74 research outputs found
Thermocapillary rupture in falling liquid films at moderate Reynolds numbers
An experimental study of the flow of a water film over a heated surface for Re = 15-50 was performed. The influence of the development of thermocapillary instability on the wave amplitudes, the deformation of the surface of the liquid film, and the formation of the first stable dry spot on the heater are investigated. It is shown that the interaction of waves with thermocapillary structures can lead to an increase in the critical heat flux corresponding to the rupture of the liquid film, as compared with the data known in the literature
Homogeneous singularities inside collapsing wormholes
We analyze analytically and numerically the origin of the singularity in the
course of the collapse of a wormhole with the exotic scalar field Psi with
negative energy density, and with this field Psi together with the ordered
magnetic field H. We do this under the simplifying assumptions of the spherical
symmetry and that in the vicinity of the singularity the solution of the
Einstein equations depends only on one coordinate (the homogeneous
approximation). In the framework of these assumptions we found the principal
difference between the case of the collapse of the ordinary scalar field Phi
with the positive energy density together with an ordered magnetic field H and
the collapse of the exotic scalar field Psi together with the magnetic field H.
The later case is important for the possible astrophysical manifestation of the
wormholes.Comment: 10 pages, 5 figures each of which has a),b),c),and d) sub-figures. To
be published in "Physical review. D, Particles, fields, gravitation, and
cosmology
A new method for reconstructing the density distribution of matter in the disks of spiral galaxies from the rotation velocity curve in it
In this paper we propose a new method for reconstructing the surface density
of matter in flat disks of spiral galaxies. The surface density is expressed
through observational rotation velocity curves of visible matter in the disks
of spiral galaxies. The new method is not based on quadrature of special
functions. The found solution is used for processing and analysis of
observational data from several spiral galaxies. The new method can be used to
more accurately estimate the amount of dark matter in spiral galaxies.Comment: 18 pages, 6 figure
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