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相关论文: On the cosmological distance and redshift between …

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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

A cosmology calculator that computes times and distances as a function of redshift for user-defined cosmological parameters is available on the World Wide Web. This note gives the formulae used by the cosmology calculator and discusses some…

天体物理学 · 物理学 2010-04-21 Edward L. Wright

The Universe is not completely homogeneous. Even if it is sufficiently so on large scales, it is very inhomogeneous at small scales, and this has an effect on light propagation, so that the distance as a function of redshift, which in many…

宇宙学与河外天体物理 · 物理学 2020-01-08 Phillip Helbig

Using cosmological relativity theory, we derive the formula for the cosmological redshift written explicitly in terms of 1 - "Omega", where "Omega" = "rho"/"rho"_c is the ratio of the average mass density to the critical "closure" density.…

天体物理学 · 物理学 2007-05-23 Moshe Carmeli

Formulae for the line-of-sight and transverse comoving distances, proper motion distance, angular diameter distance, luminosity distance, k-correction, distance modulus, comoving volume, lookback time, age, and object intersection…

天体物理学 · 物理学 2007-05-23 David W. Hogg

We study the validity of cosmic distance duality relation between angular diameter and luminosity distances. To test this duality relation we use the latest Union2 Supernovae Type Ia (SNe Ia) data for estimating the luminosity distance. The…

宇宙学与河外天体物理 · 物理学 2015-05-27 Remya Nair , Sanjay Jhingan , Deepak Jain

This paper gives a compilation of physical mechanisms which have been proposed to explain the spectral red-shift of distant astronomical objects. Over sixty selected mechanisms are listed for the purpose of quantitative comparisons. Some of…

宇宙学与河外天体物理 · 物理学 2018-01-24 Louis Marmet

The standard cosmological parallax--distance formula, as found in the literature, including text-books and reference books on cosmology, requires a correction. This correction stems from the fact that in the standard text-book derivation it…

宇宙学与河外天体物理 · 物理学 2015-09-04 Ashok K. Singal

From the first observations made by Slipher, our understanding and interpretation of the cosmological redshift was evolving until reaching the current consensus, through the expanding universe and the emergence of modern physical cosmology…

宇宙学与河外天体物理 · 物理学 2020-02-28 Gabriel R. Bengochea

The inner product provides a conceptually and algorithmically simple method for calculating the comoving distance between two cosmological objects given their redshifts, right ascension and declination, and arbitrary constant curvature. The…

天体物理学 · 物理学 2009-11-06 Boudewijn F. Roukema

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

We show that the usual relation between redshift and angular-diameter distance can be obtained by considering light from a source to be gravitationally lensed by material that lies in the telescope beam as it passes from source to observer…

天体物理学 · 物理学 2008-02-03 Fedja Hadrovic , James Binney

We investigate some possible relations between physical observables and estimate the "cosmic variance" which affects these measurements. We focus on redshift and angular-distance and we discuss the difference in considering the redshift as…

宇宙学与河外天体物理 · 物理学 2018-06-26 Giuseppe Fanizza

Aims: we propose that the condition of relative motion between us and the objects that we observe in the Universe should generate relativistic aberration on the photons that such objects emit, varying the observed flux similarly to the…

宇宙学与河外天体物理 · 物理学 2024-04-05 Nicolò Cedola

For more that seventy years, the measurements of fluxes of galaxies at different wavelengths and derived colours have been used to estimate their corresponding cosmological distances. From the fields of galaxy and AGN evolution to precision…

星系天体物理 · 物理学 2018-06-06 Mara Salvato , Olivier Ilbert , Ben Hoyle

In this work we present the first results from a new ray-tracing tool to calculate cosmological distances in the context of fully nonlinear general relativity. We use this tool to study the ability of the general cosmographic representation…

宇宙学与河外天体物理 · 物理学 2023-03-15 Hayley J. Macpherson

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

The results from the Supernova Cosmology Project indicate a relation between cosmic distance and redshift that corresponds to an accelerating Universe, and, as a consequence, the presence of an energy component with negative pressure. This…

天体物理学 · 物理学 2007-05-23 Daniel Enstrom , Sverker Fredriksson , Johan Hansson

There are now several analyses reporting quantized differences in the redshifts between pairs of galaxies. In the simplest cases, these differential redshifts are found to be harmonics of fundamental periods of approximately 72 km/s and…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Firmin J. Oliveira

The redshift of light is calculated for an anisotropic cosmological spacetime. Two different approaches are considered. In the first one, electromagnetic waves are modeled using the geometrical optics (high--frequency) approximation. This…

广义相对论与量子宇宙学 · 物理学 2018-05-10 Sergio A. Hojman , Felipe A. Asenjo
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