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The discovery of the accelerating universe indicates strongly the presence of a scalar field which is not only expected to solve today's version of the cosmological constant problem, or the fine-tuning and the coincidence problems, but also…

广义相对论与量子宇宙学 · 物理学 2010-02-24 Yasunori Fujii , Kensuke Homma

The cosmological evolution of free massless vector or tensor (but not gauge) fields minimally coupled to gravity is analyzed. It is shown that there are some unstable solutions for these fields in De Sitter background. The back reaction of…

天体物理学 · 物理学 2009-12-30 A. D. Dolgov

The accelerating expansion of the universe is the most surprising cosmological discovery in many decades. In this short review, we briefly summarize theories for the origin of cosmic acceleration and the observational methods being used to…

宇宙学与河外天体物理 · 物理学 2014-01-03 Michael J. Mortonson , David H. Weinberg , Martin White

On the basis of a recent cosmological model, the puzzle of galactic rotational velocities at their edges is explained without invoking dark matter. A rationale for the existence of structures like galaxies and superclusters is also…

天体物理学 · 物理学 2007-05-23 B. G. Sidharth

A new cosmological scenario driven by a slow rolling homogeneous scalar field whose exponential potential $V(\Phi)$ has a quadratic dependence on the field $\Phi$ in addition to the standard linear term is discussed. The derived equation of…

天体物理学 · 物理学 2009-11-11 F. C. Carvalho , J. S. Alcaniz , J. A. S. Lima , R. Silva

We present an extension of $f(T)$ gravity, allowing for a general coupling of the torsion scalar $T$ with the trace of the matter energy-momentum tensor $\mathcal{T}$. The resulting $f(T,\mathcal{T})$ theory is a new modified gravity, since…

广义相对论与量子宇宙学 · 物理学 2014-12-12 Tiberiu Harko , Francisco S. N. Lobo , G. Otalora , Emmanuel N. Saridakis

The issues of quintessence and cosmic acceleration can be discussed in the framework of theories which do not include necessarily scalar fields. It is possible to define pressure and energy density for new components considering effective…

天体物理学 · 物理学 2008-11-26 S. Capozziello , S. Carloni , A. Troisi

The common attribute of all Big Bang cosmologies is that they are based on the assumption that the universe is expanding. However examination of the evidence for this expansion clearly favours a static universe. The major topics considered…

综合物理 · 物理学 2014-07-10 David F. Crawford

We review matter bounce scenarios where the matter content is dark matter and dark energy. These cosmologies predict a nearly scale-invariant power spectrum with a slightly red tilt for scalar perturbations and a small tensor-to-scalar…

宇宙学与河外天体物理 · 物理学 2016-12-28 Yi-Fu Cai , Antonino Marciano , Dong-Gang Wang , Edward Wilson-Ewing

Scalar-tensor~(ST) theories of gravity are natural phenomenological extensions to general relativity. Although these theories are severely constrained both by solar system experiments and by binary pulsar observations, a large set of ST…

广义相对论与量子宇宙学 · 物理学 2016-02-10 Carlos Palenzuela , Steve Liebling

The cosmological model best capable of fitting current observational data features two separate epochs during which the Universe is accelerating. During the earliest stages of the Universe, such acceleration is known as cosmological…

天体物理学 · 物理学 2009-10-31 Andrew R Liddle

Nearly seventy per cent of the energy density in the universe is unclustered and exerts negative pressure. This conclusion -- now supported by numerous observations -- poses the greatest challenge for theoretical physics today. I discuss…

天体物理学 · 物理学 2009-07-09 T. Padmanabhan

We describe what cosmology looks like in the context of the geometric theory of gravity (GSG) based on a single scalar field. There are two distinct classes of cosmological solutions. An interesting feature is the possibility of having a…

广义相对论与量子宇宙学 · 物理学 2015-02-17 E. Bittencourt , U. Moschella , M. Novello , J. D. Toniato

Several kinds of astronomical observations, interpreted in the framework of the standard Friedmann-Robertson-Walker cosmology, have indicated that our universe is dominated by a Cosmological Constant. The dimming of distant Type Ia…

天体物理学 · 物理学 2014-11-18 Subir Sarkar

Typical cosmological models are based on the postulate that space is homogeneous. Space however contains overdense regions in which matter is concentrating, leaving underdense regions of almost void. The evolution of the scale factor of the…

宇宙学与河外天体物理 · 物理学 2022-05-27 Vincent Deledicque

One possible description for the current accelerated expansion of the universe is quintessence dynamics. The basic idea of quintessence consists of analyzing cosmological scenarios driven by scalar fields. In this work we present some…

广义相对论与量子宇宙学 · 物理学 2014-04-10 P. H. R. S. Moraes , J. R. L. Santos

Certain results of observational cosmology cast critical doubt on the foundations of standard cosmology but leave most cosmologists untroubled. Alternative cosmological models that differ from the Big Bang have been published and defended…

综合物理 · 物理学 2009-05-18 Martin Lopez-Corredoira

It is argued that the Brans-Dicke theory may explain the present accelerated expansion of the universe without resorting to a cosmological constant or quintessence matter

广义相对论与量子宇宙学 · 物理学 2009-10-31 Narayan Banerjee , Diego Pavon

The recent simultaneous detection of gravitational waves and a gamma ray burst from a neutron star merger significantly shrank the space of viable scalar-tensor theories by demanding that the speed of gravity is equal to that of light. The…

宇宙学与河外天体物理 · 物理学 2018-04-06 Marco Crisostomi , Kazuya Koyama

We note that in general there exist two basic aspects in any branch of physics, including cosmology - one dealing with the attributes of basic constituents and forces of nature, the other dealing with how structures arise from them and how…

广义相对论与量子宇宙学 · 物理学 2007-05-23 B. L. Hu