中文
相关论文

相关论文: A GREAT model comparison against the cosmological …

200 篇论文

The unimodular theory of gravity is an alternative perspective to traditional Einstein's general relativity and opens new possibilities for exploring its implications in cosmology. In this paper, we investigate the unimodular gravity (UG)…

宇宙学与河外天体物理 · 物理学 2024-02-09 Naveen K. Singh , Gopal Kashyap

An overview is presented of a recently proposed "radically conservative" solution to the problem of dark energy in cosmology. The proposal yields a model universe which appears to be quantitatively viable, in terms of its fit to supernovae…

天体物理学 · 物理学 2017-08-23 David L. Wiltshire

We test the theoretical predictions of several cosmological models against different observables to compare the indirect estimates of the current expansion rate of the Universe determined from model fitting with the direct measurements…

宇宙学与河外天体物理 · 物理学 2016-11-09 Vladimir V. Luković , Rocco D'Agostino , Nicola Vittorio

We have shown that the varying physical constant model is consistent with the recently published variational approach wherein Einstein equations are modified to include the variation of the speed of light c, gravitational constant G and…

宇宙学与河外天体物理 · 物理学 2020-09-21 Rajendra P. Gupta

Observational constraints guide one forcefully to examine models in which the matter density is substantially less than critical density. Particularly noteworthy are those which are consistent with inflation. For these models, microwave…

天体物理学 · 物理学 2007-05-23 J. P. Ostriker , Paul J. Steinhardt

Measurements of the current expansion rate of the Universe, $H_0$, using standard candles, disagree with those derived from observations of the Cosmic Microwave Background (CMB). This discrepancy, known as the Hubble tension, is substantial…

宇宙学与河外天体物理 · 物理学 2024-02-05 Sergio Torres-Arzayus

We provide a new extension of general relativity (GR) which has the remarkable property of being more constrained than GR plus a cosmological constant, having one less free parameter. This is implemented by allowing the cosmological…

广义相对论与量子宇宙学 · 物理学 2019-10-09 Stephon Alexander , Marina Cortês , Andrew R. Liddle , João Magueijo , Robert Sims , Lee Smolin

A range of cosmological observations demonstrate an accelerated expansion of the Universe, and the most likely explanation of this phenomenon is a cosmological constant. Given the importance of understanding the underlying physics, it is…

宇宙学与河外天体物理 · 物理学 2021-04-07 Karoline Loeve , Kristine Simone Nielsen , Steen H. Hansen

Delta Gravity is a gravitational model based on an extension of General Relativity given by a new symmetry called $\tilde{\delta}$. In this model, new matter fields are added to the original matter fields, motivated by the additional…

宇宙学与河外天体物理 · 物理学 2021-07-01 Jorge Alfaro , Marco San Martín , Carlos Rubio

In this {\sl Letter} we construct the Hubble diagram (HD) for the standard Friedmann-Lema\^itre-Robertson-Walker (FLRW) cosmological model after enforcing it with the general relativistic energy conditions, heeding to investigate whether it…

We provide preliminary quantitative evidence that a new solution to averaging the observed inhomogeneous structure of matter in the universe [gr-qc/0702082, arxiv:0709.0732], may lead to an observationally viable cosmology without exotic…

天体物理学 · 物理学 2008-11-26 Ben M. Leith , S. C. Cindy Ng , David L. Wiltshire

We use the new gamma-ray bursts (GRBs) data, combined with the baryon acoustic oscillation(BAO) observation from the spectroscopic Sloan Digital Sky Survey (SDSS) data release, the newly obtained $A$ parameter at $z=0.6$ from the WiggleZ…

宇宙学与河外天体物理 · 物理学 2012-12-27 Yu Pan , Shuo Cao , Yungui Gong , Kai Liao , Zong-Hong Zhu

In this work, we revisit/reinterpret/extend the model-independent analysis method (which we now call spread - luminosity distance fitting, spread-LDF) from our previous work. We apply it to the updated supernova type Ia catalogue, Pantheon+…

广义相对论与量子宇宙学 · 物理学 2025-12-02 A. Kazım Çamlıbel , M. Akif Feyizoğlu , İbrahim Semiz

We apply the technique of parameter-splitting to existing cosmological data sets, to check for a generic failure of dark energy models. Given a dark energy parameter, such as the energy density Omega_Lambda or equation of state w, we split…

天体物理学 · 物理学 2008-11-26 Sheng Wang , Lam Hui , Morgan May , Zoltan Haiman

Recently, some divergent conclusions about cosmic acceleration were obtained using type Ia supernovae (SNe Ia), with opposite assumptions on the intrinsic luminosity evolution. In this paper, we use strong gravitational lensing systems to…

宇宙学与河外天体物理 · 物理学 2019-02-20 Z. L. Tu , J. Hu , F. Y. Wang

In this paper, by considering an absorption probability independent of photon wavelength, we show that current type Ia supernovae (SNe Ia) and gamma ray burst (GRBs) observations plus high-redshift measurements of the cosmic microwave…

宇宙学与河外天体物理 · 物理学 2018-02-07 R. F. L. Holanda , S. H. Pereira , Deepak Jain

We carry out a Bayesian model selection analysis of different dark energy parametrizations using the recent luminosity distance data of high redshift supernovae from Riess et al. 2007 and from the new ESSENCE Supernova Survey. Including…

天体物理学 · 物理学 2008-11-26 Paolo Serra , Alan Heavens , Alessandro Melchiorri

Astronomical observations reveal a major deficiency in our understanding of physics $-$ the detectable mass is insufficient to explain the observed motions in a huge variety of systems given our current understanding of gravity, Einstein's…

宇宙学与河外天体物理 · 物理学 2022-07-07 Indranil Banik , Hongsheng Zhao

New observational constraints on the cosmic matter density $\Omega_m$ and an effectively redshift-independent equation of state parameter $w_x$ of the dark energy are obtained while simultaneously testing the strong and null energy…

In this paper, we use a newly compiled sample of ultra-compact structure in radio quasars and strong gravitational lensing systems with quasars acting as background sources to constrain six spatially flat and non-flat cosmological models…

宇宙学与河外天体物理 · 物理学 2022-12-07 Tonghua Liu , Shuo Cao , Xiaolei Li , Hao Zheng , Yuting Liu , Wuzheng Guo , Chenfa Zheng