4,314 research outputs found
Ising t-J model close to half filling: A Monte Carlo study
Within the recently proposed doped-carrier representation of the projected
lattice electron operators we derive a full Ising version of the t-J model.
This model possesses the global discrete Z_2 symmetry as a maximal spin
symmetry of the Hamiltonian at any values of the coupling constants, t and J.
In contrast, in the spin anisotropic limit of the t-J model, usually referred
to as the t-J_z model, the global SU(2) invariance is fully restored at J_z=0,
so that only the spin-spin interaction has in that model the true Ising form.
We discuss a relationship between those two models and the standard isotropic
t-J model. We show that the low-energy quasiparticles in all three models share
the qualitatively similar properties at low doping and small values of J/t. The
main advantage of the proposed Ising t-J model over the t-J_z one is that the
former allows for the unbiased Monte Carlo calculations on large clusters of up
to 10^3 sites. Within this model we discuss in detail the destruction of the
antiferromagnetic order by doping as well as the interplay between the AF order
and hole mobility. We also discuss the effect of the exchange interaction and
that of the next nearest neighbour hoppings on the destruction of the AF order
at finite doping. We show that the short-range AF order is observed in a wide
range of temperatures and dopings, much beyond the boundaries of the AF phase.
We explicitly demonstrate that the local no double occupancy constraint plays
the dominant role in destroying the magnetic order at finite doping. Finally, a
role of inhomogeneities is discussed.Comment: 24 pages, 10 figure
Dynamics of Enceladus and Dione inside the 2:1 Mean-Motion Resonance under Tidal Dissipation
In a previous work (Callegari and Yokoyama 2007, Celest. Mech. Dyn. Astr.
vol. 98), the main features of the motion of the pair Enceladus-Dione were
analyzed in the frozen regime, i.e., without considering the tidal evolution.
Here, the results of a great deal of numerical simulations of a pair of
satellites similar to Enceladus and Dione crossing the 2:1 mean-motion
resonance are shown. The resonance crossing is modeled with a linear tidal
theory, considering a two-degrees-of-freedom model written in the framework of
the general three-body planar problem. The main regimes of motion of the system
during the passage through resonance are studied in detail. We discuss our
results comparing them with classical scenarios of tidal evolution of the
system. We show new scenarios of evolution of the Enceladus-Dione system
through resonance not shown in previous approaches of the problem.Comment: 36 pages, 12 figures. Accepted in Celestial Mechanics and Dynamical
Astronom
A new analysis of the GJ581 extrasolar planetary system
We have done a new analysis of the available observations for the GJ581
exoplanetary system. Today this system is controversial due to choices that can
be done in the orbital determination. The main ones are the ocurrence of
aliases and the additional bodies - the planets f and g - announced in Vogt et
al. 2010. Any dynamical study of exoplanets requires the good knowledge of the
orbital elements and the investigations involving the planet g are particularly
interesting, since this body would lie in the Habitable Zone (HZ) of the star
GJ581. This region,for this system, is very attractive of the dynamical point
of view due to several resonances of two and three bodies present there. In
this work, we investigate the conditions under which the planet g may exist. We
stress the fact that the planet g is intimately related with the orbital
elements of the planet d; more precisely, we conclude that it is not possible
to disconnect its existence from the determination of the eccentricity of the
planet d. Concerning the planet f, we have found one solution with period
days, but we are judicious about any affirmation concernig this
body because its signal is in the threshold of detection and the high period is
in a spectral region where the ocorruence of aliases is very common. Besides,
we outline some dynamical features of the habitable zone with the dynamical map
and point out the role played by some resonances laying there.Comment: 12 pages, 9 figure
Chirikov Diffusion in the Asteroidal Three-Body Resonance (5,-2,-2)
The theory of diffusion in many-dimensional Hamiltonian system is applied to
asteroidal dynamics. The general formulations developed by Chirikov is applied
to the Nesvorn\'{y}-Morbidelli analytic model of three-body (three-orbit)
mean-motion resonances (Jupiter-Saturn-asteroid system). In particular, we
