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相关论文: Testing quantised inertia on galactic scales

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The property of inertia has never been fully explained. A model for inertia (MiHsC or quantised inertia) has been suggested that assumes that 1) inertia is due to Unruh radiation and 2) this radiation is subject to a Hubble-scale Casimir…

综合物理 · 物理学 2015-06-15 M. E. McCulloch

It is shown here that a model for inertial mass, called quantised inertia, or MiHsC (Modified inertia by a Hubble-scale Casimir effect) predicts the rotational acceleration of the 153 good quality galaxies in the SPARC dataset (2016 AJ 152…

星系天体物理 · 物理学 2017-09-18 M. E. McCulloch

It has recently been observed that there are no disc galaxies with masses less than 10^9 M_solar and this cutoff has not been explained. It is shown here that this minimum mass can be predicted using a model that assumes that 1) inertia is…

宇宙学与河外天体物理 · 物理学 2015-05-18 M. E. McCulloch

We argue that soft gravitational radiation leads to a misidentification of the angular momentum of stars seen in distant galaxies, and that this could be interpreted as an additional mass inside the orbit of the star. It is tempting to…

高能物理 - 理论 · 物理学 2018-10-16 Tom Banks , Willy Fischler

The flyby anomalies are unexplained velocity increases of 3.9, 13.5, 0.1 and 1.8 mm/s observed near closest approach during the Earth flybys of the Galileo, NEAR, Cassini and Rosetta spacecraft. Here, these flybys are modelled using a…

天体物理学 · 物理学 2011-09-15 M. E. McCulloch

Dwarf satellite galaxies of the Milky Way appear to be gravitationally bound, but their stars' orbital motion seems too fast to allow this given their visible mass. This is akin to the larger-scale galaxy rotation problem. In this paper, a…

综合物理 · 物理学 2017-03-06 M. E. McCulloch

The flyby anomalies are unexplained velocity jumps of 3.9, -4.6, 13.5, -2, 1.8 and 0.02 mm/s observed near closest approach during the Earth flybys of six spacecraft. These flybys are modelled here using a theory that assumes that inertia…

天体物理学 · 物理学 2009-11-13 M. E. McCulloch

The missing gravity in galaxies requires dark matter, or alternatively a modification of gravity or inertia. These theoretical possibilities of fundamental importance may be distinguished by the statistical relation between the observed…

星系天体物理 · 物理学 2022-12-21 Kyu-Hyun Chae

Rotation curves of spiral galaxies \emph{i}) fall off much less steeply than the Keplerian curves do, and \emph{ii}) have asymptotic speeds almost proportional to the fourth root of the mass of the galaxy, the Tully-Fisher relation. These…

广义相对论与量子宇宙学 · 物理学 2010-11-02 Y. Sobouti , A. Hasani Zonoozi , H. Haghi

As an alternative to dark matter models we use generalized Jordan-Brans-Dicke scalar-vector-tensor (JBD-SVT) gravity model to study the behavior of the rotational velocities of test particles moving around galaxies. To do so we consider an…

广义相对论与量子宇宙学 · 物理学 2019-06-05 Hossein Ghaffarnejad , Razieh Dehghani

The Tajmar anomaly is an unexplained acceleration observed by gyroscopes close to, but isolated from, rotating rings cooled to 5K. The observed ratio between the gyroscope and ring accelerations was 3+/-1.2*10^-8 for clockwise rotations and…

宇宙学与河外天体物理 · 物理学 2015-05-28 M. E. McCulloch

Galaxies are huge physical systems having dimensions of many tens of thousands of light years. Thus any change at the galactic center will be noticed at the rim only tens of thousands of years later. Those retardation effects seem to be…

综合物理 · 物理学 2021-11-01 A. Yahalom

We propose an action-based $ f(R) $ modification of Einstein's gravity which admits of a modified Schwarzschild-deSitter metric. In the weak field limit this amounts to adding a small logarithmic correction to the newtonian potential. A…

天体物理学 · 物理学 2009-11-11 Y. Sobouti

A disk-shaped universe (encompassing the observable universe) rotating globally with an angular speed equal to the Hubble constant is postulated. It is shown that dark energy and dark matter are cosmic inertial effects resulting from such a…

综合物理 · 物理学 2016-06-03 Serkan Zorba

Observations show that for disk galaxies the fourth power of the circular velocity of stars around the core of the galaxy is proportional to the luminosity L. This is known as the Tully-Fisher law. Since L is proportional to the mass M of…

天体物理学 · 物理学 2007-05-23 Silvia Behar , Moshe Carmeli

We show that ultra-light scalar dark matter (fuzzy dark matter) in galaxies has a quantum mechanical typical acceleration scale about $10^{-10}\,\mbox{ms}^{-2}$, which leads to the baryonic Tully-Fisher relation. Baryonic matter at central…

星系天体物理 · 物理学 2019-07-02 Jae-Weon Lee , Hyeong-Chan Kim , Jungjai Lee

The Tajmar effect is an unexplained acceleration observed by accelerometers and laser gyroscopes close to rotating supercooled rings. The observed ratio between the gyroscope and ring accelerations was 3+/-1.2x10^-8. Here, a new model for…

宇宙学与河外天体物理 · 物理学 2011-09-21 M. E. McCulloch

Alterations of the gravity Lagrangian introduced in modified torsion gravity theories---also referred to as $f(T)$ gravity---allows for an accelerated expansion in a matter dominated Universe. In this framework, the cosmic speed up is…

宇宙学与河外天体物理 · 物理学 2014-04-23 Stefano Camera , Vincenzo F. Cardone , Ninfa Radicella

We use a new deprojection formula to infer the gravitational potential around isolated galaxies from weak gravitational lensing. The results imply circular velocity curves that remain flat for hundreds of kpc, greatly extending the classic…

星系天体物理 · 物理学 2024-06-21 Tobias Mistele , Stacy McGaugh , Federico Lelli , James Schombert , Pengfei Li

This work explores modified inertia in the context of galactic dynamics by investigating the consequences of introducing quantum-motivated bounds on acceleration. Building on earlier ideas related to maximal acceleration and quantum speed…

广义相对论与量子宇宙学 · 物理学 2026-02-24 Jonathan Gillot
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