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相关论文: Redshift and Energy Conservation

200 篇论文

Over the past decade, the disparity between the value of the cosmic expansion rate directly determined from measurements of distance and redshift or instead from the standard $\Lambda$CDM cosmological model calibrated by measurements from…

宇宙学与河外天体物理 · 物理学 2022-11-10 Marc Kamionkowski , Adam G. Riess

Achieving relativistic flight to enable extrasolar exploration is one of the dreams of humanity and the long term goal of our NASA Starlight program. We derive a fully relativistic solution for the motion of a spacecraft propelled by…

天体物理仪器与方法 · 物理学 2018-04-04 Neeraj Kulkarni , Philip Lubin , Qicheng Zhang

A mildly inhomogeneous universe with a cosmological constant may look like it contains evolving dark energy. We show that could be the case by modelling the inhomogeneities and their effects in three different ways: as clumped matter…

宇宙学与河外天体物理 · 物理学 2026-01-29 Yonadav Barry Ginat , Pedro G. Ferreira

We focus on uncertainties in supernova measurements, in particular of individual magnitudes and redshifts, to review to what extent supernovae measurements of the expansion history of the universe are likely to allow us to constrain a…

天体物理学 · 物理学 2011-05-12 Lawrence M. Krauss , Katherine Jones-Smith , Dragan Huterer

Distances in cosmology are usually inferred from observed redshifts - an estimate that is dependent on the local peculiar motion - giving a distorted view of the three dimensional structure and affecting basic observables such as the…

天体物理学 · 物理学 2008-12-18 J. Richard Shaw , Antony Lewis

The origin of the observed acceleration of the expansion of the universe is a major problem of modern cosmology and theoretical physics. Simple estimations of the contribution of vacuum to the density energy of the universe in quantum field…

宇宙学与河外天体物理 · 物理学 2013-06-11 Arnaud Dupays , Brahim Lamine , Alain Blanchard

A major recent evelopment in observational cosmology has been an accurate measurement of the luminosity distance-redshift relation out to redshifts z=0.8 from Type Ia supernova standard candles. The results have been argued as evidence for…

天体物理学 · 物理学 2016-01-13 Neil Trentham

We present here the transformations required to recast the Robertson-Walker metric and Friedmann-Robertson-Walker equations in terms of observer-dependent coordinates for several commonly assumed cosmologies. The overriding motivation is…

宇宙学与河外天体物理 · 物理学 2018-09-26 Fulvio Melia , Majd Abdelqader

In the timescape scenario cosmic acceleration is understand as an apparent effect, due to gravitational energy gradients that grow when spatial curvature gradients become significant with the nonlinear growth of cosmic structure. This…

宇宙学与河外天体物理 · 物理学 2010-07-14 David L. Wiltshire

We review the evidence for recently accelerating cosmological expansion or "dark energy", either a negative pressure constituent in General Relativity (Dark Energy) or modified gravity (Dark Gravity), without any Dark Energy constituent. If…

天体物理学 · 物理学 2007-05-23 Sidney Bludman

It is known since 1968 that the interaction of a pulse of light with matter redshifts the spectrum; the theory is clarified, to obtain the conditions for which, with incoherent light, one gets a redshift similar to a Doppler shift rather…

天体物理学 · 物理学 2007-05-23 Jacques Moret-Bailly

A recently proposed Asymptotically Safe cosmology provides an elegant mechanism towards understanding the nature of dark energy and its associated cosmic coincidence problem. The underlying idea is that the accelerated expansion of the…

宇宙学与河外天体物理 · 物理学 2019-03-06 Fotios K. Anagnostopoulos , Spyros Basilakos , Georgios Kofinas , Vasilios Zarikas

A general-relativistic theory of cosmology, the dynamical variables of which are those of Hubble's, namely distances and redshifts, is presented. The theory describes the universe as having a three-phase evolution with a decelerating…

天体物理学 · 物理学 2007-05-23 S. Behar , M. Carmeli

We consider the fate of the observable universe in the light of the discovery of a dark energy component to the cosmic energy budget. We extend results for a cosmological constant to a general dark energy component and examine the…

天体物理学 · 物理学 2009-11-07 Dragan Huterer , Glenn D. Starkman , Mark Trodden

The Schr\"odinger-Newton equation is a proposed model to explain the localization of macroscopic particles by suppressing quantum dispersion with the particle's own gravitational attraction. On cosmic scales, however, dark energy also acts…

广义相对论与量子宇宙学 · 物理学 2020-04-01 Kelvin , Kelvin Onggadinata , Matthew J. Lake , Tomasz Paterek

Dark energy is inferred from a Hubble expansion which is slower at epochs which are earlier than ours. But evidence reviewed here shows $H_0$ for nearby galaxies is actually less than currently adopted and would instead require {\it…

天体物理学 · 物理学 2007-12-20 H. Arp

We give a rigorous derivation of the general-relativistic formula for the two-way Doppler tracking of a spacecraft in Friedmann-Lemaitre-Robertson-Walker and in McVittie spacetimes. The leading order corrections of the so-determined…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Matteo Carrera , Domenico Giulini

Discussed is the classical theoretical description of the experimentally established thermal redshift of spectral lines. Straightforward calculation of the observable spectrum from a canonical ensamble of monochromatic radiators yileds…

量子物理 · 物理学 2009-10-30 Vesselin I. Dimitrov

If general relativity is the correct theory of physics on large scales, then there is a differential equation that relates the Hubble expansion function, inferred from measurements of angular diameter distance and luminosity distance, to…

天体物理学 · 物理学 2011-02-01 Mustapha Ishak , Amol Upadhye , David N. Spergel

The redshift of galaxies is in general explained by the expansion of space. The flat space time theory of gravitation suggests an additional interpretation. In this theory gravitation is explained analogously to Maxwell's theory on a flat…

综合物理 · 物理学 2007-05-31 Walter Petry