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      Gravity with extra dimensions and dark matter interpretation: A straightforward approach

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          Abstract

          Any connection between dark matter and extra dimensions can be cognizably evinced from the associated effective energy-momentum tensor. In order to investigate and test such relationship, a higher dimensional spacetime endowed with a factorizable general metric is regarded to derive a general expression for the stress tensor -- from the Einstein-Hilbert action -- and to elicit the effective gravitational potential. A particular construction for the case of six dimensions is provided, and it is forthwith revealed that the missing mass phenomenon may be explained, irrespective of the dark matter existence. Moreover, the existence of extra dimensions in the universe accrues the possibility of a straightforward mechanism for such explanation. A configuration which density profile coincides with the Newtonian potential for spiral galaxies is constructed, from a 4-dimensional isotropic metric plus extra-dimensional components. A Miyamoto-Nagai \emph{ansatz} is used to solve Einstein equations. The stable rotation curves associated to such system are computed, in full compliance to the observational data, without fitting techniques. The density profiles are reconstructed and compared to that ones obtained from the Newtonian potential.

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          Brane worlds: the gravity of escaping matter

          In the framework of a five-dimensional model with one 3-brane and an infinite extra dimension, we discuss a process in which matter escapes from the brane and propagates into the bulk to arbitrarily large distances. An example is a decay of a particle of mass \(2m\) residing on the brane into two particles of mass \(m\) that leave the brane and accelerate away. We calculate, in the linearized theory, the metric induced by these particles on the brane. This metric does not obey the four-dimensional Einstein equations and corresponds to a spherical gravity wave propagating along the four-dimensional future light cone. The four-dimensional space-time left behind the spherical wave is flat, so the gravitational field induced in the brane world by matter escaping from the brane disappears in a causal way.
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            Constraints on the Dark Matter from Optical Rotation Curves

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              Analysis of Rotation Curves in the Framework of the Gravitational Suppression Model

              We present an analysis of suitable rotation curves (RCs) of eight galaxies, aimed at checking the consistency and universality of the gravitational suppression (GraS) hypothesis, a phenomenological model for a new interaction between dark matter and baryons. Motivated by the puzzle of the core versus cusp distribution of dark matter in the center of halos, this hypothesis claims to reconcile the predictions from N-body \Lambda cold dark matter simulations with kinematic observations. The GraS model improves the kinematic fitting residuals, but the mass parameters are unphysical and put the theory in difficulty.
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                Author and article information

                Journal
                26 March 2012
                Article
                10.1155/2013/713508
                1203.5736
                18db6767-91a5-4363-92e5-c7e10e522560

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                ISRN High Energy Physics Volume 2013 (2013), Article ID 713508, 9 pages
                13 pages, 6 figures
                gr-qc astro-ph.CO astro-ph.GA hep-ph

                Cosmology & Extragalactic astrophysics,General relativity & Quantum cosmology,Galaxy astrophysics,High energy & Particle physics

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