investigate the diffusion \emph{along} and \emph{across} the separatrices of
the (5,-2,-2) resonance of the (490) Veritas asteroidal family and their
relationship to diffusion in semi-major axis and eccentricity. The estimations
of diffusion were obtained using the Melnikov integral, a Hadjidemetriou-type
sympletic map and numerical integrations for times up to years.Comment: 27 pages, 6 figure
Topological Hall effect induced by classical large-spin background: path-integral approach
The coherent-state path-integral technique is employed to study
lattice electrons strongly coupled to a quantum spin background. In the
large-spin limit it is replaced with its classical counterpart that breaks the
time-reversal symmetry. The fermions propagating through a classical large-spin
texture may then exhibit the topological Hall effect which arises even for a
zero scalar spin chirality of the underlying spin background.Comment: 6 pages, 9 figure
Subsídio metodológico à integração da gestão de recursos hídricos com a gestão territorial, considerando as políticas florestal, agrícola e municipal urbana
Na tentativa de apoiar a efetivação da gestão de recursos hídricos no Brasil, segundo a Lei 9433/1997, pesquisas vêm sendo desenvolvidas em contribuição à integração da gestão de recursos hídricos com a gestão municipal/territorial. Neste contexto, o presente estudo, dando continuidade a trabalho com metodologia desenvolvida para integração ente a política de recursos hídricos com a política urbana, buscou expandir a integração de instrumentos da gestão de recursos
hídricos com outras políticas setoriais, fortemente incidentes em regiões rurais, através da adaptação de modelo conceitual. Tomando-se as políticas agrícola e florestal como exemplo daquelas fortemente atuantes em regiões rurais, e como referência procedimentos metodológicos de análise e agrupamento de, e avaliação
de interface entre, instrumentos de gestão de políticas, as principais etapas que compreenderam o desenvolvimento do trabalho foram: 1- identificação, análise e agrupamento de instrumentos de gestão das políticas agrícola e florestal; e 2- avaliação das inter-relações entre grupos de instrumentos de gestão de recursos hídricos com grupos de instrumentos de gestão agrícola, florestal e urbana. O desenvolvimento de extensiva pesquisa bibliográfica e documental foi de grande
relevância em suporte à realização de todas as fases da pesquisa. Entre as principais conclusões do trabalho destaca-se: a adaptação do Modelo Conceitual para a integração entre a política de recursos hídricos e a política urbana mostrou-se promissor no que se refere à identificação de possibilidades de integração de grupos de instrumentos de gestão de recursos hídricos com grupos de instrumentos de gestão de outras políticas setoriais (uma ou mais) incidentes em regiões urbana e/ou rurais), avaliadas individualmente ou em conjunto, com base na afinidade entre as finalidades de tais grupos. Por fim, são feitas algumas recomendações para o desenvolvimento de futuros estudos
Capybara (Hydrochoerus hydrochaeris) distribution in agroecosystems: a cross-scale habitat analysis.
On the dynamics of Extrasolar Planetary Systems under dissipation. Migration of planets
We study the dynamics of planetary systems with two planets moving in the
same plane, when frictional forces act on the two planets, in addition to the
gravitational forces. The model of the general three-body problem is used.
Different laws of friction are considered. The topology of the phase space is
essential in understanding the evolution of the system. The topology is
determined by the families of stable and unstable periodic orbits, both
symmetric and non symmetric. It is along the stable families, or close to them,
that the planets migrate when dissipative forces act. At the critical points
where the stability along the family changes, there is a bifurcation of a new
family of stable periodic orbits and the migration process changes route and
follows the new stable family up to large eccentricities or to a chaotic
region. We consider both resonant and non resonant planetary systems. The 2/1,
3/1 and 3/2 resonances are studied. The migration to larger or smaller
eccentricities depends on the particular law of friction. Also, in some cases
the semimajor axes increase and in other cases they are stabilized. For
particular laws of friction and for special values of the parameters of the
frictional forces, it is possible to have partially stationary solutions, where
the eccentricities and the semimajor axes are fixed.Comment: Accepted in Celestial Mechanics and Dynamical Astronom
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