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相关论文: Redshift-space density versus real-space velocity …

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Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the key parameters that describe the galaxy density field and its spatial correlations in redshift space. Methods. We use the Bayesian formalism…

We describe the construction of an N-body simulation that mimics the true velocity and mass-density fields in a box of side 256\hmpc about the Local Group , and the production of mock catalogs that mimic in detail current catalogs of…

天体物理学 · 物理学 2009-10-28 Tsafrir Kolatt , Avishai Dekel , Galit Ganon , Jeffrey Willick

We present a simple model for the shape of the distribution function of galaxy peculiar velocities. We show how both nonlinear and linear theory terms combine to produce a distribution which has an approximately Gaussian core with…

天体物理学 · 物理学 2009-10-31 Ravi K. Sheth , Antonaldo Diaferio

We review the quantitative science that can be and has been done with redshift and peculiar velocity surveys of galaxies in the nearby universe. After a brief background setting the cosmological context for this work, the first part of this…

天体物理学 · 物理学 2016-08-30 Michael A. Strauss , Jeffrey A. Willick

The geometry of Freedman-Roberston-Walker cosmological models is fixed by the mass density parameter, Omega_M, and the cosmological constant, Omega_Lambda. The classical volume-redshift cosmological relation is a sensitive…

天体物理学 · 物理学 2007-05-23 R. G. Carlberg

We introduce a formalism, valid both for dark matter and collapsed objects, that allows us to describe redshift space distortions in the context of the Effective Field Theory of Large Scale Structures (EFTofLSS). Expressing density…

宇宙学与河外天体物理 · 物理学 2014-09-08 Leonardo Senatore , Matias Zaldarriaga

We present a public code to generate a mock galaxy catalog in redshift space assuming a log-normal probability density function (PDF) of galaxy and matter density fields. We draw galaxies by Poisson-sampling the log-normal field, and…

宇宙学与河外天体物理 · 物理学 2017-10-11 Aniket Agrawal , Ryu Makiya , Chi-Ting Chiang , Donghui Jeong , Shun Saito , Eiichiro Komatsu

Redshift-space distortions (RSD) offers an exciting opportunity to test the gravity on cosmological scales. In the presence of galaxy bias, however, the RSD measurement at large scales, where the linear theory prediction is safely applied,…

宇宙学与河外天体物理 · 物理学 2021-08-25 Yong-Seon Song , Yi Zheng , Atsushi Taruya

We investigate the evolution of matter density perturbations and some properties of the peculiar velocity field for a special class of exponential potentials in a scalar field model for quintessence, for which a general exact solution is…

天体物理学 · 物理学 2008-11-26 Claudio Rubano , Mauro Sereno

Low redshift surveys of galaxy peculiar velocities provide a wealth of cosmological information. We revisit the idea of extracting this information by directly measuring the redshift-space momentum power spectrum from such surveys. We…

宇宙学与河外天体物理 · 物理学 2019-06-19 Cullan Howlett

We derive an analytic expression for the two-point correlation function in redshift space which (i) is nonlinear; (ii) is valid on the full sky, i.e. the distant-observer limit is not assumed; (iii) can account for the effect of…

宇宙学与河外天体物理 · 物理学 2023-11-08 Lawrence Dam , Camille Bonvin

We only see a small fraction of the matter in the universe, but the rest gives itself away by the impact of its gravity. The distortions from pure Hubble flow (or peculiar velocities) that this matter creates have the potential to be a…

天体物理学 · 物理学 2009-06-23 Karen L. Masters

The era of real-time cosmology has begun. It is now possible to directly measure the apparent drift of high-redshift astronomical sources across the sky $\textit{in real time}$. This so-called $\textit{position drift}$ provides a valuable…

宇宙学与河外天体物理 · 物理学 2026-01-01 Alexander Oestreicher , Chris Clarkson , Julian Adamek , Sofie Marie Koksbang

We present a method for reconstructing cosmological densityn for and velocity fields using the Lagrangian Zel'dovich formalism. . The method involves finding the least action solution for straight line particle paths in an evolving density…

天体物理学 · 物理学 2015-06-24 R. A. C. Croft , E. Gaztanaga

The peculiar velocities of galaxies distort the clustering pattern anisotropically in redshift space. This effect on the statistics of isodensity contours is examined by linear theory. The statistics considered in this paper are the three-…

天体物理学 · 物理学 2016-08-30 Takahiko Matsubara

The peculiar velocity of the Local Group, reconstructed from inhomogeneities in the local density field, differs in direction and magnitude from the velocity inferred from the Cosmic Microwave Background dipole. We investigate whether…

宇宙学与河外天体物理 · 物理学 2010-03-04 Aidan C Crook , Alessandra Silvestri , Phillip Zukin

In this paper, we develop a theory of redshift distortion of the galaxy power spectrum in the discrete wavelet transform (DWT) representation. Because the DWT power spectrum is dependent of both the scale and shape (configuration) of the…

天体物理学 · 物理学 2009-11-07 Xiao-Hu Yang , Long-Long Feng , Yao-Quan Chu , Li-Zhi Fang

We further develop the description of redshift space distortions within the Effective Field Theory of Large Scale Structures. First, we generalize the counterterms to include the effect of baryonic physics and primordial non-Gaussianity.…

宇宙学与河外天体物理 · 物理学 2018-04-04 Matthew Lewandowski , Leonardo Senatore , Francisco Prada , Cheng Zhao , Chia-Hsun Chuang

It is widely believed that the cosmological redshift is not a Doppler shift. However, Bunn & Hogg have recently pointed out that to settle properly this problem, one has to transport parallelly the velocity four-vector of a distant galaxy…

宇宙学与河外天体物理 · 物理学 2015-05-14 Michał Chodorowski

We show by direct calculation that the common Equivalence Principle explanation for why gravity must deflect light is quantitatively incorrect by a factor of three in Schwarzschild geometry. It is therefore possible, at least as a matter of…

广义相对论与量子宇宙学 · 物理学 2024-03-08 Steven A. Balbus