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1.
A new class of exact solutions of Einstein’s field equations with a bulk viscous fluid for an LRS Bianchi type-Ia obtained
by using a time dependent deceleration parameter and cosmological term Λ. The coefficient of bulk viscosity is assumed to
be a power function of mass density (ξ=ξ
0
ρ
n
). We have obtained a general solution of the field equations from which six models of the universe are derived: exponential,
polynomial and sinusoidal form respectively. The behaviour of these models of the universe are also discussed in the frame
of reference of recent supernovae Ia observations.
相似文献
2.
The properties of locally rotationally symmetric Bianchi type-II perfect fluid space-times are analyzed in Barber’s second
self-creation theory by using a special law of variation for Hubble’s parameter that yields a constant value of deceleration
parameter. By assuming the equation of state p=γ
ρ, many new solutions are obtained for different era—Zel’dovich, radiation, vacuum and vacuum energy dominated. The solutions
with power-law and exponential expansion are discussed. A detailed study of geometrical and physical parameters is carried
out. The nature of singularity is also clarified in each case. 相似文献
3.
4.
Measurements of meteoroid velocities and decelerations have been obtained from post-t
0 diffraction patterns present in echo signatures obtained from the multi-site AMOR radar operated at the University of Canterbury’s
research facility. The system allows the sampling of a meteoroid’s velocity at separated points along the body’s trajectory
to yield decelerations. The technique has potential value in providing data on the relation between trajectory behaviour,
drag characteristics, the physical structure of meteoroids and stream membership or orbit type. 相似文献
5.
An exact Bianchi type-V perfect fluid cosmological model is obtained in a scalar tensor theory proposed by Sen (Z. Phys. 149:311,
1957) based on Lyra Manifold in case of β is a constant and it is shown that this cosmological model exists only in the case of Radiation Universe (ρ=3p) if β is a function of ‘t’ using negative constant deceleration parameter. Some physical and geometrical properties of these models are discussed. 相似文献
6.
A special law of variation for Hubble’s parameter is presented in a spatially homogeneous and anisotropic Bianchi type-I space-time
that yields a constant value of deceleration parameter. Using the law of variation for Hubble’s parameter, exact solutions
of Einstein’s field equations are obtained for Bianchi-I space-time filled with perfect fluid in two different cases where
the universe exhibits power-law and exponential expansion. It is found that the solutions are consistent with the recent observations
of type Ia supernovae. A detailed study of physical and kinematical properties of the models is carried out. 相似文献
7.
We have studied the evolution of homogeneous and anisotropic Bianchi type-I cosmological models filled with perfect fluid
in Barber second self-creation theory by assuming a special law of variation for Hubble’s parameter that yield a constant
value of deceleration parameter. Some physical consequences of the models have been discussed in case of Zel’dovich fluid
and radiation dominated fluid. 相似文献
8.
9.
C. P. Singh 《Astrophysics and Space Science》2009,323(2):197-203
In this paper we consider a locally-rotationally-symmetric (LRS) Bianchi type-V perfect fluid model with variable cosmological
‘constant’ representing the energy density of vacuum. The field equations are solved with and without heat conduction by using
a variation law for the mean Hubble parameter, which is related to the average scale factor of the metric and yields a constant
value of the deceleration parameter. A constant value of deceleration parameter generates power-law form of average scale
factor which is used to find the exact solutions with and without heat conduction with decaying vacuum density. The solutions
presented here satisfy all the necessary conditions for the physically acceptability. The thermodynamical relations in decaying
vacuum fluid model are also studied in detail. 相似文献
10.
The generalized thermal theory for gravitational convection, produced from instantaneous buoyancy sources on sloping boundaries, developed in Dai and Garcia (2010) is examined in this note. An assumption implicitly made therein, that detrained fluid carries no momentum, was inappropriate and the solution was not physical in special cases. The generalized thermal theory is now improved by considering the momentum carried away by detrained mixed fluid. An asymptotic velocity–distance relation for gravity currents further downslope in the deceleration phase is provided and agreement with reported experimental data is found. 相似文献