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It is very likely that the quantum description of spacetime is quite different from what we perceive at large scales, $l\gg (G\hbar/c^3)^{1/2}$. The long wave length description of spacetime, based on Einstein's equations, is similar to the…

广义相对论与量子宇宙学 · 物理学 2009-11-10 T. Padmanabhan

We have assumed that in a physical universe a blackhole is created some where. We conjecture that this blackhole will then separate itself from the physical universe and will build up an extra dimensional entity associated with the physical…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. M. Harunar Rashid , Arshad Momen , A. L. Choudhury

The possibility that the expansion rate of the Universe, as reflected by the Red Shift, could be produced by the existence of the dilaton field is explored. The analysis starts from previously studied solutions of the Einstein equations for…

高能物理 - 理论 · 物理学 2007-05-23 Alejandro Cabo , Alexis Amezaga

We present a unified evolution of the universe from very early times until the present epoch by including both the leading local correction $R^2$ and the leading non-local term $R\frac{1}{\square^2}R$ to the classical gravitational action.…

广义相对论与量子宇宙学 · 物理学 2018-05-09 Alessandro Codello , Rajeev Kumar Jain

The quantity and quality of cosmic structure observations have greatly accelerated in recent years. Further leaps forward will be facilitated by imminent projects, which will enable us to map the evolution of dark and baryonic matter…

A quantum expansion parameter, analogous to the Hubble parameter in cosmology, is defined for a free particle quantum wavefunction. By considering the universe as an initial single Gaussian quantum wavepacket whose mass is that of…

宇宙学与河外天体物理 · 物理学 2012-02-28 A. D. Ernest

The cosmological redshifts z in the frequencies of spectral lines from distant galaxies as compared with their values observed in terrestrial laboratories, which are due to the scale factor a(t), frequently are interpret as a…

综合物理 · 物理学 2011-12-07 Branislav Vlahovic

It is shown that topological changes in space-time are necessary to make General Relativity compatible with the Newtonian limit and to solve the hierarchy of the fundamental interactions. We detail how topology and topological changes…

广义相对论与量子宇宙学 · 物理学 2012-12-10 M. D. Maia

Emergent gravity views spacetime as an entity emergent from a more complete theory of interacting fundamental constituents valid at much finer resolution or higher energies, usually assumed to be above the Planck energy. In this view…

广义相对论与量子宇宙学 · 物理学 2010-03-12 B. L. Hu

Phenomena currently attributed to Dark Energy (DE) and Dark Matter (DM) are merely a result of the interplay between gravitational energy density, generated by the contraction of space by matter, and the energy density of the Cosmological…

天体物理学 · 物理学 2008-12-25 Shlomo Barak , Elia M Leibowitz

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

A underlying dynamical structure for both relativity and quantum theory-``superrelativity'' has been proposed in order to overcome the well known incompatibility between these theories. The relationship between curvature of spacetime…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Peter Leifer

It has been speculated that gravity could be an emergent phenomenon, with classical general relativity as an effective, macroscopic theory, valid only for classical systems at large temporal and spatial scales. As in classical continuum…

广义相对论与量子宇宙学 · 物理学 2015-06-24 Huan Yang , Larry R. Price , Nicolas D. Smith , Rana X Adhikari , Haixing Miao , Yanbei Chen

In this paper we suppose that the cosmological constant will change when the universe expends. For a general consideration, the cosmological constant is assumed to be a function of scale factor and Hubble constant. According to the ADM…

宇宙学与河外天体物理 · 物理学 2010-08-03 Jin-Zhang Tang , Qiang Xu

It is widely believed that the large redshifts for distant supernovae are explained by the vacuum energy dominance, or, in other words, by the cosmological constant in Einstein's equations, which is responsible for the anti-gravitation…

广义相对论与量子宇宙学 · 物理学 2008-11-26 B. P. Kosyakov

After a brief introduction to the sixteenth and seventeenth century views of the Universe and the nineteenth century paradox of Olbers, we start the history of the cosmic expansion with Hubble's epochal discovery of the recession velocities…

天体物理学 · 物理学 2008-02-15 Matts Roos

The discovery that the expansion of the universe is accelerating in time is a major discovery which still awaits adequate explanation. It is generally agreed that this implies a cosmic repulsion as a result of the existence of a…

综合物理 · 物理学 2008-11-26 R. F. O'Connell

Using a collapsing matter model at the center of an expanding universe as described by Weinberg we assume a special type of generated pressure. This pressure transmits into the surrounding expanding universe. Under certain restriction the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. Latif Choudhury

From the first observations made by Slipher, our understanding and interpretation of the cosmological redshift was evolving until reaching the current consensus, through the expanding universe and the emergence of modern physical cosmology…

宇宙学与河外天体物理 · 物理学 2020-02-28 Gabriel R. Bengochea

Quantum gravity, as a fundamental theory of space-time, is expected to reveal how the universe may have started, perhaps during or before an inflationary epoch. It may then leave a potentially observable (but probably minuscule) trace in…

广义相对论与量子宇宙学 · 物理学 2015-12-17 Martin Bojowald
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