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相关论文: Can TeVeS avoid Dark Matter on galactic scales?

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The validity of MOND and TeVeS models of modified gravity has been recently tested by using lensing techniques, with the conclusion that a non-trivial component in the form of dark matter is needed in order to match the observations. In…

宇宙学与河外天体物理 · 物理学 2015-06-05 Ignacio Ferreras , Nick Mavromatos , Mairi Sakellariadou , Muhammad Furqaan Yusaf

We constrain the one-parameter class of TeVeS models by testing the theory against both rotation curve and strong gravitational lensing data on galactic scales, remaining fully relativistic in our formalism. The upshot of our analysis is…

星系天体物理 · 物理学 2009-11-10 Ignacio Ferreras , Nick E. Mavromatos , Mairi Sakellariadou , Muhammad Furqaan Yusaf

To further test MOdified Newtonian Dynamics (MOND) on galactic scales -- originally proposed to explain the rotation curves of disk galaxies without dark matter -- we study a sample of six strong gravitational lensing early-type galaxies…

天体物理学 · 物理学 2008-11-26 Ignacio Ferreras , Mairi Sakellariadou , Muhammad Furqaan Yusaf

Bekenstein's (2004) TeVeS theory has added an interesting twist to the search for dark matter and dark energy, modifying the landscape of gravity-related astronomy day by day. Built bottom-up rather than top-down as most gravity theories,…

天体物理学 · 物理学 2007-05-23 HongSheng Zhao

We propose to use multiple-imaged gravitational lenses to set limits on gravity theories without dark matter, specificly TeVeS (Bekenstein 2004), a theory which is consistent with fundamental relativistic principles and the phenomenology of…

天体物理学 · 物理学 2009-11-11 HongSheng Zhao , David J. Bacon , Andy N. Taylor , Keith Horne

Modified Newtonian Dynamics (MOND) and its relativistic version - TeVeS offer us an alternative perspective to understand the universe without the demand of the elusive cold dark matter. This MONDian paradigm is not only competitive with…

天体物理学 · 物理学 2008-12-31 M. C. Chiu , Y. Tian , C. M. Ko

Aims: We explore the lensing properties of asymmetric matter density distributions in Bekenstein's Tensor-Vector-Scalar theory (TeVeS). Methods: Using an iterative Fourier-based solver for the resulting non-linear scalar field equation, we…

天体物理学 · 物理学 2008-03-06 M. Feix , C. Fedeli , M. Bartelmann

The phenomena customly described with the standard $\Lambda$CDM model are broadly reproduced by an extremely simple model in TeVeS, Bekenstein's (2004) modification of General Relativity motivated by galaxy phenomenology. Our model can…

天体物理学 · 物理学 2008-11-26 HongSheng Zhao

The premier alternative to the dark matter paradigm is modified gravity. Following an introduction to the relevant phenomenology of galaxies, I review the MOND paradigm, an effective summary of the observations which any theory must…

宇宙学与河外天体物理 · 物理学 2010-01-25 Jacob D. Bekenstein

Using strong lensing data Milgrom's MOdified Newtonian Dynamics (MOND) or its covariant TeVeS (Tensor-Vector-Scalar Theory) is being examined here as an alternative to the conventional $\Lambda$CDM paradigm. We examine 10 double-image…

星系天体物理 · 物理学 2011-05-10 Mu-Chen Chiu , Chung-Ming Ko , Yong Tian , HongSheng Zhao

The impressive success of the standard cosmological model has suggested to many that its ingredients are all one needs to explain galaxies and their systems. I summarize a number of known problems with this program. They might signal the…

宇宙学与河外天体物理 · 物理学 2013-11-06 Jacob D. Bekenstein

Among modified gravitational theories, the Tensor-Vector-Scalar (TeVeS) occupies a special place -- it is a covariant theory of gravity that produces the modified Newtonian dynamics (MOND) in the nonrelativistic weak field limit and…

高能物理 - 理论 · 物理学 2014-07-08 Masud Chaichian , Josef Kluson , Markku Oksanen , Anca Tureanu

Observations of spiral galaxies strongly support a one-to-one analytical relation between the inferred gravity of dark matter at any radius and the enclosed baryonic mass. It is baffling that baryons manage to settle the dark matter…

天体物理学 · 物理学 2008-11-26 Benoit Famaey , Gianfranco Gentile , Jean-Philippe Bruneton , HongSheng Zhao

Time delay in galaxy gravitational lensing systems has been used to determine the value of Hubble constant. As in other dynamical phenomena at the scale of galaxy, dark matter is often invoked in gravitational lensing to account for the…

宇宙学与河外天体物理 · 物理学 2013-10-10 Yong Tian , Chung-Ming Ko , Mu-Chen Chiu

Bekenstein's Tensor-Vector-Scalar (TeVeS) theory has had considerable success in explaining various phenomena without the need for dark matter. However, it is difficult to observationally discern the differences between TeVeS and…

天体物理学 · 物理学 2010-04-21 Paul D. Lasky , Hajime Sotani , Dimitrios Giannios

A relativistic theory of gravity has recently been proposed by Bekenstein, where gravity is mediated by a tensor, a vector and a scalar field, thus called TeVeS. The theory aims at modifying gravity in such a way as to reproduce Milgrom's…

天体物理学 · 物理学 2009-11-13 Constantinos Skordis

If it is hypothesised that there is no dark matter then some alternative gravitational theory must take the place of general relativity (GR) on the largest scales. Dynamical measurements can be used to investigate the nature of such a…

天体物理学 · 物理学 2008-11-26 Daniel J. Mortlock , Edwin L. Turner

The tensor-vector-scalar (TeVeS) model is considered a viable theory of gravity. It produces the Milgrom's modified Newtonian dynamics in the nonrelativistic weak field limit and is free from ghosts. This model has been tested against…

宇宙学与河外天体物理 · 物理学 2015-10-14 Xiao-dong Xu , Bin Wang , Pengjie Zhang

An alternative theory of gravity has recently been proposed by Bekenstein, named Tensor-Vector-Scalar (TeVeS) theory, which can explain many galactic and cosmological observations without the need for dark matter. Whilst this theory passes…

广义相对论与量子宇宙学 · 物理学 2009-11-13 Hajime Sotani

Certain covariant theories of the modified Newtonian dynamics paradigm seem to require an additional hot dark matter (HDM) component - in the form of either heavy ordinary neutrinos or more recently light sterile neutrinos (SNs) with a mass…

宇宙学与河外天体物理 · 物理学 2016-05-24 Martin Feix , HongSheng Zhao , Cosimo Fedeli , José Luis Garrido Pestaña , Henk Hoekstra
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