7,368 research outputs found
Brane cosmology with a van der Waals equation of state
The evolution of a Universe confined onto a 3-brane embedded in a
five-dimensional space-time is investigated where the cosmological fluid on the
brane is modeled by the van der Waals equation of state. It is shown that the
Universe on the brane evolves in such a manner that three distinct periods
concerning its acceleration field are attained: (a) an initial accelerated
epoch where the van der Waals fluid behaves like a scalar field with a negative
pressure; (b) a past decelerated period which has two contributions, one of
them is related to the van der Waals fluid which behaves like a matter field
with a positive pressure, whereas the other contribution comes from a term of
the Friedmann equation on the brane which is inversely proportional to the
scale factor to the fourth power and can be interpreted as a radiation field,
and (c) a present accelerated phase due to a cosmological constant on the
brane.Comment: 9 pages, 2 figures, to be published in General Relativity and
Gravitatio
A model for a non-minimally coupled scalar field interacting with dark matter
In this work we investigate the evolution of a Universe consisted of a scalar
field, a dark matter field and non-interacting baryonic matter and radiation.
The scalar field, which plays the role of dark energy, is non-minimally coupled
to space-time curvature, and drives the Universe to a present accelerated
expansion. The non-relativistic dark matter field interacts directly with the
dark energy and has a pressure which follows from a thermodynamic theory. We
show that this model can reproduce the expected behavior of the density
parameters, deceleration parameter and luminosity distance.Comment: 3 pages, 4 figures. To appear in Brazilian Journal of Physic
Irreversible processes and the accelerated-decelerated phases of the Universe
A model for the Universe is proposed where it is considered as a mixture of
scalar and matter fields. The particle production is due to an irreversible
transfer of energy from the gravitational field to the matter field and
represented by a non-equilibrium pressure. This model can simulate three
distinct periods of the Universe: (a) an accelerated epoch where the energy
density of the scalar field prevails over the matter field, (b) a past
decelerated period where the energy density of the matter field becomes more
predominant than the scalar energy density, and (c) a present acceleration
phase where the scalar energy density overcomes the energy density of the
matter field.Comment: 6 pages, 2 figures, to be published in Brazilian Journal of Physic
Irreversible Processes in a Universe modelled as a mixture of a Chaplygin gas and radiation
The evolution of a Universe modelled as a mixture of a Chaplygin gas and
radiation is determined by taking into account irreversible processes. This
mixture could interpolate periods of a radiation dominated, a matter dominated
and a cosmological constant dominated Universe. The results of a Universe
modelled by this mixture are compared with the results of a mixture whose
constituents are radiation and quintessence. Among other results it is shown
that: (a) for both models there exists a period of a past deceleration with a
present acceleration; (b) the slope of the acceleration of the Universe
modelled as a mixture of a Chaplygin gas with radiation is more pronounced than
that modelled as a mixture of quintessence and radiation; (c) the energy
density of the Chaplygin gas tends to a constant value at earlier times than
the energy density of quintessence does; (d) the energy density of radiation
for both mixtures coincide and decay more rapidly than the energy densities of
the Chaplygin gas and of quintessence.Comment: 8 pages, 1 figure, to be published in GR
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