1,853 research outputs found
General circular velocity relation of a test particle in a 3D gravitational potential: application to the rotation curves analysis and total mass determination of UGC 8490 and UGC 9753
In this paper we derive a novel circular velocity relation for a test
particle in a 3D gravitational potential applicable to every system of
curvilinear coordinates, suitable to be reduced to orthogonal form. As an
illustration of the potentiality of the determined circular velocity expression
we perform the rotation curves analysis of UGC 8490 and UGC 9753 and we
estimate the total and dark matter mass of these two galaxies under the
assumption that their respective dark matter halos have spherical, prolate and
oblate spheroidal mass distributions. We employ stellar population synthesis
models and the total HI density map to obtain the stellar and HI+He+metals
rotation curves of both galaxies. The subtraction of the stellar plus gas
rotation curves from the observed rotation curves of UGC 8490 and UGC 9753
generates the dark matter circular velocity curves of both galaxies. We fit the
dark matter rotation curves of UGC 8490 and UGC 9753 through the newly
established circular velocity formula specialised to the spherical, prolate and
oblate spheroidal mass distributions, considering the Navarro, Frenk and White,
Burkert, Di Cintio, Einasto and Stadel dark matter halos. Our principal
findings are the following: globally, cored dark matter profiles Burkert and
Einasto prevail over cuspy Navarro, Frenk and White and Di Cintio. Also,
spherical/oblate dark matter models fit better the dark matter rotation curves
of both galaxies than prolate dark matter halos.Comment: 23 pages, 16 figures, published in MNRAS Main Journa
Numerical simulations of flow and mass transport processes in the anterior chamber in the presence of an iris-fixated intraocular lens
An off-shell I.R. regularization strategy in the analysis of collinear divergences
We present a method for the analysis of singularities of Feynman amplitudes
based on the Speer sector decomposition of the Schwinger parametric integrals
combined with the Mellin-Barnes transform. The sector decomposition method is
described in some details. We suggest the idea of applying the method to the
analysis of collinear singularities in inclusive QCD cross sections in the
mass-less limit regularizing the forward amplitudes by an off-shell choice of
the initial particle momenta. It is shown how the suggested strategy works in
the well known case of the one loop corrections to Deep Inelastic Scattering.Comment: 25 pages, 3 figure
2D kinematics of the edge-on spiral galaxy ESO 379-G006
We present a kinematical study of the nearly edge-on galaxy ESO 379-G006 that
shows the existence of extraplanar ionized gas. With Fabry-Perot spectroscopy
at H-alpha, we study the kinematics of ESO 379-G006 using velocity maps and
position-velocity diagrams parallel to the major and to the minor axis of the
galaxy. We build the rotation curve of the disk and discuss the role of
projection effects due to the fact of viewing this galaxy nearly edge-on. The
twisting of the isovelocities in the radial velocity field of the disk of ESO
379-G006 as well as the kinematic asymmetries found in some position-velocity
diagrams parallel to the minor axis of the galaxy suggest the existence of
deviations to circular motions in the disk that can be modeled and explained
with the inclusion of a radial inflow probably generated by a bar or by spiral
arms. We succeeded in detecting extraplanar Diffuse Ionized Gas in this galaxy.
At the same time, from the analysis of position-velocity diagrams, we found
some evidence that the extraplanar gas could lag in rotation velocity with
respect to the midplane rotation.Comment: 61 pages, 15 figures. Accepted for publication in A
A Finite Element Study of Electromagnetic Riveting
Electromagnetic riveting, used in some aerospace assembly processes, involves rapid deformation, leading to the finished rivet configuration. Analysis of this process is described for the case of an aluminum rivet joining typical aluminum structural elements. The analysis is based on a finite element method that includes the effects of heating, due to rapid plastic deformation of the material, on the material properties. Useful details of material deformation and thermal history and the final rivet and structure configuration and states of stress and strain are obtained. These results have significant implications in the design, implementation, and improvement of practical fastening processes in the aerospace industry
A 3D porous media liver lobule model: the importance of vascular septa and anisotropic permeability for homogeneous perfusion
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