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相关论文: Gravity-Driven Acceleration of the Cosmic Expansio…

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The union of high-energy particle theories and gravitation often gives rise to an evolving strength of gravity. The standard picture of the earliest universe would certainly deserve revision if the Planck mass, which defines the strength of…

广义相对论与量子宇宙学 · 物理学 2008-02-03 Janna J. Levin

Modern data is showing increasing evidence that the Universe is accelerating. So far, all attempts to account for the acceleration have required some fundamental dimensionless quantities to be extremely small. We show how a class of scalar…

天体物理学 · 物理学 2010-04-08 Andreas Albrecht , Constantinos Skordis

The discovery that the cosmic expansion is accelerating has been followed by an intense theoretical and experimental response in physics and astronomy. The discovery implies that our most basic notions about how gravity work are violated on…

宇宙学与河外天体物理 · 物理学 2010-01-15 Robert R. Caldwell , Marc Kamionkowski

An inflationary epoch driven by the kinetic energy density in a dynamical Planck mass is studied. In the conformally related Einstein frame it is easiest to see the demands of successful inflation cannot be satisfied by kinetic inflation…

高能物理 - 理论 · 物理学 2010-11-01 Janna Levin

The accelerated expansion of the universe has been established through observations of supernovae, the growth of structure, and the cosmic microwave background. The most popular explanation is Einsteins cosmological constant, or dynamic…

综合物理 · 物理学 2021-09-08 Steen H. Hansen

We show that scalar field fluctuations alone can drive cosmic acceleration, provided the universe is spatially closed and the Compton wavelength of the field exceeds the radius of curvature. This mechanism may open new perspectives on…

广义相对论与量子宇宙学 · 物理学 2026-02-12 Daniel Jiménez-Aguilar

Cosmic acceleration can be achieved not only with a sufficiently flat scalar field potential but through kinetic terms coupled to gravity. These derivative couplings impose a shift symmetry on the scalar field, aiding naturalness. We write…

宇宙学与河外天体物理 · 物理学 2011-11-29 Giulia Gubitosi , Eric V. Linder

The principles of General Relativity allow for a non-vanishing cosmological constant, which can possibly be interpreted at least partially in terms of quantum-fluctuations of matter fields. Depending on sign and magnitude it can cause…

天体物理学 · 物理学 2007-05-23 Domenico Giulini , Norbert Straumann

In creating his gravitational field equations Einstein unjustifiedly assumed that inertial mass, and its energy equivalent, is a source of gravity. Denying this assumption allows modifying the field equations to a form in which a positive…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Homer G. Ellis

A new model of nonlinear electrodynamics with a dimensional parameter $\beta$ coupled to gravity is considered. We show that an accelerated expansion of the universe takes place if the nonlinear electromagnetic field is the source of the…

广义相对论与量子宇宙学 · 物理学 2016-01-26 S. I. Kruglov

The current acceleration of the universe leads us to investigate higher dimensional gravity theory, which is able to explain acceleration from a theoretical view point without the need of introducing dark energy by hand. We argue that the…

广义相对论与量子宇宙学 · 物理学 2009-06-26 S. Chatterjee , D. Panigrahi

For variable gravity models the strength of gravity, as measured by Newton's ``constant'' or the Planck mass, depends on the value of a scalar field, the cosmon. We discuss two simple four-parameter models with a quadratic or constant…

宇宙学与河外天体物理 · 物理学 2014-01-15 C. Wetterich

Homogeneous cosmological solutions are obtained in five dimensional space time assuming equations of state $ p = k\rho $ and $ p_{5}= \gamma\rho$ where p is the isotropic 3 - pressure and $p_{5}$, that for the fifth dimension. Using…

广义相对论与量子宇宙学 · 物理学 2009-11-11 D. Panigrahi , Y. Z. Zhang , S. Chatterjee

We trace the origin of the cosmological constant problem to the assumption that Newton's constant $G$ sets the scale for cosmology. And then we show that once this assumption is relaxed, the very same cosmic acceleration which has served to…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Philip D. Mannheim

Based on some observations, the apparent energy, associated with gravity, of vacuums is defined, with that of normal vacuums to be zero and that of the vacuums losing some energy to be negative. An important application of the energy is its…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Yi-Ping Qin

We show that cosmic acceleration can arise due to very tiny corrections to the usual gravitational action of General Relativity of the form $R^n$, with $n<0$. This eliminates the need for dark energy, though it does not address the…

天体物理学 · 物理学 2009-11-10 Sean M. Carroll , Vikram Duvvuri , Mark Trodden , Michael S. Turner

Recent astronomical observations of distant supernovae light-curves suggest that the expansion of the universe has recently begun to accelerate. Acceleration is created by an anti-gravitational repulsive stress, like that produced by a…

天体物理学 · 物理学 2009-10-31 John Barrow , Rachel Bean , Joao Magueijo

Starting from pure multidimensional gravity with curvature-nonlinear terms but no matter fields in the initial action, we obtain a cosmological model with two effective scalar fields related to the size of two extra factor spaces. The model…

广义相对论与量子宇宙学 · 物理学 2010-04-21 K. A. Bronnikov , S. G. Rubin , I. V. Svadkovsky

A gravity-driven inflation is shown to arise from a simple higher dimensional universe. In vacuum, the shear of $n>1$ contracting dimensions is able to inflate the remaining three spatial dimensions. Said another way, the expansion of the…

广义相对论与量子宇宙学 · 物理学 2009-10-22 Janna Levin

Increasing evidence suggests that most of the energy density of the universe consists of a dark energy component with negative pressure, a ``cosmological constant" that causes the cosmic expansion to accelerate. In this paper, we address…

天体物理学 · 物理学 2009-09-15 C. Armendariz-Picon , V. Mukhanov , Paul J. Steinhardt
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