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The null findings of the terrestrially conducted Michelson-Morley type experiments have been influential to determining which physical theory best fits reality. Here, we propose the use of parallax and ranging techniques of distance…

综合物理 · 物理学 2009-09-29 Akinbo Ojo

In this paper we prove a number of exact relations between optical observables, such as trigonometric parallax, position drift and the proper motion of a luminous source in addition to the variations of redshift and the viewing angle. These…

广义相对论与量子宇宙学 · 物理学 2025-05-13 Mikołaj Korzyński , Nezihe Uzun

The general expression of the angular distance between two point sources as measured by an arbitrary observer is given. The modelling presented here is rigorous, covariant and valid in any space-time. The sources of light may be located at…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Pierre Teyssandier , Christophe Le Poncin-Lafitte

We first review the current knowledge of Hipparcos systematic and random errors, in particular small-scale correlations. Then, assuming Gaussian parallax errors and using examples from the recent Hipparcos literature, we show how random…

天体物理学 · 物理学 2007-05-23 F. Arenou , X. Luri

We derive angle differences between two null geodesics, propagating from light sources to an observer, on the de Sitter spacetime with multi-lensing objects. Assuming the lensing objects are mass monopoles on the de Sitter background, we…

广义相对论与量子宇宙学 · 物理学 2020-10-30 Rio Saitou , Hiromi Saida

We consider the standard problem of observational astronomy, i.e. the observations of light emission from a distant region of spacetime in general relativity. The goal is to describe the changes between the measurements of the light…

广义相对论与量子宇宙学 · 物理学 2019-04-02 Michele Grasso , Mikołaj Korzyński , Julius Serbenta

Gravitational-wave astronomy allows us to study objects and events invisible to electromagnetic waves. So far, only signals triggered by coalescing binaries have been detected. However, as the interferometers' sensitivities improve over…

高能天体物理现象 · 物理学 2023-03-08 Magdalena Sieniawska , David Ian Jones , Andrew Lawrence Miller

The Gaia satellite will soon probe parallax on cosmological distances. Using the covariant formalism and considering the angle between a pair of sources, we find parallax for both spacelike and timelike separation between observation…

宇宙学与河外天体物理 · 物理学 2014-03-19 Syksy Rasanen

Two recently proposed techniques, involving the measurement of the cosmic parallax and redshift drift, provide novel ways of directing probing (over a time-span of several years) the background metric of the universe and therefore shed…

宇宙学与河外天体物理 · 物理学 2010-04-06 Miguel Quartin , Luca Amendola

In this paper, we prove that two different observers don't equally measure the distance between two points A and B. For this, we introduce some postulates and obtain a new formula to show distance between A and B. In this formula, radius of…

综合物理 · 物理学 2007-05-23 M. Akbari , M. T. Darvishi

The distance to the stars is a fundamental parameter, which is determined via two primary methods - parallax and luminosity. While the parallax is a direct trigonometric method, the luminosity distance is usually influenced by interstellar…

星系天体物理 · 物理学 2024-12-30 Ralf Siebenmorgen , Frank Heymann , Rolf Chini

Information exchanged between observers in the universe typically travels along the null rays of the associated light signals. One may therefore decompose the luminosity distance of a given radiation source along these null geodesics,…

广义相对论与量子宇宙学 · 物理学 2022-11-23 Jessica Santiago , Christos G. Tsagas

Astrometric surveys such as Gaia and LSST will measure parallaxes for hundreds of millions of stars. Yet they will not measure a single distance. Rather, a distance must be estimated from a parallax. In this didactic article, I show that…

天体物理仪器与方法 · 物理学 2016-03-09 C. A. L. Bailer-Jones

Recently, Rindler and Ishak have argued that the bending of light is, in principle, changed by the presence of a cosmological constant since one must consider not only the null geodesic equation, but also the process of measurement. I agree…

广义相对论与量子宇宙学 · 物理学 2007-11-27 Kayll Lake

We show that distances of objects at cosmological distances can be measured directly using interferometry. Our approach to interferometric parallax comes from analysis of 4-point amplitude and intensity correlations that can be generated…

天体物理学 · 物理学 2008-11-26 Pankaj Jain , John P. Ralston

Under very general assumptions of metric theory of spacetime, photons traveling along null geodesics and photon number conservation, two observable concepts of cosmic distance, i.e. the angular diameter and the luminosity distances are…

宇宙学与河外天体物理 · 物理学 2016-05-16 Kai Liao , Zhengxiang Li , Shuo Cao , Marek Biesiada , Xiaogang Zheng , Zong-Hong Zhu

In this paper, we present the analysis of the binary gravitational microlensing event OGLE-2015-BLG-0196. The event lasted for almost a year and the light curve exhibited significant deviations from the lensing model based on the…

It is now a known fact that if we happen to be living in the middle of a large underdense region, then we will observe an "apparent acceleration", even when any form of dark energy is absent. In this paper, we present a "Minimal Void"…

天体物理学 · 物理学 2009-09-24 Stephon Alexander , Tirthabir Biswas , Alessio Notari , Deepak Vaid

From the equivalence principle (EP) and experiments on gravitational (G) time dilation (GTD) it is proved that the standards of observers located in different ``distances'' from the earth are physically different with respect to each other.…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Rafael A. Vera

Energy statistics are estimators of the energy distance that depend on the distances between observations. The idea behind energy statistics is to consider a statistical potential energy that would parallel Newton's gravitational potential…

统计方法学 · 统计学 2017-03-24 Ruite Guo , Vic Patrangenaru
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