10,520 research outputs found
Analysis of water absorbency into knitted spacer structures
The absorbency properties of knitted structures are very important in designing garments that both remove liquid sweat from the skin and provide tactile and sensorial comfort to the wearer. Water absorbency by knitted spacer structures was experimentally investigated using a gravimetric absorbency tester to record absorbency rate, total absorbency, and time taken to saturate the structure. The geometry of spacer structures was analyzed and a model created to define the capillary characteristic in the spacer yarn. Absorbency into the spacer structures was modeled using the fabric parameters, the capillary radius, and the properties of water. Experimental and theoretical results were compared to validate the models
Searching for unknown open clusters in the Tycho-2 catalog
We present 11 new open cluster candidates found in a systematic search for
unknown star clusters using the astrometric and photometric data included in
the Tycho2 catalog. The possible existence of these stellar aggregates is
supported by the analysis of proper motions, color-magnitude diagrams, stellar
density distributions, and by the visual inspection of the Digitized Sky Survey
(DSS) plates. With these tools we were able to determine mean absolute proper
motions as well as preliminary reddenings, distances and ages for the majority
of the candidates. We found that most of them are possibly nearby (closer than
about 600 pc) open clusters never studied before.Comment: 14 pages, 6 figures. Accepted by A&
A new form of the rotating C-metric
In a previous paper, we showed that the traditional form of the charged
C-metric can be transformed, by a change of coordinates, into one with an
explicitly factorizable structure function. This new form of the C-metric has
the advantage that its properties become much simpler to analyze. In this
paper, we propose an analogous new form for the rotating charged C-metric, with
structure function G(\xi)=(1-\xi^2)(1+r_{+}A\xi)(1+r_{-}A\xi), where r_\pm are
the usual locations of the horizons in the Kerr-Newman black hole. Unlike the
non-rotating case, this new form is not related to the traditional one by a
coordinate transformation. We show that the physical distinction between these
two forms of the rotating C-metric lies in the nature of the conical
singularities causing the black holes to accelerate apart: the new form is free
of torsion singularities and therefore does not contain any closed timelike
curves. We claim that this new form should be considered the natural
generalization of the C-metric with rotation.Comment: 13 pages, LaTe
Small Kerr-anti-de Sitter black holes are unstable
Superradiance in black hole spacetimes can trigger instabilities. Here we
show that, due to superradiance, small Kerr-anti-de Sitter black holes are
unstable. Our demonstration uses a matching procedure, in a long wavelength
approximation.Comment: 7 pages, 1 figure, RevTeX
Symmetries and Ambiguities in the linear sigma model with light quarks
We investigate the role of undetermined finite contributions generated by
radiative corrections in a linear sigma model with quarks.
Although some of such terms can be absorbed in the renormalization procedure,
one such contribution is left in the expression for the pion decay constant.
This arbitrariness is eliminated by chiral symmetry.Comment: 9 pages. Added references through the text; an author was added due
to an important contribution; corrected typos; the title also was changed.
Submitted to Modern Physics Letter
Perturbations and absorption cross-section of infinite-radius black rings
We study scalar field perturbations on the background of non-supersymmetric
black rings and of supersymmetric black rings. In the infinite-radius limit of
these geometries, we are able to separate the wave equation, and to study wave
phenomena in its vicinities. In this limit, we show that (i) both geometries
are stable against scalar field perturbations, (ii) the absorption
cross-section for scalar fields is equal to the area of the event horizon in
the supersymmetric case, and proportional to it in the non-supersymmetric
situation.Comment: ReVTeX4. 15 pages, 3 figures. References added. Published versio
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