7,125 research outputs found
Models of relativistic particle with curvature and torsion revisited
Models, describing relativistic particles, where Lagrangian densities depend
linearly on both the curvature and the torsion of the trajectories, are
revisited in D=3 space forms. The moduli spaces of trajectories are completely
and explicitly determined using the Lancret program. The moduli subspaces of
closed solitons in the three sphere are also determined.Comment: 13 page
Breaking a Chaotic Cryptographic Scheme Based on Composition Maps
Recently, a chaotic cryptographic scheme based on composition maps was
proposed. This paper studies the security of the scheme and reports the
following findings: 1) the scheme can be broken by a differential attack with
chosen-plaintext, where is the size of
plaintext and is the number of different elements in plain-text; 2) the
scheme is not sensitive to the changes of plaintext; 3) the two composition
maps do not work well as a secure and efficient random number source.Comment: 9 pages, 7 figure
Large reduction with the Twisted Eguchi-Kawai model
We examine the breaking of symmetry recently reported for the Twisted
Eguchi-Kawai model (TEK). We analyse the origin of this behaviour and propose
simple modifications of twist and lattice action that could avoid the problem.
Our results show no sign of symmetry breaking and allow us to obtain values of
the large infinite volume string tension in agreement with extrapolations
from results based upon straightforward methods.Comment: latex file 14 pages, 4 figure
Combinatorics of lattice paths with and without spikes
We derive a series of results on random walks on a d-dimensional hypercubic
lattice (lattice paths). We introduce the notions of terse and simple paths
corresponding to the path having no backtracking parts (spikes). These paths
label equivalence classes which allow a rearrangement of the sum over paths.
The basic combinatorial quantities of this construction are given. These
formulas are useful when performing strong coupling (hopping parameter)
expansions of lattice models. Some applications are described.Comment: Latex. 25 page
La boîte à outils géotechnique de demain: conception des structures géotechniques selon EN 1997: 202x
This paper shows how three new concepts – ‘Design Cases’ (introduced in prEN 1990), the ‘Geotechnical Design Model’ (prEN 1997-1), and the ‘Ground Model’ (prEN 1997-2) – are combined (in prEN 1997-3) to provide a comprehensive and flexible set of tools for the design of specific geotechnical structures. The paper presents flow charts divided between: a) reliability management, b) ground modelling, c) verification of the design, and d) structure execution, which provide guidelines for navigating prEN 1990 and prEN 1997.Postprint (published version
Menos es más (complejidad). Una reflexión sobre la concepción de complejidad predominante en el pensamiento decrecentista
Asociado a los límites biofísicos es frecuente encontrar la idea de que el decrecimiento supone una descomplejización del sistema social. Creemos que esta idea se fundamenta en una concepción del concepto de complejidad asociada a variables cuantitativas y a la idea de que lo “primitivo” y “menos complejo” incrementa la resiliencia de la población. Proponemos utilizar la noción de complejidad sustentada en la obra de Edgar Morin, concepción que nos ayuda a entender que el decrecimiento no supone, inevitablemente, un decremento de la complejidad del sistema social
VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A), sigma Oph, BM Sco, and HD 206859
We add four warmer late-type supergiants to our previous
spectro-interferometric studies of red giants and supergiants.
V766 Cen (=HR 5171 A) is found to be a high-luminosity log(L/L_sun)=5.8+-0.4
source of Teff 4290+-760 K and radius 1490+-540 Rsun located close to both the
Hayashi and Eddington limits; this source is consistent with a 40 Msun
evolutionary track without rotation and current mass 27-36 Msun. It exhibits
NaI in emission arising from a shell of radius 1.5 Rphot and a photocenter
displacement of about 0.1 Rphot. V766 Cen shows strong extended molecular (CO)
layers and a dusty circumstellar background component. This suggest an
optically thick pseudo-photosphere at about 1.5 Rphot at the onset of the wind.
V766 Cen is a red supergiant located close to the Hayashi limit instead of a
yellow hypergiant already evolving back toward warmer Teff as previously
discussed.
The stars sigma Oph, BM Sco, and HD 206859 are found to have lower
luminosities of about log(L/Lsun)=3.4-3.5 and Teff of 3900-5300 K,
corresponding to 5-9 Msun tracks. They do not show extended molecular layers as
observed for higher luminosity red supergiants of our sample. BM Sco shows an
unusually strong contribution by an over-resolved circumstellar dust component.
These stars are more likely high-mass red giants instead of red supergiants.
This leaves us with an unsampled locus in the HR diagram corresponding to
luminosities log(L/Lsun)~3.8-4.8 or masses 10-13 Msun, possibly corresponding
to the mass region where stars explode as type II-P supernovae during the RSG
stage.
Our previously found relation of increasing strength of extended molecular
layers with increasing luminosities is now confirmed to extend to double our
previous luminosities and up to the Eddington limit. This might further point
to steadily increasing radiative winds with increasing luminosity.
[Abridged]Comment: 16 pages, 14 figures, accepted for publication in Astronomy and
Astrophysics (A&A
Radio detection of the young binary HD 160934
Precise determination of dynamical masses of pre-main-sequence (PMS) stars is
essential to calibrate stellar evolution models that are widely used to derive
theoretical masses of young low-mass objects. Binary stars in young, nearby
loose associations are particularly good candidates for this calibration since
all members share a common age. Interestingly, some of these young binaries
present a persistent and compact radio emission, which makes them excellent
targets for astrometric VLBI studies. We aim to monitor the orbital motion of
the binary system HD 160934, a member of the AB Doradus moving group. We
observed HD 160934 with the Very Large Array and the European VLBI Network at
8.4 and 5 GHz, respectively. The orbital information derived from these
observations was analyzed along with previously reported orbital measurements.
We show that the two components of the binary, HD 160934 A and HD 160934 c,
display compact radio emission at VLBI scales, providing precise information on
the relative orbit. Revised orbital elements were estimated. Future VLBI
monitoring of this pair should determine precise model-independent mass
estimates for the A and c components, which will serve as calibration tests for
PMS evolutionary models.Comment: 5 pages, 5 figures, accepted for publication in A&
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