahoo

Based on a thoeretical model in which scalar fields play crucial roles, we propose a mechanism to better understand a cosmological constant expected to be small (nearly comparable with the critical density) but nonzero as suggested strongly…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Yasunori Fujii

The $f(R)$ theory of gravitation developed perturbatively around the general theory of relativity with cosmological constant (the \text{$\Lambda$}CDM model) in a flat FLWR geometry is considered. As a result, a general explicit cosmological…

广义相对论与量子宇宙学 · 物理学 2025-02-25 Pham Van Ky , Nguyen Thi Hong Van , Nguyen Anh Ky

In the early seventies, Alan Sandage defined cosmology as the search for two numbers: Hubble parameter ${{H}_{0}}$ and deceleration parameter ${{q}_{0}}$. The first of the two basic cosmological parameters (the Hubble parameter) describes…

广义相对论与量子宇宙学 · 物理学 2015-02-04 Yu. L. Bolotin , V. A. Cherkaskiy , O. A. Lemets , D. A. Yerokhin , L. G. Zazunov

Non-conservation of dark matter can lead to late-time cosmic acceleration. This mechanism is known as the matter creation theory and this replaces the need of dark energy and modified gravity theories. We consider a two-fluid system…

广义相对论与量子宇宙学 · 物理学 2025-12-02 Sudip Halder , Jaume de Haro , Supriya Pan , Tapan Saha , Subenoy Chakraborty

The fundamental constants of electromagnetism, gravity and quantum mechanics can be related empirically by the numerical approximation $\ln(V_e/V_P)\approx \alpha^{-1}$, where $\alpha$ is the low energy value of the electromagnetic fine…

综合物理 · 物理学 2018-01-31 L. Eaves

We examine in the context of general relativity the dynamics of a spatially flat Robertson-Walker universe filled with a classical minimally coupled scalar field \phi of exponential potential ~ e^{-\mu\phi} plus pressureless baryonic…

广义相对论与量子宇宙学 · 物理学 2009-11-10 A. Kehagias , G. Kofinas

We explore a toy model mechanism of geometric cancellation, alleviating the (classical) cosmological constant problem. To do so, we assume at primordial times that vacuum energy fuels an inflationary quadratic hilltop potential nonminimally…

广义相对论与量子宇宙学 · 物理学 2024-06-12 Alessio Belfiglio , Roberto Giambò , Orlando Luongo

We systematically study the evolution of the Friedmann-Robertson-Walker (FRW) universe coupled with a cosmological constant $\Lambda$ and a perfect fluid that has the equation of state $p=w\rho$, where $p$ and $\rho$ denote, respectively,…

The creation of ultra-light dark particles in the late-time FLRW spacetime provides a cosmological model in accordance with precise observational tests. The matter creation backreaction implies in this context a vacuum energy density…

宇宙学与河外天体物理 · 物理学 2012-10-11 Saulo Carneiro

A range of cosmological observations demonstrate an accelerated expansion of the Universe, and the most likely explanation of this phenomenon is a cosmological constant. Given the importance of understanding the underlying physics, it is…

宇宙学与河外天体物理 · 物理学 2021-04-07 Karoline Loeve , Kristine Simone Nielsen , Steen H. Hansen

In a recent paper (Vigoureux et al. Int. J. Theor. Phys. 47:928, 2007) it has been suggested that the velocity of light and the expansion of the universe are two aspects of one single concept connecting space and time in the expanding…

宇宙学与河外天体物理 · 物理学 2011-03-22 David Viennot , Jean-Marie Vigoureux

In this work, we investigate cosmologies where the gravitational constant varies in time, with the aim of explaining the accelerated expansion without a cosmological constant. We achieve this by considering a phenomenological extension to…

宇宙学与河外天体物理 · 物理学 2020-03-18 Ekim Taylan Hanımeli , Brahim Lamine , Alain Blanchard , Isaac Tutusaus
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