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In cosmology based on general relativity, the universe is modeled as a fluid. The transition from the Einstein field equation to its large-scale (cosmological) version is thus analogous to the transition, for a system consisting of a large…

综合物理 · 物理学 2018-10-18 Gregory Ryskin

The recent measurements of the Hubble constant based on the standard $\Lambda$CDM cosmology reveal an underlying disagreement between the early-Universe estimates and the late-time measurements. Moreover, as these measurements improve, the…

综合物理 · 物理学 2020-11-25 Ram Gopal Vishwakarma

A nonhomogeneous universe with vacuum energy, but without spacetime expansion, is utilized together with gravitational and Doppler redshifts as the basis for proposing a new interpretation of the Hubble relation and the 2.7K Cosmic…

天体物理学 · 物理学 2009-10-30 Robert V. Gentry

If gravitons are super-strong interacting particles and the low-temperature graviton background exists, the basic cosmological conjecture about the Dopplerian nature of redshifts may be false. In this case, a full magnitude of cosmological…

高能物理 - 理论 · 物理学 2007-05-23 Michael A. Ivanov

The Hubble constant, which measures the expansion rate, together with the total energy density of the Universe, sets the size of the observable Universe, its age, and its radius of curvature. Excellent progress has been made recently toward…

天体物理学 · 物理学 2008-11-26 Wendy L. Freedman

This report continues recent Peebles-Turner debate "Is cosmology solved?" and considers the first results for Sandage's program for "Practical cosmology". A review of conceptual problems of modern cosmological models is given, among them:…

天体物理学 · 物理学 2009-10-31 Yurij V. Baryshev

A wide range of large scale observations hint towards possible modifications on the standard cosmological model which is based on a homogeneous and isotropic universe with a small cosmological constant and matter. These observations, also…

宇宙学与河外天体物理 · 物理学 2014-01-21 Leandros Perivolaropoulos

In view of late-time cosmic acceleration, a dark energy cosmological model is revisited wherein Einstein's cosmological constant is considered as a candidate of dark energy. Exact solution of Einstein field equations (EFEs) is derived in a…

广义相对论与量子宇宙学 · 物理学 2019-11-22 S. K. J. Pacif , Md Salahuddin Khan , L. K. Paikroy , Shalini Singh

The coincidence problem of late cosmic acceleration constitutes a serious riddle with regard to our understanding of the evolution of the Universe. Here we argue that this problem may someday be solved -or better understood- by expressing…

天体物理学 · 物理学 2008-11-26 Sergio del Campo , Ramon Herrera , Diego Pavon

We revisit the quantum cosmological constant problem and highlight the important roles played by the dS horizon of zero point energy. We argue that fields which are light enough to have dS horizon of zero point energy comparable to the FLRW…

广义相对论与量子宇宙学 · 物理学 2022-09-30 Hassan Firouzjahi

It is introduced a hypothesis that the gravitational potential in the universe changes linearly with the time. This enables to explain the Hubble red shift and the anomalous acceleration of Pioneer 10 and 11.

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

We apply the new dynamics of 3-space to cosmology by deriving a Hubble expansion solution. This dynamics involves two constants; G and alpha - the fine structure constant. This solution gives an excellent parameter-free fit to the recent…

综合物理 · 物理学 2007-06-27 Reginald T Cahill

Dark energy is one of the greatest scientific mysteries of today. The idea that dark energy originates from quantum vacuum fluctuations has circulated since the late '60s, but theoretical estimations of vacuum energy have disagreed with the…

广义相对论与量子宇宙学 · 物理学 2021-09-10 Dror Berechya , Ulf Leonhardt

The current state of cosmology is easy to summarize: a very successful standard model -- the hot big-bang cosmology -- that accounts for the evolution of the Universe from 10^{-2} sec until the present; bold ideas based upon early-Universe…

天体物理学 · 物理学 2009-10-30 Michael S. Turner

There is sufficient amount of internal evidence in the nature of gravitational theories to indicate that gravity is an emergent phenomenon like, e.g, elasticity. Such an emergent nature is most apparent in the structure of gravitational…

宇宙学与河外天体物理 · 物理学 2015-06-05 T. Padmanabhan

The article addresses a possibility of obtaining cosmologically relevant effects from the quantum nature of the Hubble horizon. Following the observation made by E.~Bianchi and C.~Rovelli in Phys.\ Rev.\ D {\bf 84} (2011) 027502 we explore…

广义相对论与量子宇宙学 · 物理学 2019-09-04 Michal Artymowski , Jakub Mielczarek

If we separate energy in a holographic theory into an extensive part and an intrinsic part, where the extensive part is given by the cosmological constant, and assume entropy be given by the Gibbon-Hawking formula, the Cardy-Verlinde…

高能物理 - 理论 · 物理学 2009-11-10 Ke Ke , Miao Li

I show that a cumulative contraction or expansion must result from repetitive tidal action in a curved stress field, depending on the direction of the curvature. The resulting expansion of solid materials onboard deep space probes and the…

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

The Hubble tension refers to the discrepancy in the value of the Hubble constant $H_0$ inferred from the cosmic microwave background observations, assuming the concordance $\Lambda$CDM model of the Universe, and that from the distance…

宇宙学与河外天体物理 · 物理学 2024-03-19 Yashi Tiwari , Basundhara Ghosh , Rajeev Kumar Jain

The Hubble diagram is one of the cornerstones of observational cosmology. It is usually analysed assuming that, on average, the underlying relation between magnitude and redshift matches the prediction of a…

宇宙学与河外天体物理 · 物理学 2017-04-05 Pierre Fleury , Chris Clarkson , Roy Maartens