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It is shown that the observed cmb dipole implies the existence of a center for the expansion of the universe, and that it can be explained by a combination of peculiar velocity and Hubble flow.

天体物理学 · 物理学 2007-10-30 Yukio Tomozawa

We explore the dynamics and evolution of the Universe at early and late times, focusing on both dark energy and extended gravity models and their astrophysical and cosmological consequences. Modified theories of gravity not only provide an…

{\it The universe is expanding} is known (through Galaxy observations) since 1929 through Hubble's discovery ($V = H D$). Recently in 1999, it is found (through Supernovae observations) that the universe is not simply expanding but is…

综合物理 · 物理学 2010-10-20 R. C. Gupta , Anirudh Pradhan

In an expanding universe the vacuum energy density \rho_{\Lambda} is expected to be a dynamical quantity. In quantum field theory in curved space-time \rho_{\Lambda} should exhibit a slow evolution, determined by the expansion rate of the…

高能物理 - 唯象学 · 物理学 2015-06-04 Harald Fritzsch , Joan Sola

Hubble's law, which states a linear increase in velocities with distances, can physically be understood in terms of an acceleration cH. This work proposes a connection between this "universal" acceleration seen in the solar system and the…

综合物理 · 物理学 2021-11-09 Y. G. Yi

We consider the fate of the observable universe in the light of the discovery of a dark energy component to the cosmic energy budget. We extend results for a cosmological constant to a general dark energy component and examine the…

天体物理学 · 物理学 2009-11-07 Dragan Huterer , Glenn D. Starkman , Mark Trodden

The novel idea is that the undergoing accelerated expansion of the universe happens due to infrared quantum gravity modifications at intermediate astrophysical scales of galaxies or galaxy clusters, within the framework of Asymptotically…

广义相对论与量子宇宙学 · 物理学 2021-02-16 Fotios K. Anagnostopoulos , Georgios Kofinas , Vasilios Zarikas

It is argued that fluctuations of quantum fields in four-dimensional space do not give rise to dark energy, but are rather a negligible contribution to dark matter. By (relativistic) dark matter we mean that the relation between pressure…

高能物理 - 唯象学 · 物理学 2011-07-18 Kimball A. Milton

In the standard model of universe the increase in mass of our observed expansive and isotropic relativistic Universe is explained by the hypothetical assumption of matter objects emerging on the horizon (of the most remote visibility).…

广义相对论与量子宇宙学 · 物理学 2008-12-19 V. Skalsky

We study the possibility to probe the spatial geometry of the Universe by supernova measurement of the cubic correction to the luminosity distance. We illustrate with an accelerating universe model with infinite-volume extra dimensions, for…

高能物理 - 理论 · 物理学 2009-11-10 Bin Wang , Yungui Gong , Ru-Keng Su

The possibility that spacetime is extended beyond the familiar 3+1-dimensions has intrigued physicists for a century. Indeed, the consequences of a dimensionally richer spacetime would be profound. Recently, new theories with higher…

高能物理 - 唯象学 · 物理学 2008-11-26 JoAnne Hewett , Maria Spiropulu

We assume the spacetime foam picture in which vacuum is filled with virtual wormholes. In the presence of an external field the distribution of wormholes changes. We consider an anisotropic distribution of wormholes and analyze its relation…

广义相对论与量子宇宙学 · 物理学 2016-06-14 E. P. Savelova

In this paper we study the viability of an entropic cosmological model. The effects of entropic gravity are derived from a modified entropy-area relationship with a volumetric entropy term. This model describes a late time limit cosmic…

广义相对论与量子宇宙学 · 物理学 2024-03-07 Javier Chagoya , I. Díaz-Saldaña , J. C. López-Domínguez , M. Sabido

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

The origins of recently reported anisotropy of the local velocity field of nearby galaxies (velocities < 500 km/s corresponding to the distance less than 8 Mpc) are studied. The exact solution of the Newtonian equation for the expanding…

天体物理学 · 物理学 2009-04-15 Monika Biernacka , Piotr Flin , Victor Pervushin , Andrey Zorin

The expansion of the Universe is the basis of modern cosmology. This chapter outlines the theory behind the expansion of the universe, including the cosmological principle, distances, velocities, and accelerations. We provide basic…

宇宙学与河外天体物理 · 物理学 2025-09-15 Tamara M. Davis

We review a cosmology in which particles are fluctuationally created from a background Zero Point Field. This cosmology is consistent with recent observations of an ever expanding and accelerating universe, as also the recently confirmed…

综合物理 · 物理学 2015-06-26 B. G. Sidharth

We investigate non-singular bounce and cyclic cosmological evolutions in a universe governed by the extended nonlinear massive gravity, in which the graviton mass is promoted to a scalar-field potential. The extra freedom of the theory can…

宇宙学与河外天体物理 · 物理学 2012-11-05 Yi-Fu Cai , Caixia Gao , Emmanuel N. Saridakis

In this article we review the discovery of the accelerating universe using type Ia supernovae. We then outline ways in which dark energy - component that causes the acceleration - is phenomenologically described. We finally describe…

宇宙学与河外天体物理 · 物理学 2016-11-15 Dragan Huterer

Whether our universe with present day acceleration can eventually collapse is very interesting problem. We are also interesting in such problems, whether the universe is closed? Why it is so flat? How long to expend a period for a cycle of…

天体物理学 · 物理学 2007-05-23 De-Hai Zhang
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