363 research outputs found
Rewriting systems and biautomatic structures for Chinese, hypoplactic, and sylvester monoids
This paper studies complete rewriting systems and biautomaticity for three interesting classes of finite-rank homogeneous monoids: Chinese monoids, hypoplactic monoids, and sylvester monoids. For Chinese monoids, we first give new presentations via finite complete rewriting systems, using more lucid constructions and proofs than those given independently by Chen & Qui and Güzel Karpuz; we then construct biautomatic structures. For hypoplactic monoids, we construct finite complete rewriting systems and biautomatic structures. For sylvester monoids, which are not finitely presented, we prove that the standard presentation is an infinite complete rewriting system, and construct biautomatic structures. Consequently, the monoid algebras corresponding to monoids of these classes are automaton algebras in the sense of Ufnarovskij
Small quark stars in the chromodielectric model
Equations of state for strange quark matter in beta equilibrium at high
densities are used to investigate the structure (mass and radius) of compact
objects. The chromodielectric model is used as a general framework for the
quark interactions, which are mediated by chiral mesons, and , and by a confining chiral singlet dynamical field, . Using a
quartic potential for , two equations of state for the same set of model
parameters are obtained, one with a minimum at around the nuclear matter
density and the other at . Using the latter
equation of state in the Tolman-Oppenheimer-Volkoff equations we found
solutions corresponding to compact objects with km and . The phenomenology of recently discovered X-ray sources is compatible
with the type of quark stars that we have obtained.Comment: 8 pages, AIP macros; Talk delivered at the Pan American Advanced
Studies Institute (PASI) Conference "New States of Matter in Hadronic
Interactions", Campos do Jordao, Brazil, January 200
Gravitational waves in the theory of gravity
There is a host of alternative theories of gravitation in the literature,
among them the recently elaborated by Harko and collaborators. In
these theories the and are respectively the Ricci scalar and the trace
of the energy momentum tensor. There is already in literature a series of
studies of different forms of the functions as well as their
cosmological consequences. However, there is not so far in the literature
studies related to the gravitational waves in gravity. Here we
consider such an issue, in particular studying the putative extra polarization
models that can well appear in such theories. To do that, we consider different
functional forms for .Comment: 7 pages, no figures, accepted for publication in Physical Review
Constraining relativistic models through heavy ion collisions
Relativistic models can be successfully applied to the description of compact
star properties in nuclear astrophysics as well as to nuclear matter and finite
nuclei properties, these studies taking place at low and moderate temperatures.
Nevertheless, all results are model dependent and so far it is unclear whether
some of them should be discarded. Moreover, in the regime of hot hadronic
matter very few calculations exist using these relativistic models, in
particular when applied to particle yields in heavy ion collisions.
In the present work we comment on the known constraints that can help the
selection of adequate models in this regime and investigate the main
differences that arise when the particle production during a Au+Au collision at
RHIC is calculated with different models.Comment: 9 pages, 1 figure, 3 table
Finite Nuclei in a Relativistic Mean-Field Model with Derivative Couplings
We study finite nuclei, at the mean-field level, using the Zimanyi-Moskowski
model and one of its variations (the ZM3 model). We calculate energy levels and
ground-state properties in nuclei where the mean-field approach is reliable.
The role played by the spin-orbit potential in sorting out mean-field model
descriptions is emphasized.Comment: 17 pages, 9 figures, 30 kbytes. Uses EPSF.TEX. To appear in Zeit. f.
Phys. A (Hadrons and Nuclei
Stellar equilibrium configurations of white dwarfs in the gravity
In this work we investigate the equilibrium configurations of white dwarfs in
a modified gravity theory, na\-mely, gravity, for which and
stand for the Ricci scalar and trace of the energy-momentum tensor,
respectively. Considering the functional form , with
being a constant, we obtain the hydrostatic equilibrium equation for
the theory. Some physical properties of white dwarfs, such as: mass, radius,
pressure and energy density, as well as their dependence on the parameter
are derived. More massive and larger white dwarfs are found for
negative values of when it decreases. The equilibrium configurations
predict a maximum mass limit for white dwarfs slightly above the Chandrasekhar
limit, with larger radii and lower central densities when compared to standard
gravity outcomes. The most important effect of theory for massive
white dwarfs is the increase of the radius in comparison with GR and also
results. By comparing our results with some observational data of
massive white dwarfs we also find a lower limit for , namely, .Comment: To be published in EPJ
Object transportation by a human and a mobile manipulator : a dynamical systems approach
In this paper we address the problem of humanrobot joint transportation of large payloads. The human brings to the task knowledge on the goal destination and global path planning. The robot has no prior knowledge of the environment
and must autonomously help the human, while simultaneously
avoiding static and/or dynamic obstacles that it encounters. For
this purpose a dynamic control architecture, formalized as a
coupled system of non-linear differential equations, is designed
to control the behavior of the mobile manipulator in close loop
with the acquired sensorial information. Verbal communication
is integrated that allows the robot to communicate its limitations.
Results show the robot’s ability to generate stable, smooth and
robust behavior in unstructured and dynamic environments.
Furthermore, the robot is able to explain the difficulties it
encounters and thus contribute to success of the task and to
enhance the human-robot physical interaction.FP6-IST2-EU-project JAST (project no 003747)Portuguese Science and Technology Foundation (FCT) and FEDER project COOPDYN (POSI/SRI/38081/2001)
Hadronic Entropy Enhancement and Low Density QGP
Recent studies show that for central collisions the rising of the incident
energy from AGS to RHIC decreases the value of the chemical potential in the
Hadron-QGP phase diagram. Thus, the formation of QGP at RHIC energies in
central collisions may be expected to occur at very small values of the
chemical potential. Using many different relativistic mean-field hadronic
models (RMF) at this regime we show that the critical temperature for the
Hadron-QGP transition is hadronic model independent. We have traced back the
reason for this and conclude that it comes from the fact that the QGP entropy
is much larger than the hadronic entropy obtained in all the RMF models. We
also find that almost all of these models present a strong entropy enhancement
in the hadronic sector coming from the baryonic phase transition to a
nucleon-antinucleon plasma. This result is in agreement with the recent data
obtained in the STAR collaboration at RHIC where it was found a rich
proton-antiproton matter
Seleção de fungos entomopatogênicos para o controle de Dactylopius opuntiae Cockerel (Hemiptera: Dactylopiidae) no Semi-Árido nordestino.
O objetivo deste trabalho foi selecionar fungos entomopatogênicos para controle de ninfas migrantes de Dactylopius opuntiae
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