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The strong equivalence principle is extended in application to averaged dynamical fields in cosmology to include the role of the average density in the determination of inertial frames. The resulting cosmological equivalence principle is…

广义相对论与量子宇宙学 · 物理学 2008-11-26 David L. Wiltshire

On the largest scales there is evidence of discrete structure, examples of this are superclusters and voids and also by redshift taking discrete values. In this paper it is proposed that discrete redshift can be explained by using the…

天体物理学 · 物理学 2011-04-04 Mark D. Roberts

We derive the metric of an expanding universe with zero accelerations by pure kinematic method. By doing so we expatiate physics related with co-moving coordinate system in details. The most important discovery or our study is, in an…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Ding-fang Zeng

The cosmic curvature $\Omega_{K,0}$, which determines the spatial geometry of the universe, is an important parameter in modern cosmology. Any deviation from $\Omega_{K,0}=0$ would have a profound impact on primordial inflation paradigm and…

宇宙学与河外天体物理 · 物理学 2023-04-14 Peng-Ju Wu , Jing-Zhao Qi , Xin Zhang

We establish a relationship between the multipoles of the expansion rate fluctuation field $\eta,$ which capture in an accurate way deviations from isotropy in the redshift-distance relation, and the multipoles of the covariant cosmographic…

宇宙学与河外天体物理 · 物理学 2025-01-06 Basheer Kalbouneh , Christian Marinoni , Roy Maartens

We examine the cosmological implications of measurements of the void-galaxy cross-correlation at redshift $z=0.57$ combined with baryon acoustic oscillation (BAO) data at $0.1<z<2.4$. We find direct evidence of the late-time acceleration…

宇宙学与河外天体物理 · 物理学 2020-07-01 Seshadri Nadathur , Will J. Percival , Florian Beutler , Hans Winther

Higher order theories of gravity have recently attracted a lot of interest as alternative candidates to explain the observed cosmic acceleration without the need of introducing any scalar field. A critical ingredient is the choice of the…

天体物理学 · 物理学 2009-11-10 S. Capozziello , V. F. Cardone , A. Troisi

In this paper, the dynamical behavior of the accelerated expansion of the universe is studied within the framework of $f(T)$ gravity by considering a well-motivated functional form of $f(T)$. A specific form of the Hubble parameter is…

广义相对论与量子宇宙学 · 物理学 2026-03-20 Khomesh R. Patle , G. P. Singh

A measurement of the redshift drift constitutes a model-independent probe of fundamental cosmology. Several approaches are being considered to make the necessary observations, using (i) the Extremely Large Telescope (ELT), (ii) the Cosmic…

宇宙学与河外天体物理 · 物理学 2024-12-13 Fulvio Melia

We present the luminosity distance series expansion to third order in redshift for a general space-time with no assumption on the metric tensor or the field equations prescribing it. It turns out that the coefficients of this general…

宇宙学与河外天体物理 · 物理学 2021-06-25 Asta Heinesen

Cosmologists are exploring two possible sets of explanations for the remarkable observation of cosmic acceleration: dark energy fills space or general relativity fails on cosmological scales. We define a null test parameter $\epsilon(k,a)…

天体物理学 · 物理学 2008-11-26 Viviana Acquaviva , Amir Hajian , David N. Spergel , Sudeep Das

Astronomical measurements of the Omegas for mass density, cosmological constant lambda and curvature k are shown to be sufficient to produce a unique and detailed cosmological model describing dark energy influences based on the Friedman…

综合物理 · 物理学 2010-01-14 James G. Gilson

The number of galaxies at a given flux as a function of the redshift, $z$, is derived when the $z$-distance relation is non-standard. In order to compare different models, the same formalism is also applied to the standard cosmology. The…

宇宙学与河外天体物理 · 物理学 2015-09-07 L. Zaninetti

f(R) gravity is one of the simplest viable modifications to General Relativity: it passes local astrophysical tests, predicts both the early-time cosmic inflation and the late-time cosmic acceleration, and also describes dark matter. In…

宇宙学与河外天体物理 · 物理学 2024-03-22 Didam Duniya , Amare Abebe , Alvaro de la Cruz-Dombriz , Peter Dunsby

The GRAVITY Collaboration achieved the remarkable detection of the orbital precession of the S2 star around the Galactic centre supermassive black hole, providing yet another proof of the validity of the General Relativity. The departure…

广义相对论与量子宇宙学 · 物理学 2021-11-18 Ivan de Martino , Riccardo della Monica , Mariafelicia de Laurentis

The challenging issue of determining the correct $f(R)$ among several possibilities is here revised by means of numerical reconstructions of the modified Friedmann equations around the redshift interval $z\in[0,1]$. Frequently, a severe…

宇宙学与河外天体物理 · 物理学 2015-06-24 Liberato Pizza

The number of galaxies with measured redshifts > 1 is at present rapidly increasing, allowing for measurements of their correlation function. The correlations function is measured in redshift space, as a function of angular separation and…

天体物理学 · 物理学 2009-10-31 Vibhat Nair

Fluctuations in sky maps of the galaxy redshifts, dubbed as angular redshift fluctuations (ARF), contain precise information about the growth rate of structures and the nature of gravity in the Universe. Specifically, ARF constrain the…

宇宙学与河外天体物理 · 物理学 2021-03-31 Carlos Hernández-Monteagudo , Jonás Chaves-Montero , Raúl E. Angulo , Giovanni Aricò

We probe the cosmic expansion scenario within the framework of $f(R, L_{m})$ gravity by employing a well-motivated functional form of $f(R, L_{m}) = \frac{R}{2} + L_{m}^{\lambda}$. Specifically, we introduce three novel cosmological models…

广义相对论与量子宇宙学 · 物理学 2026-05-27 Khomesh R. Patle , G. P. Singh

In this work we perform an observational data analysis on the $f(R,T)$ gravity with the aim of constraining the parameter space of the model. Five different models are considered and the 30 point $z-H(z)$ cosmic chronometer data is used in…

广义相对论与量子宇宙学 · 物理学 2021-05-24 Prabir Rudra , Kinsuk Giri
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