中文
相关论文

相关论文: INDICATIONS OF DARK MATTER DERIVED FROM LARGE SCAL…

200 篇论文

Peculiar velocity measurements are the only tool available in the low-redshift Universe for mapping the large-scale distribution of matter and can thus be used to constrain cosmology. Using redshifts from the 2M++ redshift compilation, we…

宇宙学与河外天体物理 · 物理学 2015-06-24 Jonathan Carrick , Stephen J. Turnbull , Guilhem Lavaux , Michael J. Hudson

By correcting the redshift--dependent distances for peculiar motions through a number of peculiar velocity field models, we recover the true distances of a wide, all-sky sample of nearby galaxies (~ 6400 galaxies with velocities cz<5500…

天体物理学 · 物理学 2009-10-30 C. Marinoni , P. Monaco , G. Giuricin , B. Costantini

Peculiar velocities are an important probe of the mass distribution in the Universe and the growth rate of structure, directly measuring the effects of gravity on the largest scales and providing a test for theories of gravity. Comparing…

宇宙学与河外天体物理 · 物理学 2024-04-30 Paula Boubel , Matthew Colless , Khaled Said , Lister Staveley-Smith

In this contribution we review the large body of work carried out over the past two decades to probe the dark matter in the local universe using redshift survey and peculiar velocity data. While redshift surveys have evolved rapidly over…

天体物理学 · 物理学 2007-05-23 L. da Costa

Our statistical studies comprise the mean relative velocity and velocity correlation for pairs of galaxies as a function of separation, and a bulk flow analysis determined on spheres of $10 h^{-1}$ $Mpc$ radius. In order to test the…

天体物理学 · 物理学 2009-10-30 Nelson Padilla , Manuel Merchán , Diego G. Lambas

The large-scale dynamics of matter is inferred from the observed peculiar velocities of galaxies via the POTENT procedure. The smoothed fields of velocity and mass-density fluctuations are recovered from the current data of about 3000…

天体物理学 · 物理学 2007-05-23 Avishai Dekel

A new method is proposed for directly measuring the expansion rate of the universe through very precise measurement of the fluence of extremely stable sources. The method is based on the definition of the luminosity distance and its change…

宇宙学与河外天体物理 · 物理学 2012-05-08 Shi Qi , Tan Lu

We investigate the extent to which correlated distortions of the luminosity distance-redshift relation due to large-scale bulk flows limit the precision with which cosmological parameters can be measured. In particular, peculiar velocities…

天体物理学 · 物理学 2009-11-11 Asantha Cooray , Robert R. Caldwell

We constructed a Bayesian hyper-parameter statistical method to quantify the difference between predicted velocities derived from the observed galaxy distribution in the \textit{IRAS}-PSC$z$ redshift survey and peculiar velocities measured…

宇宙学与河外天体物理 · 物理学 2015-06-05 Yin-Zhe Ma , Enzo Branchini , Douglas Scott

Cosmological parameters can be measured by comparing peculiar velocities with those predicted from a galaxy density field. Previous work has tested the accuracy of this approach with N-body simulations, but generally on idealised mock…

宇宙学与河外天体物理 · 物理学 2024-03-27 Amber M. Hollinger , Michael J. Hudson

A formalism that simultaneously searches for the monopolar and dipolar peculiar velocities is presented. The formalism is applied to (1) the Mark III catalogue, (2) Lauer and Postman's Abell cluster catalogue, and (3) Riess et al.'s Type Ia…

天体物理学 · 物理学 2009-10-28 Xiangdong Shi

Although a simple argument implies that the distribution of dark matter in galactic halos is characterized by discrete flows and caustics, their presence is often ignored in discussions of galactic dynamics and of dark matter detection…

天体物理学 · 物理学 2008-11-26 Aravind Natarajan , Pierre Sikivie

Masses of galaxies are beginning to be measured systematically at redshifts z > 0.3. Such data provide powerful and unique links and clues to theories, simulations, and our understanding of early galaxy formation and evolution.…

天体物理学 · 物理学 2007-05-23 David C. Koo

We give a brief review of recent developments in the study of the large-scale velocity field of galaxies since the international workshop on Cosmic Flows held in July 1999 in Victoria, B.C. Peculiar velocities (PVs) yield a tight and unique…

天体物理学 · 物理学 2007-05-23 Stephane Courteau , Avishai Dekel

We have measured the cosmic momentum power spectrum from the peculiar velocities of galaxies in the SFI sample. The SFI catalog contains field spiral galaxies with radial peculiar velocities derived from the I-band Tully-Fisher relation. As…

天体物理学 · 物理学 2009-11-13 Chan-Gyung Park , Changbom Park

It has been argued recently that the galaxy peculiar velocity field provides evidence of excessive power on scales of $50\hmpc$, which seems to be inconsistent with the standard $\Lambda$CDM cosmological model. We discuss several…

宇宙学与河外天体物理 · 物理学 2015-06-11 Yin-Zhe Ma , Douglas Scott

The transverse peculiar velocities caused by the mass distribution of large-scale structure provide a test of the theoretical matter power spectrum and the cosmological parameters that contribute to its shape. Typically, the matter density…

宇宙学与河外天体物理 · 物理学 2018-11-28 Alexandra Truebenbach , Jeremy Darling

We describe a new method of overcoming problems inherent in peculiar velocity surveys by using data compression as a filter with which to separate large-scale, linear flows from small-scale noise that biases the results systematically. We…

天体物理学 · 物理学 2007-05-23 Hume A Feldman , Richard Watkins , Adrian Melott , Will Chambers

IRAS flux densities, redshifts, and infrared luminosities are reported for all sources identified in the IRAS Revised Bright Galaxy Sample (RBGS), a complete flux-limited survey of all extragalactic objects with total 60 micron flux density…

天体物理学 · 物理学 2011-07-18 D. B. Sanders , J. M. Mazzarella , D. -C. Kim , J. A. Surace , B. T. Soifer

We review the increasing evidence for the cosmological relevance of the cold local Hubble flow. New observations, N-body simulations and other theoretical arguments are discussed, supporting our previous suggestion that the cosmological…

天体物理学 · 物理学 2009-11-11 Pekka Teerikorpi , Arthur D. Chernin , Yurij V. Baryshev