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相关论文: Eddington-Malmquist bias in a cosmological context

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In this paper we outline the framework of mathematical statistics with which one may study the properties of galaxy distance estimators. We describe, within this framework, how one may formulate the problem of distance estimation as a…

天体物理学 · 物理学 2009-10-28 M. A. Hendry , J. F. L. Simmons

It is shown that the Hubble constant can be derived from the standard luminosity function of galaxies as well as from a new luminosity function as deduced from the mass-luminosity relationship for galaxies. An analytical expression for the…

宇宙学与河外天体物理 · 物理学 2011-09-20 Lorenzo Zaninetti

We discuss physical interpretation of {\Lambda}CDM cosmology from a Machian model of the universe containing nothing but visible matter (ordinary matter, radiation). The Friedmann equation can be derived from a Machian definition of energy,…

广义相对论与量子宇宙学 · 物理学 2016-06-28 Herman Telkamp

The spatial distribution of galaxies we observed is subject to the given condition that we, human beings are sitting right in a galaxy -- the Milky Way. Thus the ergodicity assumption is questionable in interpretation of the observed galaxy…

宇宙学与河外天体物理 · 物理学 2015-05-18 Jun Pan , Pengjie Zhang

Recent calculations using non-linear relativistic cosmological perturbation theory show biases in the mean luminosity distance and distance modulus at low redshift. We show that these effects may be understood very simply as a…

宇宙学与河外天体物理 · 物理学 2015-09-30 Nick Kaiser , Michael J. Hudson

We present a brief history of the construction of models of the universe, followed by calculations of quantitative characteristics of basic geometric and kinematic properties of the Standard Cosmological Model ($\Lambda$CDM). Using the…

广义相对论与量子宇宙学 · 物理学 2026-04-23 D. I. Nagirner , S. G. Jorstad , A. V. Dementyev

The homogeneous, isotropic, and flat $\Lambda$CDM universe favored by observations of the cosmic microwave background can be described using only Euclidean geometry, locally correct Newtonian mechanics, and the basic postulates of special…

宇宙学与河外天体物理 · 物理学 2018-06-27 J. J. Condon , A. M. Matthews

H.A. Wilson, then R.H. Dicke, proposed to describe gravitation by a spatial change of the refractive index of the vacuum around a gravitational mass. Dicke extended this formalism in order to describe the apparent expansion of the Universe…

综合物理 · 物理学 2018-06-06 X. Sarazin , F. Couchot , A. Djannati-Atai , M. Urban

The Hubble diagram is one of the cornerstones of observational cosmology. It is usually analysed assuming that, on average, the underlying relation between magnitude and redshift matches the prediction of a…

宇宙学与河外天体物理 · 物理学 2017-04-05 Pierre Fleury , Chris Clarkson , Roy Maartens

The Friedmann equation is derived for a Newtonian universe. Changing mass density to energy density gives exactly the Friedmann equation of general relativity. Accounting for work done by pressure then yields the two Einstein equations that…

天体物理学 · 物理学 2015-06-24 Thomas F. Jordan

We point out that although conventional stars are primarily fed by burning of nuclear fuel at their cores, in a strict sense, the process of release of stored gravitational energy, known as, Kelvin - Helmholtz (KH) process is either also…

天体物理学 · 物理学 2009-11-11 Abhas Mitra

The calculation of distances is of fundamental importance in extragalactic astronomy and cosmology. However, no practical implementation for the general case has previously been available. We derive a second-order differential equation for…

天体物理学 · 物理学 2016-08-30 Rainer Kayser , Phillip Helbig , Thomas Schramm

As the universe expands astronomical observables such as brightness and angular size on the sky change in ways that differ from our simple Cartesian expectation. We show how observed quantities depend on the expansion of space and…

宇宙学与河外天体物理 · 物理学 2015-06-04 Jodi Christiansen , Andy Siver

In this letter, we propose a new generalized mass-to-horizon relation to be used in the context of entropic cosmologies and holographic principle scenarios. We show that a general scaling of the mass with the Universe horizon as $M=\gamma…

广义相对论与量子宇宙学 · 物理学 2024-05-02 Hussain Gohar , Vincenzo Salzano

After a brief introduction to the sixteenth and seventeenth century views of the Universe and the nineteenth century paradox of Olbers, we start the history of the cosmic expansion with Hubble's epochal discovery of the recession velocities…

天体物理学 · 物理学 2008-02-15 Matts Roos

In this paper we review the two main approaches to the problem of Malmquist bias which have been adopted in the cosmology literature, and show how these two formulations of the problem represent fundamentally different views of the nature…

天体物理学 · 物理学 2007-05-23 Martin A. Hendry , John F. L. Simmons , Andrew M. Newsam

The cosmological concordance model is consistent with all available observational data, including the apparent distance and redshift relationship for distant supernovae, but it is curious how the Milne cosmological model is able to make…

综合物理 · 物理学 2007-05-23 Alasdair Macleod

Considering a n-dimensional general spacetime, we deduce its 4-dimensional Einstein equation and Friedman equations, and discover a general dual relation between the scale factor $a(t)$ of our universe and the scale factor $B(t)$ of extra…

广义相对论与量子宇宙学 · 物理学 2015-01-20 Yong-Chang Huang , LiuJi Li

The motion equation of standard cosmology, the Friedmann equation, is based on the stein's equations of gravitational fields. However, British physicist E. A. Milne pointed in 1943 that the same equation could be deduced simply based on the…

综合物理 · 物理学 2010-05-31 Mei Xiaochun

One of the keys to understanding the universe is the proper measurement of the relation between the luminosity distance $d_L$ and the angular diameter distance $d_A$. In 1933 Etherington deduced from general relativity the reciprocity…

综合物理 · 物理学 2023-05-04 Juan De Vicente
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