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相关论文: A Physical Interpretation of MOND

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Recent improvements in astronomical observations lead to the conclusion that the Hubble constant lies between 60 and 80 Mpc km$^{-1}$ sec$^{-1}$ and the age of the universe between 11 and 14 Gigayears. Taken together with recent…

广义相对论与量子宇宙学 · 物理学 2007-05-23 H. Pierre Noyes

To study some characteristics of the interstellar medium, observational data of pulsars with large Faraday rotation values (|RM|> 300 rad / m2) were used. It was suggested and justified that large |RM| values can be due to the contribution…

星系天体物理 · 物理学 2018-08-13 R. R. Andreasyan , H. R. Andreasyan , G. M. Paronyan

The stability of galaxies is either explained by the existence of dark matter or caused by a modification of Newtonian acceleration (MOND). Here we show that the modification of the Newtonian dynamics can equally well be obtained by a…

星系天体物理 · 物理学 2024-04-24 Søren Toxvaerd

It is shown that screening the background of super-strong interacting gravitons ensures the Newtonian attraction, if a part of single gravitons is pairing and graviton pairs are destructed by collisions with a body. If the considered…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Michael A. Ivanov

We investigate the distance-redshift relation in the simple void model. As discussed by Moffat and Tatarski, if the observer stays at the center of the void, the observed Hubble parameter is not so different from the background Hubble…

天体物理学 · 物理学 2016-08-30 Ken-ichi Nakao , Naoteru Gouda , Takeshi Chiba , Satoru Ikeuchi , Takashi Nakamura , Masaru Shibata

The dwarf galaxy NGC1052-DF2 has recently been identified as potentially lacking dark matter. If correct, this could be a challenge for MOND, which predicts that low surface brightness galaxies should evince large mass discrepancies.…

星系天体物理 · 物理学 2018-08-01 B. Famaey , S. McGaugh , M. Milgrom

Background boucing cosmologies in the framework of General Relativity, driven by a single scalar field filling the Universe, and with a quasi-matter domination period, i.e., depicting the so-called Matter Bounce Scenario, are reconstructed…

广义相对论与量子宇宙学 · 物理学 2017-03-22 Jaume de Haro

We use 28 Hubble parameter, $H(z)$, measurements at intermediate redshifts $0.07 \leq z \leq 2.3$ to determine the present-day Hubble constant $H_0$ in four cosmological models. We measure $H_0 = 68.3^{ +2.7}_{ -2.6 }, 68.4^{ +2.9 }_{ -3.3…

宇宙学与河外天体物理 · 物理学 2017-01-26 Yun Chen , Suresh Kumar , Bharat Ratra

Vectorial analysis relating to derivation of deflection of light is presented. Curvilinear acceleration is distinguished from the Newtonian polar conic acceleration. The difference between the two is due to the curvature term. Lorentz…

综合物理 · 物理学 2014-12-09 Vikram H. Zaveri

Our cosmology contains Big Bang relic fluctuations by a loss of time-translation symmetry on a Hubble time scale. The contribution to the vacuum is identified with dynamical dark energy $\Lambda\simeq \alpha_p\Lambda_0$ by an IR coupling…

宇宙学与河外天体物理 · 物理学 2024-08-26 Maurice H. P. M. van Putten

The primary argument levelled against Milgrom's MOND is that it has no theoretical support, even though considerable effort has been expended in attempting to provide it. Against that criticism, MOND irrefutably enjoys an expanding…

星系天体物理 · 物理学 2020-06-16 D F Roscoe

We have had the chance to live through a fascinating revolution in measuring the fundamental empirical cosmological Hubble law. The key progress is analysed : 1) improvement of observational means (ground-based radio and optical…

宇宙学与河外天体物理 · 物理学 2018-01-10 Georges Paturel , Pekka Teerikorpi , Yurij Baryshev

Cosmological theories for the origin and evolution of structure in the Universe are highly predictive of the form of the angular power spectrum of cosmic microwave background fluctuations. We present new results from a comprehensive study…

天体物理学 · 物理学 2007-05-23 Stephen Hancock , Graca Rocha

Modified Newtonian Dynamics (MoND) is an empirically modification of Newtonian gravity at largest scales in order to explain rotation curves of galaxies, as an alternative to nonbaryonic dark matter. But MoND theories can hardly connect…

宇宙学与河外天体物理 · 物理学 2010-07-21 Nelson Falcon

As the advent of precision cosmology, the Hubble constant ($H_0$) inferred from the Lambda Cold Dark Matter fit to the Cosmic Microwave Background data is increasingly in tension with the measurements from the local distance ladder. To…

星系天体物理 · 物理学 2021-12-08 Wei-Jian Lu , Yi-Ping Qin

One of the greatest challenges of science is to understand the current accelerated expansion of the Universe. In this work, we show that by considering the quantum nature of the gravitational field, its wavelength can be associated with an…

综合物理 · 物理学 2022-11-08 Tonatiuh Matos , Laura L-Parrilla

Modified Newtonian Dynamics (MOND) is an alternative to the dark matter hypothesis that attempts to explain the "missing gravity" problem in astrophysics and cosmology through a modification to objects' dynamics. Since its conception in…

宇宙学与河外天体物理 · 物理学 2025-05-29 Harry Desmond

We present here a general relativistic mechanism for accelerated cosmic expansion and the Hubble's constant. It is shown that spacetime vorticity coupled to the magnetic field density in galaxies causes the galaxies to recede from one…

宇宙学与河外天体物理 · 物理学 2019-03-20 Babur M. Mirza

Measurements of the linear diameters of 12 nearby spiral galaxies with distances determined from primary indicators suggest that both the Milky Way Galaxy and M31 are in the middle of the range of sizes for such galaxies. By comparing the…

天体物理学 · 物理学 2009-09-25 S. P. Goodwin , J. Gribbin , M. A. Hendry

The correlation between the luminosities and rotation velocities of galaxies can be used to estimate distances to late-type galaxies. It is an appropriate moment to re-evaluate this method given the great deal of new information available.…

天体物理学 · 物理学 2014-10-13 R. Brent Tully , M. J. Pierce
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