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相关论文: The shrinking Hubble constant

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Strong gravitational lensing has been a powerful probe of cosmological models and gravity. To date, constraints in either domain have been obtained separately. We propose a new methodology through which the cosmological model, specifically…

宇宙学与河外天体物理 · 物理学 2020-07-08 Tao Yang , Simon Birrer , Bin Hu

A spherical cosmological model with a local void on scales of $\sim 200$ Mpc and with an inhomogeneous Hubble constant was proposed in recent two papers. This model explains consistently the observed properties of the cosmic bulk flow, the…

天体物理学 · 物理学 2009-10-31 Kenji Tomita

Adopting the low-redshift observational datasets, including the Pantheon sample of Type Ia supernovae, baryon acoustic oscillation measurements, and the tomographic Alcock-Paczynski method, we determine the Hubble constant to be…

宇宙学与河外天体物理 · 物理学 2019-11-22 Xue Zhang , Qing-Guo Huang

An independent determination of the Hubble constant is crucial given the persistent tension between early- and late-Universe measurements. In this study, we analyze the dynamics of the Centaurus~A (CenA) and M83 galaxies, along with their…

宇宙学与河外天体物理 · 物理学 2026-01-14 Adrian Faucher , David Benisty , David F. Mota

The determination of the Hubble constant has been a central goal in observational astrophysics for nearly 100 years. Extraordinary progress has occurred in recent years on two fronts: the cosmic distance ladder measurements at low redshift…

宇宙学与河外天体物理 · 物理学 2014-10-14 C. L. Bennett , D. Larson , J. L. Weiland , G. Hinshaw

One of hot topics in the last years is a systematic discrepancy in the determination of Hubble parameter by various methods. Namely, the values derived "directly" from the distance scale based on Cepheids and supernovae--and referring to…

宇宙学与河外天体物理 · 物理学 2018-04-03 Yurii V. Dumin

One of main sources of uncertainty in modern cosmology is the present rate of the universe's expansion, H0, called the Hubble constant. Once again, different observational techniques bring about different results, causing new 'Hubble…

物理学史与哲学 · 物理学 2023-12-29 Jorge L. Cervantes-Cota , Salvador Galindo-Uribarri , George F. Smoot

Since the expansion of the universe was first established by Edwin Hubble and Georges Lemaitre about a century ago, the Hubble constant H0 which measures its rate has been of great interest to astronomers. Besides being interesting in its…

宇宙学与河外天体物理 · 物理学 2021-12-15 Paul Shah , Pablo Lemos , Ofer Lahav

In homogeneous cosmological models the wavelength $\lambda$ of a photon exchanged between two fundamental observers changes in proportion to expansion of the space $D$ between them, so $\Delta\log(\lambda / D) = 0$. This is exactly the same…

宇宙学与河外天体物理 · 物理学 2015-06-18 Nick Kaiser

The product of two empirical constants, the dimensionless fine structure constant and the von Klitzing constant (an electrical resistance), turns out to be an exact dimensionless number. Then the accuracy and cosmological time variation (if…

综合物理 · 物理学 2014-11-20 Antonio Alfonso-Faus

Tension between cosmic microwave background-based and distance ladder-based determinations of the Hubble constant ${\rm H}_{\rm 0}$ motivates pursuit of independent methods that are not subject to the same systematic effects. A promising…

宇宙学与河外天体物理 · 物理学 2023-10-23 Kate Napier , Keren Sharon , Håkon Dahle , Matthew Bayliss , Michael D. Gladders , Guillaume Mahler , Jane R. Rigby , Michael Florian

As the 2015 results of Plancks mission have recently been made available, it is interesting to check the evolution of the scale factor and of the Hubble parameter in the light of these results. Two models in line with Einsteins field…

综合物理 · 物理学 2017-06-08 Guibert U. Crevecoeur

The redshift-distance modulus relation, the Hubble Diagram, derived from Cosmological General Relativity has been extended to arbitrarily large redshifts. Numerical methods were employed and a density function was found that results in a…

综合物理 · 物理学 2008-10-03 John G. Hartnett

The longitudinal Doppler shift is a measure of hyperbolic distance. Transformations of uniform motion are determined by the Doppler shift, while its square root transforms to a uniformly accelerated frame. A time-velocity space metric is…

综合物理 · 物理学 2008-05-16 B. H. Lavenda

We present explicit expressions for the calculation of cosmological look back time, for zero cosmological constant and arbitrary density parameter $\Omega$, which, in the limit as redshift becomes infinite, give the age of the universe. The…

天体物理学 · 物理学 2007-05-23 Kevin Krisciunas

The Supernova Cosmology Project has discovered over twenty-eight supernovae (SNe) at 0.35 <z < 0.65 in an ongoing program that uses Type Ia SNe as high-redshift distance indicators. Here we present measurements of the ratio between the…

We present a method to compute the probability distribution function of the (true) Hubble constant and the age of the universe, given the estimate of the Hubble constant in our nearby galaxy samples. Our method takes into account both the…

天体物理学 · 物理学 2009-10-28 T. Nakamura , Y. Suto

The evolution of the Hubble parameter $H(z)$ with redshift $z$ is estimated from the Pantheon+ data of Type Ia supernovae, for the $\Lambda$CDM model and the three special cases of the eternal coasting (EC) cosmological model with three…

宇宙学与河外天体物理 · 物理学 2024-12-23 Ardra Edathandel Sasi , Moncy Vilavinal John

The description of the cosmological expansion and its possible local manifestations via treating the proper conformal transformations as a coordinate transformation from a comoving Lorentz reference frame to an uniformly accelerated one is…

广义相对论与量子宇宙学 · 物理学 2008-06-03 L. M. Tomilchik

Theories with ingredients like the Higgs mechanism, gravitons, and inflaton fields rejuvenate the idea that relativistic kinematics is dynamically emergent. Eternal inflation treats the Hubble constant H as depending on location.…

广义相对论与量子宇宙学 · 物理学 2015-05-19 Sascha Vongehr