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相关论文: Testing the theory of gravity with DESI: estimator…

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We review recent progress in the construction of modified gravity models as alternatives to dark energy as well as the development of cosmological tests of gravity. Einstein's theory of General Relativity (GR) has been tested accurately…

宇宙学与河外天体物理 · 物理学 2016-03-24 Kazuya Koyama

The Dark Energy Spectroscopic Instrument (DESI) provides an unprecedented opportunity to test deviations from general relativity (GR) that introduce a new physical scale within its redshift range. Using the connection between a Yukawa-like…

A key task in cosmology is to test the validity of general relativity (GR) at cosmological scales and, therefore, to distinguish between dark energy and modified gravity (MG) as the driver of the late-time cosmic acceleration. The decay…

宇宙学与河外天体物理 · 物理学 2025-11-07 Xinyi Zhao , Pengjie Zhang , Fuyu Dong

Tests of gravity on large-scales in the universe can be made using both imaging and spectroscopic surveys. The former allow for measurements of weak lensing, galaxy clustering and cross-correlations such as the ISW effect. The latter probe…

宇宙学与河外天体物理 · 物理学 2010-01-27 Jacek Guzik , Bhuvnesh Jain , Masahiro Takada

The recent discovery of gravitational waves marks the culmination of a sequence of successful tests of the general theory of relativity (GR) since its formulation in 1915. Yet these tests remain confined to the scale of stellar systems or…

宇宙学与河外天体物理 · 物理学 2019-01-10 Jian-hua He , Luigi Guzzo , Baojiu Li , Carlton M. Baugh

In this paper, we conduct a statistical analysis of various cosmological models within the framework of f (R) gravity theories, motivated by persistent challenges in modern cosmology, such as the unknown mechanisms driving the late-time…

宇宙学与河外天体物理 · 物理学 2025-08-04 Francisco Plaza , Lucila Kraiselburd

Modified theories of gravity provide us with a unique opportunity to generate innovative tests of gravity. In Chameleon f(R) gravity, the gravitational potential differs from the weak-field limit of general relativity (GR) in a mass…

宇宙学与河外天体物理 · 物理学 2016-04-26 Alejo Stark , Christopher J. Miller , Nicholas Kern , Daniel Gifford , Gong-Bo Zhao , Baojiu Li , Kazuya Koyama , Robert C. Nichol

Redshift-space distortions (RSD) offer an attractive method to measure the growth of cosmic structure on large scales, and combining with the measurement of the cosmic expansion history, it can be used as cosmological tests of gravity. With…

宇宙学与河外天体物理 · 物理学 2014-10-22 Atsushi Taruya , Kazuya Koyama , Takashi Hiramatsu , Akira Oka

Modifications of general relativity provide an alternative explanation to dark energy for the observed acceleration of the universe. We review recent developments in modified gravity theories, focusing on higher dimensional approaches and…

宇宙学与河外天体物理 · 物理学 2015-05-18 Bhuvnesh Jain , Justin Khoury

The Dark Energy Spectroscopic Instrument (DESI) survey will measure spectroscopic redshifts for millions of galaxies across roughly $14,000 \, \mathrm{deg}^2$ of the sky. Cross-correlating targets in the DESI survey with complementary…

Modified gravity theories may provide an alternative to dark energy to explain cosmic acceleration. We argue that the observational program developed to test dark energy needs to be augmented to capture new tests of gravity on astrophysical…

宇宙学与河外天体物理 · 物理学 2015-05-27 Bhuvnesh Jain

Future galaxy surveys hope to distinguish between the dark energy and modified gravity scenarios for the accelerating expansion of the Universe using the distortion of clustering in redshift space. The aim is to model the form and size of…

宇宙学与河外天体物理 · 物理学 2011-01-06 Elise Jennings , Carlton M. Baugh , Silvia Pascoli

Despite the success of general relativity (GR), the unexplained nature of dark energy on cosmological scales leaves open the question of whether GR provides a complete description of gravity. This quest is further motivated by growing…

We review recent developments and results in testing general relativity (GR) at cosmological scales. The subject has witnessed rapid growth during the last two decades with the aim of addressing the question of cosmic acceleration and the…

宇宙学与河外天体物理 · 物理学 2019-12-09 Mustapha Ishak

$E_G$ is a summary statistic that combines cosmological observables to achieve a test of gravity that is relatively model-independent. Here, we consider the power of a measurement of $E_G$ using galaxy-galaxy lensing and galaxy clustering…

宇宙学与河外天体物理 · 物理学 2026-03-24 C. D. Leonard , S. Alam , R. Mandelbaum , M. M. Rau , S. Singh , C. M. A. Zanoletti , the LSST Dark Energy Science Collaboration

In the last two decades, Modified Gravity (MG) models have been proposed to explain the accelerated expansion of the Universe. However, one of the main difficulties these theories face is that they must reduce to General Relativity (GR) at…

广义相对论与量子宇宙学 · 物理学 2021-10-27 Alejandro Aviles

We present the first computation of the gravity model testing parameter $E_G$ on realistic simulated modified gravity galaxy mocks. The analysis is conducted using two twin simulations presented in arXiv:1805.09824(1): one based on general…

宇宙学与河外天体物理 · 物理学 2025-05-19 C. Viglione , P. Fosalba , I. Tutusaus , L. Blot , J. Carretero , P. Tallada , F. Castander

Gravitational waves (GWs) provide a new tool to probe the nature of dark energy (DE) and the fundamental properties of gravity. We review the different ways in which GWs can be used to test gravity and models for late-time cosmic…

宇宙学与河外天体物理 · 物理学 2018-12-24 Jose María Ezquiaga , Miguel Zumalacárregui

General Relativity (GR) describes gravitation well at the energy scales which we have so far been able to achieve or detect. However, we do not know whether GR is behind the physics governing stronger gravitational field regimes, such as…

广义相对论与量子宇宙学 · 物理学 2012-09-13 Priscilla Canizares , Jonathan R. Gair , Carlos F. Sopuerta
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